Detection of Aerosols at Microbar Pressures in an Exoplanet Atmosphere
| Autor: | Adriana Valio, Raissa Estrela, Mark R. Swain, Elyar Sedaghati, Gael M. Roudier, Robert A. West |
|---|---|
| Přispěvatelé: | National Aeronautics and Space Administration (US), Sao Paulo Research Foundation, California Institute of Technology, Ministerio de Economía y Competitividad (España), European Commission |
| Jazyk: | angličtina |
| Rok vydání: | 2021 |
| Předmět: |
Earth and Planetary Astrophysics (astro-ph.EP)
Physics Exoplanet atmospheres (487) Haze Microphysics Exoplanets (498) FOS: Physical sciences Astronomy and Astrophysics Astrophysics Transmission spectroscopy (2133) Exoplanet Aerosol Jupiter symbols.namesake Space and Planetary Science symbols Exoplanet atmospheric composition (2021) Astrophysics::Earth and Planetary Astrophysics Rayleigh scattering Wide Field Camera 3 Space Telescope Imaging Spectrograph Physics::Atmospheric and Oceanic Physics Astrophysics - Earth and Planetary Astrophysics |
| Zdroj: | Digital.CSIC. Repositorio Institucional del CSIC instname |
| Popis: | The formation of hazes at microbar pressures has been explored by theoretical models of exoplanet atmospheres to explain Rayleigh scattering and/or featureless transmission spectra; however observational evidence of aerosols in the low-pressure formation environments has proved elusive. Here, we show direct evidence of aerosols existing at ∼1 microbar pressures in the atmosphere of the warm sub-Saturn WASP-69b using observations taken with the Space Telescope Imaging Spectrograph and Wide Field Camera 3 instruments on the Hubble Space Telescope. The transmission spectrum shows a wavelength-dependent slope induced by aerosol scattering that covers 11 scale heights of spectral modulation. Drawing on the extensive studies of haze in our solar system, we model the transmission spectrum based on a scaled version of Jupiter's haze-density profile to show that the WASP-69b transmission spectrum can be produced by scattering from an approximately constant density of particles extending throughout the atmospheric column from 40 millibar to microbar pressures. These results are consistent with theoretical expectations based on microphysics of the aerosol particles that have suggested haze can exist at microbar pressures in exoplanet atmospheres. © 2021. The American Astronomical Society. All rights reserved. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. R.E. and M.S. acknowledge support for a portion of this effort from NASA ADAP award 907524. R.E. acknowledges the Sao Paulo Research Foundation for the fellowship #2018/09984-7. This work has been supported in part by the California Institute of Technology Jet Propulsion Laboratory Exoplanet Science Initiative. This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004; 2021). All rights reserved. With funding from the Spanish government through the Severo Ochoa Centre of Excellence accreditation SEV-2017-0709. |
| Databáze: | OpenAIRE |
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