| タイトル | A Post-Stardust Mission View of Jupiter Family Comets |
| 本文（外部サイト） | http://hdl.handle.net/2060/20120003314 |
| 著者（英） | Zolensky, M. |
| 著者所属（英） | NASA Johnson Space Center |
| 発行日 | 2011-01-01 |
| 言語 | eng |
| 内容記述 | Before the Stardust Mission, many persons (including the mission team) believed that comet nuclei would be geologically boring objects. Most believed that comet nucleus mineralogy would be close or identical to the chondritic interplanetary dust particles (IDPs), or perhaps contain mainly amorphous nebular condensates or that comets might even be composed mainly of preserved presolar material [1]. Amazingly, the results for Comet Wild 2 (a Jupiter class comet) were entirely different. Whether this particular comet will ultimately be shown to be typical or atypical will not be known for a rather long time, so we describe our new view of comets from the rather limited perspective of this single mission. |
| NASA分類 | Space Sciences (General) |
| レポートNO | JSC-CN-25955 |
| 権利 | No Copyright |
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