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- W3100290159 startingPage "L31" @default.
- W3100290159 abstract "Transmission spectroscopy of exoplanets is a tool to characterize rocky planets and explore their habitability. Using the Earth itself as a proxy, we model the atmospheric cross section as a function of wavelength, and show the effect of each atmospheric species, Rayleigh scattering, and refraction from 115 to 1000 nm. Clouds do not significantly affect this picture because refraction prevents the lowest 12.75 km of the atmosphere, in a transiting geometry for an Earth-Sun analog, to be sampled by a distant observer. We calculate the effective planetary radius for the primary eclipse spectrum of an Earth-like exoplanet around a Sun-like star. Below 200 nm, ultraviolet (UV) O2 absorption increases the effective planetary radius by about 180 km, versus 27 km at 760.3 nm, and 14 km in the near-infrared (NIR) due predominantly to refraction. This translates into a 2.6% change in effective planetary radius over the UV–NIR wavelength range, showing that the UV is an interesting wavelength range for future space missions." @default.
- W3100290159 created "2020-11-23" @default.
- W3100290159 creator A5027931079 @default.
- W3100290159 creator A5040297972 @default.
- W3100290159 date "2013-07-18" @default.
- W3100290159 modified "2023-10-18" @default.
- W3100290159 title "TRANSMISSION SPECTRUM OF EARTH AS A TRANSITING EXOPLANET FROM THE ULTRAVIOLET TO THE NEAR-INFRARED" @default.
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- W3100290159 doi "https://doi.org/10.1088/2041-8205/772/2/l31" @default.
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