Albedo Maps of Comets p/ Halley and p/ Giacobini-Zinner

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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