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. 2021 Oct 22;11:20894. doi: 10.1038/s41598-021-99240-w

Table 1.

List of key parameters for the model calculations.

C N H C/N C/H
BSE [μg/g-Earth] 42–730a,b,c 0.83–2.5a,b,c 44–450a,b,c 40 ± 8a,d 1.3 ± 0.3 a,e
CI chondrites [ppm] 20,000–50,000f 500–2,000f 4,700–10,500g 14.5 ± 2.5d 2–8h
CI model [ppm] 35,000 1,500 6,900 23 5
Enstatite chondrites [ppm] 2,000–7,000f 100–500f 90–600i 13.7± 12.1d
EC model [ppm] 4,000 250 400 16 10
Oxidised model
Si 1.6j,k 1.0l M98 modelm
Dimet/sil 500n,o 20p 6.5q
Intermediate model
Si 0.55o 5.0p M98modell
Dimet/sil 1000n,o 20p 6.5q
Reduced model
Si 0.22r 50l 5.0s
Dimet/sil 3,000n,o 20p 6.5q

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 Si (the units are (Pi/1MPa)1/2ppm for reduced SH and Pi/1MPappm for the others, where Pi is the partial pressure of each molecule i), and the partitioning coefficients Di 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.