Abstract
Hydrogen, carbon, nitrogen, and oxygen isotopic compositions are heterogeneous among comet 81P/Wild 2 particle fragments; however, extreme isotopic anomalies are rare, indicating that the comet is not a pristine aggregate of presolar materials. Nonterrestrial nitrogen and neon isotope ratios suggest that indigenous organic matter and highly volatile materials were successfully collected. Except for a single 17O-enriched circumstellar stardust grain, silicate and oxide minerals have oxygen isotopic compositions consistent with solar system origin. One refractory grain is 16O-enriched, like refractory inclusions in meteorites, suggesting that Wild 2 contains material formed at high temperature in the inner solar system and transported to the Kuiper belt before comet accretion.
| Original language | English |
|---|---|
| Pages (from-to) | 1724-1728 |
| Number of pages | 5 |
| Journal | Science |
| Volume | 314 |
| Issue number | 5806 |
| DOIs | |
| Publication status | Published - 15 Dec 2006 |
| Externally published | Yes |