For the first time, astronomers have detected the presence of complex organic molecules, the building blocks of life, in a protoplanetary disk surrounding a young star.
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This is suggesting once again that the conditions that spawned our Earth and Sun are not unique in the universe.
This discovery, made with the Atacama Large Millimeter/submillimeter Array (ALMA), reveals that the protoplanetary disk surrounding the million-year-old star MWC 480 is brimming with methyl cyanide (CH3CN), a complex carbon-based molecule.
Both this molecule and its simpler cousin hydrogen cyanide (HCN) were found in the cold outer reaches of the star's newly formed disk, in a region that astronomers believe is analogous to our own Kuiper Belt—the realm of icy planetesimals and comets beyond Neptune.
Scientists understand that comets retain a pristine record of the early chemistry of our solar system from the period of planet formation. As the planets evolved, it's believed that comets and asteroids from the outer solar system seeded the young Earth with water and organic molecules, helping set the stage for life to eventually emerge.
"Studies of comets and asteroids show that the solar nebula that spawned our Sun and planets was rich in water and complex organic compounds," noted Karin Öberg, an astronomer with the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., and lead author on a paper published in the journal Nature.
"We now have evidence that this same chemistry exists elsewhere in the universe, in regions that could form solar systems not unlike our own." This is particularly intriguing, Öberg notes, since the molecules found in MWC 480 are also found in similar concentrations in our own solar system's comets.
The star MWC 480, which is about twice the mass of the Sun, is located approximately 455 light-years away in the Taurus star-forming region. Its surrounding disk is in the very early stages of development - having recently coalesced out of a cold, dark nebula of dust and gas.
Studies with ALMA and other telescopes have yet to detect any obvious signs of planet formation in it, though higher resolution observations may reveal structures similar to HL Tau, which is of a similar age.
Astronomers have known that cold, dark interstellar clouds are very efficient factories of complex organic molecules—including a group of molecules known as cyanides. Cyanides, and most especially methyl cyanide, are important because they contain carbon-nitrogen bonds, which are essential for the formation of amino acids, the foundation of proteins.
It has been unclear, however, if these same complex organic molecules commonly form and survive in the energetic environment of a newly forming solar system, where shocks and radiation can easily break chemical bonds.
With ALMA's remarkable sensitivity, the astronomers now know that these molecules not only survive, but thrive.
Importantly, the molecules ALMA detected are much more abundant than would be found in interstellar clouds. According to the researchers, there's enough methyl cyanide around MWC 480 to fill all of Earth's oceans. This tells astronomers that protoplanetary disks are very efficient at forming complex organic molecules and that they are able to form them on a relatively fast timescale. ■