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Dynamical Zodiacal Cloud Models Constrained by High Resolution Spectroscopy of the Zodiacal LightWe have developed a set of self-consistent dynamical models of the Zodiacal cloud, following the orbital evolution of dust particles. Three populations were considered, originating from the Kuiper belt, asteroids and comets. Using the models developed, we investigated how the solar spectrum is changed by scattering by the zodiacal cloud grains and compared the obtained spectra with the observations.
Document ID
20050169817
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Ipatov, S. I. (Maryland Univ. MD, United States)
Kutyrev, A. S. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Madsen, G. J. (Wisconsin Univ. Madison, WI, United States)
Mather, J. C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Moseley, S. H. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Reynolds, R. J. (Wisconsin Univ. Madison, WI, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2005
Publication Information
Publication: Lunar and Planetary Science XXXVI, Part 9
Subject Category
Astronomy
Funding Number(s)
CONTRACT_GRANT: NSF AST-02-04973
CONTRACT_GRANT: NAG5-12265
Distribution Limits
Public
Copyright
Public Use Permitted.

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