Constraints on the volatile distribution within Shackleton crater at the lunar south pole-Reference-Cited by-同舟云学术

Constraints on the volatile distribution within Shackleton crater at the lunar south pole

Published:2012-06 Issue:7403 Volume:486 Page:378-381
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Zuber Maria T.,Head James W.,Smith David E.,Neumann Gregory A.,Mazarico Erwan,Torrence Mark H.,Aharonson Oded,Tye Alexander R.,Fassett Caleb I.,Rosenburg Margaret A.,Melosh H. Jay

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature11216.pdf

Reference31 articles.

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2. Arnold, J. R. Ice in the lunar polar regions. J. Geophys. Res. 84, 5659–5668 (1979)

3. Spudis, P. D., Plescia, J., Josset, J.-L. & Beauvivre, S. Geology of Shackleton Crater and the south pole of the Moon. Geophys. Res. Lett.. 36, L14201, http://dx.doi.org/10.1029/2008GL034468 (2008)

4. Nozette, S. et al. The Clementine bistatic radar experiment. Science 274, 1495–1498 (1996)

5. Stacy, N. J. S., Campbell, D. B. & Ford, P. G. Arecibo radar mapping of the lunar poles: a search for ice deposits. Science 276, 1527–1530 (1997)

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