Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...187..665h&link_type=abstract
Astronomy and Astrophysics, Vol.187, NO. 1+2/NOV, P. 665, 1987
Astronomy and Astrophysics
Astrophysics
11
Scientific paper
Near-simultaneous infrared and visual images of P/Halley are combined to create a map of the spatial variation of average albedo (which is generally a factor of four larger than the geometric albedo defined by Hanner et al., 1981). The map is compared with a similar map of P/Giacobini-Zinner (P/G-Z) obtained previously. P/G-Z showed a minimum in albedo of 0.07 with an increase by a factor of 2 over an angular distance of 30". The lowest albedos in P/G-Z were offset from the nucleus in the anti-sunward direction, coincident with a dust tail observed in the infrared. The P/Halley albedos are higher than those found for P/G-Z, ranging from 0.2-0.4, but both comets have relatively low albedo in the anti-sunward direction (along the tail). We attribute the albedo distribution to large, dark, fluffy grains confined to the orbital plane close to the nucleus. The high albedo values in P/Halley may be due to enhanced flux in the visual image because of the comet's very small phase angle.
Campins Humberto
Cruikshank Dale P.
Decher Rudolf
Hammel Heidi Beth
Storrs Alex D.
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