Observations of the spectrum of Jupiter from 1500 to 2000 A with the IUE
The far-UV spectrum of Jupiter recorded by these observations with the International Ultraviolet Explorer samples only the upper levels of the planet's atmosphere. There are several absorptions caused by C/sub 2/H/sub 2/ and indications that NH/sub 3/ may also be present at these altitudes. We...
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| Veröffentlicht in: | Astrophys. J., Lett. Ed.; (United States) Lett. Ed.; (United States), 1980-02, Vol.236, p.L39 |
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| container_title | Astrophys. J., Lett. Ed.; (United States) |
| container_volume | 236 |
| creator | Owen, T. Caldwell, J. Rivolo, A. R. Moore, V. Lane, A. L. Sagan, C. Hunt, G. E. Ponnamperuma, C. |
| description | The far-UV spectrum of Jupiter recorded by these observations with the International Ultraviolet Explorer samples only the upper levels of the planet's atmosphere. There are several absorptions caused by C/sub 2/H/sub 2/ and indications that NH/sub 3/ may also be present at these altitudes. We find (C/sub 2/H/sub 2/)/(H/sub 2/)=22 x 10/sup -9/ and (NH/sub 3/)/(H/sub 2/)< or =0.5 x 10/sup -9/ for specific absorptions in this spectral region. Ph/sub 3/ may also play a role as a continuum absorber, and we can set a new upper limit of |
| doi_str_mv | 10.1086/183194 |
| format | Article |
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R. ; Moore, V. ; Lane, A. L. ; Sagan, C. ; Hunt, G. E. ; Ponnamperuma, C.</creator><creatorcontrib>Owen, T. ; Caldwell, J. ; Rivolo, A. R. ; Moore, V. ; Lane, A. L. ; Sagan, C. ; Hunt, G. E. ; Ponnamperuma, C. ; Laboratory for Planetary Atmospheres Research, State University of New York, Stony Brook</creatorcontrib><description>The far-UV spectrum of Jupiter recorded by these observations with the International Ultraviolet Explorer samples only the upper levels of the planet's atmosphere. There are several absorptions caused by C/sub 2/H/sub 2/ and indications that NH/sub 3/ may also be present at these altitudes. We find (C/sub 2/H/sub 2/)/(H/sub 2/)=22 x 10/sup -9/ and (NH/sub 3/)/(H/sub 2/)< or =0.5 x 10/sup -9/ for specific absorptions in this spectral region. Ph/sub 3/ may also play a role as a continuum absorber, and we can set a new upper limit of <5 x 10/sup -9/ on (H/sub 2/S)/(H/sub 2/). 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R.</creatorcontrib><creatorcontrib>Moore, V.</creatorcontrib><creatorcontrib>Lane, A. L.</creatorcontrib><creatorcontrib>Sagan, C.</creatorcontrib><creatorcontrib>Hunt, G. E.</creatorcontrib><creatorcontrib>Ponnamperuma, C.</creatorcontrib><creatorcontrib>Laboratory for Planetary Atmospheres Research, State University of New York, Stony Brook</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J., Lett. Ed.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Owen, T.</au><au>Caldwell, J.</au><au>Rivolo, A. R.</au><au>Moore, V.</au><au>Lane, A. L.</au><au>Sagan, C.</au><au>Hunt, G. E.</au><au>Ponnamperuma, C.</au><aucorp>Laboratory for Planetary Atmospheres Research, State University of New York, Stony Brook</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observations of the spectrum of Jupiter from 1500 to 2000 A with the IUE</atitle><jtitle>Astrophys. J., Lett. Ed.; (United States)</jtitle><date>1980-02-15</date><risdate>1980</risdate><volume>236</volume><spage>L39</spage><pages>L39-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>The far-UV spectrum of Jupiter recorded by these observations with the International Ultraviolet Explorer samples only the upper levels of the planet's atmosphere. There are several absorptions caused by C/sub 2/H/sub 2/ and indications that NH/sub 3/ may also be present at these altitudes. We find (C/sub 2/H/sub 2/)/(H/sub 2/)=22 x 10/sup -9/ and (NH/sub 3/)/(H/sub 2/)< or =0.5 x 10/sup -9/ for specific absorptions in this spectral region. Ph/sub 3/ may also play a role as a continuum absorber, and we can set a new upper limit of <5 x 10/sup -9/ on (H/sub 2/S)/(H/sub 2/). These results are consistent with existing models for Jovian photochemistry and atmospheric structure, but they emphasize the need for additional theoretical and laboratory studies.</abstract><cop>United States</cop><doi>10.1086/183194</doi><oa>free_for_read</oa></addata></record> |
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| ispartof | Astrophys. J., Lett. Ed.; (United States), 1980-02, Vol.236, p.L39 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_183194 |
| source | Alma/SFX Local Collection |
| subjects | 640107 - Astrophysics & Cosmology- Planetary Phenomena ABSORPTION ACETYLENE ALKYNES AMMONIA ATMOSPHERES CHEMICAL COMPOSITION CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS HYDRIDES HYDROCARBONS HYDROGEN COMPOUNDS JUPITER PLANET NITROGEN COMPOUNDS NITROGEN HYDRIDES ORGANIC COMPOUNDS PHOSPHINES PHOSPHORUS COMPOUNDS PLANETARY ATMOSPHERES PLANETS SPECTRA ULTRAVIOLET SPECTRA |
| title | Observations of the spectrum of Jupiter from 1500 to 2000 A with the IUE |
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