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Meteorites and their parent bodies: evidence from oxygen isotopes
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Clayton, R. N. |
| Copyright Year | 1978 |
| Description | Isotopic abundance variations among meteorites are used to establish genetic associations between meteorite classes. Oxygen isotope distributions between group II E irons with H-group ordinary chondrites and enstatic meteorites indicate that the parent bodies were formed out of pre-solar material that was not fully mixed at the time condensation occurred within the solar nebula. |
| File Size | 465577 |
| Page Count | 7 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19780021066 |
| Archival Resource Key | ark:/13960/t2m669m8x |
| Language | English |
| Publisher Date | 1978-01-01 |
| Access Restriction | Open |
| Subject Keyword | Lunar And Planetary Exploration Solar Corona Enstatite Planetary Evolution Meteoritic Composition Chondrites Iron Meteorites Chronology Solar System Oxygen Isotopes Isotopic Labeling Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
