Results 141 to 150 of about 908,915 (272)
Separating Super-puffs versus Hot Jupiters among Young Puffy Planets
The Astrophysical JournalDiscoveries of close-in young puffy ( R _p ≳ 6 R _⊕ ) planets raise the question of whether they are bona fide hot Jupiters or puffed-up Neptunes, potentially placing constraints on the formation location and timescale of hot Jupiters.
Amalia Karalis +2 more
doaj +1 more source
EPJ Web of Conferences, 2013 The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infrared Telescope (UKIRT). We conduct Monte Carlo transit injection and detection simulations for short period (
Murgas F. +13 more
doaj +1 more source
Magnetohydrodynamical Torsional Oscillations from Thermoresistive Instability in Hot Jupiters
The Astrophysical Journal, 2023 Hot Jupiter atmospheres may be subject to a thermoresistive instability where an increase in the electrical conductivity due to ohmic heating results in runaway of the atmospheric temperature.
Raphaël Hardy +2 more
doaj +1 more source
Engineering Reports, Volume 7, Issue 10, October 2025.Characterization of Himalayan pine needle composites: Mechanical, tribological, and microstructural evaluation under liquid exposure. The graphical abstract illustrates the process of studying Himalayan pine needle composites through mechanical and tribological testing.
Pawan Kumar Rakesh +4 more
wiley +1 more source
The Astronomical JournalA significant fraction of hot Jupiters have orbital axes misaligned with their host stars’ spin axes. The large stellar obliquities of these giants have long been considered potential signatures of high-eccentricity migration, which is expected to clear ...
Brandon T. Radzom +7 more
doaj +1 more source
Atmospheric Circulation of Hot Jupiters: Dayside–Nightside Temperature Differences. II. Comparison with Observations [PDF]
, 2016 The full-phase infrared light curves of low-eccentricity hot Jupiters show a trend of increasing fractional dayside–nightside brightness temperature difference with increasing incident stellar flux, both averaged across the infrared and in each ...
T. Komacek, A. Showman, Xianyu Tan
semanticscholar +1 more source
THE IMPRINT OF EXOPLANET FORMATION HISTORY ON OBSERVABLE PRESENT-DAY SPECTRA OF HOT JUPITERS [PDF]
, 2016 The composition of a planet’s atmosphere is determined by its formation, evolution, and present-day insolation. A planet’s spectrum therefore may hold clues on its origins.
C. Mordasini +4 more
semanticscholar +1 more source
Flexible Polyurethane Foams Reinforced With Recycled Waste Tire Material
Polymer Engineering &Science, Volume 65, Issue 10, Page 5491-5506, October 2025.Ground tire rubber powder obtained through water jet pulverization mixed with PU foam possesses tunable mechanical and acoustic properties suitable for automotive, construction, and aerospace applications. ABSTRACT We explore the use of ground tire rubber (GTR) powder obtained through water jet pulverization (WJP), referred to as WJP‐GTR, and reveal ...
Y. Nezili +8 more
wiley +1 more source
Spin and Obliquity Evolution of Hot Jupiter Hosts from Resonance Locks
The Astrophysical JournalWhen a hot Jupiter orbits a star whose effective temperature exceeds ∼6100 K, its orbit normal tends to be misaligned with the stellar spin axis. Cooler stars typically have smaller obliquities, which may have been damped by hot Jupiters in resonance ...
J. J. Zanazzi, Eugene Chiang
doaj +1 more source
Structure and Evolution of Internally Heated Hot Jupiters
, 2017 Hot Jupiters receive strong stellar irradiation, producing equilibrium temperatures of $1000 - 2500 \ \mathrm{Kelvin}$. Incoming irradiation directly heats just their thin outer layer, down to pressures of $\sim 0.1 \ \mathrm{bars}$.
Komacek, Thaddeus D., Youdin, Andrew N.
core +1 more source