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A&A 420, L5-L8 (2004)
DOI: 10.1051/0004-6361:20040147
Letter
An R-type asteroid within near-Earth objects?
S. Marchi, M. Lazzarin and S. MagrinDipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
e-mail: [marchi;lazzarin;magrin]@pd.astro.it
(Received 10 March 2004 / Accepted 16 April 2004)
Abstract
We present visible and near-infrared spectroscopy of 2001 XR31,
a previously unclassified small near-Earth object (NEOs).
Its spectrum resembles that of basaltic body, with the distinctive
1 and 2
m pyroxene absorption bands, similar to those
found on V-type bodies. However, the spectrum of 2001 XR31 is
somewhat peculiar and we discuss whether
it can belong to another class of basaltic bodies, namely the rare R-class.
Key words: minor planet -- asteroids -- near-Earth objects
Offprint request: S. Marchi, marchi@pd.astro.it
© ESO 2004
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