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.

The National Academies of Sciences, Engineering, and Medicine
500 Fifth St. N.W. | Washington, D.C. 20001

Copyright © National Academy of Sciences. All rights reserved.
Terms of Use and Privacy Statement