Results 71 to 80 of about 2,846 (170)

Investigating the Origins of Hot Neptunes from Radial Velocity Data

open access: yesThe 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

Exploring Warm Jupiter Migration Pathways with Eccentricities. II. Correlations with Host Star Properties and Orbital Separation

open access: yesThe Astronomical Journal
Warm Jupiters with orbital periods of ≈10–365 days represent a population of giant planets located well within the water ice line but beyond the region of tidal influence of their host star relevant for high-eccentricity tidal migration.
Marvin Morgan   +2 more
doaj   +1 more source

A Hot Jupiter in a Nearly Polar Orbit [PDF]

open access: bronze, 2013
Brett Addison   +7 more
openalex   +1 more source

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

open access: yesThe 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

Constraints onTESSalbedos for five hot Jupiters [PDF]

open access: bronze, 2022
Martin Blažek   +12 more
openalex   +1 more source

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

open access: yesThe 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   +8 more
doaj   +1 more source

A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion [PDF]

open access: green, 2015
David K. Sing   +20 more
openalex   +1 more source

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

open access: yesThe 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   +14 more
doaj   +1 more source

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