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  • richardmitnick 1:49 pm on February 7, 2020 Permalink | Reply
    Tags: "These dwarf planets are just as strange as Pluto", 2007 OR10, , , , , , Makemake, Orcus, Quaoar, Sedna,   

    From Astronomy Magazine: “These dwarf planets are just as strange as Pluto” 

    From Astronomy Magazine

    February 3, 2020
    Eric Betz

    A new generation of ground-based telescopes and proposed space missions could soon reveal their secrets.

    The dwarf planet Pluto, imaged by NASA’s New Horizons mission. NASA/Johns Hopkins University Applied Physics
    Laboratory/Southwest Research Institute

    NASA/New Horizons spacecraft

    Deep in the outer solar system, billions of miles from Earth, lurks a realm of small, icy worlds called dwarf planets. Astronomers know relatively little about these dim and distant objects, but in recent years, new evidence has revealed that the tiny planets can hold a surprising range of features, from oceans and mountains to canyons, dunes and volcanoes.

    Much of what astronomers know about dwarf planets comes from the NASA New Horizons spacecraft’s 2015 Pluto flyby. Pluto thrilled scientists with its towering mountain ranges made of ice. Its surprising geological complexity leaves astronomers eager to see the diversity of similar worlds in the Kuiper Belt — a donut-shaped region beyond Neptune packed with icy space rocks both large and small.

    Kuiper Belt. Minor Planet Center

    So far, the International Astronomical Union, the astronomy world’s official record keeper, recognizes just five dwarf planets: Ceres, Eris, Haumea, Makemake, and Pluto. But astronomers keep finding new dwarf planet candidates every year.

    What is a dwarf planet? According to the IAU, a dwarf planet is a world orbiting the Sun that’s big enough for its gravity to make round, but may “orbit in a zone that has many other objects in it.”

    Here’s a rundown of some of the most potentially exciting and unexplored dwarf planets.

    2007 OR10

    Like other icy planetesimals in the Kuiper Belt, 2007 OR10 takes a wild ride around our solar system. A year on this dwarf planet candidate lasts 550 Earth years and takes it almost as close to the Sun as Neptune before plunging more than twice as far out as Pluto.

    Scientists still aren’t sure about its diameter, but estimates put it at about two-thirds of Pluto’s. That leaves 2007 OR10 as the largest unnamed world in the solar system. (An online vote last year hosted by Brown and his team of co-discoverers suggested the name Gonggong, after a Chinese water god known for sowing chaos.)
    Standing on its surface, the icy ground would look dark and red, like Pluto. Indeed, 2007 OR10 is one of the reddest worlds astronomers know of. That reddish hue hints at the presence of complex organic compounds astronomers call tholins. Carl Sagan first discovered tholins, which form when ultraviolet light hits carbon-rich molecules like methane, in the lab during an experiment aimed at replicating the conditions of early Earth. The tarry substance is found on Pluto and likely exists on worlds throughout the Kuiper Belt.

    Research published in 2011 also showed that 2007 OR10 has a fresh surface covered in water ice. Astronomers think it’s evidence of cryovolcanoes, where slushy ice erupts from below the surface like lava.

    An artist’s impression of 2007 OR10. Its reddish hue may come from compounds known as tholins. NASA


    This frigid world, named for a Rapa Nui god, is among the largest objects known in the Kuiper Belt. Surface temperatures on Makemake (pronounced MAH-keh MAH-keh) match up well with Pluto’s, reaching as low as negative 230 degrees Celsius. A year on Makemake lasts about 300 Earth years.

    What little is known about Makemake’s surface suggests the world is covered in bright ices that are extremely cold, while its moon, MK2, is as black as charcoal. Some research has suggested the potential dwarf planet is also littered with pellets of methane as much as half an inch across.

    This illustration shows Makemake’s bright red surface and the inferred darker surface of the moon, known as MK2.
    NASA/SwRI/Alex Parker


    Today, Triton isn’t a dwarf planet and it isn’t in the Kuiper Belt. Instead, it’s a large, icy moon of the planet Neptune with some seriously peculiar properties. Its orbit carries in the opposition direction of other large moons in the solar system, called retrograde motion, and it has a geologically active surface with strong signs of ice volcanoes.

    Triton’s similarities to Pluto, as well as its orbit, lead astronomers to suspect that the moon initially formed as a dwarf planet in the Kuiper Belt and was later captured by Neptune. But whereas Pluto is thought to have an ancient ocean that froze over time, astronomers think Triton may still have a liquid water ocean beneath its surface thanks to Neptune’s intense gravity.

    If true, that would make Triton one of the most habitable known worlds. And whereas NASA likely won’t have a mission to Pluto’s other far-flung cousins in the outer solar system in the near future, scientists are already seriously considering a mission dedicated to visiting Neptune. “We would learn a lot about dwarf planets with a mission to Neptune,” Stern says.

    A mosaic photo of Neptune’s moon Triton taken by the Voyager 2 spacecraft.

    NASA/Voyager 2



    Sedna is one of the reddest objects in the solar system — likely a sign of tholins — and it has one of the strangest orbits known. The potential dwarf planet takes roughly 11,400 years to circle the Sun, meaning just about one year has passed there since the dawn of agriculture on Earth.

    Sedna’s orbit leads some to rank it as the most important find in the region beyond Neptune. That’s because it’s unlikely that the world formed where it is now. One possibility is that a passing star may have knocked Sedna out of the Oort Cloud — a circumstellar cloud of icy space rocks orbiting far from the Sun — and onto its current orbit. It’s hard to guess at what its surface looks like because astronomers have never seen a large object from that region up close.

    “I call Sedna a fossil record of the earliest solar system,” Mike Brown, the Caltech astronomer who co-discovered Sedna, said in a Discover Magazine interview back in 2006. “Eventually, when other fossil records are found, Sedna will help tell us how the Sun formed and the number of stars that were close to the Sun when it formed.”

    An artist’s conception of Sedna, one of the reddest objects known in our solar system. NASA/JPL-Caltech/R. Hurt


    It’s now been roughly two decades since Quaoar was discovered. And while this dwarf planet spans just half the diameter of Pluto, that doesn’t necessarily make it a less interesting world. Right now, Quaoar is orbiting at about 42 astronomical units, where 1 AU equals the Earth-Sun distance.

    Quaoar is roughly the same size as Pluto’s large moon Charon, where the New Horizons mission recently revealed a stunning diversity of landscapes, from mountains to canyons, valleys, craters and plains. Charon is also covered in water ice and features a giant tectonic belt of canyons that stretch four times longer than the Grand Canyon and twice as deep. Astronomers suspect this gash, called Argo Chasma, formed when an ocean froze inside Charon and cracked the dwarf planet open like a soda can left in the freezer too long.

    In the years since Quaoar’s discovery, astronomers have detected water ice there. And some scientists suggest it may have cryovolcanoes. Its relatively bright surface also hints that the world may have been geologically active in the not-too-distant past.

    An artist’s illustration of Quaoar (pronounced “kwa-whar”). NASA and G. Bacon (STScI)


    Some have called Orcus the “anti-Pluto” because of their many similarities but opposing orbits. Right now, Orcus is at its farthest point from the Sun, while Pluto is near the closest point of its orbit. Both worlds eventually pass even closer to the Sun than Neptune. And on Pluto, these close passes create a thin but temporary atmosphere.

    Like Pluto and Eris, Orcus also boasts a large moon, named Vanth, which may be the third largest moon orbiting beyond Neptune. Vanth’s orbit clings to Orcus at an uncomfortably close 5,600 miles (9,000 km) — the dwarf planet itself is just some 600 miles (965 km) in diameter.

    If Earth’s own Moon orbited at a similar distance relative to size, it would sit several times closer than it does now.

    And these two objects seem to have very different surfaces. Whereas Vanth has a reddish hue common to Kuiper Belt objects, Orcus has a much lighter surface with signs of water ice. Is this system a slightly smaller version of the Pluto-Charon system? Or are these worlds something else entirely? Only a higher-resolution view will reveal the truth.

    Orcus can be seen in the green circle at top right. California Institute of Technology

    See the full article here .


    Please help promote STEM in your local schools.

    Stem Education Coalition

    Astronomy is a magazine about the science and hobby of astronomy. Based near Milwaukee in Waukesha, Wisconsin, it is produced by Kalmbach Publishing. Astronomy’s readers include those interested in astronomy and those who want to know about sky events, observing techniques, astrophotography, and amateur astronomy in general.

    Astronomy was founded in 1973 by Stephen A. Walther, a graduate of the University of Wisconsin–Stevens Point and amateur astronomer. The first issue, August 1973, consisted of 48 pages with five feature articles and information about what to see in the sky that month. Issues contained astrophotos and illustrations created by astronomical artists. Walther had worked part time as a planetarium lecturer at the University of Wisconsin–Milwaukee and developed an interest in photographing constellations at an early age. Although even in childhood he was interested to obsession in Astronomy, he did so poorly in mathematics that his mother despaired that he would ever be able to earn a living. However he graduated in Journalism from the University of Wisconsin Stevens Point, and as a senior class project he created a business plan for a magazine for amateur astronomers. With the help of his brother David, he was able to bring the magazine to fruition. He died in 1977.

  • richardmitnick 11:28 am on July 23, 2018 Permalink | Reply
    Tags: , , , , Did a Stellar Intruder Deform Our Outer Solar System?, , , Sedna   

    From Scientific American: “Did a Stellar Intruder Deform Our Outer Solar System?” 

    Scientific American

    From Scientific American

    July 23, 2018
    Shannon Hall

    New results suggest a massive star once swung dangerously close to our sun—helping to shape the mysterious features we see today.

    The odd orbit of the dwarf planet Sedna (shown here in an artist’s conceptualization) and other outer solar system objects suggests a visiting star may have swerved too close to the sun long ago. Credit: NASA and JPL-Caltech

    There is a mystery brewing in the far reaches of our solar system.

    Astronomers have long thought the eight planets orbit in nearly perfect circles because they once formed within the swirling disk of dust and gas that surrounded the young sun. But in 2003 scientists discovered something strange: a dwarf planet known as Sedna whose elongated orbit takes it from twice Pluto’s distance to more than 20 times its distance from the sun. And it is not alone. In the years since astronomers have uncovered nearly two dozen distant icy objects whose orbits are oblong and strangely tilted compared to the plane of the solar system. To explain such oddities, scientists speculated that maybe these worlds are scars from a violent past, a sign something—perhaps a passing star—knocked them off course in our solar system’s infancy. Or maybe there is a distant ninth planet whose gravity sculpts their peculiar orbits.

    The latter hypothesis has gained traction over the past several years, leaving the first in the dust, says Susanne Pfalzner, an astronomer at the Max Planck Institute for Radio Astronomy in Germany. Anomalies in the orbits of some small outer solar system objects have amassed evidence for a “Planet Nine” roughly 10 times Earth’s mass. Meanwhile a stellar interloper has been considered too unlikely—until now. Pfalzner and her colleagues recently published a paper to the preprint server arXiv that has been accepted by The Astrophysical Journal showing stars might buzz our solar system far more often than previously thought. Not only do the results lend credibility to a stellar flyby but they just might also explain how the elusive Planet Nine would have landed in its odd orbit in the first place.

    Effect of a prograde, parabolic fly-by of a star with a) M=0.5 M, b) M2= 1, Mand c) M2= 5 Mthat is inclined by 60 degree and has a angle of periastron equal zero. The perihelion distance is always chosen in such a way as to lead to a 30-35 AU disc. The top row indicates the eccentricity distribution of the matter with a central area of most particles on circular orbits and more eccentric orbits at larger distances form the Sun. The eccentricities are indicated by the different colours given in the bar. The origin of the different eccentricity populations in the original disc can be seen in bottom row, where matter indicated in grey becomes unbound from the Sun. Note that in c) the path of the perturber is not visible because it is outside the shown frame. Credit: arXiv:1807.02960 [astro-ph.GA]

    Astronomers know the sun has not always been so solitary. It was born within a cluster of hundreds to perhaps tens of thousands of stars that dispersed only 10 million years later. So while the sun was still entombed within that cluster, stars would have rocked to and fro in a dizzying dance that easily could have brought one waltzing into our nascent solar system. But after the cluster broke apart the likelihood of such an encounter dropped nearly to zero, or so the thinking went. But Pfalzner and her colleagues now argue the odds of an encounter remained quite high after the cluster had started to disperse. After many long computer simulations they found there is a 20 to 30 percent chance a star perhaps as massive as the sun would swing nearly as close as Pluto at 50 to 150 astronomical units. (One AU is the mean distance from Earth to the sun, or 93 million miles.) And there is no doubt such a close approach would surely shake our young solar system.

    Although the large planets would remain unbothered (much like the sun is only slightly jostled by the minor gravities of the eight planets), the encounter would perturb the solar system’s smaller objects—tossing them around and placing them in odd orbits in the distant reaches of the solar system. What is more: the simulations also re-created a second trend astronomers have observed in the solar system, that outer objects tend to cluster together in space. They travel together in tight-knit groups that all cross the plane of the solar system at roughly the same spot before swinging outward to the same distant point. In short, simulations including a stellar interloper can perfectly re-create the observations to date. “But whether they’ll last for 4.5 billion years” or over the solar system’s entire life span, “is the million-dollar question,” says Scott Kenyon, an astronomer at Harvard–Smithsonian Center for Astrophysics who was not involved in the research. And Pfalzner agrees. She would like to model the long-term behavior next to see whether those changes will hold over the solar system’s entire lifetime. It could be that a flyby clusters objects for a cosmic moment before they randomize again. If that is the case, then a planet is the best explanation for the observations.

    Scientists are eagerly tracking down more data with a number of different observing campaigns. A handful of teams, for example, are already scouring large chunks of the heavens in search of more oddities in the outer solar system. Scott Sheppard, an astronomer at the Carnegie Institution for Science who was not involved in the study, cannot contain his excitement over the upcoming Large Synoptic Survey Telescope—an 8.4-meter-wide scope that will likely uncover hundreds of new solar system rocks.


    LSST Camera, built at SLAC

    LSST telescope, currently under construction on the El Peñón peak at Cerro Pachón Chile, a 2,682-meter-high mountain in Coquimbo Region, in northern Chile, alongside the existing Gemini South and Southern Astrophysical Research Telescopes.

    “That’s really going to open up the floodgates for trying to discover these distant objects,” he says.

    Meanwhile Kenyon is hopeful the Gaia spacecraft, which is in the process of charting one billion stars to unprecedented accuracy, will help find our sun’s long-lost siblings.

    ESA/GAIA satellite

    That will allow scientists to better understand the stellar cluster in which our young solar system formed, along with the likelihood another star zoomed too close. “Gaia is the new savior on the block,” he says. A recent Gaia study even traced the paths of nearby stars into the past and projected those paths into the future, only to find that 25 stars speed dangerously close to home over a 10-million-year time period. That tally is seven times as much nearby stellar traffic as previously thought. Then, of course, there are a number of surveys searching for the elusive Planet Nine itself.

    But Pfalzner argues the discovery of another major member of the solar system will not rule out a stellar flyby. “It’s not an either–or scenario,” she says. “If Planet Nine exists, this would not be in any way a contradiction to the flyby model, but possibly even a point in favor for it.” Her team argues Planet Nine’s predicted orbit, which is also both eccentric (stretched out) and inclined (tilted from the solar system’s plane), was likely shaped by the stellar interloper itself. So she and others will continue to hunt for both Planet Nine and further oddities.

    And although astronomers might disagree over the specifics of our solar system’s origin story, they are all certain the treasure trove of objects already discovered in the outer solar system is only the beginning. Sedna was the tip of the iceberg, Sheppard says. “There’s just so much sky we haven’t covered to date that it’s more likely than not there’s something pretty big out there.”

    See the full article here .


    Please help promote STEM in your local schools.

    Stem Education Coalition

    Scientific American, the oldest continuously published magazine in the U.S., has been bringing its readers unique insights about developments in science and technology for more than 160 years.

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