Measurements of surface reflectance of permanently shadowed areas near Mercury's north pole reveal regions of anomalously dark and bright deposits at 1064 nm wavelength. These reflectance anomalies are concentrated on polewardfacing slopes and are spatially collocated with areas of high radar b...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.1072.2395 2023-05-15T17:39:44+02:00 Gregory A Neumann John F Cavanaugh Xiaoli Sun Erwan M Mazarico David E Smith Maria T Zuber Dandan Mao David A Paige Sean C Solomon Carolyn M Ernst Olivier S Barnouin The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1072.2395 http://www-geodyn.mit.edu/zubersite/pdfs/neumannetalsci.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1072.2395 http://www-geodyn.mit.edu/zubersite/pdfs/neumannetalsci.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www-geodyn.mit.edu/zubersite/pdfs/neumannetalsci.pdf text ftciteseerx 2020-04-26T00:23:48Z Measurements of surface reflectance of permanently shadowed areas near Mercury's north pole reveal regions of anomalously dark and bright deposits at 1064 nm wavelength. These reflectance anomalies are concentrated on polewardfacing slopes and are spatially collocated with areas of high radar backscatter postulated to be the result of near-surface water ice. Correlation of observed reflectance with modeled temperatures indicates that the optically bright regions are consistent with surface water ice, whereas dark regions are consistent with a surface layer of complex organic material that likely overlies buried ice and provides thermal insulation. Impacts of comets or volatile-rich asteroids could have provided both the dark and bright deposits. Text North Pole Unknown North Pole |
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Measurements of surface reflectance of permanently shadowed areas near Mercury's north pole reveal regions of anomalously dark and bright deposits at 1064 nm wavelength. These reflectance anomalies are concentrated on polewardfacing slopes and are spatially collocated with areas of high radar backscatter postulated to be the result of near-surface water ice. Correlation of observed reflectance with modeled temperatures indicates that the optically bright regions are consistent with surface water ice, whereas dark regions are consistent with a surface layer of complex organic material that likely overlies buried ice and provides thermal insulation. Impacts of comets or volatile-rich asteroids could have provided both the dark and bright deposits. |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Gregory A Neumann John F Cavanaugh Xiaoli Sun Erwan M Mazarico David E Smith Maria T Zuber Dandan Mao David A Paige Sean C Solomon Carolyn M Ernst Olivier S Barnouin |
spellingShingle |
Gregory A Neumann John F Cavanaugh Xiaoli Sun Erwan M Mazarico David E Smith Maria T Zuber Dandan Mao David A Paige Sean C Solomon Carolyn M Ernst Olivier S Barnouin |
author_facet |
Gregory A Neumann John F Cavanaugh Xiaoli Sun Erwan M Mazarico David E Smith Maria T Zuber Dandan Mao David A Paige Sean C Solomon Carolyn M Ernst Olivier S Barnouin |
author_sort |
Gregory A Neumann |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1072.2395 http://www-geodyn.mit.edu/zubersite/pdfs/neumannetalsci.pdf |
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North Pole |
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http://www-geodyn.mit.edu/zubersite/pdfs/neumannetalsci.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1072.2395 http://www-geodyn.mit.edu/zubersite/pdfs/neumannetalsci.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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