Abstract
The observed 26Mg and 16O anomalies in meteorites can be consistently understood if a supernova occurred within a few million years of the condensation of the Solar System. Grains condensing in the ejecta from this supernova may be an integral aspect of this process.
| Original language | English |
|---|---|
| Pages (from-to) | 116-118 |
| Number of pages | 3 |
| Journal | Nature |
| Volume | 269 |
| Issue number | 5624 |
| DOIs | |
| State | Published - 1977 |
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