The secular variation of cometary magnitude

Details The secular variation of cometary magnitude The secular variation of cometary magnitude

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...53..444h&link_type=abstract

Icarus (ISSN 0019-1035), vol. 53, March 1983, p. 444-452.

Other

19

Astrometry, Comets, Magnitude, Secular Variations, Orbits, Solar Position, Comets, Magnitude, Calculations, Short Period Comets, Decay, Analysis, Mathematical Models

Scientific paper

This paper calculates the mean variation in absolute magnitude per perihelion passage, ΔH10, for short-period comets from the data of Vsekhsvyatskii and finds a value of 0.30 ± 0.06. Other mechanisms used for estimating cometary decay are reviewed an it is concluded that a more probable value for ΔH10 is about 0.002. Reasons for the discrepancy between these two values are given.

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