Comet Sugano-Saigusa-Fujikawa (1983V) - A small, puzzling comet
Spectroscopic and infrared observations of Comet Sugano-Saigusa-Fujikawa (1983V) were obtained during its close approach to the earth on June 11-14, 1983. The forbidden O I production rates of 1.8 + or - 0.9 x 10 to the 26th atoms/s observed on June 12.3 and 7 + or - 3.5 x 10 to the 26th atoms/s on...
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| Veröffentlicht in: | Astron. J.; (United States) 1987-10, Vol.94 (4), p.1081-1087 |
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| creator | Hanner, M. S. Newburn, R. L. Veeder, G. J. Spinrad, H. |
| description | Spectroscopic and infrared observations of Comet Sugano-Saigusa-Fujikawa (1983V) were obtained during its close approach to the earth on June 11-14, 1983. The forbidden O I production rates of 1.8 + or - 0.9 x 10 to the 26th atoms/s observed on June 12.3 and 7 + or - 3.5 x 10 to the 26th atoms/s on June 13.4 lead to derived water-production rates of 3 x 10 to the 27th mol/s on June 12 and 1.1 x 10 to the 28th mol/s on June 13. The abundances of the minor species NH2, CN, C2, and C3 are unusually low relative to forbidden O I. The upper limit to the average nuclear radius from infrared and visual photometry on June 12-13 (assuming that the entire signal came from the nucleus) is about 370 m. The dust/gas mass ratio was less than 0.01 on June 12 and less than 0.005 on June 13. |
| doi_str_mv | 10.1086/114544 |
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S. ; Newburn, R. L. ; Veeder, G. J. ; Spinrad, H.</creator><creatorcontrib>Hanner, M. S. ; Newburn, R. L. ; Veeder, G. J. ; Spinrad, H. ; California Univ., Berkeley ; California Institute of Technology, Pasadena</creatorcontrib><description>Spectroscopic and infrared observations of Comet Sugano-Saigusa-Fujikawa (1983V) were obtained during its close approach to the earth on June 11-14, 1983. The forbidden O I production rates of 1.8 + or - 0.9 x 10 to the 26th atoms/s observed on June 12.3 and 7 + or - 3.5 x 10 to the 26th atoms/s on June 13.4 lead to derived water-production rates of 3 x 10 to the 27th mol/s on June 12 and 1.1 x 10 to the 28th mol/s on June 13. The abundances of the minor species NH2, CN, C2, and C3 are unusually low relative to forbidden O I. The upper limit to the average nuclear radius from infrared and visual photometry on June 12-13 (assuming that the entire signal came from the nucleus) is about 370 m. 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The upper limit to the average nuclear radius from infrared and visual photometry on June 12-13 (assuming that the entire signal came from the nucleus) is about 370 m. 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S.</creatorcontrib><creatorcontrib>Newburn, R. L.</creatorcontrib><creatorcontrib>Veeder, G. J.</creatorcontrib><creatorcontrib>Spinrad, H.</creatorcontrib><creatorcontrib>California Univ., Berkeley</creatorcontrib><creatorcontrib>California Institute of Technology, Pasadena</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Medline</collection><collection>MEDLINE</collection><collection>MEDLINE (Ovid)</collection><collection>MEDLINE</collection><collection>MEDLINE</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Astron. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hanner, M. S.</au><au>Newburn, R. L.</au><au>Veeder, G. J.</au><au>Spinrad, H.</au><aucorp>California Univ., Berkeley</aucorp><aucorp>California Institute of Technology, Pasadena</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Comet Sugano-Saigusa-Fujikawa (1983V) - A small, puzzling comet</atitle><jtitle>Astron. J.; (United States)</jtitle><addtitle>Astron J</addtitle><date>1987-10-01</date><risdate>1987</risdate><volume>94</volume><issue>4</issue><spage>1081</spage><epage>1087</epage><pages>1081-1087</pages><issn>0004-6256</issn><abstract>Spectroscopic and infrared observations of Comet Sugano-Saigusa-Fujikawa (1983V) were obtained during its close approach to the earth on June 11-14, 1983. The forbidden O I production rates of 1.8 + or - 0.9 x 10 to the 26th atoms/s observed on June 12.3 and 7 + or - 3.5 x 10 to the 26th atoms/s on June 13.4 lead to derived water-production rates of 3 x 10 to the 27th mol/s on June 12 and 1.1 x 10 to the 28th mol/s on June 13. The abundances of the minor species NH2, CN, C2, and C3 are unusually low relative to forbidden O I. The upper limit to the average nuclear radius from infrared and visual photometry on June 12-13 (assuming that the entire signal came from the nucleus) is about 370 m. The dust/gas mass ratio was less than 0.01 on June 12 and less than 0.005 on June 13.</abstract><cop>Legacy CDMS</cop><pmid>11542132</pmid><doi>10.1086/114544</doi><tpages>7</tpages></addata></record> |
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| source | MEDLINE; NASA Technical Reports Server; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
| subjects | 640107 - Astrophysics & Cosmology- Planetary Phenomena Astronomical Phenomena Astronomy Astrophysics Carbon CHEMICAL COMPOSITION CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COMETS COSMIC DUST Cosmic Dust - analysis COSMIC GASES DUSTS FLUIDS GASES HYDROGEN COMPOUNDS INFRARED SPECTRA INTERPLANETARY SPACE MASS Meteoroids Models, Theoretical Nitrogen Compounds Oxygen OXYGEN COMPOUNDS SPACE Space life sciences SPECTRA Spectrophotometry, Infrared WATER |
| title | Comet Sugano-Saigusa-Fujikawa (1983V) - A small, puzzling comet |
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