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Mercury Radar Imaging: Evidence for Polar Ice

Slade, Martin A., Butler, Bryan J., Muhleman, Duane O.·1992·Science

Abstract

The first unambiguous full-disk radar mapping of Mercury at 3.5-centimeter wavelength, with the Goldstone 70-meter antenna transmitting and 26 antennas of the Very Large Array receiving, has provided evidence for the presence of polar ice. The radar experiments, conducted on 8 and 23 August 1991, were designed to image the half of Mercury not photographed by Mariner 10. The orbital geometry allowed viewing beyond the north pole of Mercury; a highly reflective region was clearly visible on the north pole during both experiments. This polar region has areas in which the circular polarization ratio (μ c ) was 1.0 to 1.4; values < ∼0.1 are typical for terrestrial planets. Such high values of μ c have hitherto been observed in radar observations only from icy regions of Mars and icy outer planet satellites.

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Metadata

Authors
Slade, M. A., Butler, B. J., & Muhleman, D. O.
Venue
Science
Published
1992-10-23
Volume
258
Issue
5082
Pages
635-640
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W1978389347
Cited by
345
References
0
FWCI
9.83
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Mercury Radar Imaging: Evidence for Polar Ice. https://app.cochat.ai/papers/10.1126/science.258.5082.635
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Slade, M. A., Butler, B. J., & Muhleman, D. O. (1992). Mercury Radar Imaging: Evidence for Polar Ice. Science. https://doi.org/10.1126/science.258.5082.635

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