The brightness of P/Halley and the surface activity of the nucleus at previous apparitions

Details The brightness of P/Halley and the surface activity of the nucleus at previous apparitions The brightness of P/Halley and the surface activity of the nucleus at previous apparitions

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234..173h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Sept. 1, 1988, p. 173-176.

Astronomy and Astrophysics

Astronomy

5

Brightness Distribution, Comet Nuclei, Halley'S Comet, Surface Properties, Giotto Mission, Magnitude

Scientific paper

The variation in the absolute magnitude of Halley's comet over the last
2000 yr can be explained in terms of a variation in the percentage of
the total area of the nucleus that is active. On average this percentage
is 3.4 but it has probably varied from as little as 0.76 to as high as
10.0.

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