Results 161 to 170 of about 908,915 (272)

Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia [PDF]

, 1998
M. Roos‐Serote, P. Drossart, Thérèse Encrenaz, E. Lellouch, R. W. Carlson, K. H. Baines, L. W. Kamp, R. Mehlman, Glenn S. Orton, S. B. Calcutt, P. G. J. Irwin, F. W. Taylor, Andrew Weir   +12 more
openalex   +1 more source

Two-dimensional Models of Microphysical Clouds on Hot Jupiters. I. Cloud Properties

The Astrophysical Journal
We present a new two-dimensional, bin-scheme microphysical model of cloud formation in the atmospheres of hot Jupiters that includes the effects of longitudinal gas and cloud transport.
Diana Powell, Xi Zhang
doaj   +1 more source

Mechanisms affecting the composition of Hot Jupiters atmospheres

EPJ Web of Conferences, 2013
Opacities and thus local chemical composition play a key role when characterizing exoplanet atmospheres from observations. When the gas is in chemical equilibrium the chemical abundances depend strongly on the temperature profile.
Showman Adam P., Guillot Tristan, Parmentier Vivien   +2 more
doaj   +1 more source

Atmospheric Circulation of Hot Jupiters [PDF]

, 2004
T. Guillot
openalex   +1 more source

Mapping the Atmospheres of Hot Jupiters

, 2007
To appear in "Extreme Solar Systems", eds. D. Fischer, F. Rasio, S. Thorsett, A. Wolszczan (ASP Conf. Series).
openaire   +4 more sources

Investigating the Origins of Hot Neptunes from Radial Velocity Data

The Astronomical Journal
Hot Neptunes are extrasolar planets that are similar in size to Neptune in our solar system but are much closer to their host stars, completing an orbit in 10 days or less. The origin of hot Neptunes is not fully understood.
Sophie Y. Zheng
doaj   +1 more source

A Larger Sample Confirms Small Planets around Hot Stars Are Misaligned

The Astrophysical Journal Letters
The distribution of stellar obliquities provides critical insight into the formation and evolution pathways of exoplanets. In the past decade, it was found that hot stars hosting hot Jupiters are more likely to have high obliquities than cool stars, but ...
Emma M. Louden, Songhu Wang, Joshua N. Winn, Erik A. Petigura, Howard Isaacson, Luke Handley, Samuel W. Yee, Corey Beard, Joseph M. Akana Murphy, Gregory Laughlin   +9 more
doaj   +1 more source

Exoplanet Ephemerides Change Observations (ExoEcho). I. Transit Timing Analysis of 37 Exoplanets Using HST/WFC3 Data

The Astronomical Journal
The ExoEcho project is designed to study the photodynamics of exoplanets by leveraging high-precision transit timing data from ground- and space-based telescopes.
Xinyue Ma, Wenqin Wang, Zixin Zhang, Cong Yu, Dichang Chen, Jiwei Xie, Shangfei Liu, Li Zhou, Bo Ma   +8 more
doaj   +1 more source

On the Dayside Thermal Emission of Hot Jupiters [PDF]

, 2005
Sara Seager, L. J. Richardson, Bradley M. S. Hansen, Kristen Menou, J. Y.‐K. Cho, Drake Deming   +5 more
openalex   +1 more source

The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201

The Astrophysical Journal Letters
Measuring the obliquities of stars hosting giant planets may shed light on the dynamical history of planetary systems. Significant efforts have been made to measure the obliquities of FGK stars with hot Jupiters, mainly based on observations of the ...
Tianjun Gan, Sharon X. Wang, Fei Dai, Joshua N. Winn, Shude Mao, Siyi Xu, Enric Pallé, Jacob L. Bean, Madison Brady, Nina Brown, Cicero Lu, Rafael Luque, Teo Mocnik, Andreas Seifahrt, Guđmundur K. Stefánsson   +14 more
doaj   +1 more source