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martedì 8 agosto 2017

# s-esobio: self-assembled azotosomes by convective activity, a kind of proto-life on Titan.

<< vinyl cyanide (C2H3CN; also known as acrylonitrile or propenenitrile) would be the best candidate species for the formation of (..) cell-like membranes, known as “azotosomes” >>

AA << report the first spectroscopic detection of vinyl cyanide in Titan’s atmosphere, obtained using archival data from the Atacama Large Millimeter/submillimeter Array (ALMA), collected from February to May 2014 >>

AA << detect the three strongest rotational lines of C2H3CN in the frequency range of 230 to 232 GHz, each with >4σ confidence >>

the << production rate of vinyl cyanide and its saturation mole fraction imply the availability of sufficient dissolved material to form ~107 cell membranes/cm3 in Titan’s sea Ligeia Mare (Titan's second largest liquid body) >>

<< Reactions of hydrocarbons with hydrogen, both readily available on Titan, release energy, which could provide support for methanogenic life. The sedimentation time of atmospheric organics depends on the particle size and convective activity in the troposphere. This coupling of Titan’s atmosphere and surface completes the picture regarding the astrobiological importance of (..) detection of vinyl cyanide in Titan’s middle/upper atmosphere >>

Maureen Y. Palmer, Martin A. Cordiner, et al. ALMA detection and astrobiological potential of vinyl cyanide on Titan. Science Advances  28 Jul 2017: Vol. 3, no. 7, e1700022
doi: 10.1126/sciadv.1700022

http://advances.sciencemag.org/content/3/7/e1700022.full

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