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- W1663384925 abstract "Spectral photometry is a powerful tool for establishing links between meteorites and their parent bodies (asteroids, comets, the Moon, Mars). The primary information used to interpret asteroid reflectance spectra comes from absorption bands that are diagnostic of the cosmically significant minerals pyroxene and olivine. Then there are secondary effects that can alter the size of the bands and the slope of the continuum. These effects are primarily due to particle size, surface roughness, and temperature which are poorly characterized in the literature. These effects are important because our knowledge of the physical condition of the surface of bodies such as asteroids and comets is limited. Understanding how light scattering changes the features in the reflectance spectra is then useful for interpreting spectra. A lot of effort has gone into characterizing and modeling the effect of particle size on the reflectance spectra with some success. The reason for this is because most asteroids over 100 m in size are thought to be covered by a layer of impact generated particles. However, there has been little characterization of the meteorite samples in terms of their solid surface roughness." @default.
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- W1663384925 date "2010-06-01" @default.
- W1663384925 modified "2023-09-25" @default.
- W1663384925 title "Reflectance spectra of meteorites" @default.
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