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Cometary Activity at 25.7 AU: Hale-Bopp 11 Years after Perihelion*

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Published 2008 March 27 © 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Gy. M. Szabó et al 2008 ApJ 677 L121 DOI 10.1086/588095

1538-4357/677/2/L121

Abstract

Eleven years after its perihelion, comet C/1995 O1 (Hale-Bopp) is still active. Between 2007 October 20 and 22, we detected a diffuse coma of 180 × 103 km in diameter with a slight elongation toward the north-south direction. The integrated brightness was 20.04 mag in RC, implying Afρ = 300 m and albedo × dust surface aRC = 4300 km2. The coma was relatively red at VR = 0.66 mag, which is consistent with that of the dust in other comets. The observed properties and the overall fading in brightness between 10 and 26 AU follow the predicted behavior of CO-driven activity. This is the most distant cometary activity ever observed.

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Footnotes

  • Based on data obtained at the Siding Spring Observatory.

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10.1086/588095