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Enceladus: BiosignaturesSaturn's moon Enceladus is a new world for Astrobiology. Through the study of Enceladus' plumes new insights into its habitability will be gained. The four core parameters for life include: water, carbon, nitrogen, and energy; all were found in the plume. Carbon and nitrogen in the plume exist in forms easily usable by biological systems (CH4, HCN, NH3, H2, CO2, and organics up to C6). The first step to search for evidence of life is to define potential biosignatures for Enceladus.
Document ID
20140017289
Acquisition Source
Ames Research Center
Document Type
Abstract
Authors
Mancinelli, Rocco L.
(Bay Area Environmental Research Inst. Moffett Field, CA, United States)
Mckay, Chris P.
(NASA Ames Research Center Moffett Field, CA United States)
Davilla, Alfonso
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Date Acquired
December 11, 2014
Publication Date
October 13, 2014
Subject Category
Space Sciences (General)
Exobiology
Report/Patent Number
ARC-E-DAA-TN17216
Report Number: ARC-E-DAA-TN17216
Meeting Information
Meeting: European Astrobiology Conference (EANA)
Location: Edinburgh, Scotland
Country: United Kingdom
Start Date: October 13, 2014
End Date: October 16, 2014
Sponsors: Edinburgh Univ.
Funding Number(s)
CONTRACT_GRANT: NNX12AD05A
WBS: WBS 736466.01.09.01.32
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Amino Acids
Enceladus
Biosignatures
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