Article ID Journal Published Year Pages File Type
1774338 Icarus 2011 14 Pages PDF
Abstract

The Chandrayaan-1 X-ray Spectrometer (C1XS) flown on-board the first Indian lunar mission Chandrayaan-1, measured X-ray fluorescence spectra during several episodes of solar flares during its operational period of ∼9 months. The accompanying X-ray Solar Monitor (XSM) provided simultaneous spectra of solar X-rays incident on the Moon which are essential to derive elemental chemistry. In this paper, we present the surface abundances of Mg, Al, Si, Ca and Fe, derived from C1XS data for a highland region on the southern nearside of the Moon. Analysis techniques are described in detail including absolute X-ray line flux derivation and conversion into elemental abundance. The results are consistent with a composition rich in plagioclase with a slight mafic mineral enhancement and a Ca/Al ratio that is significantly lower than measured in lunar returned samples. We suggest various possible scenarios to explain the deviations.

► First results from Chandrayaan-1 X-ray Spectrometer. ► Elemental composition for a region in the southern nearside highlands. ► Derived values suggests a hitherto unsampled composition.

Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
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