| タイトル | EPOXI at Comet Hartley 2 |
| 本文（外部サイト） | http://hdl.handle.net/2060/20110015409 |
| 著者（英） | Kelley, Michael S.; Wellnitz, Dennis D.; Bodewits, Dennis; Besse, Sebastien; Belton, Michael J. S.; Melosh, H. Jay; Kissel, Jochen; Thomas, Peter C.; Meech, Karen J.; Yeomans, Donald K.; Collins, Steven M.; Feaga, Lori M.; Hermalyn, Brendan; Hampton, Donald; Veverka, Joseph; McFadden, Jessica M.; Farnham, Tony F.; Schultz, Peter H.; Klaasen, Kenneth P.; A'Hearn, Michael F.; Bowling, Timothy J.; Carcish, Brian T.; Delamere, W. Alan; Groussin, Oliver; Sunshine, Jessica M. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2011-03-16 |
| 言語 | eng |
| 内容記述 | Understanding how comets work, i,e., what drives their activity, is crucial to using comets to study the early solar system. EPOXI flew past comet 103P/Hartley 2, one with an unusually small but very active nucleus. taking both images and spectra. Unlike large, relatively inactive nuclei, this nncleus is outgassing primarily due to CO2, which drags chnnks of ice out of the nnclens. It also shows significant differences in the relative abundance of volatiles from various parts of the nucleus. |
| NASA分類 | Astronomy |
| レポートNO | GSFC.CP.5023.2011 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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