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The Search for Extant Life on Mars: A Human Exploration ObjectiveA search for evidence of extant life on Mars should be conducted prior to and as part of human exploration missions. Potentially habitable environments for modern life occur on Mars. Despite a vigorous campaign of exploration of the surface over the last 3 decades, no mission has attempted to search for signatures of extant life since the Viking landers in 1976. Finding an example of extant life beyond Earth would be one of the greatest scientific discoveries of all
time. This is especially important because (once discovered) the biochemistry and metabolism of the life form can be studied. Earth and Mars exchange materials over geologic time because impacts eject rock and crustal materials into space that are eventually deposited on other planets and moons [1]. Therefore, Earth and Mars could share life with a common origin and similar biochemistry; if this is the case, life on Mars likely experienced billions of years of evolution in isolation from Earth. Alternatively, Mars may host a distinct genesis of life which could be evident from its different biochemistry. Either discovery would change our understanding of life in the solar system and beyond.

The Mars 2020/Perseverance sample collection mission is not optimized for finding extant life because the site for sample collection, Jezero Crater, was chosen for its ancient habitability and likelihood to host fossil evidence of life. Furthermore, the samples collected will not be returned for at least a decade. Within that period, technology development for human exploration will likely be underway and it is possible that humans will land on Mars without an updated knowledge of extant life on Mars, which may pose a risk both to those mission crews and to Earth when they return. Thus, it is important to perform a search for extant life on Mars prior to humans landing at a site where life may persist. Salts and shallow ground ice are particularly important environments to evaluate for extant life prior to human missions because they may be encountered and
interacted with by human crews.
Document ID
20220005419
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
C.R. Stoker
(Ames Research Center Mountain View, California, United States)
J.L. Heldmann
(Ames Research Center Mountain View, California, United States)
C. P. McKay
(Ames Research Center Mountain View, California, United States)
Alfonso F Davila
(Ames Research Center Mountain View, California, United States)
Date Acquired
April 6, 2022
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: Science Objective for Human Exploration
Location: Denver, CO
Country: US
Start Date: May 4, 2022
End Date: May 6, 2022
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 811073.02.52.01.48
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Technical Review
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