Near-infrared spectroscopy of probable impact melt from three large lunar highland craters
- 1 September 1985
- Vol. 63 (3) , 442-452
- https://doi.org/10.1016/0019-1035(85)90056-9
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Remote sensing of lunar pyroclastic mantling depositsIcarus, 1985
- Strength of mineral absorption features in the transmitted component of near‐infrared reflected light: First results from RELABJournal of Geophysical Research, 1983
- Bunte Breccia of the Ries: Continuous deposits of large impact cratersReviews of Geophysics, 1983
- The Manicouagan Impact Structure: An analysis of its original dimensions and formJournal of Geophysical Research, 1983
- Copernicus Crater Central Peak: Lunar Mountain of Unique CompositionScience, 1982
- Moon: Near‐infrared spectral reflectance, A first good lookJournal of Geophysical Research, 1981
- Spectral reflectance of highland rock types at Apollo 17: Evidence from Boulder 1, Station 2Earth, Moon, and Planets, 1975
- Visible and near-infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the solar systemJournal of Geophysical Research, 1974
- Spectral reflectance systematics for mixtures of powdered hypersthene, labradorite, and ilmeniteJournal of Geophysical Research, 1974
- Vitrification darkening of rock powders: implications for optical properties of the lunar surfaceEarth, Moon, and Planets, 1973