日本地球惑星科学連合2022年大会

講演情報

[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-AE 天文学・太陽系外天体

[P-AE17] 系外惑星

2022年5月26日(木) 10:45 〜 12:15 105 (幕張メッセ国際会議場)

コンビーナ:生駒 大洋(国立天文台 科学研究部)、コンビーナ:成田 憲保(東京大学)、藤井 友香(国立天文台)、座長:藤井 友香(国立天文台)

11:15 〜 11:30

[PAE17-03] Unveiling non-gray surface of cloudy exoplanets: the influence of wavelength-dependent surface albedo and cloud scattering properties on retrieval solutions

*Fei Wang1,2,3Yuka Fujii4,5Jinping He1,2 (1.National Astronomical Observatory of China / Nanjing Institute of Astronomical Optics and Technology、2.CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing, 210042, China.、3. University of Chinese Academy of Sciences, Beijing, 100049,China、4.Division of Science, National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan.、5.Earth-Life Science Institute, Tokyo Institute of Technology, Ookayama, Meguro, Tokyo 152-8550, Japan.)

キーワード:Exoplanet, Direct imaging, Bayesian statistics

Direct-imaging spectra hold rich information about a planet's atmosphere and surface, and several space-based missions aiming at such observations will become a reality in the near future. Previous spectral retrieval works have resulted in key atmospheric constraints under the assumption of a gray surface, but the effect of wavelength-dependent surface albedo on retrieval has not been shown. We explore the influence of the coupling effect of cloud and wavelength-dependent surface albedo on retrieval performance via modeling suites of Earth-like atmospheres with varying cloud and surface albedo parameterizations. We show that the retrieval degeneracy between the cloud properties and wavelength-dependent surface albedo leads to biased results of atmospheric composition and cloud properties. The multi-epoch visible band observations offer limited improvement in disentangling this degeneracy. However, the constraints on atmospheric composition from the combination of UV band (R ∼ 6) + visible band (R ∼ 140) are consistent with input values to within 1 σ. If short bandpass data is lacking, an alternative solution to reduce the retrieval uncertainties would be to have the prior constraints on planetary cloud fraction with less than 20% uncertainty. Under the assumption of known cloud scattering properties, the retrieved surface spectral albedos also show promising constraints on the surface composition when the surface cover is Earth-like vegetated areas or the ocean, which may aid in characterizing the planet's habitability.