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
APA
Chicago
ICMJE
MLA
NLM
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.
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