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Table 4

Molecular abundances.

Molecule Name Abundance relative to water in %
67P in 2021 67P in 2015(a) Rosetta(b) in comets
HCN Hydrogen cyanide 0.09 ± 0.01 0.11 ± 0.02 0.2 0.08–0.25
HNC Hydrogen isocyanide <0.006 0.0015–0.035
HNCd < 0.009(c)
CH3CN Methyl cyanide 0.017 ± 0.003 <0.30 0.0059 0.008–0.054
HC3N Cyanoacetylene <0.019 0.0004 0.002–0.068
HNCO Isocyanic acid 0.045 ± 0.013 0.027 0.009–0.080
NH2CHO Formamide <0.033 0.004 0.016–0.022

CO Carbon monoxide <4.6 0.3–3 0.4–35
H2CO Formaldehyde 0.06 ± 0.01 <0.8 0.5
H2COd 0.28 ± 0.05(d) <1.5(d) 0.5 0.13- 1.4(d)
CH3OH Methanol 1.2 ± 0.1 2.1 ± 0.6 0.5–1.5 0.7–6.1
HCOOH Formic acid <0.21 0.013 0.03–0.18
CH3CHO Acetaldehyde <0.14 0.047 0.05–0.08

H2S Hydrogen sulphide 0.16 ± 0.03 < 2.0 2.0 0.09–1.5
CS Carbon monosulphide 0.05 ± 0.01 < 0.25 0.02(e) 0.05–0.20
OCS Carbonyl sulphide <0.54 0.07 0.05–0.40
SOd Sulphur monoxide <0.22(f) 0.071 0.04–0.30(f)
SO2 Sulphur dioxide <0.23 0.127 0.03–0.23
H2CS Thioformaldehyde <0.1 0.0027 0.009–0.090

Notes. (a)Based on IRAM data with molec s−1 (Biver et al. 2019). (b)Based on Biver et al. (2019), Rubin et al. (2019), and Läuter et al. (2020).(c) Assuming a daughter distribution with Lp = 1000 km (Cordiner et al. 2014, 2017).(d) Assuming a daughter distribution with Lp = 1.2–2.0 × Ld(H2CO). (e)From CS2 with ROSINA.(f) Assuming a daughter distribution with Lp = Ld(SO2).

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