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Science 12 July 1985:
Vol. 229. no. 4709, pp. 160 - 163
DOI: 10.1126/science.229.4709.160

Articles

Near-Earth Asteroids: Possible Sources from Reflectance Spectroscopy

LUCY A. MCFADDEN 1, MICHAEL J. GAFFEY 2, and THOMAS B. MCCORD 2

1 Astronomy Program, University of Maryland, College Park 20742
2 Planetary Geosciences Division, Hawaii Institute of Geophysics, University of Hawaii, Honolulu 96822

Spectra of near-Earth asteroids were compared to spectra of selected asteroids, planets, and satellites to determine possible source regions. The diversity of reflectance spectra of the near-Earth asteroids implies different mineralogical compositions and hence more than one source region. The presence of near-Earth asteroid spectral signatures similar to those of certain main-belt asteroids supports models that derive some of these asteroids from the 5:2 Kirkwood gap and the Flora family by gravitational perturbations. Planetary and satellite surfaces are different in composition than the near-Earth asteroids, which is in agreement with theoretical arguments that such bodies should not be sources. Some near-Earth asteroids supply portions of Earth's meteorite flux, but other sources must also contribute.

Submitted on October 10, 1984
Accepted on March 8, 1985


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