Results 131 to 140 of about 2,811,519 (263)
Exoplanet winds: Modelling atmospheric dynamics via resolved spectral lines
This thesis benchmarked a new probe of atmospheric dynamics in exoplanet atmospheres by resolving the spectral lines stemming from these far atmospheres and then modelling their line shape taking into account the broadening from atmospheric winds. This gives us a window into atmospheric winds for these far away worlds only limited by the depths of the ...
openaire +2 more sources
The HD 191939 Exoplanet System is Well Aligned and Flat
We report the sky-projected spin–orbit angle λ for HD 191939 b, the innermost planet in a six-planet system, using Keck/KPF to detect the Rossiter–McLaughlin (RM) effect.
Jack Lubin+27 more
doaj +1 more source
The barycentric motion of exoplanet host stars: tests of solar spin-orbit coupling
Empirical evidence suggests a tantalising but unproven link between various indicators of solar activity and the barycentric motion of the Sun. The latter is exemplified by transitions between regular and more disordered motion modulated by the motions ...
Baliunas+51 more
core +1 more source
Inertia of Ionospheric Conductance During Electron Precipitation Events
Abstract Using the SuperThermal Electron Transport (STET) model coupled with the Super‐thermal Proton Electron Atomic Hydrogen—tRansport in the Ionosphere and Thermosphere (SPEAH‐RIT) codes, we demonstrate that temporal variability of ionospheric conductance is defined by several time scales: the temporal variations of the magnetospheric source, the ...
George V. Khazanov+2 more
wiley +1 more source
Formation of Ultra-short-period Planets in Hot Jupiter Systems: Application to WASP-47
The WASP-47 system is notable as the first known system hosting both inner and outer low-mass planetary companions around a hot Jupiter, with an ultra-short-period (USP) planet as the innermost planetary companion.
Su Wang+4 more
doaj +1 more source
Geodynamics of Super‐Earth GJ 486b
Abstract Many super‐Earths are on very short orbits around their host star and, therefore, more likely to be tidally locked. Because this locking can lead to a strong contrast between the dayside and nightside surface temperatures, these super‐Earths could exhibit mantle convection patterns and tectonics that could differ significantly from those ...
Tobias G. Meier+10 more
wiley +1 more source
Abstract Iron hydrides are a potentially dominant component of the metallic cores of planets, primarily because of hydrogen's ubiquity in the universe and affinity for iron. Using ab initio molecular dynamics, we examine iron hydrides with 0.1, 0.33, 0.5, and 0.6 mol fraction hydrogen up to 100 GPa between 3,000 and 5,000 K to describe how hydrogen ...
Emma R. Stoutenburg+3 more
wiley +1 more source
A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World
The discovery of planetary systems beyond the solar system has revealed a diversity of architectures, most of which differ significantly from our system.
Stephen R. Kane+7 more
doaj +1 more source
Inhomogeneous cloud formation and wavelength-dependent phenomena are expected to shape hot Jupiter atmospheres. We present a general circulation model with multiwavelength “picket fence” radiative transfer and radiatively active, temperature-dependent ...
Isaac Malsky+7 more
doaj +1 more source
Correction: Secular orbital dynamics of the innermost exoplanet of the $$\upsilon $$-Andromedæ system [PDF]
Rita Mastroianni, Ugo Locatelli
openalex +1 more source