NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Rapid Radiolytic Degradation of Amino Acids in the Martian Shallow Subsurface: Implications for the Search for Extinct LifeAmino acids are fundamental to life as we know them as the monomers of proteins and enzymes. They are also readily synthesized under a variety of plausible prebiotic conditions and are common in carbon-rich meteorites. Thus, they represent a reasonable class of organics to target in the search for prebiotic chemistry or chemical evidence of life on Mars. However, regardless of their origin, amino acids and other organic molecules present in near-surface regolith and rocks on Mars can be degraded by exposure to cosmic rays that can penetrate to a depth of a few meters. We exposed several pure amino acids in dry and hydrated silicate mixtures and in mixtures of silicates with perchlorate salts to gamma radiation at various temperatures and radiation doses representative of the martian near-subsurface. We found that irradiation of amino acids mixed with dry silica powder increased the rate of amino acid radiolysis, with the radiolysis constants of amino acids in silicate mixtures at least a factor of 10 larger compared with the radiolysis constants of amino acids alone. The addition of perchlorate salts to the silicate samples or hydration of silicate samples further accelerated the rate of amino acid destruction during irradiation and increased the radiolysis constants by a factor of *1.5. Our results suggest that even low-molecular-weight amino acids could degrade in just *20 million years in the top 10 cm of the martian surface regolith and rock, and even faster if the material contains elevated abundances of
hydrated silicate minerals or perchlorates. We did not detect evidence of amino acid racemization after gamma radiation exposure of the samples, which indicates that the chirality of some surviving amino acids may still be preserved. Our experimental results suggest serious challenges for the search of ancient amino acids and other potential organic biosignatures in the top 2 m of the martian surface.
Document ID
20220014699
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Alexander A. Pavlov ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Hannah L. McLain
(Catholic University of America Washington D.C., District of Columbia, United States)
Daniel P. Glavin
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Anais Roussel
(Georgetown University Washington D.C., District of Columbia, United States)
Jason P. Dworkin ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Jamie E. Elsila ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Katarina M. Yocum
(University of Wisconsin–Madison Madison, Wisconsin, United States)
Date Acquired
September 28, 2022
Publication Date
September 22, 2022
Publication Information
Publication: Astrobiology
Publisher: Mary Ann Liebert
Volume: 22
Issue: 9
Issue Publication Date: September 1, 2022
ISSN: 1531-1074
e-ISSN: 1557-8070
Subject Category
Life Sciences (General)
Lunar And Planetary Science And Exploration
Funding Number(s)
WBS: 811073.02.52.01.04.06
CONTRACT_GRANT: 80GSFC21M0002
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
NASA Peer Committee
No Preview Available