Colour, albedo and nucleus size of Halley's comet View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1985-05

AUTHORS

Dale P. Cruikshank, W. K. Hartmann, David J. Tholen

ABSTRACT

Halley's comet (1982 i) is now bright enough for broadband photometry by large infrared telescopes1–3. We report here on photometry of the comet in the B (0.44 µm), J (0.55 µm), V (1.25 µm) and K (2.2 µm) broadband filters during a time when the coma was very weak and presumed to contribute negligibly to the broadband photometry. The V – J and J – K colours suggest that the colour of the nucleus of Halley's comet is similar to that of the D-type asteroids, which in turn suggests that the surface of the nucleus is of albedo < 0.1. More... »

PAGES

122-124

References to SciGraph publications

  • 1974-03. Physical properties of the natural satellites in SPACE SCIENCE REVIEWS
  • 1980-02. The composition of the Trojan asteroids in NATURE
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1038/315122a0

    DOI

    http://dx.doi.org/10.1038/315122a0

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1030707738


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