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DOI | 10.1126/science.7871428 |
HST spectroscopic observations of Jupiter after the collision of comet Shoemaker-Levy 9 | |
Noll K.S.; McGrath M.A.; Trafton L.M.; Atreya S.K.; Caldwell J.J.; Weaver H.A.; Yelle R.V.; Barnet C.; Edgington S. | |
发表日期 | 1995 |
ISSN | 0036-8075 |
起始页码 | 1307 |
结束页码 | 1313 |
卷号 | 267期号:5202 |
英文摘要 | Ultraviolet spectra obtained with the Hubble Space Telescope identified at least 10 molecules and atoms in the perturbed stratosphere near the G impact site, most never before observed in Jupiter. The large mass of sulfur-containing material, more than 1014 grams in S2 alone, indicates that many of the sulfur-containing molecules S2, CS2, CS, H2S, and S+ may be derived from a sulfur-bearing parent molecule native to Jupiter. If so, the fragment must have penetrated at least as deep as the predicted NH4SH cloud at a pressure of approximately 1 to 2 bars. Stratospheric NH3 was also observed, which is consistent with fragment penetration below the cloud tops. Approximately 107 grams of neutral and ionized metals were observed in emission, including Mg II, Mg I, Si I, Fe I, and Fe II. Oxygen-containing molecules were conspicuous by their absence; upper limits for SO2, SO, CO, SiO, and H2O are derived. |
英文关键词 | Sio; ammonia; carbon disulfide; iron; magnesium; oxygen; sulfur; water; article; astronomy; atmosphere; microclimate; spectroscopy; Ammonia; Atmosphere; Carbon Disulfide; Extraterrestrial Environment; Iron; Jupiter; Magnesium; Oxygen; Solar System; Spectrum Analysis; Sulfur; Support, U.S. Gov't, Non-P.H.S.; Water |
语种 | 英语 |
来源期刊 | Science
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/244896 |
作者单位 | Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States; Department of Astronomy, University of Texas, Austin, TX 78712, United States; Atmosph., Oceanic, Space Sci. Dept., University of Michigan, Ann Arbor, MI 48109, United States; Inst. for Space and Terrestrial Sci., Space Astrophysics Laboratory, 4850 Keele Street, North York, Ont. M3J 3K1, Canada; NASA/Ames Research Center, Moffett Field, CA 94035, United States |
推荐引用方式 GB/T 7714 | Noll K.S.,McGrath M.A.,Trafton L.M.,et al. HST spectroscopic observations of Jupiter after the collision of comet Shoemaker-Levy 9[J],1995,267(5202). |
APA | Noll K.S..,McGrath M.A..,Trafton L.M..,Atreya S.K..,Caldwell J.J..,...&Edgington S..(1995).HST spectroscopic observations of Jupiter after the collision of comet Shoemaker-Levy 9.Science,267(5202). |
MLA | Noll K.S.,et al."HST spectroscopic observations of Jupiter after the collision of comet Shoemaker-Levy 9".Science 267.5202(1995). |
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