Results 111 to 120 of about 908,915 (272)
Prophetic promise: the lineal return of ‘lopp'd branches’ in Shakespeare's Cymbeline
Abstract This paper identifies the early‐modern conception of prophecy as a word‐magic performed across generations, a verbal promise that anticipates its own realisation in posterity. Just as Francis Bacon upheld the generative power of prophetic utterances by noting their ‘springing and germinant accomplishment throughout many ages’, Shakespeare's ...
Rana Banna
wiley +1 more source
Limited Hysteresis in the Atmospheric Dynamics of Hot Jupiters
Over the past two decades, a coherent picture has emerged of the atmospheric dynamics of hot Jupiters from a combination of three-dimensional general circulation models and astronomical observations.
Thaddeus D. Komacek
doaj +1 more source
We present high-resolution dayside thermal emission observations of the exoplanet KELT-20b/MASCARA-2b using the MAROON-X spectrograph. Applying the cross-correlation method with both empirical and theoretical masks and a retrieval analysis, we confirm ...
David Kasper +12 more
doaj +1 more source
On Possible Types of Magnetospheres of Hot Jupiters [PDF]
Accepted in Astronomy Reports, 23 pages, 10 ...
Andrey Zhilkin, D. V. Bisikalo
openaire +3 more sources
A Secular Resonant Origin for the Loneliness of Hot Jupiters [PDF]
Despite decades of inquiry, the origin of giant planets residing within a few tenths of an astronomical unit from their host stars remains unclear. Traditionally, these objects are thought to have formed further out before subsequently migrating inwards.
Batygin, Konstantin +1 more
core +3 more sources
Boulders on Bennu: Low Apparent Thermal Inertia Caused by Thermal Fatigue Fractures
Abstract Boulders covering the surfaces of asteroids Bennu and Ryugu have apparent thermal inertias substantially lower than their meteorite analogs. This has led to the inference that boulders on Bennu may be unlike any known meteorite. However, samples returned from Ryugu have a thermal inertia 3.5 times higher than the apparent thermal inertia ...
Catherine M. Elder
wiley +1 more source
The degree of alignment between a star’s spin axis and the orbital plane of its planets (the stellar obliquity) is related to interesting and poorly understood processes that occur during planet formation and evolution.
Nicholas Saunders +55 more
doaj +1 more source
For the majority of short-period exoplanets transiting massive stars with radiative envelopes, the spin angular momentum of the host star is greater than the planetary orbital angular momentum.
Alexander P. Stephan, B. Scott Gaudi
doaj +1 more source
Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets [PDF]
In this paper we search for distant massive companions to known transiting hot Jupiters that may have influenced the dynamical evolution of these systems. We present new radial velocity observations for a sample of 51 hot Jupiters obtained using the Keck
Bakos, Gáspár Á. +12 more
core +3 more sources
Formation of Silicate and Titanium Clouds on Hot Jupiters [PDF]
We present the first application of a bin-scheme microphysical and vertical transport model to determine the size distribution of titanium and silicate cloud particles in the atmospheres of hot Jupiters.
D. Powell +3 more
semanticscholar +1 more source

