The Lu–Hf and Sm–Nd isotopic composition of CHUR: Constraints from unequilibrated chondrites and implications for the bulk composition of terrestrial planets

By A. Bouvier, J. Vervoort, P. Patchett. 2008

2,862 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/433d471c611cac2bf717636303834b240c4184a3

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. T. O. S. University
2. Research School of Earth Sciences
3. D. Geology
4. T. Yoshizaki
5. William F. McDonough Department of Earth Science
6. Japan.
7. College Park
8. Usa

In Geophysics

1. T. O. S. University
2. Research School of Earth Sciences
3. D. Geology
4. T. Yoshizaki
5. William F. McDonough Department of Earth Science
6. Japan.
7. College Park
8. Usa

In Nuclear and High Energy Physics

1. T. O. S. University
2. Usa

Citations in the corpus

• The composition of Mars (2019, background): “n and their relative abundances show limited variation (generally <10%) among chondritic meteorites (e.g., Masuda, 1957; Coryell et al., 1963; Larimer and Wasson, 1988; Wasson and Kallemeyn, 1988; Bouvier et al., 2008b). Thus, if you establish the absolute concentration of one RLE, you can calcul”