Did you know that chemical building blocks for life on Earth might have come from the centre of the Milky Way?
German researchers used 20 x 12 metre dishes at the ALMA radio telescope in Chile to detect radiowaves emitted from Sagittarius B2, a huge star-forming cloud near the centre of our galaxy.
Among the spectra were signature radiowaves for iso-propyl cyanide.
This is the first branched carbon molecule discovered in interstellar space that is similar to organic molecules associated with life on Earth (e.g. amino acids).
Therefore, it is possible that life-giving organic compounds might have been produced in huge gas clouds like Sagittarius B2, then hitched a ride on meteorites/comets to seed life on Earth.
If it happened here, this makes it more likely it also happened elsewhere in the galaxy.
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Background
All life on Earth is based on organic compounds containing carbon (e.g. amino acids, DNA, fats, sugars, ATP, etc).
Carbon was chosen by nature because it is abundant (4th in the universe, 15th on Earth, 2nd in humans) and forms up to four bonds per atom with itself (forming chains) and other elements (forming compounds). This flexibility and stability means it can produce an almost infinite number of molecules/compounds.
So where did they come from? And could they have given rise to life elsewhere in the universe?
Several carbon-based organic compounds have previously been detected in space, but they have all been straight-chained carbon molecules.
Carbon compounds associated with life on Earth are usually branched.
Materials and Methods
German researchers used 20 x 12 metre dishes at the Atacama Large Millimetre Array (ALMA) radiotelescope in Chile to detect radiowaves emitted from Sagittarius B2, a huge star-forming cloud near the centre of the Milky Way galaxy. The spectra detected were compared to spectra from control samples on Earth or computer-predicted spectra.
Results
Among the spectra of many molecules from Sagittarius B2 were radiowaves for iso-propyl cyanide.
This is the first branched carbon molecule discovered in interstellar space that is similar to organic molecules associated with life on Earth.
The iso-propyl cyanide forms in or on dust-grain ices at around 55-75 Kelvin (-218° to -198°C), according to their models.
Discussion
Branched organic compounds have also been discovered in meteorites.
Therefore, it is possible that life-giving organic compounds might have been produced in huge gas clouds like Sagittarius B2, then hitched a ride on meteorites to seed life on Earth.
If it happened here, this makes it more likely it also happened elsewhere in the galaxy.
More sensitive telescopes may one day be able to measure amino acids in interstellar space. If so, this further increases the chance that life originated in space (at least the building blocks).
Article
Detection of a branched alkyl molecule in the interstellar medium: iso-propyl cyanide
Belloche et al., 2014 Science 345:1584-7
Keywords
Organic, compound, molecule, carbon, life, star, Earth, galaxy, universe, interstellar, meteorite, branched, amino acid, radiowave, radiotelescope, radio, telescope
Subject
Science, Earth and Space, ST2-9ES, ACSSU048, ST3-8ES, ACSSU078, SC4-12ES, ACSSU115, SC4-14LW, ACSSU111, ACSSU149, SC5-12ES, ACSSU188, SC5-15LW, ACSSU185, SC5-17CW, ACSSU178, ACSSU179