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The Icebreaker Life Mission to Mars: A Search for Biomolecular Evidence for LifeThe search for evidence of life on Mars is the primary motivation for the exploration of that planet. The results from previous missions, and the Phoenix mission in particular, indicate that the ice-cemented ground in the north polar plains is likely to be the most recently habitable place that is currently known on Mars. The near-surface ice likely provided adequate water activity during periods of high obliquity, ~ 5 Myr ago. Carbon dioxide and nitrogen is present in the atmosphere, and nitrates may be present in the soil. Perchlorate in the soil together with iron in basaltic rock provides a possible energy source for life. Furthermore, the presence of organics must once again be considered, as the results of the Viking GCMS are now suspect given the discovery of the thermally reactive perchlorate. Ground-ice may provide a way to preserve organic molecules for extended periods of time, especially organic biomarkers. The Mars Icebreaker Life mission focuses on the following science goals: 1. Search for specific biomolecules that would be conclusive evidence of life. 2. A general search for organic molecules in the ground ice. 3. Determine the processes of ground ice formation and the role of liquid water. 4. Understand the mechanical properties of the Mars polar ice-cemented soil. 5. Assess the recent habitability of the environment with respect to required elements to support life, energy sources, and possible toxic elements. And 6. Compare the elemental composition of the northern plains with mid-latitude sites. The Icebreaker Life payload has been designed around the Phoenix spacecraft and is targeted to a site near the Phoenix landing site. However, the Icebreaker payload could be supported on other Mars landing systems. Preliminary studies of the SpaceX Dragon lander show that it could support the Icebreaker payload for a landing either at the Phoenix site or at mid-latitudes. Duplicate samples could be cached as a target for possible return by a Mars Sample Return mission. If the samples were shown to contain organic biomarkers interest in returning them to Earth would be high.
Document ID
20140011650
Acquisition Source
Ames Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Mckay, Christopher P.
(NASA Ames Research Center Moffett Field, CA United States)
Stoker, Carol R.
(NASA Ames Research Center Moffett Field, CA United States)
Glass, Brian J.
(NASA Ames Research Center Moffett Field, CA United States)
Dave, Arwen I.
(Lockheed Martin Corp. Moffett Field, CA, United States)
Davila, Alfonso F.
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Heldmann, Jennifer L.
(NASA Ames Research Center Moffett Field, CA, United States)
Marinova, Margarita M.
(Bay Area Environmental Research Inst. Moffett Field, CA, United States)
Fairen, Alberto G
(California Inst. of Tech. Pasadena, CA, United States)
Quinn, Richard C
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Zacny, Kris A.
(Honeybee Robotics Pasadena, CA, United States)
Paulsen, Gale
(Honeybee Robotics Pasadena, CA, United States)
Smith, Peter H.
(Arizona Univ. Tucson, AZ, United States)
Parro, Victor
(Instituto Nacional de Tecnica Aeroespacial Madrid, Spain)
Andersen, Dale T.
(Search for Extraterrestrial Intelligence Inst. Mountain View, CA, United States)
Hecht, Michael H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lacelle, Denis
(Ottawa Univ. Ontario, Canada)
Pollard, Wayne H.
(McGill Univ. Montreal, Quebec, Canada)
Date Acquired
September 12, 2014
Publication Date
October 26, 2012
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN9251
Funding Number(s)
WBS: WBS 857464
CONTRACT_GRANT: NAS7-03001
CONTRACT_GRANT: NNX10AT88A
CONTRACT_GRANT: NNX11AJ32A
CONTRACT_GRANT: NNM10AA11C
CONTRACT_GRANT: NAS2-02090
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Life detection
In situ measurement
Mars
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