Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth

Earth and Planetary Science Letters

Volumn 312, Issue 3-4, 2011, Pages 390-400

  Burkhardt, Christoph ^a   Kleine, Thorsten ^a,b   Oberli, Felix ^a   Pack, Andreas ^c   Bourdon, Bernard ^a,d   Wieler, Rainer ^a  

^a ETH ZURICH   (Switzerland)

^b UNIVERSITY OF MÜNSTER   (Germany)

^c UNIVERSITY OF GÖTTINGEN   (Germany)

^d UNIVERSITÉ DE LYON   (France)

Author keywords

Earth composition; Meteorites; Mo isotopes; Nucleosynthesis; Solar nebula

Indexed keywords

CA-AL-RICH INCLUSIONS; CARBONACEOUS CHONDRITES; COMPOSITION OF THE EARTH; COVARIATION; DIVERSE MATERIALS; EARLY DIFFERENTIATION; HIGH PRECISION; ISOTOPE VARIATION; ISOTOPIC COMPOSITION; ISOTOPIC DATA; ISOTOPIC HOMOGENEITY; MARTIAN METEORITES; MOLYBDENUM ISOTOPES; NUCLEOSYNTHESIS; ORIGIN OF THE EARTH; OUTER SOLAR SYSTEM; PARENT BODIES; R-PROCESS; S-PROCESS; S-PROCESS CARRIER; SOLAR NEBULA; TERRESTRIAL PLANETS; TIME-SCALES;

ALUMINUM; EARTH (PLANET); HAFNIUM; ISOTOPES; MOLYBDENUM; NEODYMIUM; OSMIUM; PLANETS;

METEORITES;

CARBONACEOUS CHONDRITE; CORRELATION; EFFICIENCY MEASUREMENT; ISOTOPIC ANALYSIS; ISOTOPIC COMPOSITION; MARS; METEORITE; MOLYBDENUM; OXYGEN ISOTOPE; PARENT BODY; PLANETARY EVOLUTION;

EID: 81355149338     PISSN: 0012821X     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.epsl.2011.10.010     Document Type: Article

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