Elemental abundances and minimum mass of heavy elements in the envelope of HD 189733b

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Table 2:

Elemental and molecular abundances in the protoplanetary disk.
Species X	X/H₂	Species X	X/H₂
C	$5.82 \times 10^{-4}$	CO₂	$7.01 \times 10^{-5}$
N	$1.60 \times 10^{-4}$	CH₃OH	$1.40 \times 10^{-5}$
O	$1.16 \times 10^{-3}$	CH₄	$7.01 \times 10^{-6}$
S	$3.66 \times 10^{-5}$	NH₃	$5.33 \times 10^{-5}$
P	$6.88 \times 10^{-7}$	N₂	$5.33 \times 10^{-5}$
H₂O	$5.15 \times 10^{-4}$	H₂S	$1.83 \times 10^{-5}$
CO	$4.91 \times 10^{-4}$	PH₃	$6.88 \times 10^{-7}$

Elemental abundances derive from Lodders (2003). Molecular abundances are determined from our nominal gas phase composition.

Source LaTeX | All tables | In the text

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