Evidence for water ice near the lunar poles
By W. Feldman, Sylvestre Maurice, D. Lawrence, R. Little, S. Lawrence, O. Gasnault, R. Wiens, B. Barraclough, R. Elphic, T. Prettyman and 2 more. 2001
338 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology
View Paper: https://www.semanticscholar.org/paper/5935a184975f3ca4b5ea3d23faceee41f7846cd9
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In Astronomy and Astrophysics
- Ian A. Crawford
- S. Squyres
- Dan J. McCleese
- Ashwin R. Vasavada
- B. Jakosky
- J. Schofield
- W. Feldman
- S. Calcutt
In Ecology
Citations in the corpus
- The Mars Odyssey Gamma-Ray Spectrometer Instrument Suite (2004, methodology): “The fluxes of epithermal neutrons measured by Lunar Prospector were used to infer the presence of H at the poles of the Moon (Feldman et al., 2001).”
- The Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment (2010, background): “These data have been interpreted to be consistent with the presence of roughly 1.5% water-equivalent hydrogen in the uppermost ∼50 cm of the lunar regolith if concentrated in the floors of craters unresolved by the spectrometer’s footprint (Feldman et al. 2001).”
- Lunar resources (2014, methodology): “Indirect evidence for ice in permanently shadowed polar craters was provided by the neutron spectrometer on the Lunar Prospector Spacecraft (Feldman et al., 1998, 2001).”