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Cited by 206

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Arecibo Radar Mapping of the Lunar Poles: A Search for Ice Deposits

Stacy, N. J. S., Campbell, D. B., Ford, P. G.·1997·Science

Abstract

The Arecibo 12.6-centimeter wavelength radar system was used to image the polar regions of the moon at a resolution of 125 meters in a search for ice deposits in areas of possible permanent shadow from the sun. No areas greater than 1 square kilometer were found with high radar backscatter cross sections and high circular polarization ratios, properties suggestive of the presence of ice. A number of areas smaller than 1 square kilometer were found with these properties, but optical images from spacecraft missions have shown some of these features to be in sunlight. Arecibo radar images of Sinus Iridum at latitude 47°N also showed a number of small features with similar properties. The coincidence of some of these features with the radar-facing slopes of craters and their presence in sunlit areas suggests that very rough surfaces rather than ice deposits are responsible for their unusual radar properties.

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Crossref · 10.1126/science.276.5318.1527

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Metadata

Authors
Stacy, N. J. S., Campbell, D. B., & Ford, P. G.
Venue
Science
Published
1997-06-06
Volume
276
Issue
5318
Pages
1527-1530
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W1979129737
Cited by
206
References
1
FWCI
8.88
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Arecibo Radar Mapping of the Lunar Poles: A Search for Ice Deposits. https://app.cochat.ai/papers/10.1126/science.276.5318.1527
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Stacy, N. J. S., Campbell, D. B., & Ford, P. G. (1997). Arecibo Radar Mapping of the Lunar Poles: A Search for Ice Deposits. Science. https://doi.org/10.1126/science.276.5318.1527

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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