Complex organic molecules detected in interstellar space

Join Our Community of Science Lovers!

This article was published in Scientific American’s former blog network and reflects the views of the author, not necessarily those of Scientific American



On supporting science journalism

If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today.


Two of the most complex molecules ever found outside the solar system have been turned up by astronomers peering into Sagittarius B2 (Sgr B2), a massive, vigorous star-forming region near the heart of the Milky Way.

Arnaud Belloche, an astronomer at the Max Planck Institute for Radio Astronomy in Bonn, Germany, and his colleagues detected the spectral signature of ethyl formate (far left in image) and n-propyl cyanide (at right in image) in electromagnetic radiation from Sgr B2. Both are relatively large organic (carbon-based) molecules—ethyl formate (C2H5OCHO) has 11 atoms and n-propyl cyanide (n-C3H7CN) has 12. Only cyanodecapentayne (HC11N), discovered in 1997, boasts more atoms among known interstellar molecules with 13.

Belloche and his co-authors suspect that the organics formed piecemeal on dust grains in the interstellar medium from pre-made building blocks. The mechanism could produce even more complex molecules, such as the amino acids that form proteins on Earth, but the signatures of such organics have yet to be found.

The researchers used the IRAM 30-meter telescope on Pico Veleta in southern Spain, near the city of Granada, which detects emissions in the millimeter regime—short-wavelength radio waves. Their results were presented this week at the European Week of Astronomy and Space Science at the University of Hertfordshire in England and are in press at the journal Astronomy & Astrophysics.

Sgr B2 has been a gold mine of organic compounds—the authors report that most complex molecules so far turned up in interstellar space were first discovered in a hot, dense cloud in the region called the "Large Molecule Heimat," which is where the new research revealed ethyl formate and n-propyl cyanide.

In an interview with the Guardian, Belloche noted that ethyl formate is present in raspberries. The chemical "does happen to give raspberries their flavour," Belloche told the newspaper, "but there are many other molecules that are needed to make space raspberries." At the very least, perhaps ethyl formate makes space smell nice—according to the Occupational Safety and Health Administration, the chemical has "a pleasant, fruity odor."

Molecules (hydrogen: white; carbon: gray; oxygen: red; nitrogen: blue): Oliver Baum, University of Cologne 

It’s Time to Stand Up for Science

If you enjoyed this article, I’d like to ask for your support. Scientific American has served as an advocate for science and industry for 180 years, and right now may be the most critical moment in that two-century history.

I’ve been a Scientific American subscriber since I was 12 years old, and it helped shape the way I look at the world. SciAm always educates and delights me, and inspires a sense of awe for our vast, beautiful universe. I hope it does that for you, too.

If you subscribe to Scientific American, you help ensure that our coverage is centered on meaningful research and discovery; that we have the resources to report on the decisions that threaten labs across the U.S.; and that we support both budding and working scientists at a time when the value of science itself too often goes unrecognized.

In return, you get essential news, captivating podcasts, brilliant infographics, can't-miss newsletters, must-watch videos, challenging games, and the science world's best writing and reporting. You can even gift someone a subscription.

There has never been a more important time for us to stand up and show why science matters. I hope you’ll support us in that mission.

Thank you,

David M. Ewalt, Editor in Chief, Scientific American

Subscribe