Cometary activity at 25.7 AU: Hale--Bopp 11 years after perihelion

Abstract

Eleven years after its perihelion, comet C/1995 O1 (Hale-Bopp) is still active. Between October 20--22, 2007, we detected a diffuse coma of 180x10^3$kmindiameterwithaslightelongationtowardN/Sdirection.Theintegratedbrightnesswas20.04magin{R}_C,implyingAf\rho =300mandalbedoxdustsurface$a_RC$=4300 km^2. The coma was relatively red at V-R=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 AU and 26 AU follow the predicted behaviour of CO-driven activity (Capria et al. 2002). This is the most distant cometary activity ever observed.

v2: typos corrected. 13 pages, 5 figures, 1 table, ApJ Letters, in press

References in corpus (2)

• Photometry of cometary nuclei: Rotation rates, colours and a comparison with Kuiper Belt Objects
• Optical observations of 23 distant Jupiter Family Comets, including 36P/Whipple at multiple phase angles

Cited by in corpus (1)

• The Active Centaurs