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Asteroid lightcurve inversionOne of the most fundamental physical properties of any asteroid is its shape. Lightcurves provide the only source of shape information for most asteroids. Unfortunately, the functional form of a lightcurve is determined by the viewing/illumination geometry and the asteroid's light scattering characteristics as well as its shape, and in general it is impossible to determine an asteroid's shape from lightcurves. A technique called convex-profile inversion (CPI) that obtains a convex profile, P, from any lightcurve is introduced. If certain ideal conditions are satisfied, then P is an estimator for the asteroid's mean cross section, C, a convex set defined as the average of all cross sections C(z) cut by planes a distance z above the asteroids's equatorial plane. C is therefore a 2-D average of the asteroid's 3-D shape.
Document ID
19870013944
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Ostro, Steven J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Connelly, Robert
(Cornell Univ. Ithaca, N.Y., United States)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986
Subject Category
Optics
Accession Number
87N23377
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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