Author/Authors :
Ballhaus، نويسنده , , Chris and Laurenz، نويسنده , , Vera and Münker، نويسنده , , Carsten and Fonseca، نويسنده , , Raْl O.C. and Albarède، نويسنده , , Francis and Rohrbach، نويسنده , , Arno and Lagos، نويسنده , , Markus and Schmidt، نويسنده , , Max W. and Jochum، نويسنده , , Klaus Peter and Stoll، نويسنده , , Brigitte and Weis، نويسنده , , Ulrike and Helmy، نويسنده , , Hassan M.، نويسنده ,
Abstract :
The 238U/204Pb ratio of the Earthʹs mantle is conventionally seen as reflecting the loss of lead to the Earthʹs core, implying that this element is siderophile. A contrasting view holds that lead may be depleted because it did not fully condense at the accretion temperatures of the early Earth. Experiments reported here show that lead is indeed quite siderophile at high temperature. At the same time, it is noted that no plausible set of physical conditions exists where the present-day abundances of all moderately volatile elements of the mantle could have been in chemical equilibrium with a metallic iron melt. It is argued that a large proportion of the moderately volatile elements, including Pb, were added late, during the waning stages of core formation. In consequence, caution is advised in using the 238U/204Pb and the Pb isotope ratios of the mantle to date the differentiation of the Earth in silicate mantle and metallic core (Hofmann, 2001).
Keywords :
core formation , late addition , Volatile elements , Earthיs accretion , U/Pb