NASA NTRS · 20060040920
Microwave Instrument for the Rosetta Orbiter (MIRO)
Abstract
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.
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Gulkis, S., Frerking, M., Janssen, M., Hartogh, P., Beaudin, G., Koch, T., Salinas, Y., Kahn, C.. 1999-01-01. Microwave Instrument for the Rosetta Orbiter (MIRO). https://ntrs.nasa.gov/citations/20060040920
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