Universität zu Köln

Cubillos, Patricio E., Fossati, Luca ORCID: 0000-0003-4426-9530, Erkaev, Nikolai V., Malik, Matej, Tokano, Tetsuya, Lendl, Monika, Johnstone, Colin P., Lammer, Helmut and Wyttenbach, Aurelien ORCID: 0000-0001-9003-7699 (2017). Aerosol Constraints on the Atmosphere of the Hot Saturn-mass Planet WASP-49b. Astrophys. J., 849 (2). BRISTOL: IOP PUBLISHING LTD. ISSN 1538-4357

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Abstract

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 constrain 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 mu m. 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 (100x solar metallicity), 10(-4) bar (solar), and 10(-3) bar (0.1x 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 100x solar metallicity); Cr and MnS (at solar and 0.1x solar); and forsterite, enstatite, and alabandite (at 0.1x solar).

Item Type:	Journal Article
Creators:	Creators Email ORCID ORCID Put Code Cubillos, Patricio E. UNSPECIFIED UNSPECIFIED UNSPECIFIED Fossati, Luca UNSPECIFIED orcid.org/0000-0003-4426-9530 UNSPECIFIED Erkaev, Nikolai V. UNSPECIFIED UNSPECIFIED UNSPECIFIED Malik, Matej UNSPECIFIED UNSPECIFIED UNSPECIFIED Tokano, Tetsuya UNSPECIFIED UNSPECIFIED UNSPECIFIED Lendl, Monika UNSPECIFIED UNSPECIFIED UNSPECIFIED Johnstone, Colin P. UNSPECIFIED UNSPECIFIED UNSPECIFIED Lammer, Helmut UNSPECIFIED UNSPECIFIED UNSPECIFIED Wyttenbach, Aurelien UNSPECIFIED orcid.org/0000-0001-9003-7699 UNSPECIFIED
URN:	urn:nbn:de:hbz:38-211326
DOI:	10.3847/1538-4357/aa9019
Journal or Publication Title:	Astrophys. J.
Volume:	849
Number:	2
Date:	2017
Publisher:	IOP PUBLISHING LTD
Place of Publication:	BRISTOL
ISSN:	1538-4357
Language:	English
Faculty:	Unspecified
Divisions:	Unspecified
Subjects:	no entry
Uncontrolled Keywords:	Keywords Language COLLISION-INDUCED ABSORPTION; INDUCED INFRARED-SPECTRA; GIANT PLANETS; BROWN DWARFS; H-2-HE PAIRS; TRANSMISSION SPECTRUM; TEMPERATURES; EXOPLANETS; CHEMISTRY; DATABASE Multiple languages Astronomy & Astrophysics Multiple languages
Refereed:	Yes
URI:	http://kups.ub.uni-koeln.de/id/eprint/21132