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• W2005020221 abstract "Recent spectroscopic observations indicate that the M-type asteroid 21 Lutetia has a primitive, carbonaceous-chondrite-like (C-type) surface composition for which a low geometric albedo would be expected; this is incompatible with the IRAS albedo of . From new thermal-infrared spectrophotometric measurements and detailed thermophysical modeling we infer that Lutetia has a diameter of km and a geometric albedo of , in excellent agreement with the IRAS value. We can thus rule out a low albedo typical of a C-type taxonomic classification. Furthermore, we find that Lutetia's thermal properties are well within the range expected for large asteroids; we find no evidence for unusually high thermal inertia." @default.
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• W2005020221 date "2006-02-10" @default.
• W2005020221 modified "2023-09-30" @default.
• W2005020221 title "The size and albedo of Rosetta fly-by target 21 Lutetia from new IRTF measurements and thermal modeling" @default.
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• W2005020221 doi "https://doi.org/10.1051/0004-6361:20053742" @default.
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