Sulfates in the North Polar Region of Mars Detected by OMEGA/Mars Express
The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) imaging spectrometer observed the northern circumpolar regions of Mars at a resolution of a few kilometers. An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorpti...
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 2005-03, Vol.307 (5715), p.1584-1586 |
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| creator | Langevin, Yves Poulet, François Bibring, Jean-Pierre Gondet, Brigitte |
| description | The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) imaging spectrometer observed the northern circumpolar regions of Mars at a resolution of a few kilometers. An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorptions at wavelengths of 1.45, 1.75, 1.94, 2.22, 2.26, and 2.48 micrometers. These signatures can be unambiguously attributed to calcium-rich sulfates, most likely gypsum. This region corresponds to the dark longitudinal dunes of Olympia Planitia. These observations reveal that water alteration played a major role in the formation of the constituting minerals of northern circumpolar terrains. |
| doi_str_mv | 10.1126/science.1109091 |
| format | Article |
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An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorptions at wavelengths of 1.45, 1.75, 1.94, 2.22, 2.26, and 2.48 micrometers. These signatures can be unambiguously attributed to calcium-rich sulfates, most likely gypsum. This region corresponds to the dark longitudinal dunes of Olympia Planitia. These observations reveal that water alteration played a major role in the formation of the constituting minerals of northern circumpolar terrains.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1109091</identifier><identifier>PMID: 15718428</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>United States: American Association for the Advancement of Science</publisher><subject>Absorption spectra ; Analysis ; Atmosphere ; Calcium Sulfate ; Carbon Dioxide ; Dunes ; Extraterrestrial Environment ; Geologic Sediments ; Geology ; Gypsum ; Mars ; Mars (Planet) ; Mars probes ; Mercury (Planet) ; Minerals ; Observations ; Observatories ; Planets ; Pluto (Planet) ; Polar regions ; Research Article and Reports ; Signatures ; Spacecraft ; Spectral reflectance ; Spectral signatures ; Spectroscopy ; Spectroscopy, Near-Infrared ; Spectrum Analysis ; Sulfates ; Surface ; Surface (Geology) ; Surface water ; Surfaces ; Temperature ; Venus (Planet) ; Water ; Wavelengths</subject><ispartof>Science (American Association for the Advancement of Science), 2005-03, Vol.307 (5715), p.1584-1586</ispartof><rights>Copyright 2005 American Association for the Advancement of Science</rights><rights>COPYRIGHT 2005 American Association for the Advancement of Science</rights><rights>COPYRIGHT 2005 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Mar 11, 2005</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a894t-1f8eb8d2efddb84c979d068c2c0c8b030d20c4900b0c0d23cd084ed1ba2959853</citedby><cites>FETCH-LOGICAL-a894t-1f8eb8d2efddb84c979d068c2c0c8b030d20c4900b0c0d23cd084ed1ba2959853</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/3841765$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/3841765$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,780,784,803,2884,2885,27924,27925,58017,58250</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/15718428$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Langevin, Yves</creatorcontrib><creatorcontrib>Poulet, François</creatorcontrib><creatorcontrib>Bibring, Jean-Pierre</creatorcontrib><creatorcontrib>Gondet, Brigitte</creatorcontrib><title>Sulfates in the North Polar Region of Mars Detected by OMEGA/Mars Express</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) imaging spectrometer observed the northern circumpolar regions of Mars at a resolution of a few kilometers. An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorptions at wavelengths of 1.45, 1.75, 1.94, 2.22, 2.26, and 2.48 micrometers. These signatures can be unambiguously attributed to calcium-rich sulfates, most likely gypsum. This region corresponds to the dark longitudinal dunes of Olympia Planitia. These observations reveal that water alteration played a major role in the formation of the constituting minerals of northern circumpolar terrains.</description><subject>Absorption spectra</subject><subject>Analysis</subject><subject>Atmosphere</subject><subject>Calcium Sulfate</subject><subject>Carbon Dioxide</subject><subject>Dunes</subject><subject>Extraterrestrial Environment</subject><subject>Geologic Sediments</subject><subject>Geology</subject><subject>Gypsum</subject><subject>Mars</subject><subject>Mars (Planet)</subject><subject>Mars probes</subject><subject>Mercury (Planet)</subject><subject>Minerals</subject><subject>Observations</subject><subject>Observatories</subject><subject>Planets</subject><subject>Pluto (Planet)</subject><subject>Polar regions</subject><subject>Research Article and Reports</subject><subject>Signatures</subject><subject>Spacecraft</subject><subject>Spectral reflectance</subject><subject>Spectral signatures</subject><subject>Spectroscopy</subject><subject>Spectroscopy, Near-Infrared</subject><subject>Spectrum Analysis</subject><subject>Sulfates</subject><subject>Surface</subject><subject>Surface (Geology)</subject><subject>Surface water</subject><subject>Surfaces</subject><subject>Temperature</subject><subject>Venus 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An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorptions at wavelengths of 1.45, 1.75, 1.94, 2.22, 2.26, and 2.48 micrometers. These signatures can be unambiguously attributed to calcium-rich sulfates, most likely gypsum. This region corresponds to the dark longitudinal dunes of Olympia Planitia. These observations reveal that water alteration played a major role in the formation of the constituting minerals of northern circumpolar terrains.</abstract><cop>United States</cop><pub>American Association for the Advancement of Science</pub><pmid>15718428</pmid><doi>10.1126/science.1109091</doi><tpages>3</tpages></addata></record> |
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| identifier | ISSN: 0036-8075 |
| ispartof | Science (American Association for the Advancement of Science), 2005-03, Vol.307 (5715), p.1584-1586 |
| issn | 0036-8075 1095-9203 |
| language | eng |
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| source | MEDLINE; JSTOR Archive Collection A-Z Listing; American Association for the Advancement of Science |
| subjects | Absorption spectra Analysis Atmosphere Calcium Sulfate Carbon Dioxide Dunes Extraterrestrial Environment Geologic Sediments Geology Gypsum Mars Mars (Planet) Mars probes Mercury (Planet) Minerals Observations Observatories Planets Pluto (Planet) Polar regions Research Article and Reports Signatures Spacecraft Spectral reflectance Spectral signatures Spectroscopy Spectroscopy, Near-Infrared Spectrum Analysis Sulfates Surface Surface (Geology) Surface water Surfaces Temperature Venus (Planet) Water Wavelengths |
| title | Sulfates in the North Polar Region of Mars Detected by OMEGA/Mars Express |
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