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Table 4

Likely partition of carbon in the diffuse ISM dust phases.

Carbon phase Abundance
Primitive meteorites [%]

Organic matter 3–4

Pre-solar grains [ppm]

Nano-diamonds 1400 ≡ 0.14%
SiC 50
Graphite 10

Diffuse ISM abundances
[ppm and % of C in dust]

a-C:H ≳60 ppm ≡  ≳19%
a-C ~150 ppm ≡  ~49%
Nano-diamonds ≲20 ppm ≡  ≲7%
C in SiC ≲25 ppm ≡  ≲8%
Graphite ≲10 ppm ≡  ≲3%
Aromatic-rich a-C ≤5 ppm ≡  <14%

Notes. These estimates of carbon in carbon-bearing dust phases in the diffuse ISM are based upon primitive meteorite abundances, the pre-solar grains extracted from primitive meteorites and THEMIS.

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