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Title:
Surface temperature of the nucleus of Comet 9P/Tempel 1
Authors:
Groussin, O.; A'Hearn, M. F.; Li, J.-Y.; Thomas, P. C.; Sunshine, J. M.; Lisse, C. M.; Meech, K. J.; Farnham, T. L.; Feaga, L. M.; Delamere, W. A.
Affiliation:
AA(Department of Astronomy, University of Maryland, College Park, MD 20742, USA), AB(Department of Astronomy, University of Maryland, College Park, MD 20742, USA), AC(Department of Astronomy, University of Maryland, College Park, MD 20742, USA), AD(Department of Astronomy, Cornell University, Ithaca, NY 14853, USA), AE(Department of Astronomy, University of Maryland, College Park, MD 20742, USA), AF(Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA), AG(NASA Astrobiology Institute, University of Hawaii, Honolulu, HI 96822, USA), AH(Department of Astronomy, University of Maryland, College Park, MD 20742, USA), AI(Department of Astronomy, University of Maryland, College Park, MD 20742, USA), AJ(Delamere Support Services, Boulder, CO, USA)
Publication:
Icarus, Volume 191, Issue 2, p. 63-72. (Icarus Homepage)
Publication Date:
00/2007
Origin:
ELSEVIER
Abstract Copyright:
Elsevier Inc.
Comment:
Originally published in Icarus, Vol. 187, p. 16-25 (2007)
DOI:
10.1016/j.icarus.2006.08.031
Bibliographic Code:
2007Icar..191S..63G

Abstract

The Deep Impact (DI) spacecraft encountered Comet 9P/Tempel 1 on July 4th, 2005 and observed it with several instruments. In particular, we obtained infrared spectra of the nucleus with the HRI-IR spectrometer in the wavelength range of 1.0 4.9 μm. The data were taken before impact, with a maximum resolution of ˜120 m per pixel at the time of observation. From these spectra, we derived the first directly observed temperature map of a comet nucleus. The surface temperature varied from 272±7 to 336±7 K on the sunlit hemisphere, matching the surface topography and incidence angle. The derived thermal inertia is low, most probably <50 W K-1 m-2 s1/2. Combined with other arguments, it is consistent with the idea that most of rapidly varying thermal physical processes, in particular the sublimation of volatiles around perihelion, should occur close to the surface. Thermal inertia is sufficient to explain the temperature map of the nucleus of Comet Tempel 1 to first order, but other physical processes like roughness and self-radiation are required to explain the details of the temperature map. Finally, we evaluated that the Standard Thermal Model is a good approximation to derive the effective radius of a cometary nucleus with an uncertainty lower than ˜10% if combined with a thermal infrared light curve.

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