From: Bubbles to Chondrites-II. Chemical fractionations in chondrites
# | Material or Source | D/H ratio | Reference |
---|---|---|---|
 |  | ×10−4 |  |
1 | Local interstellar medium (gas) | 0.15 ±0.01 | |
2 | ProtoSolar | 0.21 ±0.05 | |
3 | Saturn (atmosphere) | 0.21 ±0.013 | |
4 | Jupiter (atmosphere) | 0.295 ±0.055 | |
5 | Uranus (atmosphere) | 0.44 ±0.04 | |
6 | Neptune (atmosphere) | 0.41 ±0.04 | |
7 | Tagish lake-11i | 0.164-1.14 | |
8 | CV | ≤0.820 | |
9 | CI | 0.643-0.976 | |
10 | CM | 0.865 ±0.036 | |
11 | CO | 0.849-1.32 | |
12 | CR | 1.71\(^{+0.17}_{-0.1}\) | |
13 | O | 2.8-3.44 | |
14 | R | 7.26 ±0.13 | |
15 | Earth Bulk | 1.49 ±0.03 | |
16 | Comet 103P/Hartley 2 | 1.61 ±0.24 | |
17 | Comet 45P/Honda-Mrkos-Pajdušáková | ≤2 | |
18 | Comet 67P/Churymov-Gerasimenko | 5.3 ±0.7 | |
19 | Comet C/2009 P1 (Garradd) | 2.06 ±0.22 | |
20 | Comet 153P/Ikeya-Zhang | ≤2.5 | |
21 | Comet C/2002 T7 (Linear) | 2.5 ±0.7 | |
22 | Comet C/1996 B2 Hyakutake | 2.9 ±0.1 | |
23 | Comet C/1995 O1 Hale-Bopp | 3.3 ±0.8 | |
24 | Comet P/Halley | 3.16 ±0.34 | |
25 | Comet 8P/Tuttle | 4.09 ±1.45 | |
26 | NGC 1333 IRAS4B (Inner) | 5.9 ±1.7 | |
27 | NGC 1333 IRAS4B (Inner) | 1-37 | |
28 | NGC 1333 IRAS4A (Inner) | 10 | |
29 | NGC 1333 IRAS4A (Inner) | 4-30 | |
29 | NGC 1333 IRAS4A (Outer) | ≈100 | |
30 | NGC 1333 IRAS4A (Inner) | 19.1 ±5.4 | |
31 | NGC 1333 IRAS4A (Inner) | 50-300 | |
32 | IRAS2A (Inner) | 7.4 ±2.1 | |
33 | IRAS2A (Inner) | ≥100 | |
33 | IRAS2A (Outer) | 900-1800 | |
34 | IRAS2A (Inner) | 30-800 | |
35 | IRAS 16293-2422 (Inner) | 9.2 ±2.6 | |
36 | IRAS 16293-2422 (Inner) | 300 | |
36 | IRAS 16293-2422 (Outer) | ≤20 | |
37 | IRAS 16293-2422 (Inner) | 140-580 | |
37 | IRAS 16293-2422 (Outer) | 20-220 |