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Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, USA.
Science. 2005 Oct 14;310(5746):265-9. doi: 10.1126/science.1118978. Epub 2005 Sep 8.
On 4 July 2005, many observatories around the world and in space observed the collision of Deep Impact with comet 9P/Tempel 1 or its aftermath. This was an unprecedented coordinated observational campaign. These data show that (i) there was new material after impact that was compositionally different from that seen before impact; (ii) the ratio of dust mass to gas mass in the ejecta was much larger than before impact; (iii) the new activity did not last more than a few days, and by 9 July the comet's behavior was indistinguishable from its pre-impact behavior; and (iv) there were interesting transient phenomena that may be correlated with cratering physics.
2005年7月4日,全球众多地面及太空天文台观测了“深度撞击”号与9P/坦普尔1号彗星的碰撞过程或其后续情况。这是一次史无前例的协同观测活动。这些数据表明:(i)撞击后出现了成分与撞击前不同的新物质;(ii)喷射物中尘埃质量与气体质量之比远大于撞击前;(iii)新的活跃状态持续不超过几天,到7月9日,彗星的行为与撞击前已无差别;(iv)出现了一些有趣的瞬态现象,可能与撞击坑形成物理过程相关。