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罗塞塔号航天器上的欧西里斯(OSIRIS)相机对深度撞击的观测。

Deep Impact observations by OSIRIS onboard the Rosetta spacecraft.

作者信息

Keller Horst Uwe, Jorda Laurent, Küppers Michael, Gutierrez Pedro J, Hviid Stubbe F, Knollenberg Jörg, Lara Luisa-Maria, Sierks Holger, Barbieri Cesare, Lamy Philippe, Rickman Hans, Rodrigo Rafael

机构信息

Max-Planck Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany.

出版信息

Science. 2005 Oct 14;310(5746):281-3. doi: 10.1126/science.1119020. Epub 2005 Sep 8.

Abstract

The OSIRIS cameras (optical, spectroscopic, and infrared remote imaging system) onboard the European Space Agency's Rosetta spacecraft observed comet 9P/Tempel 1 for 17 days continuously around the time of NASA's Deep Impact mission. The cyanide-to-water production ratio was slightly enhanced in the impact cloud, compared with that of normal comet activity. Dust particles were flowing outward in the coma at >160 meters per second, accelerated by the gas. The slope of the brightness increase showed a dip about 200 seconds after the impact. Dust Afrho values before and long after the impact confirm the slight decrease of cometary activity. The dust-to-water mass ratio was much larger than 1.

摘要

欧洲航天局“罗塞塔”号航天器上搭载的奥西里斯相机(光学、光谱和红外远程成像系统),在美国国家航空航天局“深度撞击”任务期间,持续17天对9P/坦普尔1号彗星进行了观测。与正常彗星活动相比,撞击云团中的氰化物与水的生成比率略有提高。尘埃颗粒在彗发中以每秒超过160米的速度向外流动,由气体加速。亮度增加的斜率在撞击后约200秒出现了一个下降。撞击前后及很久之后的尘埃Afrho值证实了彗星活动略有下降。尘埃与水的质量比远大于1。

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