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Thorium crust/mantle ratios

Chondritic relative abundances of strongly incompatible RLEs (lanthanum, niobium, tantalum, uranium, thorium) and their ratios to compatible RLEs in the Earth s mantle are more difficult to test. The smooth and complementary patterns of REEs in the continental crust and the residual depleted mantle are consistent with a bulk REE pattern that is flat, i.e., unfractionated when normalized to chondritic abundances. As mentioned earlier, the isotopic compositions of neodymium and hafnium are consistent with chondritic Sm/Nd and Lu/Hf ratios for bulk Earth. Most authors, however, assume that RLEs occur in chondritic relative abundances in the Earth s mantle. However, the uncertainties of RLE ratios in Cl-meteorites do exceed 10% in some cases (see Table 4) and the uncertainties of the corresponding ratios in the Earth are in same range (Jochum et ai, 1989 W eyer et ai, 2002). Minor differences (even in the percent range) in RLE ratios between the Earth and chondritic meteorites cannot be excluded, with the apparent exception of Sm/Nd and Lu/Hf ratios (Blicher-Toft and Albarede, 1997). [Pg.726]


See other pages where Thorium crust/mantle ratios is mentioned: [Pg.717]    [Pg.13]    [Pg.318]    [Pg.771]    [Pg.797]    [Pg.1003]    [Pg.1004]    [Pg.1005]    [Pg.1206]    [Pg.1370]    [Pg.1614]    [Pg.1629]    [Pg.1791]    [Pg.1883]    [Pg.2213]    [Pg.94]    [Pg.302]    [Pg.303]    [Pg.304]   
See also in sourсe #XX -- [ Pg.171 ]




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