Results 161 to 170 of about 700,042 (263)
LIGHT SCATTERING FROM EXOPLANET OCEANS AND ATMOSPHERES [PDF]
Michael E. Zugger+4 more
openalex +1 more source
JWST-TST DREAMS: Nonuniform Dayside Emission for WASP-17b from MIRI/LRS
We present the first spectroscopic characterization of the dayside atmosphere of WASP-17b in the mid-infrared using a single JWST MIRI/LRS eclipse observation.
Daniel Valentine+25 more
doaj +1 more source
The upper atmosphere of the exoplanet HD209458b revealed by the sodium D lines: temperature-pressure profile, ionization layer and thermosphere (Corrigendum) [PDF]
A. Vidal‐Madjar+9 more
openalex +1 more source
The Atmospheric Evolution of Small, Close-In Exoplanets
Submitted in part fulfilment of the requirements for the degree of Doctor of Philosophy at Imperial College London, July 2022.
openaire +4 more sources
Although Neptunian-sized (2–5 R _⊕ ) planets appear to be extremely common in the Galaxy, many mysteries remain about their overall nature. To date, only 11 Neptunian-sized planets have had their atmospheres spectroscopically characterized, and these ...
Matthew M. Murphy+3 more
doaj +1 more source
Transient conditions for biogenesis on low-mass exoplanets with escaping hydrogen atmospheres [PDF]
Robin Wordsworth
openalex +1 more source
ExoMol: molecular line lists for exoplanet and other atmospheres [PDF]
S. N. Yurchenko, Jonathan Tennyson
openalex +1 more source
Tropical Cyclones on Tidally Locked Rocky Planets: Dependence on Rotation Period
Tropical cyclones occur over the Earth’s tropical oceans, with characteristic genesis regions and tracks tied to the warm ocean surface that provide energy to sustain these storms.
Valeria Garcia+3 more
doaj +1 more source
Minimizing Star-spot Contamination of Exoplanet Transit Spectroscopy Using Alternate Normalization
Recently, M. H. Currie et al. (2023) simulated the detection of molecules in the atmospheres of temperate rocky exoplanets transiting nearby M-dwarf stars.
Drake Deming+3 more
doaj +1 more source
The recent discovery of “ultrahot” ( P < 1 day) Neptunes has come as a surprise: some of these planets have managed to retain gaseous envelopes despite being close enough to their host stars to trigger strong photoevaporation and/or Roche lobe overflow ...
Shreyas Vissapragada+18 more
doaj +1 more source