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A possible explanation for the blue spectral slope observed on B-type asteroids
M. J. Loeffler
, B. S. Prince
Astronomy and Planetary Sciences
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peer-review
6
Scopus citations
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Keyphrases
Asteroids
100%
Spectral Slope
100%
B-type
100%
Graphite
100%
Iron Oxide
80%
Dark Materials
60%
Troilite
60%
UV-VIS Spectroscopy
40%
Reflectance Spectra
40%
Spectral Changes
40%
Albedo
20%
Visible-infrared
20%
Near-infrared
20%
Sulfide
20%
Near-infrared Spectrum
20%
Regolith
20%
Silicate Minerals
20%
Bennu
20%
Visible Region
20%
Forsterite
20%
Physics
Troilite
100%
Near Infrared
66%
Reflectance
66%
Albedo
33%
Infrared Spectra
33%
Regolith
33%
Earth and Planetary Sciences
Troilite
100%
Reflectance
66%
Albedo
33%
Regolith
33%
Infrared Spectra
33%
Silicate Mineral
33%
Forsterite
33%