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Describing and Measuring the Chemical Signatures of LifeHere we discuss an approach to remotely detecting extraterrestrial life forms on other planets or their moons by detection of specific types of organic molecules. The life entities to be detected would be presently active life forms, or those that are only recently dormant. The only place beside Earth's moon where humans have actually examined surface soils for the presence of organic molecules is Mars. This was accomplished using mass-spectrometry during the Viking mission, and results were negative. The lack of organic moieties, if they ever were present, probably resulted form their destruction over geologic time frames by the extraordinarily reactive surface soils found there. Thus, on Mars, detection of organic signatures of life probably would be possible only in subsurface soils, or perhaps in polar regions.
Document ID
20010023086
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Crawford, R. L.
(Idaho Univ. Moscow, ID United States)
Paszczynski, A.
(Idaho Univ. Moscow, ID United States)
Lang, Q.
(Idaho Univ. Moscow, ID United States)
Cheng, I. F.
(Idaho Univ. Moscow, ID United States)
Barnes, B.
(Idaho Univ. Moscow, ID United States)
Anderson, T. J.
(Idaho Univ. Moscow, ID United States)
Wells, R.
(Idaho Univ. Moscow, ID United States)
Wai, C.
(Idaho Univ. Moscow, ID United States)
Corti, G.
(Idaho Univ. Moscow, ID United States)
Allenbach, L.
(Idaho Univ. Moscow, ID United States)
Date Acquired
August 20, 2013
Publication Date
July 1, 2000
Publication Information
Publication: Concepts and Approaches for Mars Exploration
Issue: Part 1
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
OTHER: JPL-1212404
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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