VIS-NIR reflectance of water ice/regolith analogue mixtures and implications for the detectability of ice mixed within planetary regoliths
Permanently shadowed regions at the poles of the Moon and Mercury have been pointed out as candidates for hosting water ice at their surface. We have measured in the laboratory the visible and near infrared spectral range (VIS‐NIR) bidirectional reflectance of intimate mixtures of water ice and the...
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Published in | Geophysical research letters Vol. 42; no. 15; pp. 6205 - 6212 |
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Main Authors | , , , , , |
Format | Journal Article |
Language | English |
Published |
Washington
Blackwell Publishing Ltd
16.08.2015
John Wiley & Sons, Inc |
Subjects | |
Online Access | Get full text |
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Summary: | Permanently shadowed regions at the poles of the Moon and Mercury have been pointed out as candidates for hosting water ice at their surface. We have measured in the laboratory the visible and near infrared spectral range (VIS‐NIR) bidirectional reflectance of intimate mixtures of water ice and the JSC‐1AF lunar simulant for different ice concentrations, particle sizes, and measurement geometries. The nonlinearity between the measured reflectance and the amount of ice in the mixture can be reproduced to some extent by the mixing formulas of standard reflectance models, in particular, those of Hapke and Hiroi, which are tested here. Estimating ice concentrations from reflectance data without knowledge of the mixing coefficients—strongly dependent on the size/shape of the grains—can result in large errors. According to our results, it is possible that considerable amounts of water ice might be intimately mixed in the regolith of the Moon and Mercury without producing noticeable photometric signatures.
Key Points
Bidirectional reflectance of ice/lunar regolith simulant binary mixtures measured in the laboratory
Strong VIS‐NIR signature of ice at high phase angle could be used to detect ice on the surface
The effect of particle size in common reflectance models is tested |
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Bibliography: | Swiss National Science Foundation - No. 200020_152560 ArticleID:GRL53248 istex:16BEE923606A5E85F6756F8F2795ADF6D312962C ark:/67375/WNG-GDZQB38H-W Texts S1 and S2 and Figures S1 and S2 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1002/2015GL064780 |