Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250b.381e&link_type=abstract
In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 2: Dust and Nucleus p 381-384 (SEE N
Astronomy and Astrophysics
Astronomy
Comet Nuclei, Halley'S Comet, Infrared Spectroscopy, Size Determination, Temperature Measurement, Vega Project, Astronomical Spectroscopy, Crusts, Surface Temperature
Scientific paper
The infrared thermal emission of the nucleus of Halley's comet was measured by the imaging channel of the IKS spectrometer in two wavelengths bands (7 - 10 μm and 9 - 14 μm) and in two perpendicular directions of analysis. The effective dimensions of the infrared emissive region in these directions are estimated from a simulation of the flyby configuration, and then compared to observations made in the visible range. A colour temperature larger than 360K was deduced using on-ground preflight calibrations. A temperature of the same order is also obtained independently, comparing the absolute value of the measured fluxes with model simulations. Such temperatures, significantly higher than the sublimating temperature of ices, are compared with surface temperatures predicted by the friable sponge model of cometary nucleus (Horanyi et al., 1984), suggesting the existence of a dust mantle layer covering at least some parts of the nucleus surface, even at 0.8 A.U.
Bibring Jean-Pierre
Combes Michel
Coron N.
Emerich Claude
Gispert Richard
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