Results 131 to 140 of about 908,915 (272)
ACCRETION OF ROCKY PLANETS BY HOT JUPITERS [PDF]
The Astrophysical Journal, 2011 The observed population of Hot Jupiters displays a stunning variety of physical properties, including a wide range of densities and core sizes for a given planetary mass. Motivated by the observational sample, this paper studies the accretion of rocky planets by Hot Jupiters, after the Jovian planets have finished their principal migration epoch and ...
Ketchum, Jacob A. +2 more
openaire +4 more sources
Ocean Worlds Maintained by Ocean Tidal Heat Expected on Several Uranian Moons
Geophysical Research Letters, Volume 52, Issue 20, 28 October 2025.Abstract In recent NASA decadal surveys, detecting oceans among Uranus' moons has been identified as a research priority in future missions. Currently, the prevailing view in planetary science is that the likelihood of finding oceans is highest on the larger moons, Titania and Oberon, due to their higher integrals of radiogenic heat sources. This study
Robert H. Tyler
wiley +1 more source
The Heating Efficiency of Hot Jupiters from a Data-driven Perspective
The Astronomical JournalThe inflated radii of hot Jupiters have been explored by various theoretical mechanisms. By connecting planetary thermal evolution models with the observed properties of hot Jupiters using hierarchical Bayesian models, a theoretical parameter called the ...
Sheng Jin +3 more
doaj +1 more source
Hot Jupiter secondary eclipses measured by Kepler
EPJ Web of Conferences, 2011 Hot-Jupiters are known to be dark in visible bandpasses, mainly because of the alkali metal absorption features. The outstanding quality of the Kepler mission photometry allows a detection (or non-detection upper limits on) giant planet secondary ...
Seager S., Demory B.-O.
doaj +1 more source
ATMOSPHERIC ESCAPE FROM HOT JUPITERS [PDF]
The Astrophysical Journal, 2009 Accepted for publication in ApJ, 22 pages, 24 figures. Added additional references--in particular, we now discuss charge-exchange as a potential source of high-velocity ...
Ruth Murray-Clay +3 more
openaire +4 more sources
Geophysical Research Letters, Volume 52, Issue 20, 28 October 2025.Abstract The outward transport of plasma and magnetic fluxes in the gas giant magnetospheres is balanced with a return flow of flux tubes emptied through magnetic reconnection. Evidence of interchange motions between inward and outward moving flux tubes have long been reported around Jupiter and Saturn.
M. Devinat +20 more
wiley +1 more source
RADIATION HYDRODYNAMICS OF HOT JUPITER ATMOSPHERES [PDF]
The Astrophysical Journal, 2010 25 pages, 4 figures, accepted for publication in ApJ (minor revisions)
Emily Rauscher, Kristen Menou
openaire +3 more sources
Prospects from TESS and Gaia to Constrain the Flatness of Planetary Systems
The Astronomical Journal, 2023 The mutual inclination between planets orbiting the same star provides key information to understand the formation and evolution of multiplanet systems.
Juan I. Espinoza-Retamal +2 more
doaj +1 more source
New avenues for thermal inversions in atmospheres of hot Jupiters [PDF]
Monthly notices of the Royal Astronomical Society, 2019 Thermal emission spectra of hot Jupiters have led to key constraints on thermal inversions (or 'stratospheres') in their atmospheres with important implications for their atmospheric processes.
S. Gandhi, N. Madhusudhan
semanticscholar +1 more source
Process Enhancement of Calcium Looping through Combined Mechanical and Chemical Sorbent Reactivation
ChemSusChem, Volume 18, Issue 19, October 1, 2025.Remilling—mechanical and chemical reactivation via wet milling after each cycle in the calcium looping process—boosts CO2 capture by 2–3 times, enhances sorbent properties, and reduces deactivation and replacement rates, as confirmed by physicochemical characterization and supported by a semiempirical model.
Dominik Groh +3 more
wiley +1 more source