Keywords

asteroids, pyroxene, meteorites, wollastonite, ferrosilite, Gaffey, mafic, mineral, composition, olivine, solar system, belt, asteroid, comets, spectra, spectrum, algorithm, programming

Abstract

Determining mafic mineral composition of asteroid bodies is a topic reviewed by M.J. Gaffey et al. (2002). The iterative procedure discussed can be implemented as an algorithm, and such efforts revealed weaknesses that are examined in this work. We seek to illustrate the limits of this method and graphically determine its predictions. There are boundaries in the formulae given where the equations break down. In ranges where mafic mixtures are predicted, a method is illustrated that allows a decoupling of these mixtures into the constituents.

Notes

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Graduation Date

2007

Semester

Fall

Advisor

Britt, Daniel

Degree

Master of Science (M.S.)

College

College of Sciences

Department

Physics

Degree Program

Physics

Format

application/pdf

Identifier

CFE0001922

URL

http://purl.fcla.edu/fcla/etd/CFE0001922

Language

English

Release Date

December 2007

Length of Campus-only Access

None

Access Status

Masters Thesis (Open Access)

Included in

Physics Commons

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