Zn and Cu isotopic variations in chondrites and iron meteorites: Early solar nebula reservoirs and parent-body processes

By J. Luck, D. Othman, F. Albarède. 2005

210 citations recorded by the source corpus.

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

View Paper: https://www.semanticscholar.org/paper/81277d6c9b58d6fd05a2c697604b4ed92689dbbf

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. C. Burkhardt
2. T. Kleine
3. B. Bourdon
4. R. Hin
5. E. Pringle
6. F. Moynier
7. N. Dauphas
8. A. Morbidelli

In Ecology

1. B. Bourdon
2. T. Kleine
3. E. Pringle
4. C. Burkhardt
5. F. Moynier

Citations in the corpus

• Evidence for Mo isotope fractionation in the solar nebula and during planetary differentiation (2014, background): “Mass-dependent isotope variations among meteorites and their components have been reported for a variety of elements, including S (Gao and Thiemens, 1993), Zn, Cu, and Ni (Luck et al., 2005; Moynier et al., 2006), Cd (Wombacher et al.”
• Isotopic fractionation and transport mechanisms of Zn in plants (2009, unknown): “, 2006) and some meteorites (Luck et al., 2005; Moynier et al., 2007).”
• Rubidium isotopic composition of the Earth, meteorites, and the Moon: Evidence for the origin of volatile loss during planetary accretion (2017, background): “This relationship for Zn indicates that the volatile element abundance variations in CC are not due to evaporation or condensation, but rather are due to the mixing of chemically and isotopically distinct primordial reservoirs consisting of refractory component and a volatile-rich (CI-like) componen”