Findings of the Mars Special Regions Science Analysis Group
Astrobiology
By: D.W. Beaty, K.L. Buxbaum, M.A. Meyer, N. Barlow, W. Boynton, B. Clark, J. Deming, P.T. Doran, K. Edgett, S. Hancock, J. Head, M. Hecht, V. Hipkin, T. Kieft, R. Mancinelli, E. McDonald, C. McKay, M. Mellon, H. Newsom, G. Ori, D. Paige, A.C. Schuerger, M. Sogin, J.A. Spry, A. Steele, K. Tanaka, and M. Voytek
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Abstract
In summary, within the upper 5 m most of Mars is either too cold or too dry to support the propagation of terrestrial life. However, there are regions that are in disequilibrium, naturally or induced, and could be classified as "special" or, if enough uncertainty exist, could not be declared as "non-special." ?? Mary Ann Liebert, Inc.
| Publication type | Article |
|---|---|
| Publication Subtype | Journal Article |
| Title | Findings of the Mars Special Regions Science Analysis Group |
| Series title | Astrobiology |
| DOI | 10.1089/ast.2006.6.677 |
| Volume | 6 |
| Issue | 5 |
| Year Published | 2006 |
| Language | English |
| Larger Work Type | Article |
| Larger Work Subtype | Journal Article |
| Larger Work Title | Astrobiology |
| First page | 677 |
| Last page | 732 |
| Google Analytic Metrics | Metrics page |