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- W2023678212 abstract "We present new infrared (2–4 μm) spectroscopic observations of Vesta obtained in 2001, 2003, and 2004. Together with previously published work, these present a picture of how Vesta's spectrum changes with sub-Earth latitude and longitude. Vesta's albedo and 2-μm band vary regularly with its rotational phase. While establishing the continuum level for Vesta in the 3-μm region is not straightforward, Vesta appears to have a spectrum consistent with the HED meteorites and not requiring a 3-μm water of hydration band. We cannot formally rule out a shallow (∼1%) band, however. We place limits on the extent to which solar-wind implantation and contamination by CM-like impactors has changed the surface spectrum of Vesta." @default.
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- W2023678212 date "2006-02-01" @default.
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- W2023678212 title "Rotationally-resolved spectroscopy of Vesta I: 2–4 μm region" @default.
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- W2023678212 doi "https://doi.org/10.1016/j.icarus.2005.09.012" @default.
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