The anomalous dust tail of comet P/Tempel 2

Details The anomalous dust tail of comet P/Tempel 2 The anomalous dust tail of comet P/Tempel 2

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211p..15e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 1, 1984, p. 15P-19P.

Astronomy and Astrophysics

Astronomy

22

Comet Tails, Cosmic Dust, Tempel 2 Comet, Infrared Spectra, Iras-Araki-Alcock Comet, Particle Emission

Scientific paper

The narrow dust tail of comet P/Tempel 2, observed by IRAS, is the
result of low-velocity emissions of large particles. Dynamical analysis
of the dust particles under the influence of solar radiation pressure
indicates that some of these emissions must have occurred at least 1500
days prior to the IRAS observations.

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