From ALMA: “Surprising Chemistry Found in Molecular Rings around Young Star”

ALMA Array

23 September 2015
Valeria Foncea

Education and Public Outreach Officer

Joint ALMA Observatory

Santiago, Chile

Tel: +56 2 467 6258

Cell: +56 9 75871963

Charles E. Blue
Public Information Officer
National Radio Astronomy Observatory
Charlottesville, Virginia, USA
Tel: +1 434 296 0314
Cell: +1 434.242.9559

Richard Hook
Public Information Officer, ESO

Garching bei München, Germany

Tel: +49 89 3200 6655

Cell: +49 151 1537 3591

Masaaki Hiramatsu

Education and Public Outreach Officer, NAOJ Chile
Tokyo, Japan

Tel: +81 422 34 3630


Temp 1
ALMA image of dual rings of DCO+ encircling the star IM Lup. The rings reveal details about the conditions of this young protoplanetary disk. The existence of the outer disk was surprising, providing new insights into the formation of heavy molecules — those based on deuterium — in this and other similar systems. Credit K. Oberg, CfA; ALMA (NRAO/ESO/NAOJ); B. Saxton (NRAO/AUI/NSF)

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have discovered two spectacular rings of molecules encircling the young, Sun-like star IM Lup. The rings are made up of one of the most common heavy ions (charged molecules) in space, DCO+ (deuterium, carbon, oxygen). In this molecule (DCO+), deuterium has replaced the normal hydrogen atom of HCO+ in a process known as hydrogen-deuterium exchange.

This chemistry reveals new insights into the conditions of the planet-forming disk surrounding this young star. “With ALMA we can directly observe this chemistry in disks that are right now in the process of making planets,” said Karin Öberg, an astronomer at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., and lead author on a paper published in the Astrophysical Journal. “The molecules have formed two spectacular rings. The inner one we expect to see; the outer one comes as a complete surprise and sheds new light into the properties of a protoplanetary disk’s outer reaches.”

The presence of a DCO+ ring nearest to the star, the astronomers note, comes from the right combination of low temperatures and abundant carbon monoxide (CO) gas, which is essential for the formation of DCO+. Closer to the star, conditions are too warm for DCO+ to form. Further out, the entire reservoir of CO freezes out, forming a layer of ice on dust grains and planetesimals.

The presence of the outer ring implies that farther and farther from the star it not only gets colder and darker, as would be expected, but it also hits a point where the disk density is so low that some light from the host star can penetrate down to the midplane of the disk. This replenishes the reservoir of CO gas and restarts the production of DCO+. Heavy, deuterium-based molecules can thus form in more places around young stars than previously thought.

This increases the utility of these molecules to tell us about the history of both our Solar System and other planetary systems in the making. “Heavy molecules are, in fact, interstellar messengers that tell us how and where different types of molecules form,” noted Öberg. “For example, based on an excess of heavy water in the Earth’s ocean we know that most of the Earth’s water comes from the pre-Solar nebula, so it’s actually older than the Sun!”

Reference: Double DCO+ rings reveal CO ice desorption in the outer disk around IM Lup, K. Öberg et al., 2015 September 4, Astrophysical Journal.

See the full article here .

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

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile. ALMA is funded in Europe by the European Organization for Astronomical Research in the Southern Hemisphere (ESO), in North America by the U.S. National Science Foundation (NSF) in cooperation with the National Research Council of Canada (NRC) and the National Science Council of Taiwan (NSC) and in East Asia by the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Academia Sinica (AS) in Taiwan.

ALMA construction and operations are led on behalf of Europe by ESO, on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI) and on behalf of East Asia by the National Astronomical Observatory of Japan (NAOJ). The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.

NRAO Small

ESO 50