Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996dps....28.0805p&link_type=abstract
American Astronomical Society, DPS meeting #28, #08.05; Bulletin of the American Astronomical Society, Vol. 28, p.1083
Astronomy and Astrophysics
Astronomy
Scientific paper
We have used the Faint Object Spectrograph on the Hubble Space Telescope (with the G270H grating, 2221 <= lambda <= 3301) to make ultraviolet studies of the comet P/Wirtanen and of the Centaur 2060-Chiron, which is possibly a former member of the Kuiper belt. The orbital parameters for the objects during the observations are given in the following table: Date Time No. V D Delta Solar Elong. (s) Exp. (mag) (AU) (AU) (degrees) Chiron 1996 Jan 23--24 4720 7 15.7 8.5 8.1 109 1996 Apr 13 1370 1 15.2 8.5 7.5 166 Wirtanen 1996 Jul 22 1430 1 19 2.7 1.8 152 The acquisition data show evidence that Wirtanen had a coma during the observation, but the data for Chiron are consistent with that of a point source. We present the color and geometric albedoes for Chiron and Wirtanen: Chiron is remarkably grey with a nuclear albedo of p=0.08 +/- 0.01 (assuming a radius of 90 km); Wirtanen's albedo is similarly grey with p<0.07 +/- 0.03 (assuming a radius of 1 km), an upper limit because an unknown fraction of flux is coming from the coma. We also will present the UV partial light curve of Chiron, obtained with the series of seven HST/FOS spectra taken in 1996 January over a time of 4 hours (about two-thirds of Chiron's synodic rotation period). There are no significant detections of coma emission (e.g., CS lambda 2576, Mgi lambda 2852, and OH lambda 3085) in either object, and the 3sigma upper limit for the OH lambda 3085 brightness of Wirtanen is {cal B} < 8 Rayleighs. In our poster we will report on upper limits for brightness and column density of coma species.
A'Hearn Michael F.
Alan Stern S.
Bertaux Jean Loup
Feldman Paul D.
Festou Michael C.
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