Cosmogenic neon from individual grains of CM meteorites: Extremely long pre-compaction exposure histories or an enhanced early particle flux
- 31 July 1990
- journal article
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 54 (7) , 2133-2140
- https://doi.org/10.1016/0016-7037(90)90276-q
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Soft X-ray observations of pre-main-sequence stars in the Chamaeleon dark cloudThe Astrophysical Journal, 1989
- Evidence in meteorites for an active early sunThe Astrophysical Journal, 1987
- Early Solar System aqueous activity: Sr isotope evidence from the Orgueil CI meteoriteNature, 1984
- Regoliths on Small Bodies in the Solar SystemAnnual Review of Earth and Planetary Sciences, 1982
- Asteroidal regolithsIcarus, 1979
- The reaction Mg(n,α)Ne at 14.1 and 14.7 MeV: cross sections and implications for meteoritesEarth and Planetary Science Letters, 1979
- Argon 40-argon 39 chronology of lithic clasts from the Kapoeta howarditeGeochimica et Cosmochimica Acta, 1979
- Formation chronology for C2 meteoritesEarth and Planetary Science Letters, 1976
- Do stony meteorites come from comets?Icarus, 1975
- The records of solar wind and solar flares in aubritesEarth and Planetary Science Letters, 1974