Atmospheres of rocky exoplanets
R Wordsworth, L Kreidberg - Annual Review of Astronomy and …, 2022 - annualreviews.org
Rocky planets are common around other stars, but their atmospheric properties remain
largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming …
largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming …
Exoplanet biosignatures: understanding oxygen as a biosignature in the context of its environment
We describe how environmental context can help determine whether oxygen (O2) detected
in extrasolar planetary observations is more likely to have a biological source. Here we …
in extrasolar planetary observations is more likely to have a biological source. Here we …
Observing the atmospheres of known temperate Earth-sized planets with JWST
CV Morley, L Kreidberg, Z Rustamkulov… - The Astrophysical …, 2017 - iopscience.iop.org
Nine transiting Earth-sized planets have recently been discovered around nearby late-M
dwarfs, including the TRAPPIST-1 planets and two planets discovered by the MEarth survey …
dwarfs, including the TRAPPIST-1 planets and two planets discovered by the MEarth survey …
Evolved climates and observational discriminants for the TRAPPIST-1 planetary system
The TRAPPIST-1 planetary system provides an unprecedented opportunity to study
terrestrial exoplanet evolution with the James Webb Space Telescope (JWST) and ground …
terrestrial exoplanet evolution with the James Webb Space Telescope (JWST) and ground …
Potential Atmospheric Compositions of TRAPPIST-1 c Constrained by JWST/MIRI Observations at 15 μm
Abstract The first James Webb Space Telescope observations of TRAPPIST-1 c showed a
secondary eclipse depth of 421±94 ppm at 15 μm, which is consistent with a bare rock …
secondary eclipse depth of 421±94 ppm at 15 μm, which is consistent with a bare rock …
The habitability of Proxima Centauri b: environmental states and observational discriminants
Proxima Centauri b provides an unprecedented opportunity to understand the evolution and
nature of terrestrial planets orbiting M dwarfs. Although Proxima Cen b orbits within its star's …
nature of terrestrial planets orbiting M dwarfs. Although Proxima Cen b orbits within its star's …
Medium-resolution integral-field spectroscopy for high-contrast exoplanet imaging-Molecule maps of the β Pictoris system with SINFONI
Context. Angular differential imaging (ADI) and spectral differential imaging (SDI) are well-
established high-contrast imaging techniques, but their application is challenging for …
established high-contrast imaging techniques, but their application is challenging for …
Detecting ocean glint on exoplanets using multiphase map**
Rotational map** and specular reflection (glint) are two proposed methods to directly
detect liquid water on the surface of habitable exoplanets. However, false positives for both …
detect liquid water on the surface of habitable exoplanets. However, false positives for both …
Radio signatures of star–planet interactions, exoplanets and space weather
Radio detections of stellar systems provide a window onto stellar magnetic activity and the
space weather conditions of extrasolar planets—information that is difficult to obtain at other …
space weather conditions of extrasolar planets—information that is difficult to obtain at other …
MOVES–IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b
Hot Jupiters provide valuable natural laboratories for studying potential contributions of high-
energy radiation to pre-biotic synthesis in the atmospheres of exoplanets. In this fourth paper …
energy radiation to pre-biotic synthesis in the atmospheres of exoplanets. In this fourth paper …