SIZE AND ORBIT DEPENDENT TRENDS IN THE REFLECTANCE COLORS OF EARTH-APPROACHING ASTEROIDS

Authors
Citation
Dl. Rabinowitz, SIZE AND ORBIT DEPENDENT TRENDS IN THE REFLECTANCE COLORS OF EARTH-APPROACHING ASTEROIDS, Icarus (New York, N.Y. 1962), 134(2), 1998, pp. 342-346
Citations number
25
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
00191035
Volume
134
Issue
2
Year of publication
1998
Pages
342 - 346
Database
ISI
SICI code
0019-1035(1998)134:2<342:SAODTI>2.0.ZU;2-B
Abstract
New observations show that reflectance colors of Earth-approaching ast eroids depend on their sizes and orbits. Most bodies larger than simil ar to 2 lan have reddish colors similar to common main-belt asteroids of spectral type S. Smaller bodies, and those that may have recently m igrated from the main belt, have relatively neutral spectra in the 0.5 - to 0.8-mu m wavelength range, These trends may result from the actio n of ''space-weathering,'' recently proposed to explain similar spectr al variations on the surfaces of S-type asteroids and the disparity be tween the colors of ordinary chondrite meteorites and their probable m ain-belt parents. (C) 1998 Academic Press.