Rapid Accretion and Early Differentiation of Mars Indicated by 142 Nd/ 144 Nd in SNC Meteorites
- 13 January 1995
- journal article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 267 (5195), 213-217
- https://doi.org/10.1126/science.7809625
Abstract
Small differences in the ratio of neodymium-142 to neodymium-144 in early formed mantle reservoirs in planetary bodies are the result of in situ decay of the extinct radionuclide samarium-146 and can be used to constrain early planetary differentiation and therefore the time scale of planetary accretion. The martian meteorite Nakhla (approximately 1.3 billion years old), the type sample of the nakhlite subgroup of the Shergottite-Nakhlite-Chassigny (SNC) meteorites, exhibits a 59 +/- 13 parts per million excess in the ratio of neodymium-142 to neodymium-144 relative to normal neodymium. This anomaly records differentiation in the martian mantle before 4539 million years ago and implies that Mars experienced no giant impacts at any time later than 27 million years after the origin of the solar system.Keywords
This publication has 41 references indexed in Scilit:
- Martian plate tectonicsJournal of Geophysical Research, 1994
- Evidence from coupled 147Sm–143Nd and 146Sm–142Nd systematics for very early (4.5-Gyr) differentiation of the Earth's mantleNature, 1992
- The random component of planetary rotationIcarus, 1991
- Accretional evolution of a planetesimal swarm: 1. A new simulationIcarus, 1991
- Rapid formation of Jupiter by diffusive redistribution of water vapor in the solar nebulaIcarus, 1988
- SNC meteorites: Clues to Martian petrologic evolution?Reviews of Geophysics, 1985
- Noble gas contents of shergottites and implications for the Martian origin of SNC meteoritesGeochimica et Cosmochimica Acta, 1984
- A new 1.3 aeon‐young achondriteGeophysical Research Letters, 1977
- Evidence for late formation and young metamorphism in the Achondrite NakhlaGeophysical Research Letters, 1974
- Thermal history of the nakhlites by the40Ar-39Ar methodEarth and Planetary Science Letters, 1973