Petrographic and chemical characterization of igneous lithic clasts from mesosiderites and howardites and comparison with eucrites and diogenites
- 1 December 1979
- journal article
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 43 (12) , 1917-1935
- https://doi.org/10.1016/0016-7037(79)90005-x
Abstract
No abstract availableKeywords
Funding Information
- National Aeronautics and Space Administration (NGR-05 007?)
This publication has 32 references indexed in Scilit:
- Olivine/liquid distribution coefficients and a test for crystal-liquid equilibriumPublished by Elsevier ,2002
- Electromagnetic heating of minor planets in the early solar systemIcarus, 1979
- Evaluation of a crust model of eucrites from the width of exsolved pyroxene.GEOCHEMICAL JOURNAL, 1977
- A classification of meteorites based on oxygen isotopesEarth and Planetary Science Letters, 1976
- THE MOAMA EUCRITE — A PYROXENE‐PLAGIOCLASE ADCUMULATEMeteoritics, 1975
- The distribution of Sr and REE between diopside and silicate liquidGeophysical Research Letters, 1974
- On the origin of eucrites and diogenitesEarth and Planetary Science Letters, 1973
- THE WASHOUGAL METEORITEMeteoritics, 1972
- Further evidence in support of the mixing model for howardite originEarth and Planetary Science Letters, 1972
- The composition of stony meteorites (X) The Ca/Al ratio in mesosideritesEarth and Planetary Science Letters, 1971