Results 121 to 130 of about 15,442 (228)
EUCLID : Dark Universe Probe and Microlensing planet Hunter
There is a remarkable synergy between requirements for Dark Energy probes by cosmic shear measurements and planet hunting by microlensing. Employing weak and strong gravitational lensing to trace and detect the distribution of matter on cosmic and ...
Batista, V +15 more
core
Short-period sub-Neptunes are common in extrasolar systems. These sub-Neptunes are generally thought to have primary atmospheres of protoplanetary-disk gas origin.
Issei Kobayashi +3 more
doaj +1 more source
We present the JWST/NIRSpec G395H transmission spectrum of the young (10–30 Myr) transiting planet V1298 Tau b (9.85 ± 0.35 R _⊕ , T _eq = 670 K). Combined Hubble Space Telescope and JWST observations reveal a haze-free, H/He-dominated atmosphere with a
Saugata Barat +21 more
doaj +1 more source
The Structure of Jupiter, Saturn, and Exoplanets: Key Questions for High-Pressure Experiments [PDF]
Jonathan J. Fortney
openalex +1 more source
Impact of photochemical hazes on the thermal structure of exoplanet atmospheres
P. Lavvas, Anthony Arfaux
openalex +1 more source
Effects of a fully 3D atmospheric structure on exoplanet transmission spectra: retrieval biases due to day–night temperature gradients [PDF]
A. Caldas +6 more
openalex +1 more source
Next-Generation Improvements in Giant Exoplanet Evolutionary and Structural Models
20 pages, 11 figures, submitted to ...
Sur, Ankan +3 more
openaire +2 more sources
Stellar Spectroscopy during Exoplanet Transits: Dissecting fine structure across stellar surfaces
Differential spectroscopy during exoplanet transits permits to reconstruct spectra of small stellar surface portions that successively become hidden behind the planet. The center-to-limb behavior of stellar line shapes, asymmetries and wavelength shifts will enable detailed tests of 3-dimensional hydrodynamic models of stellar atmospheres, such that ...
Dravins, Dainis +3 more
openaire +2 more sources
The Uncertainty in Water Mass Fraction of Wet Planets
Planets with masses between Earth and Neptune often have radii that imply the presence of volatiles, suggesting that water may be abundant in their interiors.
Michael Lozovsky
doaj +1 more source
Surface Imaging of Proxima b and Other Exoplanets: Topography, Biosignatures, and Artificial Mega-Structures [PDF]
S. V. Berdyugina, J. R. Kuhn
openalex +1 more source

