The nucleus of comet P/Schwassmann-Wachmann 1

Dale P. Cruikshank, Robert H. Brown

Research output: Contribution to journalArticle

32 Citations (Scopus)

Abstract

The thermal flux in the 20-μm Q filter band of comet P/Schwassmann-Wachmann 1 was measured some 77 days after the most recent previous eruption, and when the visual magnitude was about 17.6. Considerations of the eruptive history of the comet, and in particular its tendency to fade to a minimum threshold brightness level between eruptions, suggest that the measurement refers to an essentially bare nucleus. Using the standard photometric/radiometric technique for calculating the diameters and geometric albedos of asteroids and planetary satellites, and the assumption that the bare nucleus is measured, we find that the diameter of the nucleus is 40±5 km, and the geometric albedo is 0.13±0.04.

Original languageEnglish (US)
Pages (from-to)377-380
Number of pages4
JournalIcarus
Volume56
Issue number3
DOIs
StatePublished - 1983
Externally publishedYes

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comets
comet
albedo
volcanic eruption
planetary satellite
volcanic eruptions
nuclei
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natural satellites
asteroids
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brightness
tendencies
history
histories
filters
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ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The nucleus of comet P/Schwassmann-Wachmann 1. / Cruikshank, Dale P.; Brown, Robert H.

In: Icarus, Vol. 56, No. 3, 1983, p. 377-380.

Research output: Contribution to journalArticle

Cruikshank, Dale P. ; Brown, Robert H. / The nucleus of comet P/Schwassmann-Wachmann 1. In: Icarus. 1983 ; Vol. 56, No. 3. pp. 377-380.
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