The light curve of the short-period Comet Tempel 2 and a new selection criterion of the comet outburst activity mechanism

Details The light curve of the short-period Comet Tempel 2 and a new selection criterion of the comet outburst activity mechanism The light curve of the short-period Comet Tempel 2 and a new selection criterion of the comet outburst activity mechanism

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..375c&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 375; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 10, p. 922-927. In

Astronomy and Astrophysics

Astronomy

1

Astronomical Photometry, Light Curve, Tempel 2 Comet, Magnitude, Visual Observation

Scientific paper

The light curves of the visual integral magnitudes of the Tempel 2 short-period comet in its three apparitions (1967 X, 1983 X, and 1988 XIV) have been constructed and investigated. It is shown that, in its different apparitions, the comet preserves its form and light-curve asymmetry, the bends of its branches, symmetric relative to the perihelion, and its high outburst activity. It is found that in the comet's different apparitions, its outbursts are detected at the same heliocentric distances.

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