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Properties of the Hermean regolith: V. New optical reflectance spectra, comparison with lunar anorthosites, and mineralogical modelling
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2004 (English)In: Icarus, Vol. 168, no 2, 257-276 p.Article in journal (Refereed) Published
Abstract [en]

We present new optical (0.4-0.65 μm) spectra of Mercury and lunar pure anorthosite locations, obtained quasi-simultaneously with the Nordic Optical Telescope (NOT) in 2002. A comparative study is performed with the model of Lucey et al. (2000, J. Geo

Place, publisher, year, edition, pages
2004. Vol. 168, no 2, 257-276 p.
Identifiers
URN: urn:nbn:se:uu:diva-48017OAI: oai:DiVA.org:uu-48017DiVA: diva2:75924
Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-12

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