Electronic Resource
Springer
Earth, moon and planets
42 (1988), S. 41-47
ISSN:
1573-0794
Source:
Springer Online Journal Archives 1860-2000
Topics:
Geosciences
,
Physics
Notes:
Abstract We consider the infrared brightness of a flattened comet belt beyond the orbit of Neptune using a disk-like model with a power-law density distribution of comets. We compare this spectrum with the emission from a model zodiacal dust cloud in the ecliptic and with published IRAS data and present some consequences of dust in the comet belt.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00118038
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