Open Access
Table 1
Properties of the different populations of dust present in the model.
| Population | a | ξ | Dust-to-gas (cloud) | Processed dust fraction | Name |
|---|---|---|---|---|---|
| 1 | 1 µm | 3 g cm−3 | 1.5 × 10−3 | – | Solar nebula composition |
| 2 | 1 µm | 3 g cm−3 | 3.5 × 10−3 | – | Solar nebula composition |
| 3 | 1 µm | 3 g cm−3 | – | 89% | Refractory-depleted |
| 4 | 600 µm | 3 g cm−3 | – | 3% | Amoeboid Olivine Aggregates (AOAs) |
| 5 | 2500 µm | 3 g cm−3 | – | 8% | Ca-Al-Rich Inclusions (CAIs) |
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