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The NGST and the Zodiacal Light in the Solar System

Author
Ozernoy, Leonid
Published
[1999].
Physical Description
1 electronic document
Additional Creators
Mather, John C., Taidakova, Tanya, and Gorkavyi, Nick
Online Version

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Unclassified, Unlimited, Publicly available.
Free-to-read Unrestricted online access
Summary
We develop a physical model of the zodiacal cloud incorporating the real dust sources of asteroidal, cometary, and kuiperoidal origin. Using the inferred distribution of the zodiacal dust, we compute its thermal emission and scattering at several wavelengths (1.25, 5, and 20 micron) as a function of NGST location assumed to be at 1 AU or 3 AU. Areas on the sky with a minimum of zodiacal light are determined.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 20000019575.
NGST Science and Technology Exposition; Unknown.
Terms of Use and Reproduction
No Copyright.
View MARC record | catkey: 15970679