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Combined analysis of thorium and fast neutron data at the lunar surface.

DE2001773347

Publication Date	2001
Personal Author	Gasnault, O.; Feldman, W.
Page Count	3
Abstract	The global distribution of the radioactive elements (U, K, Th) at the lunar surface is an important parameter for an understanding of lunar evolution, because they have provided continuous heat over the lifetime of the Moon. Today, only the thorium distribution is available for the whole lunar surface (1). Another key parameter that characterize the surface of the Moon is the presence of mare basalts. These basalts are concentrated on the nearside and are represented by materials with high-Fe content, sometimes associated with high-Ti. We demonstrated elsewhere that the fast neutron measurement made by Lunar Prospector is representative of the average soil atomic mass (2) is primarily dominated by Fe and Ti in basaltic terranes, and therefore the map of the fast neutrons provides a good delineation of mare basalts. We focus here on the correlated variations of thorium abundances and fast neutron fluxes averaged over areas of 360 km in diameter, in an attempt to provide a better understanding of the thorium emplacement on the surface of the Moon.
Keywords	Moon Soil chemistry Distribution Fast neutrons Thorium Iron Titanium
Source Agency	Technical Information Center Oak Ridge Tennessee
NTIS Subject Category	54A - Astrogeology
Corporate Authors	Los Alamos National Lab., NM.; Department of Energy, Washington, DC.
Document Type	Conference Proceedings
NTIS Issue Number	200125
Contract Number	W-7405-ENG-36

Combined analysis of thorium and fast neutron data at the lunar surface.

Combined analysis of thorium and fast neutron data at the lunar surface.
DE2001773347

Publication Date	2001
Personal Author	Gasnault, O.; Feldman, W.
Page Count	3
Abstract	The global distribution of the radioactive elements (U, K, Th) at the lunar surface is an important parameter for an understanding of lunar evolution, because they have provided continuous heat over the lifetime of the Moon. Today, only the thorium distribution is available for the whole lunar surface (1). Another key parameter that characterize the surface of the Moon is the presence of mare basalts. These basalts are concentrated on the nearside and are represented by materials with high-Fe content, sometimes associated with high-Ti. We demonstrated elsewhere that the fast neutron measurement made by Lunar Prospector is representative of the average soil atomic mass (2) is primarily dominated by Fe and Ti in basaltic terranes, and therefore the map of the fast neutrons provides a good delineation of mare basalts. We focus here on the correlated variations of thorium abundances and fast neutron fluxes averaged over areas of 360 km in diameter, in an attempt to provide a better understanding of the thorium emplacement on the surface of the Moon.
Keywords	Moon Soil chemistry Distribution Fast neutrons Thorium Iron Titanium
Source Agency	Technical Information Center Oak Ridge Tennessee
NTIS Subject Category	54A - Astrogeology
Corporate Authors	Los Alamos National Lab., NM.; Department of Energy, Washington, DC.
Document Type	Conference Proceedings
NTIS Issue Number	200125
Contract Number	W-7405-ENG-36