Table 5

Rel. abundance of sulfur-bearing species with respect to water in [%].

Comet H2S OCS SO SO2 CS CS2 S2

1P/Halley 0.4[1] 0.2[2]
C/1995 O1 (Hale-Bopp) 1.5[3] 0.4[3] 0.3[3,4] 0.2[3] 0.1[6] 0.17[3] 0.02[5]
C/1996 B2 (Hyakutake) 0.8[7] 0.1[8] 0.1[6] 0.1[7] 0.01[9]
C/2001 A2 (LINEAR) 1.15[10] 0.07[10]
73P/SW3/B 0.2–0.4[11] 0.12–0.19[11]
73P/ SW3/C 0.16–0.3[11] 0.08–0.14[11]
9P/Tempel 1 before impact 0.5[12] <0.13[12]
67P summer hemisphere 0.67[13] 0.017[13] 0.004[13] 0.011[13] a) 0.003[13] 0.0004[13]
67P winter hemisphere 1.75[13] 0.098[13] 0.0014[13] 0.041[13] a) 0.024[13] 0.0013[13]

Notes. This table is based on Table 1 in Bockelée-Morvan et al. (2004), on Table 4 in Mumma & Charnley (2011) and on Table 3 in Radeva et al. (2013). References. [1] Eberhardt et al. (1994); [2] Feldman et al. (1987); [3] Bockelée-Morvan et al. (2000); [4] Lis et al. (1997b); [5] Despois et al. (2005); [6] Charnley & Rodgers (2008); [7] Biver et al. (1999); [8] Woodney et al. (1997); [9] Weaver et al. (1996); [10] Biver et al. (2006) (values at 1.1 AU); [11] Biver et al. (2008); [12] Biver et al. (2007); [13] this work; comments: a) CS cannot be resolved from CO2 by ROSINA.

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