Тип публикации: статья из журнала
Год издания: 2017
Идентификатор DOI: 10.3847/1538-4357/aa9019
Ключевые слова: methods: numerical, planets and satellites: atmospheres, planets and satellites: individual (WASP-49b), techniques: spectroscopic
Аннотация: The strong, nearly wavelength-independent absorption cross section of aerosols produces featureless exoplanet transmission spectra, limiting our ability to characterize their atmospheres. Here, we show that even in the presence of featureless spectra, we can still characterize certain atmospheric properties. Specifically, we constrПоказать полностьюain the upper and lower pressure boundaries of aerosol layers, and present plausible composition candidates. We study the case of the bloated Saturn-mass planet WASP-49 b, where near-infrared observations reveal a flat transmission spectrum between 0.7 and 1.0 μm. First, we use a hydrodynamic upper-atmosphere code to estimate the pressure reached by the ionizing stellar high-energy photons at 10-8 bar, setting the upper pressure boundary where aerosols could exist. Then, we combine HELIOS and Pyrat Bay radiative-transfer models to constrain the temperature and photospheric pressure of atmospheric aerosols, in a Bayesian framework. For WASP-49 b, we constrain the transmission photosphere (hence, the aerosol deck boundaries) to pressures above 10-5 bar (100×solar metallicity), 10-4 bar (solar), and 10-3 bar (0.1×solar) as the lower boundary, and below 10-7 bar as the upper boundary. Lastly, we compare condensation curves of aerosol compounds with the planet's pressure-temperature profile to identify plausible condensates responsible for the absorption. Under these circumstances, we find these candidates: Na2S (at 100× solar metallicity); Cr and MnS (at solar and 0.1×solar); and forsterite, enstatite, and alabandite (at 0.1×solar).
Журнал: The Astrophysical Journal
Выпуск журнала: Т. 849, № 2
Номера страниц: 145
ISSN журнала: 0004637X
Издатель: Institute of Physics and IOP Publishing Limited