A possible explanation of the light curve of comet Encke

Details A possible explanation of the light curve of comet Encke A possible explanation of the light curve of comet Encke

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..667f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Dec. 1980, p. 667-681. Research supported by the Consejo Nacional

Mathematics

Logic

6

Astronomical Photometry, Comet Nuclei, Comets, Light Curve, Albedo, Brightness, Evaporation

Scientific paper

A theoretical model was constructed for the brightness of comet Encke as a function of heliocentric distance, R, using conservation of solar energy, and assuming that C2 molecules are evaporated at the same rate as water molecules. An equation relating the total number of C2 molecules in the coma, and the total visual magnitude, m(V), was used to produce a graph of m(V) versus log R as a function of surface albedo. Theoretical results are compared with all brightness observations of comet Encke made during this century by reliable observers. Agreement between theory and observations is found to be excellent.

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