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9969 Braille: Deep Space 1 infrared spectroscopy, geometric albedo, and classification

Authors :
Buratti, B.J.
Britt, D.T.
Soderblom, L.A.
Hicks, M.D.
Boice, D.C.
Brown, R.H.
Meier, R.
Nelson, R.M.
Oberst, J.
Owen, T.C.
Rivkin, A.S.
Sandel, B.R.
Stern, S.A.
Thomas, N.
Yelle, R.V.
Source :
Icarus. Jan, 2004, Vol. 167 Issue 1, p129, 7 p.
Publication Year :
2004

Abstract

Spectra of Asteroid 9969 Braille in the 1.25-2.6 [micro]m region returned by the Deep Space 1 (DS1) Mission show a ~ 10% absorption band centered at 2 [micro]m, and a reflectance peak at 1.6 [micro]m. Analysis of these features suggest that the composition of Braille is roughly equal parts pyroxene and olivine. Its spectrum between 0.4 and 2.5 [micro]m suggests that it is most closely related to the Q taxonomic type of asteroid. The spectrum also closely matches that of the ordinary chondrites, the most common type of terrestrial meteorite. The geometric albedo of Braille is unusually high ([p.sub.v] = 0.34), which is also consistent with its placement within the rarer classes of stony asteroids, and which suggests it has a relatively fresh, unweathered surface, perhaps due to a recent collision. Keywords: Asteroids NEOs; 9969 Braille; Deep Space 1

Subjects

Subjects :
Asteroids
Astronomy
Earth sciences

Details

Language :
English
ISSN :
00191035
Volume :
167
Issue :
1
Database :
Gale General OneFile
Journal :
Icarus
Publication Type :
Academic Journal
Accession number :
edsgcl.112798727