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      Space weathering on airless bodies : SPACE WEATHERING ON AIRLESS BODIES

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      Journal of Geophysical Research: Planets
      Wiley-Blackwell

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          Bidirectional reflectance spectroscopy: 1. Theory

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            Space weathering from Mercury to the asteroid belt

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              Asteroid vesta: spectral reflectivity and compositional implications.

              The spectral reflectivity (0.30 to 1.10 microns) of several asteroids has been measured for the first time. The reflection spectrum for Vesta contains a strong absorption band centered near 0.9 micron and a weaker absorption feature between 0.5 and 0.6 micron. The reflectivity decreases strongly in the ultraviolet. The reflection spectrum for the asteroid Pallas and probably for Ceres does not contain the 0.9-micron band. Vesta shows the strongest and best-defined absorption bands yet seen in the reflection spectrum for the solid surface of an object in the solar system. The strong 0.9-micron band arises from electronic absorptions in ferrous iron on the M2 site of a magnesian pyroxene. Comparison with laboratory measurements on meteorites and Apollo 11 samples indicates that the surface of Vesta has a composition very similar to that of certain basaltic achondrites.
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                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res. Planets
                Wiley-Blackwell
                21699097
                October 2016
                October 2016
                : 121
                : 10
                : 1865-1884
                Article
                10.1002/2016JE005128
                5975224
                29862145
                2b7424c8-5c9d-4706-8598-b613c85034bb
                © 2016

                http://doi.wiley.com/10.1002/tdm_license_1

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