Small bodies and the outer planets and Appendices 1 and 2

Details Small bodies and the outer planets and Appendices 1 and 2 Small bodies and the outer planets and Appendices 1 and 2

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974psi..rept.....d&link_type=abstract

Final Report Planetary Science Inst., Tucson, AZ.

Physics

Asteroids, Cosmology, Space Debris, Spectral Reflectance, Spectral Signatures, Celestial Mechanics, Infrared Radiation, Optical Properties, Pyroxenes, Radiation Measurement

Scientific paper

Correlations of asteroid spectral reflectivity characteristics with orbital parameters have been sought. Asteroid proper elements and extreme heliocentric distance were examined. Only general trends were noted, primarily red asteroids and asteroids with IR (.95 micron) absorption bands are concentrated toward the inner part of the belt. Also, asteroids with the pyroxene band tend to have larger proper eccentricities relative to non-banded asteroids.

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