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Preventing the Forward Contamination of Mars (2006)
Space Studies Board (SSB)

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. "4 Environments on Mars Relative to Life." Preventing the Forward Contamination of Mars. Washington, DC: The National Academies Press, 2006.

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Preventing the Forward Contamination of Mars

Touma, J., and J. Wisdom. 1993. The chaotic obliquity of Mars. Science 259: 1294-1296.

Travis, B.J., N.D. Rosenberg, and J.N. Cuzzi. 2003. On the role of widespread subsurface convection in bringing liquid water close to Mars’ surface. J. Geophys. Res. 108(E4): 8040.

Treiman, A.H., R.A. Barrett, and J.L. Gooding. 1993. Preterrestrial aqueous alteration of the Lafayette (SNC) meteorite. Meteoritics 28: 86-97.


Wallendahl, A., and A.H. Treiman. 1999. Geochemical models of low-temperature alteration of martian rocks. 30th Lunar and Planetary Science Conference. Abstract No. 1268. Lunar and Planetary Institute, Houston, Tex.

Ward, W.R. 1992. Long-term orbital and spin dynamics of Mars. Pp. 298-320 in Mars, H.H. Kieffer, B.M. Jakosky, C.W. Snyder, and M.S. Matthews, eds. University of Arizona Press, Tucson, Ariz.

Weiss, B.P., Y.L. Yung, and K.H. Nealson. 2000. Atmospheric energy for subsurface life on Mars? Proc. Natl. Acad. Sci. U.S.A. 97: 1395-1399.


Yen, A.S., S.S. Kim, M.H. Hecht, M.S. Frant, and B. Murray. 2000. Evidence that the reactivity of the martian soil is due to superoxide ions. Science 289: 1909-1912.

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