Results 101 to 110 of about 53,007 (245)

Types of Gaseous Envelopes of "Hot Jupiter" Exoplanets

, 2013
As a rule, the orbital velocities of "hot Jupiters," i.e., exoplanets with masses comparable to the mass of Jupiter and orbital semi-major axes less than 0.1 AU, are supersonic relative to the stellar wind, resulting in the formation of a bow shock.
Bisikalo, D. V., Ionov, D. E., Kaigorodov, P. V., Shematovich, V. I   +3 more
core   +1 more source

Evidence for TiO in the Atmosphere of the Hot Jupiter HAT-P-65 b [PDF]

, 2021
G. Chen, Ε. Πάλλη, H. Parviainen, F. Murgas, F. Yan   +4 more
openalex   +1 more source

Prophetic Promise: The Lineal Return of ‘lopp’d branches’ in Shakespeare’s Cymbeline

Renaissance Studies, Volume 40, Issue 1, Page 55-75, February 2026.
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 force of prophetic utterances by noting their ‘springing and germinant accomplishment throughout many ages’, Shakespeare’s ...
Rana Banna
wiley   +1 more source

Constraining the atmospheric elements in hot Jupiters with Ariel [PDF]

, 2023
Fang Wang, Quentin Changeat, G. Tinetti, D. Turrini, Sam Wright   +4 more
openalex   +1 more source

Single‐Source‐Precursor Synthesis of Novel BCN and HfBCN Nanocomposites for Energy Conversion Application

Small Structures, Volume 7, Issue 1, January 2026.
We prepared monolithic BCN and HfBCN nanocomposites using a single‐source precursor approach. The HfBCN nanocomposite sintered at 1600°C achieved a record high power factor of ≈ 40 μW m–1 K–2 at 800°C, setting a benchmark in polymer‐derived ceramics (PDCs).
Wei Li, Jinxue Ding, Tianshu Jiang, Aasir Rashid, Wenjie Xie, Marc Widenmeyer, Leopoldo Molina‐Luna, Ralf Riedel, Anke Weidenkaff, Kathy Lu   +9 more
wiley   +1 more source

No variations in transit times for Qatar-1 b

, 2015
The transiting hot Jupiter planet Qatar-1 b was presented to exhibit variations in transit times that could be of perturbative nature. A hot Jupiter with a planetary companion on a nearby orbit would constitute an unprecedented planetary configuration ...
Aceituno, F. J., Dimitrov, D., Errman, R., Fernández, M., Gilbert, H., Kitze, M., Maciejewski, G., Neuhäuser, R., Ohlert, J., Pannicke, A., Puchalski, D., Raetz, St., Schmidt, J. -G., Seeliger, M.   +13 more
core   +1 more source

Testing Approximate Infrared Scattering Radiative-transfer Methods for Hot Jupiter Atmospheres

The Astrophysical Journal
The calculation of internal atmospheric (longwave) fluxes is a key component of any model of exoplanet atmospheres that requires radiative-transfer (RT) calculations.
Elspeth K. H. Lee
doaj   +1 more source

Mountain Degradation Mechanisms on Io Based on Geologic Mapping of the Cocytus Montes Region From JunoCam Imagery

Journal of Geophysical Research: Planets, Volume 131, Issue 1, January 2026.
Abstract Periodic high‐resolution imagery of Io is essential for understanding its surface evolution, from volcanic eruptions to tectonic deformation to large‐scale mass wasting. Juno flybys in 2023 and 2024 obtained imagery of the surface with the JunoCam imager at 1.8 km/pixel spatial resolution, comparable to global observations from the Galileo ...
C. H. Seeger, K. de Kleer, D. A. Williams, J. E. Perry, A. G. Davies, D. M. Nelson   +5 more
wiley   +1 more source

Velocity Shift and Signal-to-Noise Ratio Limits for High-resolution Spectroscopy of Hot Jupiters Using Keck/KPIC

The Astronomical Journal
High-resolution cross-correlation spectroscopy is a technique for detecting the atmospheres of close-in planets using the change in the projected planet velocity over a few hours. To date, this technique has most often been applied to hot Jupiters, which
Kevin S. Hong, Luke Finnerty, Michael P. Fitzgerald   +2 more
doaj   +1 more source

Synchronized Eruptions on Io: Possible Evidence of Interconnected Subsurface Magma Reservoirs

Journal of Geophysical Research: Planets, Volume 131, Issue 1, January 2026.
Abstract On 27 December 2024, Juno's JIRAM (Jovian InfraRed Auroral Mapper) instrument observed an unprecedented volcanic event in Io's southern hemisphere, covering a vast region of ∼65,000 km2, near 73°S, 140°E. Within the imaged region, only one hot spot was previously known (Pfd454).
A. Mura, R. Lopes, F. Nimmo, S. Bolton, A. Ermakov, J. T. Keane, F. Tosi, F. Zambon, R. Sordini, J. Radebaugh, J. Rathbun, W. McKinnon, S. Goossens, M. Paris, M. Mirino, A. Cicchetti, G. Piccioni, R. Noschese, G. Sindoni, C. Plainaki   +19 more
wiley   +1 more source