Freon-40 may not be a useful marker of life
Observations made with the ALMA telescope in Chile and ESA’s Rosetta mission, have detected the faint molecular fingerprint of methyl chloride in gas, a chemical commonly produced by industrial biological processes on Earth, around both an infant star and a comet. Methyl chloride, also known as Freon-40, is one of a class of molecules known as organohalogens, which are formed by organic processes on Earth. But, this is the first ever detection of them in interstellar space, dashing hopes molecule could point to life on other planets.
Life beyond Earth
Indeed, this discovery suggests that organohalogens may not be as useful markers of life as had been hoped by astrobiologists, who previously suggested searching for methyl chloride in the atmospheres of alien worlds as a possible indicator of life. However, these molecules may be significant components of the material from which planets form. This result, which appears in the journal Nature Astronomy, underscores the challenge of finding molecules that could indicate the presence of life beyond Earth.
First organohalogen in interstellar space
Using data captured by ALMA in Chile and from the ROSINA instrument on ESA’s Rosetta mission, a team of astronomers has found faint traces of methyl chloride, around both the infant star system IRAS 16293-2422, about 400 light-years away, and the famous comet 67P/Churyumov-Gerasimenko (67P/C-G), in our own Solar System. The new ALMA observation is the first detection ever of an organohalogen in interstellar space.
ESOcast: ALMA and Rosetta detect Freon-40 in space
Organohalogens consist of halogens, such as chlorine and fluorine, bonded with carbon and sometimes other elements. On Earth, these compounds are created by some biological processes, in organisms ranging from humans to fungi, as well as by industrial processes such as the production of dyes and medical drugs.
The discovery of one of these compounds, methyl chloride, in places that must predate the origin of life, can be a disappointment, as earlier research had suggested that these molecules could indicate the presence of life.
'Finding the organohalogen Freon-40 near these young, Sun-like stars was surprising,' said Edith Fayolle, a researcher with the Harvard-Smithsonian Center for Astrophysics in Cambridge, (Massachusetts, USA), and lead author of this new paper. 'We simply didn’t predict its formation and were surprised to find it in such significant concentrations. It’s clear now that these molecules form readily in stellar nurseries, providing insights into the chemical evolution of planetary systems, including our own.'
Establishing reliable markers
Exoplanet research has gone beyond the point of finding planets (more than 3000 exoplanets are now known) to looking for chemical markers that might indicate the potential presence of life. A vital step is determining which molecules could indicate life, but establishing reliable markers remains a tricky process.
'ALMA’s discovery of organohalogens in the interstellar medium also tells us something about the starting conditions for organic chemistry on planets. Such chemistry is an important step toward the origins of life,' adds Karin Öberg, a co-author on the study. 'Based on our discovery, organohalogens are likely to be a constituent of the so-called ‘primordial soup’, both on the young Earth and on nascent rocky exoplanets.'
This finding suggests that astronomers may have had things around the wrong way; rather than indicating the presence of existing life, organohalogens may be an important element in the little-understood chemistry involved in the origin of life.
The power of ALMA
Co-author Jes Jørgensen from the Niels Bohr Institute at the University of Copenhagen adds: 'This result shows the power of ALMA to detect molecules of astrobiological interest toward young stars on scales where planets may be forming. Using ALMA, we have previously found simple sugars and precursors to amino acids around different stars. The additional discovery of Freon-40 around Comet 67P/C-G strengthens the links between the pre-biological chemistry of distant protostars and our own Solar System.'
Faint radio signals
ALMA can function as an interstellar chemical analyzer by detecting the faint radio signals emitted naturally by molecules in space. Each molecule has a distinctive fingerprint, or series of spikes, in the radio spectrum. It takes incredibly sensitive instruments like ALMA to tease out the telltale of the signal of molecules like methyl chloride. The Rosetta spacecraft could detect it in the atmosphere of comet 67P/C-G using the onboard instrument known as the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA).
Highly sensitive instrument
'ROSINA was able to capture some of the molecules around the comet, separate them by mass, and count them with exquisite precision,' said Kathrin Altwegg with the University of Bern (Switzerland), and Principal Investigator of ROSINA. 'This highly sensitive instrument enabled us to detect a host of the chemicals around the comet, including the one also discovered by ALMA, far from our Solar System.'
The astronomers also compared the relative amounts of Freon-40 that contain different isotopes of carbon in the infant star system and the comet and found similar abundances. The results support the idea that a young planetary system can inherit the chemical composition of its parent star-forming cloud and opens up the possibility that organohalogens could arrive on planets in young systems during planet formation or via comet impacts.
Formation of organohalogens
'Our results show that we still have more to learn about the formation of organohalogens,' concludes Fayolle. 'This does, however, raise the question: How much of the comet’s organic content is directly inherited from the early stages of star formation? Additional searches for organohalogens around other protostars and comets need to be undertaken to help find the answer.'