Sources and physical processes responsible for OH/H2O in the lunar soil as revealed by the Moon Mineralogy Mapper (M3)
By T. McCord, L. Taylor, J. Combe, G. Kramer, Carle M. Pieters, J. Sunshine, R. Clark. 2011
167 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology
View Paper: https://www.semanticscholar.org/paper/f38e6f6d5d273325497bb5eb19689b7e17414757
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In Astronomy and Astrophysics
- Sean C. Solomon
- Clark R. Chapman
- Denton S. Ebel
- W. Feldman
- D. Domingue
- D. Lawrence
- Carle M. Pieters
- R. Clark
In Ecology
Citations in the corpus
- Thermal removal from near‐infrared imaging spectroscopy data of the Moon (2011, background): “Figures 2a and 2b show the magnitude of the thermal emission/Fsun at 1 AU and various temperatures.”
- Mercury’s Weather-Beaten Surface: Understanding Mercury in the Context of Lunar and Asteroidal Space Weathering Studies (2014, result): “This steady state is consistent with the detection of hydroxyl and water signatures over the lunar surface (Vilas et al. 2008; Clark 2009; Pieters et al. 2009; Sunshine et al. 2009; McCord et al. 2011).”
- DETECTION OF WIDESPREAD HYDRATED MATERIALS ON VESTA BY THE VIR IMAGING SPECTROMETER ON BOARD THE DAWN MISSION (2012, background): “The temporally constant longitudinal variation in 2.8 μm band depth on Vesta (Figure 3) contrasts with the temporally and latitudinally variable distribution seen on the Moon that has been used to point to a solar-wind origin (Pieters et al. 2009; Sunshine et al. 2009; McCord et al. 2011).”