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Table 3

Inferred D/H in protoplanetary ices.

Model f H2 x H2 (D/H)ices

Uranusa 0.108 0.521 (6.75+1.1/–1.2) × 10-5
Neptune 1a 0.133 0.581 (6.7 ± 1.4) × 10-5
Neptune 2a 0.055 0.343 (5.1 ± 0.75) × 10-5

Uranus I (H2O)b 0.087 0.463 (6.25 ± 1.05) × 10-5
Uranus II (H2O)b 0.065 0.387 (5.75 ± 0.9) × 10-5
Neptune I (H2O)b 0.082 0.444 (5.58 ± 1) × 10-5
Neptune II (H2O)b 0.074 0.417 (5.42 ± 0.95) × 10-5

Uranus 1c 0.116 0.541 (6.94 ± 1.3) × 10-5
Uranus 2c 0.097 0.492 (6.48 ± 1.1) × 10-5
Neptune 1c 0.150 0.614 (7.04 ± 1.6) × 10-5
Neptune 2ac 0.178 0.661 (7.71 ± 1.9) × 10-5
Neptune 2bc 0.124 0.560 (6.46 ± 1.4) × 10-5

Notes.Models from and Volumetric ratio: xH2 = nH2 / (nH2 + nH2O). Mass ratio: fH2 = MH2 / (MH2 + Mice).

(a)

Podolak et al. (1995);

(b)

Helled et al. (2011);

(c)

Nettelmann et al. (2013).

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