Evolution of the brightness of Comet Giacobini-Zinner

Details Evolution of the brightness of Comet Giacobini-Zinner Evolution of the brightness of Comet Giacobini-Zinner

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...60m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Sept.-Oct. 1985, p. 60-64. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Brightness Distribution, Evolution (Development), Giacobini-Zinner Comet, Digital Simulation, Dimensional Analysis, Solar Activity Effects, Time Dependence, View Effects

Scientific paper

Optimal expressions for brightness variations of Comet Giacobini-Zinner during 1900-1972 are obtained through mathematical simulation and dimensional analysis. These expressions made it possible to determine the absolute brightness (H0) of the comet. The seeing conditions are shown to have a significant influence on values of H0. Mathematical models are developed for the dependence of H0 on seeing conditions, phase angle, the level of solar activity, and time.

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