Literature DB >> 16150976

Deep Impact observations by OSIRIS onboard the Rosetta spacecraft.

Horst Uwe Keller1, Laurent Jorda, Michael Küppers, Pedro J Gutierrez, Stubbe F Hviid, Jörg Knollenberg, Luisa-Maria Lara, Holger Sierks, Cesare Barbieri, Philippe Lamy, Hans Rickman, Rafael Rodrigo.   

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.

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Year:  2005        PMID: 16150976     DOI: 10.1126/science.1119020

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Early inner solar system impactors: physical properties of comet nuclei and dust particles revisited.

Authors:  A C Levasseur-Regourd; J Lasue; E Desvoivres
Journal:  Orig Life Evol Biosph       Date:  2006-12       Impact factor: 1.950

  1 in total

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