Mercury Radar Imaging: Evidence for Polar Ice
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, we...
| Published in: | Science |
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| Main Authors: | , , |
| Format: | Article in Journal/Newspaper |
| Language: | English |
| Published: |
American Association for the Advancement of Science (AAAS)
1992
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| Subjects: | |
| Online Access: | http://dx.doi.org/10.1126/science.258.5082.635 https://www.science.org/doi/pdf/10.1126/science.258.5082.635 |
| Summary: | 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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