From: arXiv.org e-Print archive
Posted: Wednesday, September 3, 2014
J. T. Wilson (1), V. R. Eke (1), R. J. Massey (1), R. C. Elphic (2), B. L. Jolliff (3), D. J. Lawrence (4), E. W. Llewellin (1), J. N. McElwaine (1), L. F. A. Teodoro (2) ((1) Durham University, (2) NASA Ames, (3) WUSTL, (4) JHU-APL)
(Submitted on 3 Sep 2014)
We reconstruct the abundance of thorium near the Compton-Belkovich Volcanic Complex on the Moon, using data from the Lunar Prospector Gamma Ray Spectrometer. We enhance the resolution via a pixon image reconstruction technique, and find that the thorium is distributed over a larger (40 km×75 km) area than the (25 km×35 km) high albedo region normally associated with Compton-Belkovich. Our reconstructions show that inside this region, the thorium concentration is 15 - 33 ppm.
We also find additional thorium, spread up to 300 km eastward of the complex at∼2 ppm. The thorium must have been deposited during the formation of the volcanic complex, because subsequent lateral transport mechanisms, such as small impacts, are unable to move sufficient material. The morphology of the feature is consistent with pyroclastic dispersal and we conclude that the present distribution of thorium was likely created by the explosive eruption of silicic magma.
11 pages, 6 figures, submitted to JGR-Planets
Earth and Planetary Astrophysics (astro-ph.EP)
arXiv:1409.1209 [astro-ph.EP] (or arXiv:1409.1209v1 [astro-ph.EP] for this version)
From: Jack Wilson [v1] Wed, 3 Sep 2014 19:58:13 GMT (3634kb,D)
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