Table 1
Gas composition results: detections and upper limits.
Species | Mult. factor(1) | Mixing ratio | Col. dens. (cm−2) |
---|---|---|---|
C2H6 | 1.05 ± 0.1 | (1.35 ± 0.15) × 10−5 at ![]() |
(1.05 ± 0.1) × 1017 |
C2H2 (LTE)(2) | N/A | (3.7 ± 0.2) × 10−6 at 32 km | (2.0 ± 0.12) × 1016 |
N/A | (5.8 ± 0.4) × 10−6 at 100 km | ||
N/A | (11.0 ± 0.8) × 10−6 at 200 km | ||
C2H2 (NLTE)(3) | 1.0 | 2.2 × 10−6 at 30 km | 3.7 × 1016 |
C2H4 | <4 | <3.4 × 10−7 at ![]() |
<4.6 × 1016 |
CH3C2H | 0.105 ± 0.01 | (4.6 ± 0.5) × 10−8 at ![]() |
(3.7 ± 0.4) × 1014 |
C3H8 | <0.2 | <1.2 × 10−6 at ![]() |
<4.5 × 1015 |
C4H2 | 0.22 ± 0.2 | (1.1 ± 0.1) × 10−8 at ![]() |
(2.1 ± 0.2) × 1013 |
C6H6 | <50 | <3.0 × 10−9 at ![]() |
<7.2 × 1014 |
CO2 | <500 | <1.3 × 10−9 at ![]() |
<8.4 × 1012 |
HCN | <2 | <9.3 × 10−9 at ![]() |
<3.1 × 1014 |
HC3N | <2 | <3.6 × 10−9 at ![]() |
<3.0 × 1013 |
Notes. (1)Multiplicative factor from the Lavvas et al. (2021) model. For undetected species, “<f” indicates that the MIRI data are consistent with at most f times the Lavvas et al. (2021) model. (2)Slope profile. See text for details. (3)Fixed abundance profile. See text for details.
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