Terrestrial accretion rates and the origin of the Moon
- 1 February 2000
- journal article
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 176 (1) , 17-30
- https://doi.org/10.1016/s0012-821x(99)00317-9
Abstract
No abstract availableKeywords
This publication has 37 references indexed in Scilit:
- Formation, history and energetics of cores in the terrestrial planetsPublished by Elsevier ,2002
- 60025: relict of primitive lunar crust?Published by Elsevier ,2002
- Hf–W internal isochrons for ordinary chondrites and the initial 182Hf/180Hf of the solar systemPublished by Elsevier ,2000
- Cosmic-ray production of tungsten isotopes in lunar samples and meteorites and its implications for Hf–W cosmochemistryEarth and Planetary Science Letters, 2000
- Early evolution of the Earth and Moon: new constraints from Hf-W isotope geochemistryEarth and Planetary Science Letters, 1996
- Hafnium–tungsten chronometry and the timing of terrestrial core formationNature, 1995
- The origin of the moon and the single impact hypothesis IVIcarus, 1991
- Occurrence of Giant Impacts During the Growth of the Terrestrial PlanetsScience, 1985
- Models of the Earth's CoreScience, 1981
- Inhomogeneous accumulation of the earth from the primitive solar nebulaEarth and Planetary Science Letters, 1969