High-resolution infrared spectroscopy of Io and possible surface materials
We have obtained new spectra of Io in the 3.5- to 4.2- and 4.5- to 5.4-μm regions with a resolution (λ/Δλ) of roughly 500. The Io spectra cover a range of longitudes, and times from 1983 through 1985. Laboratory spectra of various materials have also been obtained. In this wavelength region are loca...
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| Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 1989-03, Vol.78 (1), p.27-37 |
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| container_title | Icarus (New York, N.Y. 1962) |
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| creator | Howell, Robert R. Nash, Douglas B. Geballe, Thomas R. Cruikshank, Dale P. |
| description | We have obtained new spectra of Io in the 3.5- to 4.2- and 4.5- to 5.4-μm regions with a resolution (λ/Δλ) of roughly 500. The Io spectra cover a range of longitudes, and times from 1983 through 1985. Laboratory spectra of various materials have also been obtained. In this wavelength region are located several strong bands of SO
2, known to be a major component of Io's surface, as well as the bands of several potential surface materials. In the Io spectra we identify several new features attributable to SO
2, and have obtained strengths of the
33S,
34S, and
18O isotopic bands, which appear normal. We place limits on the amounts of Na
2SO
3, and Na
2SO
4 present. Finally, we use the data to place limits on the SO
2 gas abundance in Io's atmosphere. |
| doi_str_mv | 10.1016/0019-1035(89)90067-5 |
| format | Article |
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2, known to be a major component of Io's surface, as well as the bands of several potential surface materials. In the Io spectra we identify several new features attributable to SO
2, and have obtained strengths of the
33S,
34S, and
18O isotopic bands, which appear normal. We place limits on the amounts of Na
2SO
3, and Na
2SO
4 present. Finally, we use the data to place limits on the SO
2 gas abundance in Io's atmosphere.</description><identifier>ISSN: 0019-1035</identifier><identifier>EISSN: 1090-2643</identifier><identifier>DOI: 10.1016/0019-1035(89)90067-5</identifier><identifier>CODEN: ICRSA5</identifier><language>eng</language><publisher>Legacy CDMS: Elsevier Inc</publisher><subject>640107 - Astrophysics & Cosmology- Planetary Phenomena ; ABUNDANCE ; Astronomy ; ATMOSPHERES ; CHALCOGENIDES ; CHEMICAL COMPOSITION ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; Earth, ocean, space ; Exact sciences and technology ; Jupiter ; JUPITER PLANET ; Lunar And Planetary Exploration ; OPTICAL PROPERTIES ; OXIDES ; OXYGEN COMPOUNDS ; PHYSICAL PROPERTIES ; PLANETS ; Planets, their satellites and rings. Asteroids ; REFLECTIVITY ; RESOLUTION ; SATELLITE ATMOSPHERES ; SATELLITES ; Solar system ; SPECTROSCOPY ; SULFUR COMPOUNDS ; SULFUR OXIDES ; SURFACE PROPERTIES ; SURFACES</subject><ispartof>Icarus (New York, N.Y. 1962), 1989-03, Vol.78 (1), p.27-37</ispartof><rights>1989</rights><rights>1990 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a437t-f28070a1c8fd253a74f3bd2813abcd267c93a9411b89bcec623018fd6ce16d813</citedby><cites>FETCH-LOGICAL-a437t-f28070a1c8fd253a74f3bd2813abcd267c93a9411b89bcec623018fd6ce16d813</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/0019-1035(89)90067-5$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,885,3550,27924,27925,45995</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=6584187$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/5823759$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Howell, Robert R.</creatorcontrib><creatorcontrib>Nash, Douglas B.</creatorcontrib><creatorcontrib>Geballe, Thomas R.</creatorcontrib><creatorcontrib>Cruikshank, Dale P.</creatorcontrib><creatorcontrib>NASA, Ames Research Center, Moffett Field, CA (USA)</creatorcontrib><creatorcontrib>Edinburgh Royal Observatory, (England)</creatorcontrib><creatorcontrib>Groningen Rijksuniversiteit (Netherlands)</creatorcontrib><creatorcontrib>Hawaii Univ., Honolulu (USA)</creatorcontrib><creatorcontrib>Infrared Telescope Unit, Hilo, HI (USA)</creatorcontrib><creatorcontrib>California Institute of Technology, Pasadena (USA)</creatorcontrib><title>High-resolution infrared spectroscopy of Io and possible surface materials</title><title>Icarus (New York, N.Y. 1962)</title><description>We have obtained new spectra of Io in the 3.5- to 4.2- and 4.5- to 5.4-μm regions with a resolution (λ/Δλ) of roughly 500. The Io spectra cover a range of longitudes, and times from 1983 through 1985. Laboratory spectra of various materials have also been obtained. In this wavelength region are located several strong bands of SO
2, known to be a major component of Io's surface, as well as the bands of several potential surface materials. In the Io spectra we identify several new features attributable to SO
2, and have obtained strengths of the
33S,
34S, and
18O isotopic bands, which appear normal. We place limits on the amounts of Na
2SO
3, and Na
2SO
4 present. Finally, we use the data to place limits on the SO
2 gas abundance in Io's atmosphere.</description><subject>640107 - Astrophysics & Cosmology- Planetary Phenomena</subject><subject>ABUNDANCE</subject><subject>Astronomy</subject><subject>ATMOSPHERES</subject><subject>CHALCOGENIDES</subject><subject>CHEMICAL COMPOSITION</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Jupiter</subject><subject>JUPITER PLANET</subject><subject>Lunar And Planetary Exploration</subject><subject>OPTICAL PROPERTIES</subject><subject>OXIDES</subject><subject>OXYGEN COMPOUNDS</subject><subject>PHYSICAL PROPERTIES</subject><subject>PLANETS</subject><subject>Planets, their satellites and rings. Asteroids</subject><subject>REFLECTIVITY</subject><subject>RESOLUTION</subject><subject>SATELLITE ATMOSPHERES</subject><subject>SATELLITES</subject><subject>Solar system</subject><subject>SPECTROSCOPY</subject><subject>SULFUR COMPOUNDS</subject><subject>SULFUR OXIDES</subject><subject>SURFACE PROPERTIES</subject><subject>SURFACES</subject><issn>0019-1035</issn><issn>1090-2643</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1989</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNp9kM1u1TAQRi0EEpfCG3QRIYToIuCf2LE3SKiCtqgSG1hbzmRCjXLt4MlF6tvjkKpLVrOYM5_mO4ydC_5ecGE-cC5cK7jS76y7cJybvtVP2EFwx1tpOvWUHR6R5-wF0S_OubZOHdjX6_jzri1IeT6tMacmpqmEgmNDC8JaMkFe7ps8NTe5CWlslkwUhxkbOpUpADbHsGKJYaaX7NlUB756mGfsx5fP3y-v29tvVzeXn27b0Kl-bSdpec-DADuNUqvQd5MaRmmFCgOM0vTgVHCdEIN1AyAYqbiorAEUZqzYGXu952ZaoyeIK8Id5JTqv15bqXrtKvR2h5aSf5-QVn-MBDjPIWE-kZdaKiucrmC3g1C7UsHJLyUeQ7n3gvvNrt_U-U2dt87_s-u3szcP-YEgzNVZgkiPt0bbTti-Yuc7lgIFn9ZCXjhbQzrTiW39cV9j9fUnYtnqYAIcY9najDn-_42_oiOV6g</recordid><startdate>19890301</startdate><enddate>19890301</enddate><creator>Howell, Robert R.</creator><creator>Nash, Douglas B.</creator><creator>Geballe, Thomas R.</creator><creator>Cruikshank, Dale P.</creator><general>Elsevier Inc</general><general>Elsevier</general><scope>CYE</scope><scope>CYI</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>19890301</creationdate><title>High-resolution infrared spectroscopy of Io and possible surface materials</title><author>Howell, Robert R. ; Nash, Douglas B. ; Geballe, Thomas R. ; Cruikshank, Dale P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a437t-f28070a1c8fd253a74f3bd2813abcd267c93a9411b89bcec623018fd6ce16d813</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1989</creationdate><topic>640107 - Astrophysics & Cosmology- Planetary Phenomena</topic><topic>ABUNDANCE</topic><topic>Astronomy</topic><topic>ATMOSPHERES</topic><topic>CHALCOGENIDES</topic><topic>CHEMICAL COMPOSITION</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Jupiter</topic><topic>JUPITER PLANET</topic><topic>Lunar And Planetary Exploration</topic><topic>OPTICAL PROPERTIES</topic><topic>OXIDES</topic><topic>OXYGEN COMPOUNDS</topic><topic>PHYSICAL PROPERTIES</topic><topic>PLANETS</topic><topic>Planets, their satellites and rings. Asteroids</topic><topic>REFLECTIVITY</topic><topic>RESOLUTION</topic><topic>SATELLITE ATMOSPHERES</topic><topic>SATELLITES</topic><topic>Solar system</topic><topic>SPECTROSCOPY</topic><topic>SULFUR COMPOUNDS</topic><topic>SULFUR OXIDES</topic><topic>SURFACE PROPERTIES</topic><topic>SURFACES</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Howell, Robert R.</creatorcontrib><creatorcontrib>Nash, Douglas B.</creatorcontrib><creatorcontrib>Geballe, Thomas R.</creatorcontrib><creatorcontrib>Cruikshank, Dale P.</creatorcontrib><creatorcontrib>NASA, Ames Research Center, Moffett Field, CA (USA)</creatorcontrib><creatorcontrib>Edinburgh Royal Observatory, (England)</creatorcontrib><creatorcontrib>Groningen Rijksuniversiteit (Netherlands)</creatorcontrib><creatorcontrib>Hawaii Univ., Honolulu (USA)</creatorcontrib><creatorcontrib>Infrared Telescope Unit, Hilo, HI (USA)</creatorcontrib><creatorcontrib>California Institute of Technology, Pasadena (USA)</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>Icarus (New York, N.Y. 1962)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Howell, Robert R.</au><au>Nash, Douglas B.</au><au>Geballe, Thomas R.</au><au>Cruikshank, Dale P.</au><aucorp>NASA, Ames Research Center, Moffett Field, CA (USA)</aucorp><aucorp>Edinburgh Royal Observatory, (England)</aucorp><aucorp>Groningen Rijksuniversiteit (Netherlands)</aucorp><aucorp>Hawaii Univ., Honolulu (USA)</aucorp><aucorp>Infrared Telescope Unit, Hilo, HI (USA)</aucorp><aucorp>California Institute of Technology, Pasadena (USA)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>High-resolution infrared spectroscopy of Io and possible surface materials</atitle><jtitle>Icarus (New York, N.Y. 1962)</jtitle><date>1989-03-01</date><risdate>1989</risdate><volume>78</volume><issue>1</issue><spage>27</spage><epage>37</epage><pages>27-37</pages><issn>0019-1035</issn><eissn>1090-2643</eissn><coden>ICRSA5</coden><abstract>We have obtained new spectra of Io in the 3.5- to 4.2- and 4.5- to 5.4-μm regions with a resolution (λ/Δλ) of roughly 500. The Io spectra cover a range of longitudes, and times from 1983 through 1985. Laboratory spectra of various materials have also been obtained. In this wavelength region are located several strong bands of SO
2, known to be a major component of Io's surface, as well as the bands of several potential surface materials. In the Io spectra we identify several new features attributable to SO
2, and have obtained strengths of the
33S,
34S, and
18O isotopic bands, which appear normal. We place limits on the amounts of Na
2SO
3, and Na
2SO
4 present. Finally, we use the data to place limits on the SO
2 gas abundance in Io's atmosphere.</abstract><cop>Legacy CDMS</cop><pub>Elsevier Inc</pub><doi>10.1016/0019-1035(89)90067-5</doi><tpages>11</tpages></addata></record> |
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| ispartof | Icarus (New York, N.Y. 1962), 1989-03, Vol.78 (1), p.27-37 |
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| source | Access via ScienceDirect (Elsevier); NASA Technical Reports Server |
| subjects | 640107 - Astrophysics & Cosmology- Planetary Phenomena ABUNDANCE Astronomy ATMOSPHERES CHALCOGENIDES CHEMICAL COMPOSITION CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Earth, ocean, space Exact sciences and technology Jupiter JUPITER PLANET Lunar And Planetary Exploration OPTICAL PROPERTIES OXIDES OXYGEN COMPOUNDS PHYSICAL PROPERTIES PLANETS Planets, their satellites and rings. Asteroids REFLECTIVITY RESOLUTION SATELLITE ATMOSPHERES SATELLITES Solar system SPECTROSCOPY SULFUR COMPOUNDS SULFUR OXIDES SURFACE PROPERTIES SURFACES |
| title | High-resolution infrared spectroscopy of Io and possible surface materials |
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