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Dust emission of Comet Halley at large heliocentric distancesComet Halley is currently approaching the inner solar system. Four spacecrafts (NASA's spacecraft, two Russian Vega probes and the Japanese MS-T5 spacecraft) have already been launched to encounter the comet in March 1986. Two additional Halley probes (the European Giotto spacecraft and another Japanese Planet-A probe) will be launched in mid-85 to join the armada. Observations of dust emissions from Halley's Comet are discussed. The evaporation of cometary ices causes the emission of particulates from the nucleus. These observations will be used to determine the fly-by strategy of the Giotto spacecraft by taking into account the distribution of dust in the vicinity of the nucleus and the associated hazard for the space mission.
Document ID
19850018245
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Gruen, E.
(Max-Planck-Inst. fuer Kernphysik Heidelberg, Germany)
Schwehm, G.
(ESA. European Space Operations Centre Darmstadt, Germany)
Massonne, L.
(ESA. European Space Operations Centre Darmstadt, Germany)
Fertig, J.
(ESA. European Space Operations Centre Darmstadt, Germany)
Graser, U.
(Max-Planck-Inst. fuer Astronomie Heidelberg, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Lunar and Planetary Inst. 16th Lunar and Planetary Sci. Conf.
Subject Category
Astrophysics
Accession Number
85N26556
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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