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Detailed Study of the Formation of Sugar Derivatives Produced from the UV Irradiation of Astrophysical Ice AnalogsCarbonaceous meteorites such as Murchison contain a large variety of organic compounds of astrobiological interest such as amino acids, other amphiphilic compounds, functionalized nitrogen heterocycles (including nucleobases), functionalized polycylic aromatic hydro-carbons (including quinones), and sugar derivatives. The presence of such a broad variety of organics in meteorites strongly suggests that molecules essential to life can form abiotically under astrophysical conditions. This hypothesis is strongly supported by laboratory studies in which astrophysical ice analogs (i.e., mixtures of H2O, CO, CO2, CH3OH, CH4, NH3, etc.) are subjected to ultraviolet (UV) irradiation at low temperature (less than 15 K) to simulate cold interstellar environments. These studies have shown that the organic residues recovered at room temperature after irradiation contain organic compounds that are very similar to those found in meteorites. No systematic search for the presence of sugar derivatives in laboratory residues had been carried out until the recent detection of ribose, the sugar of RNA, as well as other sugars, sugar alcohols, and sugar acids in one residue produced from the UV irradiation of an ice mixture containing H2O, CH3OH, and NH3 at 80 K. In this work, we present a detailed study of the formation of sugar derivatives contained in organic residues that are produced from the UV irradiation of ice mixtures of different starting compositions (H2O, CH3OH, CO, CO2, and/or NH3) at less than 15 K. While the presence of sugar alcohols, sugars, and sugar acids-in some cases with up to 6 carbon atoms-could be confirmed in all these residues, their distribution was shown to vary with the composition of the starting ices. In particular, only a few ices result in the formation of sugar derivatives displaying a distribution that resembles that of meteorites, in which sugar alcohols and sugar acids are very abundant while sugars are mostly absent.
Document ID
20180002065
Acquisition Source
Ames Research Center
Document Type
Abstract
Authors
Nuevo, Michel
(Bay Area Environmental Research Inst. Petaluma, CA, United States)
Cooper, George
(NASA Ames Research Center Moffett Field, CA, United States)
Saunders, John
(California Univ. Santa Cruz, CA, United States)
Buffo, Christina E.
(Wellesley Coll. MA, United States)
Materese, Christopher K.
(Bay Area Environmental Research Inst. Petaluma, CA, United States)
Sandford, Scott A.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
March 23, 2018
Publication Date
March 18, 2018
Subject Category
Inorganic, Organic And Physical Chemistry
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN49108
Meeting Information
Meeting: ACS National Meeting & Exposition
Location: New Orleans, LA
Country: United States
Start Date: March 18, 2018
End Date: March 22, 2018
Sponsors: American Chemical Society
Funding Number(s)
CONTRACT_GRANT: NNX16AO96A
WBS: WBS 811073.02.12.03.93
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Keywords
Photochemistry
Sugars
Ices
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