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  • richardmitnick 3:29 pm on May 30, 2023 Permalink | Reply
    Tags: "Software offers new way to listen for signals from the stars", , Astrophysics, , , , , , ,   

    From The College of Arts and Sciences At Cornell University: “Software offers new way to listen for signals from the stars” 

    From The College of Arts and Sciences

    At

    Cornell University

    5.30.23

    The Breakthrough Listen Investigation for Periodic Spectral Signals (BLIPSS), led by Akshay Suresh, Cornell doctoral candidate in astronomy, is pioneering a search for periodic signals emanating from the core of our galaxy, the Milky Way. The research aims to detect repetitive patterns, a way to search for extraterrestrial intelligence (SETI) within our cosmic neighborhood.

    1
    Breakthrough Listen

    _____________________________________________________________________________________
    Breakthrough Listen Project

    1

    UC Observatories Lick Automated Planet Finder fully robotic 2.4-meter optical telescope at Lick Observatory, situated on the summit of Mount Hamilton, east of San Jose, California, USA.

    Green Bank Radio Telescope, West Virginia, USA, now the center piece of the Green Bank Observatory(US), being cut loose by the National Science Foundation(US), supported by Breakthrough Listen Project, West Virginia University, and operated by the nonprofit Associated Universities, Inc.

    CSIRO-Commonwealth Scientific and Industrial Research Organisation (AU) Parkes Observatory [ Murriyang, the traditional Indigenous name] , located 20 kilometres north of the town of Parkes, New South Wales, Australia, 414.80m above sea level.

    Newly added

    University of Arizona Veritas Four Čerenkov telescopes A novel gamma ray telescope under construction at the CfA Fred Lawrence Whipple Observatory (US), Mount Hopkins, Arizona (US), altitude 2,606 m 8,550 ft. A large project known as the Čerenkov Telescope Array, composed of hundreds of similar telescopes to be situated at Roque de los Muchachos Observatory [Instituto de Astrofísica de Canarias ](ES) in the Canary Islands and Chile at European Southern Observatory Cerro Paranal(EU) site. The telescope on Mount Hopkins will be fitted with a prototype high-speed camera, assembled at the University of Wisconsin–Madison (US) and capable of taking pictures at a billion frames per second. Credit: Vladimir Vassiliev. _____________________________________________________________________________________

    The researchers developed software based on a Fast Folding Algorithm (FFA), an efficient search method offering enhanced sensitivity to periodic sequences of narrow pulses. Their paper was published May 30 in The Astronomical Journal [below].

    Pulsars — rapidly rotating neutron stars that sweep beams of radio energy across the Earth — are natural astrophysical objects that generate periodic signals but humans also use directed periodic transmissions for a variety of applications, including radar.

    Such signals would be a good way to get someone’s attention across interstellar space, standing out from the background of non-periodic signals, as well as using much less energy than a transmitter that is broadcasting continuously.

    “BLIPSS is an example of cutting-edge software as a science multiplier for SETI,” said Suresh. “Our study introduces to SETI, for the first time, the Fast Folding Algorithm; our open-source software utilizes an FFA to crunch over 1.5 million time series for periodic signals in roughly 30 minutes.”

    BLIPSS is a collaborative effort between Cornell, the SETI Institute, and Breakthrough Listen.

    SETI Institute
    About The SETI Institute
    What is life? How does it begin? Are we alone? These are some of the questions we ask in our quest to learn about and share the wonders of the universe. At the SETI Institute we have a passion for discovery and for passing knowledge along as scientific ambassadors.

    The SETI Institute is a 501 (c)(3) nonprofit scientific research institute headquartered in Mountain View, California. We are a key research contractor to NASA and the National Science Foundation (NSF), and we collaborate with industry partners throughout Silicon Valley and beyond.

    Founded in 1984, the SETI Institute employs more than 130 scientists, educators, and administrative staff. Work at the SETI Institute is anchored by three centers: the Carl Sagan Center for the Study of Life in the Universe (research), the Center for Education and the Center for Outreach.

    The SETI Institute welcomes philanthropic support from individuals, private foundations, corporations and other groups to support our education and outreach initiatives, as well as unfunded scientific research and fieldwork.

    A Special Thank You to SETI Institute Partners and Collaborators
    Campoalto, Chile, NASA Ames Research Center, NASA Headquarters, National Science Foundation, Aerojet Rocketdyne,SRI International

    Frontier Development Lab Partners
    Breakthrough Prize Foundation, The European Space Agency [La Agencia Espacial Europea] [Agence spatiale européenne][Europäische Weltraumorganisation](EU), Google Cloud, IBM, Intel, KBRwyle. Kx Lockheed Martin, NASA Ames Research Center, Nvidia, SpaceResources Luxembourg, XPrize
    In-kind Service Providers
    • Gunderson Dettmer – General legal services, Hello Pilgrim – Website Design and Development Steptoe & Johnson – IP legal services, Danielle Futselaar

    SETI/Allen Telescope Array situated at the Hat Creek Radio Observatory, 290 miles (470 km) northeast of San Francisco, California, USA, Altitude 986 m (3,235 ft), the origins of the Institute’s search.

    March 23, 2015
    By Hilary Lebow
    The NIROSETI instrument saw first light on the Nickel 1-meter Telescope at Lick Observatory on March 15, 2015. (Photo by Laurie Hatch.)

    Astronomers are expanding the search for extraterrestrial intelligence into a new realm with detectors tuned to infrared light at UC’s Lick Observatory. A new instrument, called NIROSETI, will soon scour the sky for messages from other worlds.


    Shelley Wright of UC San Diego with NIROSETI, developed at U Toronto Dunlap Institute for Astronomy and Astrophysics (CA) at the 1-meter Nickel Telescope at Lick Observatory at UC Santa Cruz

    NIROSETI team from left to right Rem Stone UCO Lick Observatory Dan Werthimer, UC Berkeley; Jérôme Maire, U Toronto; Shelley Wright, UCSD; Patrick Dorval, U Toronto; Richard Treffers, Starman Systems. (Image by Laurie Hatch).

    Laser SETI


    There is also an installation at Robert Ferguson Observatory, Sonoma, CA aimed West for full coverage [no image available].

    SETI Institute – 189 Bernardo Ave., Suite 100
    Mountain View, CA 94043
    Phone 650.961.6633 – Fax 650-961-7099
    Privacy PolicyQuestions and Comments

    Also in the hunt, but not a part of the SETI Institute
    SETI@home, a BOINC [Berkeley Open Infrastructure for Network Computing] project originated in the Space Science Lab at UC Berkeley.

    The project significantly enhances the probability of capturing evidence of extraterrestrial technology by focusing on the central region of the Milky Way, known for its dense concentration of stars and potentially habitable exoplanets. The center of the Milky Way would also be an ideal place for aliens to place a beacon to contact large swaths of the Galaxy.

    The team tested their algorithm on known pulsars and were able to detect periodic emission as expected. They then turned to a larger dataset of scans of the Galactic Center undertaken using the Breakthrough Listen instrument on the 100-meter Green Bank Telescope (GBT) in West Virginia. In contrast to pulsars, which emit across a wide swath of radio frequencies, BLIPSS looked for repeating signals in a narrower range of frequencies, covering less than one-tenth of the width of an average FM radio station.

    “The combination of these relatively narrow bandwidths with periodic patterns could be indicative of deliberate technological activities of intelligent civilizations,” said co-author Steve Croft, Breakthrough Listen project scientist. “Breakthrough Listen captures huge volumes of data, and Akshay’s technique provides a new method to help us search that haystack for needles that could provide tantalizing evidence of advanced extraterrestrial life forms.”

    “Until now, radio SETI has primarily dedicated its efforts to the search for continuous signals,” said co-author Vishal Gajjar, a SETI Institute astronomer. “Our study sheds light on the remarkable energy efficiency of a train of pulses as a means of interstellar communication across vast distances. Notably, this study marks the first-ever comprehensive endeavor to conduct in-depth searches for these signals.”

    The Astronomical Journal

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.

    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.

    Stem Education Coalition

    The College of Arts and Sciences is a division of Cornell University. It has been part of the university since its founding, although its name has changed over time. It grants bachelor’s degrees, and masters and doctorates through affiliation with the Cornell University Graduate School. Its major academic buildings are located on the Arts Quad and include some of the university’s oldest buildings. The college offers courses in many fields of study and is the largest college at Cornell by undergraduate enrollment.

    Originally, the university’s faculty was undifferentiated, but with the founding of the Cornell Law School in 1886 and the concomitant self-segregation of the school’s lawyers, different departments and colleges formed.

    Initially, the division that would become the College of Arts and Sciences was known as the Academic Department, but it was formally renamed in 1903. The College endowed the first professorships in American history, musicology, and American literature. Currently, the college teaches 4,100 undergraduates, with 600 full-time faculty members (and an unspecified number of lecturers) teaching 2,200 courses.

    The Arts Quad is the site of Cornell’s original academic buildings and is home to many of the college’s programs. On the western side of the quad, at the top of Libe Slope, are Morrill Hall (completed in 1866), McGraw Hall (1872) and White Hall (1868). These simple but elegant buildings, built with native Cayuga bluestone, reflect Ezra Cornell’s utilitarianism and are known as Stone Row. The statue of Ezra Cornell, dating back to 1919, stands between Morrill and McGraw Halls. Across from this statue, in front of Goldwin Smith Hall, sits the statue of Andrew Dickson White, Cornell’s other co-founder and its first president.

    Lincoln Hall (1888) also stands on the eastern face of the quad next to Goldwin Smith Hall. On the northern face are the domed Sibley Hall and Tjaden Hall (1883). Just off of the quad on the Slope, next to Tjaden, stands the Herbert F. Johnson Museum of Art, designed by I. M. Pei. Stimson Hall (1902), Olin Library (1959) and Uris Library (1892), with Cornell’s landmark clocktower, McGraw Tower, stand on the southern end of the quad.

    Olin Library replaced Boardman Hall (1892), the original location of the Cornell Law School. In 1992, an underground addition was made to the quad with Kroch Library, an extension of Olin Library that houses several special collections of the Cornell University Library, including the Division of Rare and Manuscript Collections.

    Klarman Hall, the first new humanities building at Cornell in over 100 years, opened in 2016. Klarman houses the offices of Comparative Literature and Romance Studies. The building is connected to, and surrounded on three sides by, Goldwin Smith Hall and fronts East Avenue.

    Legends and lore about the Arts Quad and its statues can be found at Cornelliana.

    The College of Arts and Sciences offers both undergraduate and graduate (through the Graduate School) degrees. The only undergraduate degree is the Bachelor of Arts. However, students may enroll in the dual-degree program, which allows them to pursue programs of study in two colleges and receive two different degrees. The faculties within the college are:

    Africana Studies and Research Center*
    American Studies
    Anthropology
    Archaeology
    Asian-American Studies
    Asian Studies
    Astronomy/Astrophysics
    Biology (with the College of Agriculture and Life Sciences)
    Biology & Society Major (with the Colleges of Agriculture and Life Sciences and Human Ecology)
    Chemistry and Chemical Biology
    China and Asia-pacific Studies
    Classics
    Cognitive Studies
    College Scholar Program (frees up to 40 selected students in each class from all degree requirements and allows them to fashion a plan of study conducive to achieving their ultimate intellectual goals; a senior thesis is required)
    Comparative Literature
    Computer Science (with the College of Engineering)
    Earth and Atmospheric Sciences (with the Colleges of Agriculture and Life Sciences and Engineering)
    Economics
    English
    Feminist, Gender, and Sexuality Studies
    German Studies
    Government
    History
    History of Art
    Human Biology
    Independent Major
    Information Science (with the College of Agriculture and Life Sciences and College of Engineering)
    Jewish Studies
    John S. Knight Institute for Writing in the Disciplines
    Latin American Studies
    Latino Studies
    Lesbian, Gay, Bisexual, and Transgender Studies
    Linguistics
    Mathematics
    Medieval Studies
    Modern European Studies Concentration
    Music
    Near Eastern Studies
    Philosophy
    Physics
    Psychology
    Religious Studies
    Romance Studies
    Russian
    Science and Technology Studies
    Society for the Humanities
    Sociology
    Theatre, Film, and Dance
    Visual Studies Undergraduate Concentration

    *Africana Studies was an independent center reporting directly to the Provost until July 1, 2011.

    Once called “the first American university” by educational historian Frederick Rudolph, Cornell University represents a distinctive mix of eminent scholarship and democratic ideals. Adding practical subjects to the classics and admitting qualified students regardless of nationality, race, social circumstance, gender, or religion was quite a departure when Cornell was founded in 1865.

    Today’s Cornell reflects this heritage of egalitarian excellence. It is home to the nation’s first colleges devoted to hotel administration, industrial and labor relations, and veterinary medicine. Both a private university and the land-grant institution of New York State, Cornell University is the most educationally diverse member of the Ivy League.

    On the Ithaca campus alone nearly 20,000 students representing every state and 120 countries choose from among 4,000 courses in 11 undergraduate, graduate, and professional schools. Many undergraduates participate in a wide range of interdisciplinary programs, play meaningful roles in original research, and study in Cornell programs in Washington, New York City, and the world over.

    Cornell University is a private, statutory, Ivy League and land-grant research university in Ithaca, New York. Founded in 1865 by Ezra Cornell and Andrew Dickson White, the university was intended to teach and make contributions in all fields of knowledge—from the classics to the sciences, and from the theoretical to the applied. These ideals, unconventional for the time, are captured in Cornell’s founding principle, a popular 1868 quotation from founder Ezra Cornell: “I would found an institution where any person can find instruction in any study.”

    The university is broadly organized into seven undergraduate colleges and seven graduate divisions at its main Ithaca campus, with each college and division defining its specific admission standards and academic programs in near autonomy. The university also administers two satellite medical campuses, one in New York City and one in Education City, Qatar, and The Jacobs Technion-Cornell Institute in New York City, a graduate program that incorporates technology, business, and creative thinking. The program moved from Google’s Chelsea Building in New York City to its permanent campus on Roosevelt Island in September 2017.

    Cornell is one of the few private land-grant universities in the United States. Of its seven undergraduate colleges, three are state-supported statutory or contract colleges through The State University of New York (SUNY) system, including its Agricultural and Human Ecology colleges as well as its Industrial Labor Relations school. Of Cornell’s graduate schools, only the veterinary college is state-supported. As a land grant college, Cornell operates a cooperative extension outreach program in every county of New York and receives annual funding from the State of New York for certain educational missions. The Cornell University Ithaca Campus comprises 745 acres, but is much larger when the Cornell Botanic Gardens (more than 4,300 acres) and the numerous university-owned lands in New York City are considered.

    Alumni and affiliates of Cornell have reached many notable and influential positions in politics, media, and science. As of January 2021, 61 Nobel laureates, four Turing Award winners and one Fields Medalist have been affiliated with Cornell. Cornell counts more than 250,000 living alumni, and its former and present faculty and alumni include 34 Marshall Scholars, 33 Rhodes Scholars, 29 Truman Scholars, 7 Gates Scholars, 55 Olympic Medalists, 10 current Fortune 500 CEOs, and 35 billionaire alumni. Since its founding, Cornell has been a co-educational, non-sectarian institution where admission has not been restricted by religion or race. The student body consists of more than 15,000 undergraduate and 9,000 graduate students from all 50 American states and 119 countries.

    History

    Cornell University was founded on April 27, 1865; the New York State (NYS) Senate authorized the university as the state’s land grant institution. Senator Ezra Cornell offered his farm in Ithaca, New York, as a site and $500,000 of his personal fortune as an initial endowment. Fellow senator and educator Andrew Dickson White agreed to be the first president. During the next three years, White oversaw the construction of the first two buildings and traveled to attract students and faculty. The university was inaugurated on October 7, 1868, and 412 men were enrolled the next day.

    Cornell developed as a technologically innovative institution, applying its research to its own campus and to outreach efforts. For example, in 1883 it was one of the first university campuses to use electricity from a water-powered dynamo to light the grounds. Since 1894, Cornell has included colleges that are state funded and fulfill statutory requirements; it has also administered research and extension activities that have been jointly funded by state and federal matching programs.

    Cornell has had active alumni since its earliest classes. It was one of the first universities to include alumni-elected representatives on its Board of Trustees. Cornell was also among the Ivies that had heightened student activism during the 1960s related to cultural issues; civil rights; and opposition to the Vietnam War, with protests and occupations resulting in the resignation of Cornell’s president and the restructuring of university governance. Today the university has more than 4,000 courses. Cornell is also known for the Residential Club Fire of 1967, a fire in the Residential Club building that killed eight students and one professor.

    Since 2000, Cornell has been expanding its international programs. In 2004, the university opened the Weill Cornell Medical College in Qatar. It has partnerships with institutions in India, Singapore, and the People’s Republic of China. Former president Jeffrey S. Lehman described the university, with its high international profile, a “transnational university”. On March 9, 2004, Cornell and Stanford University laid the cornerstone for a new ‘Bridging the Rift Center’ to be built and jointly operated for education on the Israel–Jordan border.

    Research

    Cornell, a research university, is ranked fourth in the world in producing the largest number of graduates who go on to pursue PhDs in engineering or the natural sciences at American institutions, and fifth in the world in producing graduates who pursue PhDs at American institutions in any field. Research is a central element of the university’s mission; in 2009 Cornell spent $671 million on science and engineering research and development, the 16th highest in the United States.

    Cornell is a member of the Association of American Universities and is classified among “R1: Doctoral Universities – Very high research activity”.

    For the 2016–17 fiscal year, the university spent $984.5 million on research. Federal sources constitute the largest source of research funding, with total federal investment of $438.2 million. The agencies contributing the largest share of that investment are The Department of Health and Human Services and the National Science Foundation, accounting for 49.6% and 24.4% of all federal investment, respectively. Cornell was on the top-ten list of U.S. universities receiving the most patents in 2003, and was one of the nation’s top five institutions in forming start-up companies. In 2004–05, Cornell received 200 invention disclosures; filed 203 U.S. patent applications; completed 77 commercial license agreements; and distributed royalties of more than $4.1 million to Cornell units and inventors.

    Since 1962, Cornell has been involved in unmanned missions to Mars. In the 21st century, Cornell had a hand in the Mars Exploration Rover Mission. Cornell’s Steve Squyres, Principal Investigator for the Athena Science Payload, led the selection of the landing zones and requested data collection features for the Spirit and Opportunity rovers. NASA-JPL/Caltech engineers took those requests and designed the rovers to meet them. The rovers, both of which have operated long past their original life expectancies, are responsible for the discoveries that were awarded 2004 Breakthrough of the Year honors by Science. Control of the Mars rovers has shifted between National Aeronautics and Space Administration ’s Jet Propulsion Laboratory at The California Institute of Technology and Cornell’s Space Sciences Building.

    Further, Cornell researchers discovered the rings around the planet Uranus, and Cornell built and operated the telescope at Arecibo Observatory located in Arecibo, Puerto Rico until 2011, when they transferred the operations to SRI International, the Universities Space Research Association and the Metropolitan University of Puerto Rico [Universidad Metropolitana de Puerto Rico].

    The Automotive Crash Injury Research Project was begun in 1952. It pioneered the use of crash testing, originally using corpses rather than dummies. The project discovered that improved door locks; energy-absorbing steering wheels; padded dashboards; and seat belts could prevent an extraordinary percentage of injuries.

    In the early 1980s, Cornell deployed the first IBM 3090-400VF and coupled two IBM 3090-600E systems to investigate coarse-grained parallel computing. In 1984, the National Science Foundation began work on establishing five new supercomputer centers, including the Cornell Center for Advanced Computing, to provide high-speed computing resources for research within the United States. As a National Science Foundation center, Cornell deployed the first IBM Scalable Parallel supercomputer.
    In the 1990s, Cornell developed scheduling software and deployed the first supercomputer built by Dell. Most recently, Cornell deployed Red Cloud, one of the first cloud computing services designed specifically for research. Today, the center is a partner on the National Science Foundation XSEDE-Extreme Science Engineering Discovery Environment supercomputing program, providing coordination for XSEDE architecture and design, systems reliability testing, and online training using the Cornell Virtual Workshop learning platform.

    Cornell scientists have researched the fundamental particles of nature for more than 70 years. Cornell physicists, such as Hans Bethe, contributed not only to the foundations of nuclear physics but also participated in the Manhattan Project. In the 1930s, Cornell built the second cyclotron in the United States. In the 1950s, Cornell physicists became the first to study synchrotron radiation.

    During the 1990s, the Cornell Electron Storage Ring, located beneath Alumni Field, was the world’s highest-luminosity electron-positron collider. After building the synchrotron at Cornell, Robert R. Wilson took a leave of absence to become the founding director of The DOE’s Fermi National Accelerator Laboratory, which involved designing and building the largest accelerator in the United States.

    Cornell’s accelerator and high-energy physics groups are involved in the design of the proposed ILC-International Linear Collider(JP) and plan to participate in its construction and operation. The International Linear Collider(JP), to be completed in the late 2010s, will complement the CERN Large Hadron Collider(CH) and shed light on questions such as the identity of dark matter and the existence of extra dimensions.
    As part of its research work, Cornell has established several research collaborations with universities around the globe. For example, a partnership with the University of Sussex(UK) (including the Institute of Development Studies at Sussex) allows research and teaching collaboration between the two institutions.

     
  • richardmitnick 9:56 am on May 30, 2023 Permalink | Reply
    Tags: "'Evil Eye' Galaxy: The Sinister Glare Can Finally Be Explained", , Astrophysics, , , It doesn't take a huge leap of imagination to see why Messier 64 is better known as the "Evil Eye galaxy"., , The discovery could be giving us a glimpse into the future of our own Milky Way galaxy.,   

    From The University of Washington Via “Science Alert (AU)” : “‘Evil Eye’ Galaxy: The Sinister Glare Can Finally Be Explained” 

    From The University of Washington

    Via

    ScienceAlert

    “Science Alert (AU)”

    5.30.23
    Michelle Starr

    1
    Hubble Space Telescope image of Messier 64, AKA the “Evil Eye” galaxy. (NASA and The Hubble Heritage Team/AURA/STScI).

    3
    A collision of two galaxies has left a merged star system with an unusual appearance as well as bizarre internal motions. Messier 64 (M64) has a spectacular dark band of absorbing dust in front of the galaxy’s bright nucleus, giving rise to its nicknames of the “Black Eye” or “Evil Eye” galaxy.

    Fine details of the dark band are revealed in this image of the central portion of M64 obtained with the Hubble Space Telescope. M64 is well known among amateur astronomers because of its appearance in small telescopes. It was first cataloged in the 18th century by the French astronomer Messier. Located in the northern constellation Coma Berenices, M64 resides roughly 17 million light-years from Earth.

    Image Credit: NASA and The Hubble Heritage Team (AURA/STScI); Acknowledgment: S. Smartt (Institute of Astronomy) and D. Richstone (U. Michigan)
    https://www.nasa.gov/

    Home


    http://www.stsci.edu/portal/
    https://umich.edu/

    It doesn’t take a huge leap of imagination to see why Messier 64 is better known as the “Evil Eye galaxy”. Sitting in the abyssal vacuum of space it seems to cast a sinister glare across the cosmos, a cloud of dust framing its visible periphery like a dark bruise.

    The galaxy is even stranger than it looks. Its hydrogen-rich outer disk orbits in the opposite direction to the galaxy’s inner disk of stars, hinting at differences in their origins.

    Now, astronomers have worked out the outer disk’s hydrogen gas came from a smaller, gas-rich satellite dwarf galaxy, one Messier 64 recently cannibalized and wrapped itself in. It’s that smaller galaxy’s material that is darkening Messier 64’s outskirts.

    The discovery could be giving us a glimpse into the future of our own Milky Way galaxy. Estimates of the mass and contents of the shredded satellite suggest that it was remarkably similar to the Small Magellanic Cloud, a Milky Way satellite dwarf galaxy that will one day be subsumed into the larger mass.

    These findings, led by astronomer Adam Smercina of the University of Washington, have been accepted into The Astrophysical Journal Letters [below].

    “We find evidence for a spectacular shell feature, and other tidal structures indicative of an ongoing, late-stage radial merger,” the researchers write.

    “We estimate the stellar mass of the progenitor galaxy to be 500 million solar masses, with a metallicity of [M/H] ≃ −1 – very similar to the mass and metallicity of the Small Magellanic Cloud.

    “The mass of Messier 64’s counter-rotating outer gas disk is also comparable to the gas mass of the Small Magellanic Cloud, suggesting that the likeliest origin of Messier 64’s unique counter-rotating disk was a recent merger with a gas-rich satellite very similar to the Small Magellanic Cloud.”

    The Astrophysical Journal Letters

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.
    Stem Education Coalition

    u-washington-campus

    The University of Washington is one of the world’s preeminent public universities. Our impact on individuals, on our region, and on the world is profound — whether we are launching young people into a boundless future or confronting the grand challenges of our time through undaunted research and scholarship. Ranked number 10 in the world in Shanghai Jiao Tong University rankings and educating more than 54,000 students annually, our students and faculty work together to turn ideas into impact and in the process transform lives and our world. For more about our impact on the world, every day.

    So what defines us —the students, faculty and community members at the University of Washington? Above all, it’s our belief in possibility and our unshakable optimism. It’s a connection to others, both near and far. It’s a hunger that pushes us to tackle challenges and pursue progress. It’s the conviction that together we can create a world of good. Join us on the journey.

    The University of Washington is a public research university in Seattle, Washington, United States. Founded in 1861, University of Washington is one of the oldest universities on the West Coast; it was established in downtown Seattle approximately a decade after the city’s founding to aid its economic development. Today, the university’s 703-acre main Seattle campus is in the University District above the Montlake Cut, within the urban Puget Sound region of the Pacific Northwest. The university has additional campuses in Tacoma and Bothell. Overall, University of Washington encompasses over 500 buildings and over 20 million gross square footage of space, including one of the largest library systems in the world with more than 26 university libraries, as well as the UW Tower, lecture halls, art centers, museums, laboratories, stadiums, and conference centers. The university offers bachelor’s, master’s, and doctoral degrees through 140 departments in various colleges and schools, sees a total student enrollment of roughly 46,000 annually, and functions on a quarter system.

    University of Washington is a member of the Association of American Universities and is classified among “R1: Doctoral Universities – Very high research activity”. According to the National Science Foundation, UW spent $1.41 billion on research and development in 2018, ranking it 5th in the nation. As the flagship institution of the six public universities in Washington state, it is known for its medical, engineering and scientific research as well as its highly competitive computer science and engineering programs. Additionally, University of Washington continues to benefit from its deep historic ties and major collaborations with numerous technology giants in the region, such as Amazon, Boeing, Nintendo, and particularly Microsoft. Paul G. Allen, Bill Gates and others spent significant time at Washington computer labs for a startup venture before founding Microsoft and other ventures. The University of Washington’s 22 varsity sports teams are also highly competitive, competing as the Huskies in the Pac-12 Conference of the NCAA Division I, representing the United States at the Olympic Games, and other major competitions.

    The university has been affiliated with many notable alumni and faculty, including 21 Nobel Prize laureates and numerous Pulitzer Prize winners, Fulbright Scholars, Rhodes Scholars and Marshall Scholars.

    In 1854, territorial governor Isaac Stevens recommended the establishment of a university in the Washington Territory. Prominent Seattle-area residents, including Methodist preacher Daniel Bagley, saw this as a chance to add to the city’s potential and prestige. Bagley learned of a law that allowed United States territories to sell land to raise money in support of public schools. At the time, Arthur A. Denny, one of the founders of Seattle and a member of the territorial legislature, aimed to increase the city’s importance by moving the territory’s capital from Olympia to Seattle. However, Bagley eventually convinced Denny that the establishment of a university would assist more in the development of Seattle’s economy. Two universities were initially chartered, but later the decision was repealed in favor of a single university in Lewis County provided that locally donated land was available. When no site emerged, Denny successfully petitioned the legislature to reconsider Seattle as a location in 1858.

    In 1861, scouting began for an appropriate 10 acres (4 ha) site in Seattle to serve as a new university campus. Arthur and Mary Denny donated eight acres, while fellow pioneers Edward Lander, and Charlie and Mary Terry, donated two acres on Denny’s Knoll in downtown Seattle. More specifically, this tract was bounded by 4th Avenue to the west, 6th Avenue to the east, Union Street to the north, and Seneca Streets to the south.

    John Pike, for whom Pike Street is named, was the university’s architect and builder. It was opened on November 4, 1861, as the Territorial University of Washington. The legislature passed articles incorporating the University, and establishing its Board of Regents in 1862. The school initially struggled, closing three times: in 1863 for low enrollment, and again in 1867 and 1876 due to funds shortage. University of Washington awarded its first graduate Clara Antoinette McCarty Wilt in 1876, with a bachelor’s degree in science.

    19th century relocation

    By the time Washington state entered the Union in 1889, both Seattle and the University had grown substantially. University of Washington’s total undergraduate enrollment increased from 30 to nearly 300 students, and the campus’s relative isolation in downtown Seattle faced encroaching development. A special legislative committee, headed by University of Washington graduate Edmond Meany, was created to find a new campus to better serve the growing student population and faculty. The committee eventually selected a site on the northeast of downtown Seattle called Union Bay, which was the land of the Duwamish, and the legislature appropriated funds for its purchase and construction. In 1895, the University relocated to the new campus by moving into the newly built Denny Hall. The University Regents tried and failed to sell the old campus, eventually settling with leasing the area. This would later become one of the University’s most valuable pieces of real estate in modern-day Seattle, generating millions in annual revenue with what is now called the Metropolitan Tract. The original Territorial University building was torn down in 1908, and its former site now houses the Fairmont Olympic Hotel.

    The sole-surviving remnants of Washington’s first building are four 24-foot (7.3 m), white, hand-fluted cedar, Ionic columns. They were salvaged by Edmond S. Meany, one of the University’s first graduates and former head of its history department. Meany and his colleague, Dean Herbert T. Condon, dubbed the columns as “Loyalty,” “Industry,” “Faith”, and “Efficiency”, or “LIFE.” The columns now stand in the Sylvan Grove Theater.

    20th century expansion

    Organizers of the 1909 Alaska-Yukon-Pacific Exposition eyed the still largely undeveloped campus as a prime setting for their world’s fair. They came to an agreement with Washington’s Board of Regents that allowed them to use the campus grounds for the exposition, surrounding today’s Drumheller Fountain facing towards Mount Rainier. In exchange, organizers agreed Washington would take over the campus and its development after the fair’s conclusion. This arrangement led to a detailed site plan and several new buildings, prepared in part by John Charles Olmsted. The plan was later incorporated into the overall University of Washington campus master plan, permanently affecting the campus layout.

    Both World Wars brought the military to campus, with certain facilities temporarily lent to the federal government. In spite of this, subsequent post-war periods were times of dramatic growth for the University. The period between the wars saw a significant expansion of the upper campus. Construction of the Liberal Arts Quadrangle, known to students as “The Quad,” began in 1916 and continued to 1939. The University’s architectural centerpiece, Suzzallo Library, was built in 1926 and expanded in 1935.

    After World War II, further growth came with the G.I. Bill. Among the most important developments of this period was the opening of the School of Medicine in 1946, which is now consistently ranked as the top medical school in the United States. It would eventually lead to the University of Washington Medical Center, ranked by U.S. News and World Report as one of the top ten hospitals in the nation.

    In 1942, all persons of Japanese ancestry in the Seattle area were forced into inland internment camps as part of Executive Order 9066 following the attack on Pearl Harbor. During this difficult time, university president Lee Paul Sieg took an active and sympathetic leadership role in advocating for and facilitating the transfer of Japanese American students to universities and colleges away from the Pacific Coast to help them avoid the mass incarceration. Nevertheless, many Japanese American students and “soon-to-be” graduates were unable to transfer successfully in the short time window or receive diplomas before being incarcerated. It was only many years later that they would be recognized for their accomplishments during the University of Washington’s Long Journey Home ceremonial event that was held in May 2008.

    From 1958 to 1973, the University of Washington saw a tremendous growth in student enrollment, its faculties and operating budget, and also its prestige under the leadership of Charles Odegaard. University of Washington student enrollment had more than doubled to 34,000 as the baby boom generation came of age. However, this era was also marked by high levels of student activism, as was the case at many American universities. Much of the unrest focused around civil rights and opposition to the Vietnam War. In response to anti-Vietnam War protests by the late 1960s, the University Safety and Security Division became the University of Washington Police Department.

    Odegaard instituted a vision of building a “community of scholars”, convincing the Washington State legislatures to increase investment in the University. Washington senators, such as Henry M. Jackson and Warren G. Magnuson, also used their political clout to gather research funds for the University of Washington. The results included an increase in the operating budget from $37 million in 1958 to over $400 million in 1973, solidifying University of Washington as a top recipient of federal research funds in the United States. The establishment of technology giants such as Microsoft, Boeing and Amazon in the local area also proved to be highly influential in the University of Washington’s fortunes, not only improving graduate prospects but also helping to attract millions of dollars in university and research funding through its distinguished faculty and extensive alumni network.

    21st century

    In 1990, the University of Washington opened its additional campuses in Bothell and Tacoma. Although originally intended for students who have already completed two years of higher education, both schools have since become four-year universities with the authority to grant degrees. The first freshman classes at these campuses started in fall 2006. Today both Bothell and Tacoma also offer a selection of master’s degree programs.

    In 2012, the University began exploring plans and governmental approval to expand the main Seattle campus, including significant increases in student housing, teaching facilities for the growing student body and faculty, as well as expanded public transit options. The University of Washington light rail station was completed in March 2015, connecting Seattle’s Capitol Hill neighborhood to the University of Washington Husky Stadium within five minutes of rail travel time. It offers a previously unavailable option of transportation into and out of the campus, designed specifically to reduce dependence on private vehicles, bicycles and local King County buses.

    University of Washington has been listed as a “Public Ivy” in Greene’s Guides since 2001, and is an elected member of the American Association of Universities. Among the faculty by 2012, there have been 151 members of American Association for the Advancement of Science, 68 members of the National Academy of Sciences, 67 members of the American Academy of Arts and Sciences, 53 members of the National Academy of Medicine, 29 winners of the Presidential Early Career Award for Scientists and Engineers, 21 members of the National Academy of Engineering, 15 Howard Hughes Medical Institute Investigators, 15 MacArthur Fellows, 9 winners of the Gairdner Foundation International Award, 5 winners of the National Medal of Science, 7 Nobel Prize laureates, 5 winners of Albert Lasker Award for Clinical Medical Research, 4 members of the American Philosophical Society, 2 winners of the National Book Award, 2 winners of the National Medal of Arts, 2 Pulitzer Prize winners, 1 winner of the Fields Medal, and 1 member of the National Academy of Public Administration. Among UW students by 2012, there were 136 Fulbright Scholars, 35 Rhodes Scholars, 7 Marshall Scholars and 4 Gates Cambridge Scholars. UW is recognized as a top producer of Fulbright Scholars, ranking 2nd in the US in 2017.

    The Academic Ranking of World Universities (ARWU) has consistently ranked University of Washington as one of the top 20 universities worldwide every year since its first release. In 2019, University of Washington ranked 14th worldwide out of 500 by the ARWU, 26th worldwide out of 981 in the Times Higher Education World University Rankings, and 28th worldwide out of 101 in the Times World Reputation Rankings. Meanwhile, QS World University Rankings ranked it 68th worldwide, out of over 900.

    U.S. News & World Report ranked University of Washington 8th out of nearly 1,500 universities worldwide for 2021, with University of Washington’s undergraduate program tied for 58th among 389 national universities in the U.S. and tied for 19th among 209 public universities.

    In 2019, it ranked 10th among the universities around the world by SCImago Institutions Rankings. In 2017, the Leiden Ranking, which focuses on science and the impact of scientific publications among the world’s 500 major universities, ranked University of Washington 12th globally and 5th in the U.S.

    In 2019, Kiplinger Magazine’s review of “top college values” named University of Washington 5th for in-state students and 10th for out-of-state students among U.S. public colleges, and 84th overall out of 500 schools. In the Washington Monthly National University Rankings University of Washington was ranked 15th domestically in 2018, based on its contribution to the public good as measured by social mobility, research, and promoting public service.

     
  • richardmitnick 8:46 am on May 30, 2023 Permalink | Reply
    Tags: "Secrets of the stars", Astrophysics, , , , How University of Washington astronomers and the world’s largest telescope and a new survey of space will upend what we thought we knew about the universe., , , The University of Washington DiRAC Institute for Data Intensive Research in Astrophysics & Cosmology   

    From The College of Arts and Sciences And The University of Washington DiRAC Institute for Data Intensive Research in Astrophysics & Cosmology At The University of Washington : “Secrets of the stars” 

    From The College of Arts and Sciences

    And

    The University of Washington Institute for Data Intensive Research in Astrophysics & Cosmology

    At

    The University of Washington

    5.30.23
    James Urton

    How University of Washington astronomers with the world’s largest telescope and a revolutionary survey of space will upend what we thought we knew about the universe.

    Beneath breathtakingly crisp views of the night sky, atop Cerro Pachón, a mountain in the foothills of the Andes in northern Chile, is a nearly finished construction project that will transform how we look at the universe. Though it resembles a postmodern office building, its domed tower is the telltale sign of an astronomical observatory.

    Next year, when its upward-turned eye opens to the heavens, the Vera C. Rubin Observatory will form the beating heart of a revolution that is sweeping astronomy. It will impact nearly every mission, every question and every research project exploring what is “out there” beyond Earth. It could even change how we view our place within the cosmos.

    Assuming, of course, astronomers can navigate their way through the unprecedented amount of data the Rubin Observatory will gather starting in 2025 — a challenge that the University of Washington is rising to meet.

    The Rubin Observatory, which features the largest mirror and digital camera ever constructed, will unleash a deluge of information about our night sky as part of the 10-year Legacy Survey of Space and Time (LSST). The University of Washington was a founding member of the LSST mission, which is no ordinary stargazing venture.

    Thanks to the observatory’s Simonyi Survey Telescope, the LSST will be the most ambitious mission ever to capture and understand the countless cosmic events that shape and reshape our universe — effectively rewriting the astronomy books we use today.

    “A generation ago, a telescope might watch just a thousand stars in a single observation run,” says James Davenport, assistant professor of astronomy in the College of Arts & Sciences. “The Rubin Observatory will observe several billion objects in the sky, giving us thousands of times more data than other telescopes could capture — and that’s just in a single night.”

    But data on its own can’t drive discovery. The astronomers need tools — algorithms, software and expertise — to sort through Rubin’s bounty.

    “It’s like someone delivering a silo of grain and saying, ‘Here, I’ve solved your hunger problem.’ You actually haven’t yet — not until we have the means to process that grain and bake loaves,” says Mario Jurić, a UW astronomy professor. “We’ll get silos of grain each night from the Rubin Observatory, and the field of astronomy needs to figure out how to transform that into bread.”

    This is where DiRAC — the UW’s Institute for Data Intensive Research in Astrophysics & Cosmology — comes in. Launched in 2017 with lead funding from the Charles and Lisa Simonyi Fund for Arts and Sciences, DiRAC is ready to help us make sense of the discoveries of Rubin and the new generation of telescopes.

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    Feeding astronomy’s hunger

    Jurić and Davenport are the director and associate director (respectively) of DiRAC, a collaborative community of scientists, engineers and students who are crafting software that can comb through those mountains of astronomical data to help scientists understand the events and changes unfolding continuously above our heads.

    Each night, the Rubin’s camera is expected to capture millions of changes in stars and other objects — too many to sort through in a lifetime.

    The astronomical events the LSST will pick up are diverse. Some will be subtle, like a dim asteroid in a frigid orbit around the sun. Others will be dramatic, like a massive star at the end of its life immolating brilliantly as a supernova.

    The tools DiRAC is developing for the Rubin project are equally diverse. Daily automated alerts, for example, will help scientists worldwide identify events that require immediate action — such as an asteroid on a collision course with Earth. Other tools will enable longer-term studies, like tracking the behavior of a specific set of stars over time in our Milky Way galaxy.

    “These are important tools to help democratize science and make it accessible,” says Jurić. “Most astronomers are not experts in writing algorithms or software to sort through large datasets. The tools we’re developing will do those jobs for them, so users can pull out the data that interests them and keep the discovery pipeline going.”

    Beyond these tool-building goals, DiRAC scientists are looking forward to applying LSST data to a host of scientific mysteries.

    5

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    Photo by Christopher Michel

    Data on its own can’t drive discovery. Astronomers need tools — algorithms, software and expertise — to sort through Rubin’s bounty. “It’s like someone delivering a silo of grain and saying, ‘Here, I’ve solved your hunger problem.’ You actually haven’t yet — not until we have the means to process that grain and bake loaves,” says Mario Jurić, UW astronomy professor and director of DiRAC. “We’ll get silos of grain each night from the Rubin Observatory, and the field of astronomy needs to figure out how to transform that into bread.”

    Finding the strange and powerful

    Many of us remember making solar-system mobiles in school, with eight (or nine, depending on our age) painted balls representing the planets — but it turns out the solar system is far more crowded than we were taught.

    After “first light” — when Rubin becomes operational in early 2025 — DiRAC scientists will use the data to understand our astronomical history, observe the present and predict the future, tracking and studying everything from protecting ourselves from near-Earth asteroids to the possibility of finding a Planet Nine lurking in the frozen reaches beyond our star.

    7
    Sarah Greenstreet

    DiRAC researcher Sarah Greenstreet works alongside teams that are creating an automated alert system for objects in motion that could impact the Earth. She notes that asteroids and other small bodies around the sun are also windows to the past — “which can help us understand how they have moved through the solar system throughout its history.”

    Other DiRAC scientists will have their gazes fixed on stars themselves. Contemporary research is challenging long-prevailing theories about how these burning furnaces form, live and die. In his own research, Davenport — who notes that he “likes weird stars” — has catalogued unexpected stellar pairings, such as a large puffy star (one that’s expanding in its twilight years) orbited by a small companion star encased in cosmic dust, or two stars whose dance around each other is twisted and turned by an unseen third companion. With the LSST watching hundreds of millions of stars each night, scientists like Davenport expect to find more of these strange systems and learn why some stars are paired up while others, like our calm sun, are not.

    “A bunch of stars out there show unusual and unexpected behavior,” says Davenport. “Is it possible that they aren’t unusual at all, but are actually very common? If so, we’ll have to go back to the theories of star formation and galaxy formation and redefine what’s ‘unusual.’”

    Still other DiRAC researchers have their eyes on even bigger prizes, including the powerful events — like black hole or neutron star mergers — that generate gravitational waves. The LSST mission will provide data about the highly energetic events that generate these waves, giving scientists valuable insight never before available.

    8
    DiRAC researcher Sarah Greenstreet is working on an automated alert system for objects in motion that could impact the Earth. She notes that asteroids are also windows to the past — “which can help us understand how they have moved through the solar system throughout its history.”

    Looking for the unexpected

    Those are just a few of the discoveries scientists expect to find. But buried within the massive datasets from LSST and the Rubin Observatory will doubtless be evidence of events, objects and phenomena that may shock and confound scientists.

    Those “anticipated unknowns,” pulled from the sky above the arid Andes and then examined at a rain-washed campus half a world away, are what most excite astronomers like Davenport. “The lasting legacy of the LSST will be in the surprises buried in the datasets that we’re helping to uncover,” he says with anticipation. “Students today will be working with these data for the rest of their careers — and that is precisely how astronomy should work.”

    What could we discover?

    A few of the astronomical mysteries the Rubin Observatory is expected to shed light on:

    7
    The amount and location of dark matter in our galaxy; what dark energy is and how it behaves.


    Light from black hole and neutron star mergers, which generate gravitational waves detected halfway across the visible universe.


    Hundreds of supernovae each night (10–100 times more than ever seen).

    10
    Solar flare.
    “Stars behaving strangely” — fading or brightening suddenly due to flare activity or interactions with a nearby star

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    Planet Nine, if it’s out there!

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.
    Stem Education Coalition

    Discovery is who we are

    DiRAC Mission Statement

    To build the world’s most advanced datasets, algorithms, and tools and use them to explore and understand the universe.

    The College of Arts & Sciences is at the heart of the University of Washington. As the UW’s largest college, Arts & Sciences produces more than half of all bachelor’s degrees on the Seattle campus. A third of our 24,000+ students are the first in their families to attend college. Faculty in our 39 academic departments are dedicated to helping students think critically, communicate clearly, and engage diverse perspectives respectfully. In Arts & Sciences, our discoveries in learning, teaching, and research engage us with our local, national and global communities — and with each other.

    The University of Washington College of Arts and Sciences provides a liberal arts education of tremendous breadth and depth to more than 22,000 students while advancing research and serving as a resource for the community. The College is made up of four academic divisions: art, humanities, natural sciences, and social sciences.

    CORE OF THE UNIVERSITY

    With more than 5,400 undergraduate courses offered in the College of Arts & Sciences annually, students can study everything from art to economics to physics. The College’s extensive academic offerings benefit the entire University community; nearly one-third of all students who take an Arts & Sciences class are pursuing a non-A&S degree.

    CUTTING-EDGE RESEARCH

    From malaria treatment to solar energy to human rights, A&S researchers are tackling many of our society’s most pressing issues. The College is home to more than 30 interdisciplinary centers and has ties to many others, enabling scholars in diverse fields to collaborate on complex research questions. A&S faculty generated about $105 million in research funds through public and private grants during the most recent fiscal year.

    INTERNATIONAL EMPHASIS

    The College teaches 60 languages and offers more than 100 study abroad programs in 36 countries, with dedicated centers in Rome, Italy and León, Spain. The Jackson School of International Studies provides interdisciplinary education, leading-edge research, public programs and outreach on all major world areas and critical international issues.

    A REGIONAL ARTS RESOURCE

    All of the University’s arts units are part of the College, including the Schools of Music, Art, and Drama, the Department of Dance, Digital Arts and Experimental Media (DXARTS), the Henry Art Gallery, the Burke Museum, and Meany Center for the Performing Arts. They offer more than 300 performances, exhibits, and public programs annually. Detailed event and ticket information is available at ArtsUW.

    PARTNERING WITH THE COMMUNITY

    The College has developed dozens of innovative partnerships with the community. These include summer programs for K-12 teachers, guided stargazings at the Jacobsen Observatory, special Meany Center performances for K-12 classes, collaborations with community organizations through project-based courses, and more.

    u-washington-campus

    The University of Washington is one of the world’s preeminent public universities. Our impact on individuals, on our region, and on the world is profound — whether we are launching young people into a boundless future or confronting the grand challenges of our time through undaunted research and scholarship. Ranked number 10 in the world in Shanghai Jiao Tong University rankings and educating more than 54,000 students annually, our students and faculty work together to turn ideas into impact and in the process transform lives and our world. For more about our impact on the world, every day.

    So what defines us —the students, faculty and community members at the University of Washington? Above all, it’s our belief in possibility and our unshakable optimism. It’s a connection to others, both near and far. It’s a hunger that pushes us to tackle challenges and pursue progress. It’s the conviction that together we can create a world of good. Join us on the journey.

    The University of Washington is a public research university in Seattle, Washington, United States. Founded in 1861, University of Washington is one of the oldest universities on the West Coast; it was established in downtown Seattle approximately a decade after the city’s founding to aid its economic development. Today, the university’s 703-acre main Seattle campus is in the University District above the Montlake Cut, within the urban Puget Sound region of the Pacific Northwest. The university has additional campuses in Tacoma and Bothell. Overall, University of Washington encompasses over 500 buildings and over 20 million gross square footage of space, including one of the largest library systems in the world with more than 26 university libraries, as well as the UW Tower, lecture halls, art centers, museums, laboratories, stadiums, and conference centers. The university offers bachelor’s, master’s, and doctoral degrees through 140 departments in various colleges and schools, sees a total student enrollment of roughly 46,000 annually, and functions on a quarter system.

    University of Washington is a member of the Association of American Universities and is classified among “R1: Doctoral Universities – Very high research activity”. According to the National Science Foundation, UW spent $1.41 billion on research and development in 2018, ranking it 5th in the nation. As the flagship institution of the six public universities in Washington state, it is known for its medical, engineering and scientific research as well as its highly competitive computer science and engineering programs. Additionally, University of Washington continues to benefit from its deep historic ties and major collaborations with numerous technology giants in the region, such as Amazon, Boeing, Nintendo, and particularly Microsoft. Paul G. Allen, Bill Gates and others spent significant time at Washington computer labs for a startup venture before founding Microsoft and other ventures. The University of Washington’s 22 varsity sports teams are also highly competitive, competing as the Huskies in the Pac-12 Conference of the NCAA Division I, representing the United States at the Olympic Games, and other major competitions.

    The university has been affiliated with many notable alumni and faculty, including 21 Nobel Prize laureates and numerous Pulitzer Prize winners, Fulbright Scholars, Rhodes Scholars and Marshall Scholars.

    In 1854, territorial governor Isaac Stevens recommended the establishment of a university in the Washington Territory. Prominent Seattle-area residents, including Methodist preacher Daniel Bagley, saw this as a chance to add to the city’s potential and prestige. Bagley learned of a law that allowed United States territories to sell land to raise money in support of public schools. At the time, Arthur A. Denny, one of the founders of Seattle and a member of the territorial legislature, aimed to increase the city’s importance by moving the territory’s capital from Olympia to Seattle. However, Bagley eventually convinced Denny that the establishment of a university would assist more in the development of Seattle’s economy. Two universities were initially chartered, but later the decision was repealed in favor of a single university in Lewis County provided that locally donated land was available. When no site emerged, Denny successfully petitioned the legislature to reconsider Seattle as a location in 1858.

    In 1861, scouting began for an appropriate 10 acres (4 ha) site in Seattle to serve as a new university campus. Arthur and Mary Denny donated eight acres, while fellow pioneers Edward Lander, and Charlie and Mary Terry, donated two acres on Denny’s Knoll in downtown Seattle. More specifically, this tract was bounded by 4th Avenue to the west, 6th Avenue to the east, Union Street to the north, and Seneca Streets to the south.

    John Pike, for whom Pike Street is named, was the university’s architect and builder. It was opened on November 4, 1861, as the Territorial University of Washington. The legislature passed articles incorporating the University, and establishing its Board of Regents in 1862. The school initially struggled, closing three times: in 1863 for low enrollment, and again in 1867 and 1876 due to funds shortage. University of Washington awarded its first graduate Clara Antoinette McCarty Wilt in 1876, with a bachelor’s degree in science.

    19th century relocation

    By the time Washington state entered the Union in 1889, both Seattle and the University had grown substantially. University of Washington’s total undergraduate enrollment increased from 30 to nearly 300 students, and the campus’s relative isolation in downtown Seattle faced encroaching development. A special legislative committee, headed by University of Washington graduate Edmond Meany, was created to find a new campus to better serve the growing student population and faculty. The committee eventually selected a site on the northeast of downtown Seattle called Union Bay, which was the land of the Duwamish, and the legislature appropriated funds for its purchase and construction. In 1895, the University relocated to the new campus by moving into the newly built Denny Hall. The University Regents tried and failed to sell the old campus, eventually settling with leasing the area. This would later become one of the University’s most valuable pieces of real estate in modern-day Seattle, generating millions in annual revenue with what is now called the Metropolitan Tract. The original Territorial University building was torn down in 1908, and its former site now houses the Fairmont Olympic Hotel.

    The sole-surviving remnants of Washington’s first building are four 24-foot (7.3 m), white, hand-fluted cedar, Ionic columns. They were salvaged by Edmond S. Meany, one of the University’s first graduates and former head of its history department. Meany and his colleague, Dean Herbert T. Condon, dubbed the columns as “Loyalty,” “Industry,” “Faith”, and “Efficiency”, or “LIFE.” The columns now stand in the Sylvan Grove Theater.

    20th century expansion

    Organizers of the 1909 Alaska-Yukon-Pacific Exposition eyed the still largely undeveloped campus as a prime setting for their world’s fair. They came to an agreement with Washington’s Board of Regents that allowed them to use the campus grounds for the exposition, surrounding today’s Drumheller Fountain facing towards Mount Rainier. In exchange, organizers agreed Washington would take over the campus and its development after the fair’s conclusion. This arrangement led to a detailed site plan and several new buildings, prepared in part by John Charles Olmsted. The plan was later incorporated into the overall University of Washington campus master plan, permanently affecting the campus layout.

    Both World Wars brought the military to campus, with certain facilities temporarily lent to the federal government. In spite of this, subsequent post-war periods were times of dramatic growth for the University. The period between the wars saw a significant expansion of the upper campus. Construction of the Liberal Arts Quadrangle, known to students as “The Quad,” began in 1916 and continued to 1939. The University’s architectural centerpiece, Suzzallo Library, was built in 1926 and expanded in 1935.

    After World War II, further growth came with the G.I. Bill. Among the most important developments of this period was the opening of the School of Medicine in 1946, which is now consistently ranked as the top medical school in the United States. It would eventually lead to the University of Washington Medical Center, ranked by U.S. News and World Report as one of the top ten hospitals in the nation.

    In 1942, all persons of Japanese ancestry in the Seattle area were forced into inland internment camps as part of Executive Order 9066 following the attack on Pearl Harbor. During this difficult time, university president Lee Paul Sieg took an active and sympathetic leadership role in advocating for and facilitating the transfer of Japanese American students to universities and colleges away from the Pacific Coast to help them avoid the mass incarceration. Nevertheless, many Japanese American students and “soon-to-be” graduates were unable to transfer successfully in the short time window or receive diplomas before being incarcerated. It was only many years later that they would be recognized for their accomplishments during the University of Washington’s Long Journey Home ceremonial event that was held in May 2008.

    From 1958 to 1973, the University of Washington saw a tremendous growth in student enrollment, its faculties and operating budget, and also its prestige under the leadership of Charles Odegaard. University of Washington student enrollment had more than doubled to 34,000 as the baby boom generation came of age. However, this era was also marked by high levels of student activism, as was the case at many American universities. Much of the unrest focused around civil rights and opposition to the Vietnam War. In response to anti-Vietnam War protests by the late 1960s, the University Safety and Security Division became the University of Washington Police Department.

    Odegaard instituted a vision of building a “community of scholars”, convincing the Washington State legislatures to increase investment in the University. Washington senators, such as Henry M. Jackson and Warren G. Magnuson, also used their political clout to gather research funds for the University of Washington. The results included an increase in the operating budget from $37 million in 1958 to over $400 million in 1973, solidifying University of Washington as a top recipient of federal research funds in the United States. The establishment of technology giants such as Microsoft, Boeing and Amazon in the local area also proved to be highly influential in the University of Washington’s fortunes, not only improving graduate prospects but also helping to attract millions of dollars in university and research funding through its distinguished faculty and extensive alumni network.

    21st century

    In 1990, the University of Washington opened its additional campuses in Bothell and Tacoma. Although originally intended for students who have already completed two years of higher education, both schools have since become four-year universities with the authority to grant degrees. The first freshman classes at these campuses started in fall 2006. Today both Bothell and Tacoma also offer a selection of master’s degree programs.

    In 2012, the University began exploring plans and governmental approval to expand the main Seattle campus, including significant increases in student housing, teaching facilities for the growing student body and faculty, as well as expanded public transit options. The University of Washington light rail station was completed in March 2015, connecting Seattle’s Capitol Hill neighborhood to the University of Washington Husky Stadium within five minutes of rail travel time. It offers a previously unavailable option of transportation into and out of the campus, designed specifically to reduce dependence on private vehicles, bicycles and local King County buses.

    University of Washington has been listed as a “Public Ivy” in Greene’s Guides since 2001, and is an elected member of the American Association of Universities. Among the faculty by 2012, there have been 151 members of American Association for the Advancement of Science, 68 members of the National Academy of Sciences, 67 members of the American Academy of Arts and Sciences, 53 members of the National Academy of Medicine, 29 winners of the Presidential Early Career Award for Scientists and Engineers, 21 members of the National Academy of Engineering, 15 Howard Hughes Medical Institute Investigators, 15 MacArthur Fellows, 9 winners of the Gairdner Foundation International Award, 5 winners of the National Medal of Science, 7 Nobel Prize laureates, 5 winners of Albert Lasker Award for Clinical Medical Research, 4 members of the American Philosophical Society, 2 winners of the National Book Award, 2 winners of the National Medal of Arts, 2 Pulitzer Prize winners, 1 winner of the Fields Medal, and 1 member of the National Academy of Public Administration. Among UW students by 2012, there were 136 Fulbright Scholars, 35 Rhodes Scholars, 7 Marshall Scholars and 4 Gates Cambridge Scholars. UW is recognized as a top producer of Fulbright Scholars, ranking 2nd in the US in 2017.

    The Academic Ranking of World Universities (ARWU) has consistently ranked University of Washington as one of the top 20 universities worldwide every year since its first release. In 2019, University of Washington ranked 14th worldwide out of 500 by the ARWU, 26th worldwide out of 981 in the Times Higher Education World University Rankings, and 28th worldwide out of 101 in the Times World Reputation Rankings. Meanwhile, QS World University Rankings ranked it 68th worldwide, out of over 900.

    U.S. News & World Report ranked University of Washington 8th out of nearly 1,500 universities worldwide for 2021, with University of Washington’s undergraduate program tied for 58th among 389 national universities in the U.S. and tied for 19th among 209 public universities.

    In 2019, it ranked 10th among the universities around the world by SCImago Institutions Rankings. In 2017, the Leiden Ranking, which focuses on science and the impact of scientific publications among the world’s 500 major universities, ranked University of Washington 12th globally and 5th in the U.S.

    In 2019, Kiplinger Magazine’s review of “top college values” named University of Washington 5th for in-state students and 10th for out-of-state students among U.S. public colleges, and 84th overall out of 500 schools. In the Washington Monthly National University Rankings University of Washington was ranked 15th domestically in 2018, based on its contribution to the public good as measured by social mobility, research, and promoting public service.

     
  • richardmitnick 8:40 pm on May 29, 2023 Permalink | Reply
    Tags: , "X-ray emissions from black hole jets vary unexpectedly challenging leading model of particle acceleration", , Astrophysics, , , ,   

    From The University of Maryland Via “phys.org” : “X-ray emissions from black hole jets vary unexpectedly challenging leading model of particle acceleration” 

    From The University of Maryland

    Via

    “phys.org”

    5.29.23

    1
    Gigantic X-rays flares offer new insight into the whirling maelstrom just outside supermassive black holes
    Stanford Kavli Institute for Particle Astrophysics and Cosmology.

    Researchers discovered only relatively recently that black hole jets emit X-rays, and how the jets accelerate particles to this high-energy state is still a mystery. Surprising new findings in Nature Astronomy [below] appear to rule out one leading theory, opening the door to reimagining how particle acceleration works in the jets—and possibly also elsewhere in the universe.

    One leading model of how jets generate X-rays expects the jets’ X-ray emissions to remain stable over long time scales (millions of years). However, the new paper found that the X-ray emissions of a statistically significant number of jets varied over just a few years.

    “One of the reasons we’re excited about the variability is that there are two main models for how X-rays are produced in these jets, and they’re completely different,” explains lead author Eileen Meyer, an astronomer at University of Maryland, Baltimore County. “One model invokes very low-energy electrons and one has very high-energy electrons. And one of those models is completely incompatible with any kind of variability.”

    For the study, the authors analyzed archival data from the Chandra X-ray Observatory, the highest-resolution X-ray observatory available.

    The research team looked at nearly all of the black hole jets for which Chandra had multiple observations, which amounted to 155 unique regions within 53 jets.

    Discovering relatively frequent variability on such short time scales “is revolutionary in the context of these jets, because that was not expected at all,” Meyer says.

    Rethinking particle acceleration

    In addition to assuming stability in X-ray emissions over time, the simplest theory for how jets generate X-rays assumes particle acceleration occurs at the center of the galaxy in the black hole “engine” that drives the jet. However, the new study found rapid changes in X-ray emissions all along the length of the jets. That suggests particle acceleration is occurring all along the jet, at vast distances from the jet’s origin at the black hole.

    “There are theories out there for how this could work, but a lot of what we’ve been working with is now clearly incompatible with our observations,” Meyer says.

    Interestingly, the results also hinted that jets closer to Earth had more variability than those much farther away. The latter are so far away, that by the time the light coming from them reaches the telescope, it is like looking back in time. It makes sense to Meyer that older jets would have less variability. Earlier in the universe’s history, the universe was smaller and ambient radiation was greater, which researchers believe could lead to greater stability of X-rays in the jets.

    Critical collaboration

    Despite Chandra’s outstanding imaging resolution, the data set posed significant challenges. Chandra observed some of the pockets of variability with only a handful of X-ray photons. And the variability in X-ray production in a given jet was typically tens of percent or so. To avoid unintentionally counting randomness as real variability, Meyer collaborated with statisticians at the University of Toronto and the Imperial College of London.

    “Pulling this result out of the data was almost like a miracle, because the observations were not designed to detect it,” Meyer says. The team’s analysis suggests that between 30 and 100 percent of the jets in the study showed variability over short time scales. “While we would like better constraints,” she says, “the variability is notably not zero.”

    The new findings poke significant holes in one of the major theories for X-ray production in black hole jets, and Meyer hopes the paper spurs future work. “Hopefully this will be a real call to the theorists,” she says, “to basically take a look at this result and come up with jet models that are consistent with what we’re finding.”

    Nature Astronomy

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.

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    Please help promote STEM in your local schools.

    Stem Education Coalition

    U Maryland Campus

    The University of Maryland is a public land-grant research university. Founded in 1856, The University of Maryland is the flagship institution of the University System of Maryland. It is also the largest university in both the state and the Washington metropolitan area, with more than 41,000 students representing all fifty states and 123 countries, and a global alumni network of over 388,000. Its twelve schools and colleges together offer over 200 degree-granting programs, including 92 undergraduate majors, 107 master’s programs, and 83 doctoral programs. The University of Maryland is a member of The Association of American Universities and competes in intercollegiate athletics as a member of the Big Ten Conference.

    The University of Maryland’s proximity to the nation’s capital has resulted in many research partnerships with the federal government; faculty receive research funding and institutional support from agencies such as The National Institutes of Health (US), The National Aeronautics and Space Administration, The National Institute of Standards and Technology, The Food and Drug Administration, The National Security Agency, and The Department of Homeland Security. It is classified among “R1: Doctoral Universities – Very high research activity” and is labeled a “Public Ivy”, denoting a quality of education comparable to the private Ivy League. The University of Maryland is ranked among the top 100 universities both nationally and globally by several indices, including its perennially top-ranked criminology and criminal justice department.

    In 2016, the University of Maryland-College Park and The University of Maryland- Baltimore formalized their strategic partnership after their collaboration successfully created more innovative medical, scientific, and educational programs, as well as greater research grants and joint faculty appointments than either campus has been able to accomplish on its own. According to The National Science Foundation, the university spent a combined $1.1 billion on research and development in 2019, ranking it 14th overall in the nation and 8th among all public institutions. As of 2021, the operating budget of the University of Maryland is approximately $2.2 billion.

    On March 6, 1856, the forerunner of today’s University of Maryland was chartered as the Maryland Agricultural College. Two years later, Charles Benedict Calvert (1808–1864), a future U.S. Representative (Congressman) from the sixth congressional district of Maryland, 1861–1863, during the American Civil War and descendant of the first Lord Baltimores, colonial proprietors of the Province of Maryland in 1634, purchased 420 acres (1.7 km^2) of the Riversdale Mansion estate nearby today’s College Park, Maryland. Later that year, Calvert founded the school and was the acting president from 1859 to 1860. On October 5, 1859, the first 34 students entered the Maryland Agricultural College. The school became a land grant college in February 1864.

    Following the Civil War, in February 1866, the Maryland legislature assumed half ownership of the school. The college thus became in part a state institution. By October 1867, the school reopened with 11 students. In 1868, the former Confederate admiral Franklin Buchanan was appointed President of the school, and in his tenure of just over a year, he reorganized it, established a system of strict economy in its business transactions, applied some of its revenues for the paying off of its debts, raised its standards, and attracted patrons through his personal influence: enrollment grew to 80 at the time of his resignation, and the school’s debt was soon paid off. In 1873, Samuel Jones, a former Confederate Major General, became president of the college.

    Twenty years later, the federally funded Agricultural Experiment Station was established there. During the same period, state laws granted the college regulatory powers in several areas—including controlling farm disease, inspecting feed, establishing a state weather bureau and geological survey, and housing the board of forestry. Morrill Hall (the oldest instructional building still in use on campus) was built the following year.

    The state took control of the school in 1916, and the institution was renamed Maryland State College. That year, the first female students enrolled at the school. On April 9, 1920, the college became part of the existing University of Maryland, replacing St. John’s College, Annapolis as the university’s undergraduate campus. In the same year, the graduate school on the College Park campus awarded its first PhD degrees and the university’s enrollment reached 500 students. In 1925 the university was accredited by The Association of American Universities.

    By the time the first black students enrolled at the university in 1951, enrollment had grown to nearly 10,000 students—4,000 of whom were women. Prior to 1951, many black students in Maryland were enrolled at The University of Maryland-Eastern Shore.

    In 1957, President Wilson H. Elkins made a push to increase academic standards at the university. His efforts resulted in the creation of one of the first Academic Probation Plans. The first year the plan went into effect, 1,550 students (18% of the total student body) faced expulsion.

    On October 19, 1957, Queen Elizabeth II of the United Kingdom attended her first and only college football game at the University of Maryland after expressing interest in seeing a typical American sport during her first tour of the United States. The Maryland Terrapins beat the North Carolina Tar Heels 21 to 7 in the historical game now referred to as “The Queen’s Game”.

    Phi Beta Kappa established a chapter at UMD in 1964. In 1969, the university was elected to The Association of American Universities. The school continued to grow, and by the fall of 1985 reached an enrollment of 38,679. Like many colleges during the Vietnam War, the university was the site of student protests and had curfews enforced by the National Guard.

    In a massive restructuring of the state’s higher education system in 1988, the school was designated as the flagship campus of the newly formed University of Maryland System (later changed to the University System of Maryland in 1997), and was formally named the University of Maryland-College Park. All of the five campuses in the former network were designated as distinct campuses in the new system. However, in 1997 the Maryland General Assembly passed legislation allowing the University of Maryland-College Park to be known simply as The University of Maryland, recognizing the campus’ role as the flagship institution of the University System of Maryland.

    The other University System of Maryland institutions with the name “University of Maryland” are not satellite campuses of the University of Maryland-College Park. The University of Maryland-Baltimore, is the only other school permitted to confer certain degrees from the “University of Maryland”.

    In 1994, the National Archives at College Park completed construction and opened on a parcel of land adjoining campus donated by the University of Maryland, after lobbying by President William Kirwan and congressional leaders to foster academic collaboration between the institutions.

    In 2004, the university began constructing the 150-acre (61 ha) “M Square Research Park,” which includes facilities affiliated with The Department of Defense , Food and Drug Administration, and the new National Center for Weather and Climate Prediction, affiliated with The National Oceanic and Atmospheric Administration. In May 2010, ground was broken on a new $128-million, 158,068-square-foot (14,685.0 m^2) Physical Science Complex, including an advanced quantum science laboratory.

    The university’s Great Expectations campaign from 2006 to 2012 exceeded $1 billion in private donations.

    The university suffered multiple data breaches in 2014. The first resulted in the loss of over 300,000 student and faculty records. A second data breach occurred several months later. The second breach was investigated by the FBI and Secret Service and found to be done by David Helkowski. Despite the attribution, no charges were filed. As a result of the data breaches, the university offered free credit protection for five years to the students and faculty affected.

    In 2012, the University of Maryland-College Park and the University of Maryland- Baltimore united under the MPowering the State initiative to leverage the strengths of both institutions. The University of Maryland Strategic Partnership Act of 2016 officially formalized this partnership.

    The University of Maryland’s University District Plan, developed in 2011 under President Wallace Loh and the College Park City Council, seeks to make the City of College Park a top 20 college town by 2020 by improving housing and development, transportation, public safety, local pre-K–12 education, and supporting sustainability projects. As of 2018, the university is involved with over 30 projects and 1.5 million square feet of development as part of its Greater College Park Initiative, worth over $1 billion in public-private investments. The university’s vision is to revitalize the campus to foster a dynamic and innovative academic environment, as well as to collaborate with the surrounding neighborhoods and local government to create a vibrant downtown community for students and faculty

    In October 2017, the university received a record-breaking donation of $219.5 million from the A. James & Alice B. Clark Foundation, ranking among the largest philanthropic gifts to a public university in the country.

    As of February 12, 2020, it has been announced that Darryll J. Pines will be the 34th President of the University of Maryland-College Park effective July 1, 2020. Darryll J. Pines is the dean of the A. James Clark School of Engineering and the Nariman Farvardin Professor of Aerospace Engineering since January 2009. Darryll J. Pines has been with the University of Maryland College Park for 25 years since he arrived in 1995 and started as an assistant professor.

    In 2021, the university announced it had achieved its record goal of $1.5 billion raised in donations since 2018 as part of its Fearless Ideas: The Campaign for Maryland for investments in faculty, students, research, scholarships, and capital projects.

    The university hosts “living-learning” programs which allow students with similar academic interests to live in the same residential community, take specialized courses, and perform research in those areas of expertise. An example is the Honors College, which is geared towards undergraduate students meeting high academic requirements and consists of several of the university’s honors programs. The Honors College welcomes students into a community of faculty and undergraduates. The Honors College offers seven living and learning programs: Advanced Cybersecurity Experience for Students, Design Cultures and Creativity, Entrepreneurship and Innovation, Honors Humanities, Gemstone, Integrated Life Sciences, and University Honors.

    Advanced Cybersecurity Experience for Students (ACES), started in 2013, is directed by Michel Cukier and run by faculty and graduate students. ACES students are housed in Prince Frederick Hall and take a 14 credit, two year curriculum that educates future leaders in the field of cybersecurity. ACES also offers a complementary two-year minor in cybersecurity.

    Design Cultures and Creativity (DCC), started in 2009, is directed by artist Jason Farman and run by faculty and graduate students. The DCC program encourages students to explore the relationship between emerging media, society, and creative practices. DCC students are housed in Prince Frederick residence hall together and take a 16 credit, two year interdisciplinary curriculum which culminates in a capstone.

    Entrepreneurship and Innovation Program (EIP) is a living and learning program for Honors College freshmen and sophomores, helping build entrepreneurial mindsets, skill sets, and relationships for the development of solutions to today’s problems. Through learning, courses, seminars, workshops, competitions, and volunteerism, students receive an education in entrepreneurship and innovation. In collaboration with faculty and mentors who have launched new ventures, all student teams develop an innovative idea and write a product plan.

    Honors Humanities is the honors program for beginning undergraduates with interests in the humanities and creative arts. The selective two-year living-learning program combines a small liberal arts college environment with the resources of a large research university.

    Gemstone is a multidisciplinary four-year research program for select undergraduate honors students of all majors. Under guidance of faculty mentors and Gemstone staff, teams of students design, direct and conduct research, exploring the interdependence of science and technology with society.

    Integrated Life Sciences (ILS) is the honors program for students interested in all aspects of biological research and biomedicine. The College of Computer, Mathematical, and Natural Sciences has partnered with the Honors College to create the ILS program, which offers nationally recognized innovations in the multidisciplinary training of life science and pre-medical students. The objective of the ILS experience is to prepare students for success in graduate, medical, dental, or other professional schools.

    University Honors (UH) is the largest living-learning program in the Honors College and allows students the greatest independence in shaping their education. University Honors students are placed into a close-knit community of the university’s faculty and other undergraduates, committed to acquiring a broad and balanced education. Students choose from over 130 seminars exploring interdisciplinary topics in three broad areas: Contemporary Issues and Challenges, Arts and Sciences in Today’s World, and Using the World as a Classroom.

    The College Park Scholars programs are two-year living-learning programs for first- and second-year students. Students are selected to enroll in one of 12 thematic programs: Arts; Business, Society, and the Economy; Environment, Technology, and Economy; Global Public Health; International Studies; Life Sciences; Media, Self, and Society; Public Leadership; Science and Global Change; Science, Discovery, and the Universe; Science, Technology, and Society. Students live in dormitories in the Cambridge Community on North Campus.

    The nation’s first living-learning entrepreneurship program, Hinman CEOs, is geared toward students who are interested in starting their own business. Students from all academic disciplines live together and are provided the resources to explore business ventures.

    The QUEST (Quality Enhancement Systems and Teams) Honors Fellows Program engages undergraduate students from business, engineering, and computer, mathematical, and physical sciences. QUEST Students participate in courses focused on cross-functional collaboration, innovation, quality management, and teamwork. The Department of Civil & Environmental Engineering (CEE) has also been long considered an outstanding engineering division of the university since its inception in 1908.

    Other living-learning programs include: CIVICUS, a two-year program in the College of Behavioral and Social Sciences based on the five principles of civil society; Global Communities, a program that immerses students in a diverse culture (students from all over the world live in a community), and the Language House, which allows students pursuing language courses to live and practice with other students learning the same language.

    The Mock Trial Team engages in intercollegiate mock trial competition. The team, which first began competing in 1990, has won five national championships (2008, 2000, 1998, 1996, 1992), which ranks the most of any university, and was also the national runner-up in 1992 and 1993.

    Research

    On October 14, 2004, the university added 150 acres (61 ha) in an attempt to create the largest research park inside the Washington, D.C., Capital Beltway, formerly known as “M Square,” and now known as the “Discovery District”.

    Many of the faculty members have funding from federal agencies such as the National Science Foundation, the National Institutes of Health, NASA, the Department of Homeland Security, the National Institute of Standards and Technology, and the National Security Agency. These relationships have created numerous research opportunities for the university including:

    Taking the lead in the nationwide research initiative into the transmission and prevention of human and avian influenza.
    Creating a new research center to study the behavioral and social foundations of terrorism with funding from the U.S. Department of Homeland Security
    Launching the joint NASA-University of Maryland Deep Impact spacecraft in early January 2005.

    The University of Maryland Libraries provide access to scholarly information resources required to meet the missions of the university.

    The University of Maryland is an international center for the study of language, hosting the largest community of language scientists in North America, including more than 200 faculty, researchers, and graduate students, who collectively comprise the Maryland Language Science Center. Since 2008 the university has hosted an NSF-IGERT interdisciplinary graduate training program that has served as a catalyst for broader integrative efforts in language science, with 50 participating students and contributions from 50 faculty. The University of Maryland is also home to two key ‘migrator’ centers that connect basic research to critical national needs in education and national security: the Center for Advanced Study of Language (CASL) and the National Foreign Language Center.

    The Center for American Politics and Citizenship provides citizens and policy-makers with research on issues related to the United States’ political institutions, processes, and policies. CAPC is a non-partisan, non-profit research institution within the Department of Government and Politics in the College of Behavioral and Social Sciences.

    The Space Systems Laboratory researches human-robotic interaction for astronautics applications, and includes the only neutral buoyancy facility at a university.

    The Joint Quantum Institute conducts theoretical and experimental research on quantum and atomic physics. The institute was founded in 2006 as a collaboration between the University of Maryland and the National Institute of Standards and Technology (NIST).

    The Center for Technology and Systems Management (CTSM) aims to advance the state of technology and systems analysis for the benefit of people and the environment. The focus is on enhancing safety, efficiency and effectiveness by performing reliability, risk, uncertainty or decision analysis studies.

    The Joint Global Change Research Institute was formed in 2001 by the University of Maryland and the DOE’s Pacific Northwest National Laboratory. The institute focuses on multidisciplinary approaches of climate change research.

    The Center for Advanced Life Cycle Engineering (CALCE) was formed in 1985 at the University of Maryland. CALCE is dedicated to providing a knowledge and resource base to support the development of electronic components, products and systems.

    The National Consortium for the Study of Terrorism and Responses to Terrorism (START) launched in 2005 as one of the Centers of Excellence supported by the Department of Homeland Security in the United States. START is focused on the scientific study of the causes and consequences of terrorism in the United States and around the world.

    The university is tied for 58th in the 2021 U.S. News & World Report rankings of “National Universities” across the United States, and it is ranked tied for 19th nationally among public universities. The Academic Ranking of World Universities ranked Maryland as 43rd in the world in 2015. The 2017–2018 Times Higher Education World University Rankings placed Maryland 69th in the world. The 2016/17 QS World University Rankings ranked Maryland 131st in the world.

    The university was ranked among Peace Corps’ 25 Top Volunteer-Producing Colleges for the tenth consecutive year in 2020. The University of Maryland is ranked among Teach for America’s Top 20 Colleges and Universities, contributing the greatest number of graduating seniors to its 2017 teaching corps. Kiplinger’s Personal Finance ranked the University 10th for in-state students and 16th for out-of-state students in its 2019 Best College Value ranking. Money Magazine ranked the university 1st in the state of Maryland for public colleges in its 2019 Best College for Your Money ranking.

    For the fourth consecutive year in 2015, the university is ranked 1st in the U.S. for the number of Boren Scholarship recipients – with 9 students receiving awards for intensive international language study. The university is ranked as a Top Producing Institution of Fulbright U.S. Students and Scholars for the 2017–2018 academic year by the United States Department of State’s Bureau of Educational and Cultural Affairs.

    In 2017, the University of Maryland was ranked among the top 50 universities in the 2018 Best Global Universities Rankings by U.S. News & World Report based on its high academic research performance and global reputation.

    In 2021, the university was ranked among the top 10 universities in The Princeton Review’s annual survey of the Top Schools for Innovation & Entrepreneurship; this was the sixth consecutive such ranking.

    WMUC-FM (88.1 FM) is the university non-commercial radio station, staffed by UMD students and volunteers. WMUC is a freeform radio station that broadcasts at 10 watts. Its broadcasts can be heard throughout the Washington metropolitan area. Notable WMUC alumni include Connie Chung, Bonnie Bernstein, Peter Rosenberg and Aaron McGruder.

     
  • richardmitnick 12:30 pm on May 29, 2023 Permalink | Reply
    Tags: "The search for habitable planets expands", , , Astrophysics, , , , , , The "soot line", The "water-ice line", The majority of detected super- Earths and sub-Neptunes lie in the “reduced carbon-rich zone.”, The team’s model theorizes about the formation of other planets born in between the “soot line” and “water-ice lines”.,   

    From The University of Michigan: “The search for habitable planets expands” 

    U Michigan bloc

    From The University of Michigan

    5.25.23
    Morgan Sherburne

    1
    Artist impression of a young planet-forming disk illustrating the respective locations of the soot and water-ice lines. Planets born interior to the “soot line” will be silicate-rich. Planets born interior to the “water-ice line”, but exterior to the soot line will be silicate and soot-rich (“Sooty Worlds”). Planets born exterior to the water-ice line will be water worlds. Image credit: Ari Gea/SayoStudio.

    A University of Michigan astronomer and his team are suggesting a new way to expand the search for habitable planets that takes into account a zone not previously considered: the space between the star and what’s called soot line in planet-forming disks.

    Worlds that form in this region—a disk of dust rotating around a central star from which planets may be built—could have surfaces rich in volatile carbon compounds quite different from Earth’s. These planets would also be rich in organic carbon, but water poor, according to Ted Bergin, who led the study that included geochemists, planetary scientists, astrochemists and exoplanet experts.

    When we search for Earth-like planets, we are particularly interested not only in bodies that look like ours, but also in those that are formed by processes similar to ours. Current models of rocky exoplanets are built using Earth-like atmospheric conditions and bulk composition, including the molecules essential for life that form from carbon-based building blocks and water. These models also focus on zones within planet-forming disks called ice lines, regions distant enough from the disk’s center star which mark where water or other key molecules transition from gas to solid phases.

    Terrestrial worlds, like our planet, formed from solids. It has long been thought that Earth, which contains only approximately 0.1% water by mass, must have formed inside the water-ice line.

    But that type of model may be too limited, Bergin said. To expand the search for habitable planets, Bergin and his research team suggest a new model that considers the soot line, a boundary closer to the solar system’s star. Between this boundary and the star, organic compounds in solids sublimate out of the solid into gas. Considering this region would also encompass rocky planets that may have more carbon than Earth has, raising questions about what that means for habitability in these kinds of planets.

    The findings by the interdisciplinary research team are published in The Astrophysical Journal Letters [below].

    “It adds a new dimension in our search for habitability. It may be a negative dimension or it may be a positive dimension,” Bergin said. “It’s exciting because it leads to all kinds of endless possibilities.”

    Just as Earth is poor in water, it is carbon poor as well, Bergin said. When forming, it likely received only 1 carbon atom per 100 available in planet-forming materials. Astronomers think the soot line explains why Earth has so little carbon. If Earth’s building blocks formed inside the soot line, the temperature and solar radiation blasted the materials that would form the young planet, turning carbon-rich compounds into gas and limiting carbon in the solids that are supplied to the forming Earth.

    The team’s model theorizes about the formation of other planets born in between the soot line and water-ice lines.

    Such a world does not appear to exist in our solar system, but our solar system is not representative of most known planetary systems around other stars, Bergin said. These other planetary systems look completely different. Their planets are closer to the sun and are much larger, ranging in size from what are called super-Earths to mini-Neptunes, he said.

    “These are either big rocks or small gas giants—that’s the most common type of planetary system. So maybe, within all those other solar systems out in the Milky Way galaxy, there exists a population of bodies that we haven’t recognized before that have much more carbon in their interiors. What are the consequences of that?” Bergin said. “What this means for habitability needs to be explored.”

    In their study, the team models what happens when a silicate-rich world with 0.1% and 1% carbon by mass and a variable water content forms in the soot line region. They found that such a planet would develop a methane-rich atmosphere through a process called outgassing. In this circumstance, organic compounds in a silicate-rich planet produce a methane-rich atmosphere.

    The presence of methane provides a fertile environment for the generation of hazes through interactions with stellar photons. This is analogous to the generation of hazes from methane in Titan in our own solar system.

    “Planets that are born within this region, which exists in every planet-forming disk system, will release more volatile carbon from their mantles,” Bergin said. “This could readily lead to the natural production of hazes. Such hazes have been observed in the atmospheres of exoplanets and have the potential to change the calculus for what we consider habitable worlds.”

    Haze around a planet might be a signpost that the planet has volatile carbon in its mantle. And more carbon, the backbone of life, in the mantle of a planet means that the planet has a chance to be considered habitable—or at least deserves a second glance, Bergin said.

    “If this is true, then there could be a common class of haze planets with abundant volatile carbon, and what that means for habitability needs to be explored,” he said. “But then there’s the other aspect: What if you have an Earth-sized world, where you have more carbon than Earth has? What does that mean for habitability, for life? We don’t know, and that’s exciting.”

    The Astrophysical Journal Letters

    1
    Figure 1. Extrapolated midplane temperatures of millimeter-sized dust as a function of radius based on measurements for three disk systems (TW Hya and CY Tau have similar profiles and are subsolar mass stars; Andrews et al. 2016; Long et al. 2018). Also shown are current confirmed exoplanets with radius measured via primary transits. Planets are culled to show only those with radii between 1 and 4 R⊕ and are plotted as a function of semimajor axis and referenced to the axis on the right (“Number of Planets”). The soot line and ice line are also shown, which have different locations depending on the system, but the majority of detected super- Earths and sub-Neptunes lie in the “reduced carbon-rich zone.”

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


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    Please support STEM education in your local school system

    Stem Education Coalition

    U MIchigan Campus

    The University of Michigan is a public research university located in Ann Arbor, Michigan, United States. Originally, founded in 1817 in Detroit as the Catholepistemiad, or University of Michigania, 20 years before the Michigan Territory officially became a state, the University of Michigan is the state’s oldest university. The university moved to Ann Arbor in 1837 onto 40 acres (16 ha) of what is now known as Central Campus. Since its establishment in Ann Arbor, the university campus has expanded to include more than 584 major buildings with a combined area of more than 34 million gross square feet (781 acres or 3.16 km²), and has two satellite campuses located in Flint and Dearborn. The University was one of the founding members of the Association of American Universities.

    Considered one of the foremost research universities in the United States, the university has very high research activity and its comprehensive graduate program offers doctoral degrees in the humanities, social sciences, and STEM fields (Science, Technology, Engineering and Mathematics) as well as professional degrees in business, medicine, law, pharmacy, nursing, social work and dentistry. Michigan’s body of living alumni (as of 2012) comprises more than 500,000. Besides academic life, Michigan’s athletic teams compete in Division I of the NCAA and are collectively known as the Wolverines. They are members of the Big Ten Conference.

    At over $12.4 billion in 2019, Michigan’s endowment is among the largest of any university. As of October 2019, 53 MacArthur “genius award” winners (29 alumni winners and 24 faculty winners), 26 Nobel Prize winners, six Turing Award winners, one Fields Medalist and one Mitchell Scholar have been affiliated with the university. Its alumni include eight heads of state or government, including President of the United States Gerald Ford; 38 cabinet-level officials; and 26 living billionaires. It also has many alumni who are Fulbright Scholars and MacArthur Fellows.

    Research

    Michigan is one of the founding members (in the year 1900) of the Association of American Universities. With over 6,200 faculty members, 73 of whom are members of the National Academy and 471 of whom hold an endowed chair in their discipline, the university manages one of the largest annual collegiate research budgets of any university in the United States. According to the National Science Foundation, Michigan spent $1.6 billion on research and development in 2018, ranking it 2nd in the nation. This figure totaled over $1 billion in 2009. The Medical School spent the most at over $445 million, while the College of Engineering was second at more than $160 million. U-M also has a technology transfer office, which is the university conduit between laboratory research and corporate commercialization interests.

    In 2009, the university signed an agreement to purchase a facility formerly owned by Pfizer. The acquisition includes over 170 acres (0.69 km^2) of property, and 30 major buildings comprising roughly 1,600,000 square feet (150,000 m^2) of wet laboratory space, and 400,000 square feet (37,000 m^2) of administrative space. At the time of the agreement, the university’s intentions for the space were not set, but the expectation was that the new space would allow the university to ramp up its research and ultimately employ in excess of 2,000 people.

    The university is also a major contributor to the medical field with the EKG and the gastroscope. The university’s 13,000-acre (53 km^2) biological station in the Northern Lower Peninsula of Michigan is one of only 47 Biosphere Reserves in the United States.

    In the mid-1960s U-M researchers worked with IBM to develop a new virtual memory architectural model that became part of IBM’s Model 360/67 mainframe computer (the 360/67 was initially dubbed the 360/65M where the “M” stood for Michigan). The Michigan Terminal System (MTS), an early time-sharing computer operating system developed at U-M, was the first system outside of IBM to use the 360/67’s virtual memory features.

    U-M is home to the National Election Studies and the University of Michigan Consumer Sentiment Index. The Correlates of War project, also located at U-M, is an accumulation of scientific knowledge about war. The university is also home to major research centers in optics, reconfigurable manufacturing systems, wireless integrated microsystems, and social sciences. The University of Michigan Transportation Research Institute and the Life Sciences Institute are located at the university. The Institute for Social Research (ISR), the nation’s longest-standing laboratory for interdisciplinary research in the social sciences, is home to the Survey Research Center, Research Center for Group Dynamics, Center for Political Studies, Population Studies Center, and Inter-Consortium for Political and Social Research. Undergraduate students are able to participate in various research projects through the Undergraduate Research Opportunity Program (UROP) as well as the UROP/Creative-Programs.

    The U-M library system comprises nineteen individual libraries with twenty-four separate collections—roughly 13.3 million volumes. U-M was the original home of the JSTOR database, which contains about 750,000 digitized pages from the entire pre-1990 backfile of ten journals of history and economics, and has initiated a book digitization program in collaboration with Google. The University of Michigan Press is also a part of the U-M library system.

    In the late 1960s U-M, together with Michigan State University and Wayne State University, founded the Merit Network, one of the first university computer networks. The Merit Network was then and remains today administratively hosted by U-M. Another major contribution took place in 1987 when a proposal submitted by the Merit Network together with its partners IBM, MCI, and the State of Michigan won a national competition to upgrade and expand the National Science Foundation Network (NSFNET) backbone from 56,000 to 1.5 million, and later to 45 million bits per second. In 2006, U-M joined with Michigan State University and Wayne State University to create the the University Research Corridor. This effort was undertaken to highlight the capabilities of the state’s three leading research institutions and drive the transformation of Michigan’s economy. The three universities are electronically interconnected via the Michigan LambdaRail (MiLR, pronounced ‘MY-lar’), a high-speed data network providing 10 Gbit/s connections between the three university campuses and other national and international network connection points in Chicago.

     
  • richardmitnick 12:00 pm on May 29, 2023 Permalink | Reply
    Tags: "A Solar System–Sized Experiment - New Proposal for Precision Cosmology and More", , Astronomers have struggled to size up the universe since Hubble first drew his famous diagram., , Astrophysics, , , , Very Very Long Baselines   

    From AAS NOVA: “A Solar System–Sized Experiment – New Proposal for Precision Cosmology and More” 

    AASNOVA

    From AAS NOVA

    5.26.23
    Ben Cassese

    Using a network of faraway telescopes in the outskirts of the solar system, astronomers could measure the distance to much farther away galaxies with exquisite precision. A recent study describes how this tactic works and explores what else we could learn with such a bold experiment.

    Very Very Long Baselines

    Distance is notoriously a tricky quantity to measure in astrophysical contexts, and astronomers have struggled to size up the universe since Hubble first drew his famous diagram.

    1
    Edwin Hubble 1929. PNAS 2003

    While they have certainly made progress over the last century, it’s natural to wonder if modern technology could enable an entirely new, more precise way to measure the gaps between galaxies.

    2
    A sketch of three detectors and a fast radio burst source. Since the wavefront is slightly curved, the same emission will strike each detector at different times. Using measurements of those differences, astronomers can back out the distance to the source. [Boone and McQuinn 2023]
    Figure 1. Example of a detector configuration that can be used to measure the distance to a source from the curvature of its wave front. The signal will arrive at detector B before it is seen at detectors A or C. By comparing the arrival times at the three detectors we can infer the distance to the source. Note that we can only measure the difference in arrival times, not the distances di directly. With two detectors the distance to the source is degenerate with the angular position on the sky θ. With three detectors in two dimensions, or four detectors in three dimensions, this degeneracy is broken and the distance to the source can be inferred.

    This thinking led Kyle Boone and Matthew McQuinn (University of Washington) to propose a bold new experiment. Their idea, described in a recent publication in The Astrophysical Journal Letters [below], is to scatter a fleet of radio telescopes throughout the solar system and instruct them to all observe the same flashing, repeating fast radio burst at the same time. Since each flash is emitted equally in all directions at the same time, the wavefront will be slightly curved when it arrives and will strike each satellite at a very slightly different time. Add up these nanosecond delays between each, and with some geometry you can back out the distance to the source.

    Such a mission would require solving numerous intense, but feasibly surmountable, engineering challenges. Chief among these, astronomers would have to know the distances between the telescopes to within just a few centimeters, a demanding requirement considering the millions of miles separating them and the many subtle forces that affect their motion. Also, each satellite would need to nurture an ultra-precise atomic clock in the face of the unforgiving vacuum of space. But, should engineers resolve these hindrances, a constellation of four or more telescopes drifting in the outer solar system could pin down the distance to each observed flash to within 1% uncertainty.

    Spanning Distances and Disciplines

    3
    The uncertainty in a measurement of the distance to a source as a function of the true distance to the source for a number of different satellite configurations. Each color represents a different possible baseline separation, and the thickness of each region marks how the uncertainty changes if the resolution of their separation varies between 0.5 and 2 cm. Note that for a source closer than 100 megaparsecs (approximately 300 million light-years), a 25 AU baseline could measure its distance to better than 1%. [Boone and McQuinn 2023]

    This experiment was conceived explicitly with precision cosmology in mind, and as Boone and McQuinn show, would be demonstrably revolutionary in that field. However, should astronomers be audacious enough to build a solar system–sized hammer, there are more than a few outstanding nails the same hardware could bludgeon. Take dark matter, for example: several models suggest that invisible clumps of the stuff should occasionally fly through the solar system at high speed. This experiment would necessarily be sensitive enough to notice the slight gravitational tug of such an encounter, meaning even a non-detection of occasional jostles could help constrain our theories of dark matter’s form. Similarly, the much debated “Planet 9” would be unable to evade such an exquisitely sensitive instrument: over time, even from hundreds of AU away, any large planets lurking in the outer solar system would eventually nudge these radio telescopes out of place.

    While this study may never grow into more than a thought experiment, such an exercise is constructive nonetheless and gives the astronomical community a chance to reflect on its current capabilities and muse about its future. That said, a more hopeful interpretation is to take this as a starting point for a grand, exacting, colossal mission that could one day uncover secrets of the universe, and our own backyard, all at once.

    4
    Figure 2. The triangular configuration of two detectors and the source used for timing. https://www.researchgate.net

    Citation

    “Solar System-scale Interferometry on Fast Radio Bursts Could Measure Cosmic Distances with Subpercent Precision,” Kyle Boone and Matthew McQuinn 2023 ApJL 947 L23.

    https://iopscience.iop.org/article/10.3847/2041-8213/acc947/pdf

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.


    Stem Education Coalition

    1

    The mission of the American Astronomical Society is to enhance and share humanity’s scientific understanding of the Universe.

    The Society, through its publications, disseminates and archives the results of astronomical research. The Society also communicates and explains our understanding of the universe to the public.
    The Society facilitates and strengthens the interactions among members through professional meetings and other means. The Society supports member divisions representing specialized research and astronomical interests.
    The Society represents the goals of its community of members to the nation and the world. The Society also works with other scientific and educational societies to promote the advancement of science.
    The Society, through its members, trains, mentors and supports the next generation of astronomers. The Society supports and promotes increased participation of historically underrepresented groups in astronomy.
    The Society assists its members to develop their skills in the fields of education and public outreach at all levels. The Society promotes broad interest in astronomy, which enhances science literacy and leads many to careers in science and engineering.

    Adopted June 7, 2009

    The society was founded in 1899 through the efforts of George Ellery Hale. The constitution of the group was written by Hale, George Comstock, Edward Morley, Simon Newcomb and Edward Charles Pickering. These men, plus four others, were the first Executive Council of the society; Newcomb was the first president. The initial membership was 114. The AAS name of the society was not finally decided until 1915, previously it was the “Astronomical and Astrophysical Society of America”. One proposed name that preceded this interim name was “American Astrophysical Society”.

    The AAS today has over 7,000 members and six divisions – the Division for Planetary Sciences (1968); the Division on Dynamical Astronomy (1969); the High Energy Astrophysics Division (1969); the Solar Physics Division (1969); the Historical Astronomy Division (1980); and the Laboratory Astrophysics Division (2012). The membership includes physicists, mathematicians, geologists, engineers and others whose research interests lie within the broad spectrum of subjects now comprising contemporary astronomy.

    In 2019 three AAS members were selected into the tenth anniversary class of TED Fellows.

    The AAS established the AAS Fellows program in 2019 to “confer recognition upon AAS members for achievement and extraordinary service to the field of astronomy and the American Astronomical Society.” The inaugural class was designated by the AAS Board of Trustees and includes an initial group of 232 Legacy Fellows.

     
  • richardmitnick 11:42 am on May 29, 2023 Permalink | Reply
    Tags: "Study doubles the number of known repeating fast radio bursts", , , Astrophysics, , , , , ,   

    From The Kavli Institute For Astrophysics and Space Research At The Massachusetts Institute of Technology: “Study doubles the number of known repeating fast radio bursts” 

    KavliFoundation

    http://www.kavlifoundation.org/institutes

    From The Kavli Institute For Astrophysics and Space Research

    At

    The Massachusetts Institute of Technology

    5.25.23
    Statistics tools support the idea that all radio bursts may repeat if observed long enough.

    Fast radio bursts (FRBs) are repeating flashes of radio waves that remain a source of mystery to astronomers. We do know a few things about them: FRBs originate from far outside the Milky Way, for instance, and they’re probably produced from the cinders of dying stars. While many astronomical radio waves have been observed to have burst only once, some waves have been seen bursting multiple times — a puzzle that has led astronomers to question if these radio waves are similar in nature and origin.

    Now, a large team of astronomers, including several from the MIT Kavli Institute for Astrophysics and Space Research and the MIT Department of Physics, have collaborated on work to decipher the origin and nature of FRBs. Their recent open-access publication in The Astrophysical Journal [below] reports the discovery of 25 new repeating FRB sources, doubling the known number of these phenomena known to scientists to 50. In addition, the team found that many repeating FRBs are inactive, producing less than one burst per week of observing time.

    The Canadian-led Canadian Hydrogen Intensity Mapping Experiment (CHIME) has been instrumental in detecting thousands of FRBs as it scans the entire northern sky. So, astronomers with the CHIME/FRB Collaboration developed a new set of statistics tools to comb through massive sets of data to find every repeating source detected so far. This provided a valuable opportunity for astronomers to observe the same source with different telescopes and study the diversity of emission. “We can now accurately calculate the probability that two or more bursts coming from similar locations are not just a coincidence,” explains Ziggy Pleunis, a Dunlap Postdoctoral Fellow at the Dunlap Institute for Astronomy and Astrophysics and corresponding author of the new work.

    The team also concluded that all FRBs may eventually repeat. They found that radio waves seen to have burst only once differed from those that were seen to have burst multiple times both in terms of duration of bursts and range of frequencies emitted, which solidifies the idea that these radio bursts have indeed different origins.

    MIT postdoc Daniele Michilli and PhD student Kaitlyn Shin, both members of MIT Assistant Professor Kiyoshi Masui’s Synoptic Radio Lab, analyzed signals from CHIME’s 1,024 antennae. The work, Michilli says, “allowed us to unambiguously identify some of the sources as repeaters and to provide other observatories with accurate coordinates for follow-up studies.”

    “Now that we have a much larger sample of repeating FRBs, we’re better equipped to understand why we might observe some FRBs to be repeaters and others to be apparently non-repeating, and what the implications are for better understanding their origins,” says Shin.

    Adds Pleunis, “FRBs are likely produced by the leftovers from explosive stellar deaths. By studying repeating FRB sources in detail, we can study the environments that these explosions occur in and understand better the end stages of a star’s life. We can also learn more about the material that is being expelled before and during the star’s demise, which is then returned to the galaxies that the FRBs live in.”

    In addition to Michilli, Shin, and Masui, MIT contributors to the study include physics graduate students Calvin Leung and Haochen Wang.

    The Astrophysical Journal

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.


    Stem Education Coalition

    The mission of the The Massachusetts Institute of Technology Kavli Institute For Astrophysics and Space Research is to facilitate and carry out the research programs of faculty and research staff whose interests lie in the broadly defined area of astrophysics and space research. Specifically, the MKI will:

    Provide an intellectual home for faculty, research staff, and students engaged in space- and ground-based astrophysics
    Develop and operate space- and ground-based instrumentation for astrophysics
    Engage in technology development
    Maintain an engineering and technical core capability for enabling and supporting innovative research
    Communicate to students, educators, and the public an understanding of and an appreciation for the goals, techniques and results of MKI’s research.

    The Foundation’s mission is implemented through an international program of research institutes, professorships, and symposia in the fields of astrophysics, nanoscience, neuroscience, and theoretical physics as well as prizes in the fields of astrophysics, nanoscience, and neuroscience.
    The mission of the The Massachusetts Institute of Technology Kavli Institute For Astrophysics and Space Research is to facilitate and carry out the research programs of faculty and research staff whose interests lie in the broadly defined area of astrophysics and space research. Specifically, the MKI will

    Provide an intellectual home for faculty, research staff, and students engaged in space- and ground-based astrophysics
    Develop and operate space- and ground-based instrumentation for astrophysics
    Engage in technology development
    Maintain an engineering and technical core capability for enabling and supporting innovative research
    Communicate to students, educators, and the public an understanding of and an appreciation for the goals, techniques and results of MKI’s research.

    The Kavli Foundation, based in Oxnard, California, is dedicated to the goals of advancing science for the benefit of humanity and promoting increased public understanding and support for scientists and their work.

    The Foundation’s mission is implemented through an international program of research institutes, professorships, and symposia in the fields of astrophysics, nanoscience, neuroscience, and theoretical physics as well as prizes in the fields of astrophysics, nanoscience, and neuroscience.

    MIT Campus

    The Massachusetts Institute of Technology is a private land-grant research university in Cambridge, Massachusetts. The institute has an urban campus that extends more than a mile (1.6 km) alongside the Charles River. The institute also encompasses a number of major off-campus facilities such as the MIT Lincoln Laboratory , the MIT Bates Research and Engineering Center , and the Haystack Observatory , as well as affiliated laboratories such as the Broad Institute of MIT and Harvard and Whitehead Institute.

    Founded in 1861 in response to the increasing industrialization of the United States, Massachusetts Institute of Technology adopted a European polytechnic university model and stressed laboratory instruction in applied science and engineering. It has since played a key role in the development of many aspects of modern science, engineering, mathematics, and technology, and is widely known for its innovation and academic strength. It is frequently regarded as one of the most prestigious universities in the world.

    As of December 2020, 97 Nobel laureates, 26 Turing Award winners, and 8 Fields Medalists have been affiliated with MIT as alumni, faculty members, or researchers. In addition, 58 National Medal of Science recipients, 29 National Medals of Technology and Innovation recipients, 50 MacArthur Fellows, 80 Marshall Scholars, 3 Mitchell Scholars, 22 Schwarzman Scholars, 41 astronauts, and 16 Chief Scientists of the U.S. Air Force have been affiliated with The Massachusetts Institute of Technology . The university also has a strong entrepreneurial culture and MIT alumni have founded or co-founded many notable companies. Massachusetts Institute of Technology is a member of the Association of American Universities (AAU).

    Foundation and vision

    In 1859, a proposal was submitted to the Massachusetts General Court to use newly filled lands in Back Bay, Boston for a “Conservatory of Art and Science”, but the proposal failed. A charter for the incorporation of the Massachusetts Institute of Technology, proposed by William Barton Rogers, was signed by John Albion Andrew, the governor of Massachusetts, on April 10, 1861.

    Rogers, a professor from the University of Virginia , wanted to establish an institution to address rapid scientific and technological advances. He did not wish to found a professional school, but a combination with elements of both professional and liberal education, proposing that:

    “The true and only practicable object of a polytechnic school is, as I conceive, the teaching, not of the minute details and manipulations of the arts, which can be done only in the workshop, but the inculcation of those scientific principles which form the basis and explanation of them, and along with this, a full and methodical review of all their leading processes and operations in connection with physical laws.”

    The Rogers Plan reflected the German research university model, emphasizing an independent faculty engaged in research, as well as instruction oriented around seminars and laboratories.

    Early developments

    Two days after The Massachusetts Institute of Technology was chartered, the first battle of the Civil War broke out. After a long delay through the war years, MIT’s first classes were held in the Mercantile Building in Boston in 1865. The new institute was founded as part of the Morrill Land-Grant Colleges Act to fund institutions “to promote the liberal and practical education of the industrial classes” and was a land-grant school. In 1863 under the same act, the Commonwealth of Massachusetts founded the Massachusetts Agricultural College, which developed as the University of Massachusetts Amherst ). In 1866, the proceeds from land sales went toward new buildings in the Back Bay.

    The Massachusetts Institute of Technology was informally called “Boston Tech”. The institute adopted the European polytechnic university model and emphasized laboratory instruction from an early date. Despite chronic financial problems, the institute saw growth in the last two decades of the 19th century under President Francis Amasa Walker. Programs in electrical, chemical, marine, and sanitary engineering were introduced, new buildings were built, and the size of the student body increased to more than one thousand.

    The curriculum drifted to a vocational emphasis, with less focus on theoretical science. The fledgling school still suffered from chronic financial shortages which diverted the attention of the MIT leadership. During these “Boston Tech” years, Massachusetts Institute of Technology faculty and alumni rebuffed Harvard University president (and former MIT faculty) Charles W. Eliot’s repeated attempts to merge MIT with Harvard College’s Lawrence Scientific School. There would be at least six attempts to absorb MIT into Harvard. In its cramped Back Bay location, MIT could not afford to expand its overcrowded facilities, driving a desperate search for a new campus and funding. Eventually, the MIT Corporation approved a formal agreement to merge with Harvard, over the vehement objections of MIT faculty, students, and alumni. However, a 1917 decision by the Massachusetts Supreme Judicial Court effectively put an end to the merger scheme.

    In 1916, The Massachusetts Institute of Technology administration and the MIT charter crossed the Charles River on the ceremonial barge Bucentaur built for the occasion, to signify MIT’s move to a spacious new campus largely consisting of filled land on a one-mile-long (1.6 km) tract along the Cambridge side of the Charles River. The neoclassical “New Technology” campus was designed by William W. Bosworth and had been funded largely by anonymous donations from a mysterious “Mr. Smith”, starting in 1912. In January 1920, the donor was revealed to be the industrialist George Eastman of Rochester, New York, who had invented methods of film production and processing, and founded Eastman Kodak. Between 1912 and 1920, Eastman donated $20 million ($236.6 million in 2015 dollars) in cash and Kodak stock to MIT.

    Curricular reforms

    In the 1930s, President Karl Taylor Compton and Vice-President (effectively Provost) Vannevar Bush emphasized the importance of pure sciences like physics and chemistry and reduced the vocational practice required in shops and drafting studios. The Compton reforms “renewed confidence in the ability of the Institute to develop leadership in science as well as in engineering”. Unlike Ivy League schools, Massachusetts Institute of Technology catered more to middle-class families, and depended more on tuition than on endowments or grants for its funding. The school was elected to the Association of American Universities in 1934.

    Still, as late as 1949, the Lewis Committee lamented in its report on the state of education at The Massachusetts Institute of Technology that “the Institute is widely conceived as basically a vocational school”, a “partly unjustified” perception the committee sought to change. The report comprehensively reviewed the undergraduate curriculum, recommended offering a broader education, and warned against letting engineering and government-sponsored research detract from the sciences and humanities. The School of Humanities, Arts, and Social Sciences and the MIT Sloan School of Management were formed in 1950 to compete with the powerful Schools of Science and Engineering. Previously marginalized faculties in the areas of economics, management, political science, and linguistics emerged into cohesive and assertive departments by attracting respected professors and launching competitive graduate programs. The School of Humanities, Arts, and Social Sciences continued to develop under the successive terms of the more humanistically oriented presidents Howard W. Johnson and Jerome Wiesner between 1966 and 1980.

    The Massachusetts Institute of Technology ‘s involvement in military science surged during World War II. In 1941, Vannevar Bush was appointed head of the federal Office of Scientific Research and Development and directed funding to only a select group of universities, including MIT. Engineers and scientists from across the country gathered at Massachusetts Institute of Technology ‘s Radiation Laboratory, established in 1940 to assist the British military in developing microwave radar. The work done there significantly affected both the war and subsequent research in the area. Other defense projects included gyroscope-based and other complex control systems for gunsight, bombsight, and inertial navigation under Charles Stark Draper’s Instrumentation Laboratory; the development of a digital computer for flight simulations under Project Whirlwind; and high-speed and high-altitude photography under Harold Edgerton. By the end of the war, The Massachusetts Institute of Technology became the nation’s largest wartime R&D contractor (attracting some criticism of Bush), employing nearly 4000 in the Radiation Laboratory alone and receiving in excess of $100 million ($1.2 billion in 2015 dollars) before 1946. Work on defense projects continued even after then. Post-war government-sponsored research at MIT included SAGE and guidance systems for ballistic missiles and Project Apollo.

    These activities affected The Massachusetts Institute of Technology profoundly. A 1949 report noted the lack of “any great slackening in the pace of life at the Institute” to match the return to peacetime, remembering the “academic tranquility of the prewar years”, though acknowledging the significant contributions of military research to the increased emphasis on graduate education and rapid growth of personnel and facilities. The faculty doubled and the graduate student body quintupled during the terms of Karl Taylor Compton, president of The Massachusetts Institute of Technology between 1930 and 1948; James Rhyne Killian, president from 1948 to 1957; and Julius Adams Stratton, chancellor from 1952 to 1957, whose institution-building strategies shaped the expanding university. By the 1950s, The Massachusetts Institute of Technology no longer simply benefited the industries with which it had worked for three decades, and it had developed closer working relationships with new patrons, philanthropic foundations and the federal government.

    In late 1960s and early 1970s, student and faculty activists protested against the Vietnam War and The Massachusetts Institute of Technology ‘s defense research. In this period Massachusetts Institute of Technology’s various departments were researching helicopters, smart bombs and counterinsurgency techniques for the war in Vietnam as well as guidance systems for nuclear missiles. The Union of Concerned Scientists was founded on March 4, 1969 during a meeting of faculty members and students seeking to shift the emphasis on military research toward environmental and social problems. The Massachusetts Institute of Technology ultimately divested itself from the Instrumentation Laboratory and moved all classified research off-campus to the MIT Lincoln Laboratory facility in 1973 in response to the protests. The student body, faculty, and administration remained comparatively unpolarized during what was a tumultuous time for many other universities. Johnson was seen to be highly successful in leading his institution to “greater strength and unity” after these times of turmoil. However six Massachusetts Institute of Technology students were sentenced to prison terms at this time and some former student leaders, such as Michael Albert and George Katsiaficas, are still indignant about MIT’s role in military research and its suppression of these protests. (Richard Leacock’s film, November Actions, records some of these tumultuous events.)

    In the 1980s, there was more controversy at The Massachusetts Institute of Technology over its involvement in SDI (space weaponry) and CBW (chemical and biological warfare) research. More recently, The Massachusetts Institute of Technology’s research for the military has included work on robots, drones and ‘battle suits’.

    Recent history

    The Massachusetts Institute of Technology has kept pace with and helped to advance the digital age. In addition to developing the predecessors to modern computing and networking technologies, students, staff, and faculty members at Project MAC, the Artificial Intelligence Laboratory, and the Tech Model Railroad Club wrote some of the earliest interactive computer video games like Spacewar! and created much of modern hacker slang and culture. Several major computer-related organizations have originated at MIT since the 1980s: Richard Stallman’s GNU Project and the subsequent Free Software Foundation were founded in the mid-1980s at the AI Lab; the MIT Media Lab was founded in 1985 by Nicholas Negroponte and Jerome Wiesner to promote research into novel uses of computer technology; the World Wide Web Consortium standards organization was founded at the Laboratory for Computer Science in 1994 by Tim Berners-Lee; the MIT OpenCourseWare project has made course materials for over 2,000 Massachusetts Institute of Technology classes available online free of charge since 2002; and the One Laptop per Child initiative to expand computer education and connectivity to children worldwide was launched in 2005.

    The Massachusetts Institute of Technology was named a sea-grant college in 1976 to support its programs in oceanography and marine sciences and was named a space-grant college in 1989 to support its aeronautics and astronautics programs. Despite diminishing government financial support over the past quarter century, MIT launched several successful development campaigns to significantly expand the campus: new dormitories and athletics buildings on west campus; the Tang Center for Management Education; several buildings in the northeast corner of campus supporting research into biology, brain and cognitive sciences, genomics, biotechnology, and cancer research; and a number of new “backlot” buildings on Vassar Street including the Stata Center. Construction on campus in the 2000s included expansions of the Media Lab, the Sloan School’s eastern campus, and graduate residences in the northwest. In 2006, President Hockfield launched the MIT Energy Research Council to investigate the interdisciplinary challenges posed by increasing global energy consumption.

    In 2001, inspired by the open source and open access movements, The Massachusetts Institute of Technology launched OpenCourseWare to make the lecture notes, problem sets, syllabi, exams, and lectures from the great majority of its courses available online for no charge, though without any formal accreditation for coursework completed. While the cost of supporting and hosting the project is high, OCW expanded in 2005 to include other universities as a part of the OpenCourseWare Consortium, which currently includes more than 250 academic institutions with content available in at least six languages. In 2011, The Massachusetts Institute of Technology announced it would offer formal certification (but not credits or degrees) to online participants completing coursework in its “MITx” program, for a modest fee. The “edX” online platform supporting MITx was initially developed in partnership with Harvard and its analogous “Harvardx” initiative. The courseware platform is open source, and other universities have already joined and added their own course content. In March 2009 the Massachusetts Institute of Technology faculty adopted an open-access policy to make its scholarship publicly accessible online.

    The Massachusetts Institute of Technology has its own police force. Three days after the Boston Marathon bombing of April 2013, MIT Police patrol officer Sean Collier was fatally shot by the suspects Dzhokhar and Tamerlan Tsarnaev, setting off a violent manhunt that shut down the campus and much of the Boston metropolitan area for a day. One week later, Collier’s memorial service was attended by more than 10,000 people, in a ceremony hosted by the Massachusetts Institute of Technology community with thousands of police officers from the New England region and Canada. On November 25, 2013, The Massachusetts Institute of Technology announced the creation of the Collier Medal, to be awarded annually to “an individual or group that embodies the character and qualities that Officer Collier exhibited as a member of The Massachusetts Institute of Technology community and in all aspects of his life”. The announcement further stated that “Future recipients of the award will include those whose contributions exceed the boundaries of their profession, those who have contributed to building bridges across the community, and those who consistently and selflessly perform acts of kindness”.

    In September 2017, the school announced the creation of an artificial intelligence research lab called the MIT-IBM Watson AI Lab. IBM will spend $240 million over the next decade, and the lab will be staffed by MIT and IBM scientists. In October 2018 MIT announced that it would open a new Schwarzman College of Computing dedicated to the study of artificial intelligence, named after lead donor and The Blackstone Group CEO Stephen Schwarzman. The focus of the new college is to study not just AI, but interdisciplinary AI education, and how AI can be used in fields as diverse as history and biology. The cost of buildings and new faculty for the new college is expected to be $1 billion upon completion.

    The Caltech/MIT Advanced aLIGO was designed and constructed by a team of scientists from California Institute of Technology , Massachusetts Institute of Technology, and industrial contractors, and funded by the National Science Foundation .

    Caltech /MIT Advanced aLigo

    It was designed to open the field of gravitational-wave astronomy through the detection of gravitational waves predicted by general relativity. Gravitational waves were detected for the first time by the LIGO detector in 2015. For contributions to the LIGO detector and the observation of gravitational waves, two Caltech physicists, Kip Thorne and Barry Barish, and Massachusetts Institute of Technology physicist Rainer Weiss won the Nobel Prize in physics in 2017. Weiss, who is also a Massachusetts Institute of Technology graduate, designed the laser interferometric technique, which served as the essential blueprint for the LIGO.

    The mission of The Massachusetts Institute of Technology is to advance knowledge and educate students in science, technology, and other areas of scholarship that will best serve the nation and the world in the twenty-first century. We seek to develop in each member of The Massachusetts Institute of Technology community the ability and passion to work wisely, creatively, and effectively for the betterment of humankind.

     
  • richardmitnick 10:36 am on May 29, 2023 Permalink | Reply
    Tags: "Biosignatures": evidence of life but simple or multicellular life., "Frank Drake - SETI visionary born on this date", , , Astrophysics, , , , , , In May 2021 John Gertz made a case for rewriting the Drake equation., The "Wow! signal", ,   

    From “EarthSky” And The SETI Institute: “Frank Drake – SETI visionary born on this date” 

    1

    From “EarthSky”

    And


    The SETI Institute

    5.28.23
    Kelly Kizer Whitt
    Deborah Byrd

    1
    Astronomer Frank Drake speaking at Cornell University in October 2017. Image via Wikipedia (CC BY-SA 4.0).

    Astronomer Frank Drake

    May 28, 2023, would be the 93rd birthday of astronomer Frank Drake. Sadly, he passed away recently, on September 2, 2022. Drake was an early visionary in the search for other civilizations in our Milky Way galaxy.

    In 1960, Drake spearheaded Project Ozma, the first modern attempt to listen for radio transmissions from otherworldly intelligences.

    2
    Previously, owned by the National Radio Astronomy Observatory (NRAO), Green Bank Observatory’s second 85-foot telescope (85-2) was, like its predecessor, the Howard E. Tatel Telescope, was built from a kit by the Blaw-Knox Corporation. Completed in February 1964, the 85-2 paired with the Tatel to form the NRAO’s first array, the Green Bank Interferometer (GBI). The GBI was changeable, because the 85-2 telescope sat on its own set of 64 wheels, and tractors could haul it up and down this stretch of road leading from the Tatel. In fact, the D7 Bulldozer in the foreground right was used as a pulling truck. Changing the distance between the 85-footers changed the resolution of the array’s combined view: farther equals higher resolution. An early computer combined the data from the two telescopes, and the cable tray for the signals runs along the far left of this photo. Today, there are three 85-foot dish antenna’s that for the GBI.

    Then, on November 1, 1961, Drake, Carl Sagan and other astronomers met at the site of the Green Bank Telescope in Green Bank, West Virginia. And at that meeting, Drake presented what has become known as the Drake equation.

    3
    NASA
    __________________________________________________________________

    Green Bank Observatory


    __________________________________________________________________

    Scientists and others found the Drake equation fascinating then … and they still do. The Drake equation is a tool for contemplating how many intelligent civilizations might be capable of communicating with us from elsewhere in the galaxy. From Drake’s formulation of the equation – and the 1961 meeting in Green Bank – the field of research and scientific organization known as SETI, the search for extraterrestrial intelligence, was born.

    What is the Drake equation?

    The Drake equation is a mathematical formula for thinking about how many civilizations beyond Earth might be able to communicate with us. Nowadays when you hear astronomers speak of life beyond Earth, they might be focused on biosignatures. That’s where they are looking for evidence of life, but for simple or multicellular life. For example, possible life forms under rocks on Mars or in the atmosphere of Venus. However, the Drake equation focuses on something different. In fact, it’s the search for advanced and communicating civilizations.

    Thus, here is the Drake equation: N = R* • fp • ne • fl • fi • fc • L

    Breaking down the Drake equation

    N = the number of civilizations in our galaxy with which communication might be possible.
    R* = the average rate of star formation in our galaxy.
    fp = the fraction of those stars that have planets.
    ne = the average number of planets that can potentially support life per star that has planets.
    fl = the fraction of planets that could support life that actually develop life at some point.
    fi = the fraction of planets with civilizations that actually go on to develop intelligent life.
    fc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space.
    L = the length of time for which such civilizations release detectable signals into space.

    As originally formulated, the Drake equation is less a true mathematical formula and more a way to start a conversation. So the value of N – the number of civilizations with which we might communicate – is difficult to determine if you don’t have solid numbers on all the factors that need to be considered.

    So do astronomers know the rate of star formation in our Milky Way? Yes, approximately. The rate of star formation is somewhere around 3 solar masses per year. Next, do they know how many stars form planets? Of course, we didn’t know that number in 1961, but now we do. In fact, the answer is thought to be that most, if not all, of them form planets.

    But, as you go onward in the equation, the state of our knowledge begins to falter. First, we don’t know the mean number of planets that could support life per star with planets. Second, we don’t know the fraction of life-supporting planets that develop life. And so on.

    Drake equation revisited

    Additionally, a wonderful thing about the Drake equation, is it continues to inspire fresh thinking about extraterrestrial life among astronomers. So in 2016, Adam Frank and Woodruff Sullivan put their heads together to publish a paper in the journal Astrobiology [below] in which they presented the Drake equation in a new light. Then they noted that technological advancements in astronomy had made better estimates possible of two Drake equation factors:

    The fraction of stars with planets, fp, is now estimated to be 1.0, meaning all stars have planets

    The number of planets per star where conditions are suitable for life, ne, is now estimated to be 0.2, meaning one in five planets can support life

    A case for rewriting the Drake equation

    In May 2021, John Gertz made a case for rewriting the Drake equation in a paper accepted for publication by the Journal of the British Interplanetary Society [below]. Here are Gertz’s thoughts on the Drake equations variables:

    R*, the mean rate of star formation changes over the history of our galaxy. Plus, what about other galaxies? The rate of star formation would be different. In his May 2021 paper, Gertz suggested changing R* to Ns. That’s for the number of candidate stars in the Milky Way that fall within our field of view. He pointed out that 80% of these stars would be stars not so very different from our sun.

    Fp, the fraction of stars that have planets, is no longer a big unknown. That’s because we now know that planets around stars are quite common.

    Ne, the number of rocky planets in a star’s habitable zone, is too limiting. Plus the presence of an atmosphere and water are important considerations. But so are the countless moons where life could exist around planets outside a star’s habitable zone. So Gertz recommends replacing this variable with Ntb. That stands for the total number of bodies that could support life on or beneath their surfaces.

    Currently, Fl, the fraction of planets that develop life, is unknowable. Also, it’s still not understood the origin of life on Earth, much less how common or rare it is in the universe.

    Fi, the fraction of planets with life that develop intelligence, is also unknowable. If we don’t know how common life may be in the universe, we don’t know how common intelligent life may be.

    More of Gertz’s suggested revisions

    Fc, the fraction of intelligent civilizations technologically capable and actively trying to communicate with us, doesn’t take into consideration the vast expanses that communication would have to travel between our home worlds. But we could also unintentionally stumble across a signal (perhaps the Wow! signal?).

    Then a better variable, Gertz says, is Fd, the fraction of technological life that is detectable by any means. However, the problem may not be the civilization sending us a message. Instead, the problem could be that we aren’t advanced enough to detect or receive it.

    L, the length of time a civilization is communicative, depends on how long they can sustain themselves before they either self-destruct or something external (asteroid, supernova or the like) takes them out. We don’t know the answer, either for ourselves or for an alien civilization. This variable is the one that Carl Sagan considered most uncertain. Gertz’s ideas about L mesh nicely with Avi Loeb’s assertion that ‘Oumuamua is of alien origin. Gertz commented:

    “The Drake equation was predicated upon the notion that there is a finite number of currently existing alien civilizations ensconced among the stars, some of whom will be signaling their presence to us using radio or optical lasers. However, this ignores another school of thought which holds that ET’s far better strategy would be to send physical probes to our solar system to surveil and ultimately make contact with us. Such probes could represent information from innumerable civilizations, many of whom may have long ago perished. If this is the case, Drake’s L is irrelevant, since the probe might far outlive its progenitor, and his N reduces to one, the single probe that makes its presence known to us through which alone we might communicate with the rest of the galaxy.”

    Gertz’s final version of the Drake equation

    What’s left is John Gertz’s updated take on the Drake equation: N = ns • fp • ntb • fl • fi • fd • L

    ns is the number of spots on the sky within our field of view.
    fp is the fraction of stars with planets.
    ntb is the average number of bodies within each that could engender life.
    fl is the fraction of those that actually do give birth to life.
    fi is the fraction of systems with life that evolves technological intelligence.
    fd is the fraction of technological life that is detectable by any means.
    L is the duration of detectability.

    Where do SETI researchers go from here?

    The plan is for radio wave and visible-light observations, combined with technological advances that will eventually let scientists survey one million nearby stars, the entire galactic plane and 100 nearby galaxies. Dedicated wide-field telescopes are one of the items on Gertz’s wish list for SETI.

    Breakthrough Listen, a project Gertz is currently involved in, is a good start.

    ___________________________________________________________________
    Breakthrough Listen Project

    1

    UC Observatories Lick Automated Planet Finder fully robotic 2.4-meter optical telescope at Lick Observatory, situated on the summit of Mount Hamilton, east of San Jose, California

    Green Bank Radio Telescope, West Virginia, now the center piece of the Green Bank Observatory, being cut loose by the National Science Foundation, supported by Breakthrough Listen Project, West Virginia University, and operated by the nonprofit Associated Universities, Inc.

    CSIRO-Commonwealth Scientific and Industrial Research Organisation (AU) Parkes Observatory [ Murriyang, the traditional Indigenous name] , located 20 kilometres north of the town of Parkes, New South Wales, Australia, 414.80m above sea level.

    SKA SARAO Meerkat telescope(SA) 90 km outside the small Northern Cape town of Carnarvon, SA.

    Newly added

    University of Arizona Veritas Four Čerenkov telescopes A novel gamma ray telescope under construction at the CfA Fred Lawrence Whipple Observatory, Mount Hopkins, Arizona, altitude 2,606 m 8,550 ft. A large project known as the Čerenkov Telescope Array, composed of hundreds of similar telescopes to be situated at Roque de los Muchachos Observatory [Instituto de Astrofísica de Canarias ](ES) in the Canary Islands and Chile at European Southern Observatory Cerro Paranal(EU) site. The telescope on Mount Hopkins will be fitted with a prototype high-speed camera, assembled at the University of Wisconsin–Madison and capable of taking pictures at a billion frames per second. Credit: Vladimir Vassiliev. ___________________________________________________________________
    It is the largest-ever scientific research program aimed at finding evidence of civilizations beyond Earth. Breakthrough Listen scans the radio spectrum with the world’s most powerful instruments. Gertz said:

    “Breakthrough Listen is a game-changer. Because of it, more SETI is accomplished in a single day than was ever before accomplished in a full year.”

    Funding will be the key to continued searches, and, with a lot of planning and maybe a little luck, to future success in finding an intelligent civilization in the wider universe.


    The Drake Equation After Sixty Years | Part 1


    The Birth-Death Drake Equation | Part 2

    Astrobiology 2016
    Journal of the British Interplanetary Society 2021


    https://www.semanticscholar.org

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


    five-ways-keep-your-child-safe-school-shootings
    Please help promote STEM in your local schools.


    Stem Education Coalition

    SETI Institute
    About The SETI Institute
    What is life? How does it begin? Are we alone? These are some of the questions we ask in our quest to learn about and share the wonders of the universe. At the SETI Institute we have a passion for discovery and for passing knowledge along as scientific ambassadors.

    The SETI Institute is a 501 (c)(3) nonprofit scientific research institute headquartered in Mountain View, California. We are a key research contractor to NASA and the National Science Foundation (NSF), and we collaborate with industry partners throughout Silicon Valley and beyond.

    Founded in 1984, the SETI Institute employs more than 130 scientists, educators, and administrative staff. Work at the SETI Institute is anchored by three centers: the Carl Sagan Center for the Study of Life in the Universe (research), the Center for Education and the Center for Outreach.

    The SETI Institute welcomes philanthropic support from individuals, private foundations, corporations and other groups to support our education and outreach initiatives, as well as unfunded scientific research and fieldwork.

    A Special Thank You to SETI Institute Partners and Collaborators
    Campoalto, Chile, NASA Ames Research Center, NASA Headquarters, National Science Foundation, Aerojet Rocketdyne,SRI International

    Frontier Development Lab Partners
    Breakthrough Prize Foundation, The European Space Agency [La Agencia Espacial Europea] [Agence spatiale européenne][Europäische Weltraumorganisation](EU), Google Cloud, IBM, Intel, KBRwyle. Kx Lockheed Martin, NASA Ames Research Center, Nvidia, SpaceResources Luxembourg, XPrize
    In-kind Service Providers
    • Gunderson Dettmer – General legal services, Hello Pilgrim – Website Design and Development Steptoe & Johnson – IP legal services, Danielle Futselaar

    SETI/Allen Telescope Array situated at the Hat Creek Radio Observatory, 290 miles (470 km) northeast of San Francisco, California, USA, Altitude 986 m (3,235 ft), the origins of the Institute’s search.

    March 23, 2015
    By Hilary Lebow
    The NIROSETI instrument saw first light on the Nickel 1-meter Telescope at Lick Observatory on March 15, 2015. (Photo by Laurie Hatch.)

    Astronomers are expanding the search for extraterrestrial intelligence into a new realm with detectors tuned to infrared light at UC’s Lick Observatory. A new instrument, called NIROSETI, will soon scour the sky for messages from other worlds.


    Shelley Wright of UC San Diego with NIROSETI, developed at U Toronto Dunlap Institute for Astronomy and Astrophysics (CA) at the 1-meter Nickel Telescope at Lick Observatory at UC Santa Cruz

    NIROSETI team from left to right Rem Stone UCO Lick Observatory Dan Werthimer, UC Berkeley; Jérôme Maire, U Toronto; Shelley Wright, UCSD; Patrick Dorval, U Toronto; Richard Treffers, Starman Systems. (Image by Laurie Hatch).

    Laser SETI


    There is also an installation at Robert Ferguson Observatory, Sonoma, CA aimed West for full coverage [no image available].

    SETI Institute – 189 Bernardo Ave., Suite 100
    Mountain View, CA 94043
    Phone 650.961.6633 – Fax 650-961-7099
    Privacy PolicyQuestions and Comments

    Deborah Byrd created the EarthSky radio series in 1991 and founded EarthSky.org in 1994. Today, she serves as Editor-in-Chief of this website. She has won a galaxy of awards from the broadcasting and science communities, including having an asteroid named 3505 Byrd in her honor. A science communicator and educator since 1976, Byrd believes in science as a force for good in the world and a vital tool for the 21st century. “Being an EarthSky editor is like hosting a big global party for cool nature-lovers,” she says.

     
  • richardmitnick 9:59 am on May 29, 2023 Permalink | Reply
    Tags: "Q&A with Project Scientist Roberta Zanin", , Astrophysics, , , ,   

    From The Čerenkov Telescope Array (CL)(ES) : “Q&A with Project Scientist Roberta Zanin” 

    From The Čerenkov Telescope Array (CL)(ES)

    5.29.23

    1
    Project Scientist Roberta Zanin.

    Building an observatory is no small feat, especially when it comes to ensuring that what is built achieves the science goals of the scientists it is going to serve. As the CTAO’s Project Scientist, Roberta Zanin is responsible for providing a link between the CTAO’s engineers and the science community to make sure that everything from the telescope specifications to the data products are designed and built to achieve the ultimate mission of the CTAO: to make unprecedented discoveries about the gamma-ray Universe. We sat down with Roberta to learn more about her and her work toward making the CTAO a world-class observatory…
    ________________________________________________________________________________________________

    Tell us about yourself and how you came into your present role.

    I decided to study Physics when I was 13 years old. At that age, I discovered what an internal combustion engine was at school and found it fascinating — I think I always had a very experimental approach to all aspects of my life! However, it was clear to me that I did not want to be an engineer, but a physicist. What I was looking for was to study and understand the basic principles of science.

    This is how I started my Physics degree at the Università di Padova (Italy), where I entered the field of astroparticle physics. Within this, I opted for gamma-ray astronomy and ended up doing my master’s thesis on the MAGIC telescopes, the preceding generation of the CTAO.

    Over the years, I participated and worked in the different instruments that compose the current generation of Imaging Atmospheric Cherenkov Telescopes or IACTs (H.E.S.S., MAGIC and VERITAS), where I had different coordination positions, especially focused on galactic physics. In fact, my field of study focused on the understanding of the very high-energy emission emitted by Galactic sources, such as rapid rotating and magnetized neutron stars (pulsars), their environment (Pulsar Wind Nebulae), or binary systems ejecting powerful jets (microquasars).

    My involvement with the CTAO started as a member of the Cherenkov Telescope Array Consortium (CTAC), where I served as Coordinator of the Galactic Working Group and worked in the development of software for data analysis and operation. When the position of Project Scientist was opened in 2019 at the CTAO gGmbH, I knew I wanted to apply: after almost 15 years dedicated to ground-based gamma-ray astronomy, being able to work directly in the definition of the first ground-based IACT observatory’s science was really exciting.

    What does a Project Scientist do, and why is it important for the future of the CTAO?

    The Project Scientist is responsible for all science-related aspects of the Observatory, which involves working on different fronts. From one side, I have to ensure that all science requirements are met during the construction phase: if, for example, the engineers need to revise the design of an instrument, I work with them to guarantee that the change’s impact on the science performance of the Observatory is acceptable. From another side, I am the Observatory’s interface with the scientific community. Thus, I collect science users’ feedback and proposals, and work together with them to define the science cases and priorities for the CTAO.

    Moreover, as Project Scientist, I had to recently evaluate the scientific implications of the Observatory’s reduced configuration. The CTAO benefits from a modular configuration and, while the ultimate goal is to have more than 100 telescopes between two sites, the approved configuration to be built based on current available funds, includes 64 telescopes. The definition of such configuration, named Alpha Configuration, and the geographical position of all elements (telescopes, calibration systems and atmospheric characterization devices) was the result of a meticulous optimization process for each array’s scientific capabilities, carried out in collaboration with the CTAC members.

    What are you working on now?

    Now that the scope of the CTAO construction project (its Alpha Configuration) has been defined, I am advancing in the definition of the Scientific Operations Concept, and this is really important: at the end, we are building this Observatory to optimize the scientific outcomes and discoveries and for that, we need to have clear processes and workflows behind observation planning, data collection, reduction and dissemination, so that observations are carried out as expected and data is properly made available to the worldwide scientific community.

    In preparation also for future data, I am working on the CTAO Science Data Challenge (SDC), our first publicly available data challenge to broaden the scientific community and allow astronomers from any field to become familiar with CTAO’s scientific capabilities and data analysis. The SDC represents an important milestone for the construction project, since it allows us to verify the requirements of the software packages, test the software algorithms (observation planning and scientific analysis tools), validate the data models and formats, test the scientific portal prototype and authentication system, among many other important parameters.

    At the same time, and thinking about the involvement of scientists at different levels of their career, we are starting the preparation of the first CTAO International School and of the second edition of the CTAO Symposium. The former’s goal is to train young scientists in gamma-ray astronomy, while the latter aims to become a meeting point for the high-energy astrophysics community, as an international conference to talk about the latest news of the CTAO and impact within multi-wavelength and multi-messenger astronomy.

    Very busy, and yet exciting, time for science with the CTAO!

    See the full article here.

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.

    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.

    Stem Education Coalition

    About The Čerenkov Telescope Array (CL)(ES)
    The Čerenkov Telescope Array (CTA) (CL) is a global initiative to build the world’s largest and most sensitive high-energy gamma-ray observatory with tens of telescopes planned on two sites: one in the northern hemisphere on the island of La Palma, Spain, and the other in the southern hemisphere near Paranal, Chile.
    CTA North at the Instituto de Astrofisica de Canarias (IAC) depiction, Roque de los Muchachos Observatory in La Palma, Spain

    Proposed CTA Telescopes, Čerenkov Telescope Array depiction at ESO’s Cerro Paranal Observatory. This image illustrates all three classes of the 99 telescopes planned for CTA South at ESO’s Paranal Observatory, Chile, as viewed from the centre of the array. This rendering is not an accurate representation of the final array layout, but it illustrates the enormous scale of the CTA telescopes and the array itself.

    The Čerenkov Telescope Array (CL)(ES) will be the foremost global observatory for very high-energy gamma-ray astronomy over the next decade and beyond and will be the first ground-based gamma-ray astronomy observatory open to the world-wide astronomical and particle physics communities. CTA will address some of the greatest mysteries in astrophysics, detecting gamma rays with an unprecedented sensitivity and expanding the cosmic source catalogue tenfold. CTA is a unique, ambitious large-scale infrastructure that will expand observations up to a region of the spectrum that has never been seen, opening an entirely new window to our Universe. The CTAO gGmbH serves to prepare the design and implementation of the CTA Observatory. The CTAO works in close cooperation with the CTA Consortium composed of 1500+ members from 31 countries, which is responsible for directing the science goals of the Observatory and is involved in the design and supply of instrumentation. The CTAO is governed by a council of shareholders from 11 countries and one intergovernmental organization, as well as associate members from two countries.

     
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