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Microwave Instrument for the Rosetta Orbiter (MIRO)The observed abundances of a large number of volatile molecules in comets supports the idea that comets were formed at very cold temperatures and at large heliocentric distances.
Document ID
20060040920
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/18371
Authors
Gulkis, S.
Frerking, M.
Janssen, M.
Hartogh, P.
Beaudin, G.
Koch, T.
Salinas, Y.
Kahn, C.
Date Acquired
August 23, 2013
Publication Date
January 1, 1999
Distribution Limits
Public
Copyright
Other
Keywords
COMET Rosetta MIRO Spectroscopy

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