SO2, silicate clouds, but no CH4 detected in a warm Neptune.
SO2, silicate clouds, but no CH4 detected in a warm Neptune.
复制标题
SO2、硅酸盐云,但在温暖的海王星中未检测到 CH4。
DOI:
10.1038/s41586-023-06849-0
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发表时间:
2024
期刊:
影响因子:
64.8
通讯作者:
Dyrek A
中科院分区:
文献类型:
--
作者:
Dyrek A
WASP-107b is a warm (∼ 740K) transiting planet with a Neptune-like mass of∼ 30.5 M⊕ and Jupiter-like radius of∼ 0.94 RJ 1, 2 whose extended atmosphere is eroding 3. Previous observations showed evidence for water vapour and a thick high-altitude condensate layer in WASP-107b’s atmosphere 4, 5. Recently, photochemically produced sulphur dioxide (SO2) was detected in the atmosphere of a hot (∼ 1,200 K) Saturn-mass planet from transmission spectroscopy near 4.05 µm 6, 7, but for temperatures below∼ 1,000 K sulphur is predicted to preferably form sulphur allotropes instead of SO2 8–10. Here we report the 9σ-detection of two fundamental vibration bands of SO2, at 7.35 µm and 8.69 µm, in the transmission spectrum of WASP-107b using the Mid-Infrared Instrument (MIRI) of the JWST. This discovery establishes WASP-107b as the second irradiated exoplanet with confirmed photochemistry, extending the temperature range of exoplanets exhibiting detected photochemistry from∼ 1,200 K down to∼ 740 K. Additionally, our spectral analysis reveals the presence of silicate clouds, which are strongly favoured (∼ 7σ) over simpler cloud setups. Furthermore, water is detected (∼ 12σ), but methane is not. These findings provide evidence of disequilibrium chemistry and indicate a dynamically active atmosphere with a super-solar metallicity.