Results 31 to 40 of about 71,492 (285)
Redox Hysteresis of Super-Earth Exoplanets from Magma Ocean Circulation [PDF]
Internal redox reactions may irreversibly alter the mantle composition and volatile inventory of terrestrial and super-Earth exoplanets and affect the prospects for atmospheric observations. The global efficacy of these mechanisms, however, hinges on the
T. Lichtenberg
semanticscholar +1 more source
Revisited mass-radius relations for exoplanets below 120 M⊕ [PDF]
The masses and radii of exoplanets are fundamental quantities needed for their characterisation. Studying the different populations of exoplanets is important for understanding the demographics of the different planetary types, which can then be linked ...
J. Otegi, F. Bouchy, R. Helled
semanticscholar +1 more source
Atmospheric regimes and trends on exoplanets and brown dwarfs [PDF]
A planetary atmosphere is the outer gas layer of a planet. Besides its scientific significance among the first and most accessible planetary layers observed from space, it is closely connected with planetary formation and evolution, surface and interior ...
Xi Zhang
semanticscholar +1 more source
Investigation of Kepler Objects of Interest Stellar Parameters from Observed Transit Durations [PDF]
The Kepler mission discovery of candidate transiting exoplanets (KOIs) enables a plethora of ensemble analysis of the architecture and properties of exoplanetary systems.
Bilinski, Christopher +2 more
core +2 more sources
VaTEST. II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars
NASA’s Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission designed to find transiting exoplanets orbiting nearby bright stars. It has identified more than 329 transiting exoplanets, and almost 6000 candidates remain unvalidated. In
Priyashkumar Mistry +50 more
doaj +1 more source
Exoplanets as Sub-GeV Dark Matter Detectors. [PDF]
We present exoplanets as new targets to discover dark matter (DM). Throughout the Milky Way, DM can scatter, become captured, deposit annihilation energy, and increase the heat flow within exoplanets.
R. K. Leane, J. Smirnov
semanticscholar +1 more source
The Transiting Exoplanet Survey Satellite (TESS) follow-up of a large number of known transiting exoplanets provides a unique opportunity to study their physical properties more precisely.
Suman Saha
doaj +1 more source
Core-powered mass-loss and the radius distribution of small exoplanets [PDF]
Recent observations identify a valley in the radius distribution of small exoplanets, with planets in the range $1.5-2.0\,{\rm R}_\oplus$ significantly less common than somewhat smaller or larger planets.
S. Ginzburg, H. Schlichting, R. Sari
semanticscholar +1 more source
Compositional Diversity of Rocky Exoplanets [PDF]
To test whether exoplanets are similar to Earth, knowledge of their host star composition is essential. Stellar elemental abundances and planetary orbital data show that of the ~5,000 known minerals, exoplanetary silicate mantles contain mostly olivine ...
K. Putirka +3 more
semanticscholar +1 more source
Sculpting the valley in the radius distribution of small exoplanets as a by-product of planet formation: the core-powered mass-loss mechanism. [PDF]
Recent observations revealed a bimodal radius distribution of small, short-period exoplanets with a paucity in their occurrence, a radius 'valley', around 1.5-2.0 R⊕.
Akash Gupta, H. Schlichting
semanticscholar +1 more source

