Table 1.
C | N | H | C/N | C/H | |
---|---|---|---|---|---|
BSE [μg/g-Earth] | 42–730 | 0.83–2.5 | 44–450 | 40 ± 8 | 1.3 ± 0.3 |
CI chondrites [ppm] | 20,000–50,000 | 500–2,000 | 4,700–10,500 | 14.5 ± 2.5 | 2–8 |
CI model [ppm] | 35,000 | 1,500 | 6,900 | 23 | 5 |
Enstatite chondrites [ppm] | 2,000–7,000 | 100–500 | 90–600 | 13.7± 12.1 | |
EC model [ppm] | 4,000 | 250 | 400 | 16 | 10 |
Oxidised model | |||||
1.6 | 1.0 | M98 model | |||
500 | 20 | 6.5 | |||
Intermediate model | |||||
0.55 | 5.0 | M98 | |||
1000 | 20 | 6.5 | |||
Reduced model | |||||
0.22 | 50 | 5.0 | |||
3,000 | 20 | 6.5 |
Observational data and model reference values for the abundances of C, N, and H in the bulk silicate Earth (BSE) and chondrites (assumed as building blocks, CI chondrites and enstatite chondrites). We set CI chondritic model, solubilities (the units are for reduced and for the others, where is the partial pressure of each molecule ), and the partitioning coefficients under each redox state by following Hirschmann5. (a) Hirschmann5, (b) Marty4, (c) Hirschmann17, (d) Bergin et al.15, (e) Hirschmann and Dasgupta124, (f) Grady and Wright81, (g) Vacher et al.82, (h) Kerridge79, (i) Piani et al.84, (j) Stolper and Holloway123, (k) Pan et al.20, (l) Libourel et al.114, (m) Moore et al.19, (n) Chi et al.100, (o) Armstrong et al.101, (p) Roskosz et al.103, (q) Okuchi102, (r) Wetzel et al.112, (s) Hirschmann et al.67.