A&A 425, L25-L28 (2004)
DOI: 10.1051/0004-6361:200400054
Letter
Visible spectral properties of asteroid 21 Lutetia, target of Rosetta Mission
M. Lazzarin, S. Marchi, S. Magrin and C. BarbieriDipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
e-mail: [lazzarin;marchi;s.magrin;barbieri]@pd.astro.it
(Received 17 June 2004 / Accepted 10 August 2004)
Abstract
Rosetta spacecraft was successfully launched on March 2nd
2004 after its launch postponement in January 2003. Owing to this
delay all the original targets, comet and asteroids, have been
changed. In particular, on its 10 years journey to the new comet
67P/Churyumov-Gerasimenko, the spacecraft will pass close to the
asteroid 21 Lutetia. In this paper we present three visible
spectra of 21 Lutetia covering its rotational period. We have not
found big surface composition variations and the overall behavior
resembles that of a C-type asteroid. However, we discovered two
main features which are present on the three spectra at around 0.43
and 0.51
m probably due to aqueous alteration and porphyrins
respectively.
Key words: visible spectroscopy -- Rosetta target
© ESO 2004

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