Abstract
New, high-precision W isotope data on iron meteorites are presented that provide important constraints on the timing of silicate-metal segregation in planetesimals. Magmatic iron meteorites all have ε
| Original language | English |
|---|---|
| Pages (from-to) | 530-542 |
| Journal | Earth and Planetary Science Letters |
| Volume | 241 |
| DOIs | |
| Publication status | Published - 2005 |
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