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


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2012-06-20

AUTHORS

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

ABSTRACT

Observations from the Lunar Orbiter Laser Altimeter reveal the Moon’s Shackleton crater to be an ancient, unusually well-preserved simple crater whose interior walls are younger than its floor and rim; the relative brightness of the floor at 1,064 nanometres is most readily explained by minimal volatile accumulation since crater formation and decreased space weathering due to permanent shadow. More... »

PAGES

378-381

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature11216

DOI

http://dx.doi.org/10.1038/nature11216

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1005507328

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/22722197


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