Abstract A preliminary analysis of infrared observations of comets P/Crommelin and P/Tempel 1 is presented. Comet P/Crommelin was observed from UKIRT over the range 1–20 micron, using standard filters. From the shape of the thermal emission spectrum, the temperature of the dust grains is estimated (T = 314 ± 33 44 K) and also the dust production rate (1.3 × 105 g s −1). Comet P/Tempel 1 was observed with the Infrared Astronomical Satellite (IRAS). The emission is found to be considerably extended and there is also evidence for temperature variation of the dust grains as indicated by the 12 to 25 micron flux ratio.
Recent infrared observations of comets with UKIRT and IRAS
Advances in Space Research ; 4 , 9 ; 203-206
1984-01-01
4 pages
Article (Journal)
Electronic Resource
English
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