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3He in permanently shadowed lunar polar surfaces

Publication ,  Journal Article
Cocks, FH
Published in: Icarus
April 1, 2010

Because of their cryogenic temperatures, analysis indicates that permanently shadowed polar lunar craters may have substantially higher levels of 3He than sunlit lunar surfaces and are conservatively estimated to contain as much as 50 ppb or more. © 2009 Elsevier Inc. All rights reserved.

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Published In

Icarus

DOI

EISSN

1090-2643

ISSN

0019-1035

Publication Date

April 1, 2010

Volume

206

Issue

2

Start / End Page

778 / 779

Related Subject Headings

  • Astronomy & Astrophysics
  • 5109 Space sciences
  • 5101 Astronomical sciences
  • 0404 Geophysics
  • 0402 Geochemistry
  • 0201 Astronomical and Space Sciences
 

Citation

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MLA
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Cocks, F. H. (2010). 3He in permanently shadowed lunar polar surfaces. Icarus, 206(2), 778–779. https://doi.org/10.1016/j.icarus.2009.12.032
Cocks, F. H. “3He in permanently shadowed lunar polar surfaces.” Icarus 206, no. 2 (April 1, 2010): 778–79. https://doi.org/10.1016/j.icarus.2009.12.032.
Cocks FH. 3He in permanently shadowed lunar polar surfaces. Icarus. 2010 Apr 1;206(2):778–9.
Cocks, F. H. “3He in permanently shadowed lunar polar surfaces.” Icarus, vol. 206, no. 2, Apr. 2010, pp. 778–79. Scopus, doi:10.1016/j.icarus.2009.12.032.
Cocks FH. 3He in permanently shadowed lunar polar surfaces. Icarus. 2010 Apr 1;206(2):778–779.
Journal cover image

Published In

Icarus

DOI

EISSN

1090-2643

ISSN

0019-1035

Publication Date

April 1, 2010

Volume

206

Issue

2

Start / End Page

778 / 779

Related Subject Headings

  • Astronomy & Astrophysics
  • 5109 Space sciences
  • 5101 Astronomical sciences
  • 0404 Geophysics
  • 0402 Geochemistry
  • 0201 Astronomical and Space Sciences