Results 151 to 160 of about 892,024 (248)
Age Analysis of Extrasolar Planets: Insight from Stellar Isochrone Models
There is growing evidence from stellar kinematics and galactic chemical evolution suggesting that giant planets ( M _P ≥ 0.3 M _J ) are relatively young compared to the most commonly occurring population of small planets ( M _P < 0.3 M _J ).
C. Swastik+4 more
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Planetary population synthesis and the emergence of four classes of planetary system architectures. [PDF]
Emsenhuber A, Mordasini C, Burn R.
europepmc +1 more source
We present a pattern emerging from stellar obliquity measurements in single-star systems: planets with high planet-to-star mass ratios ( M _P / M _* ≥ 2 × 10 ^−3 )—such as super-Jupiters, brown dwarf companions, and M dwarfs hosting Jupiter-like planets ...
Jace Rusznak+3 more
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Phase dispersion relation of the 5‐micron hot spot wave from a long‐term study of Jupiter in the visible [PDF]
J. Arregi+3 more
openalex +1 more source
A magnetic communication scenario for hot Jupiters [PDF]
S. Preusse+3 more
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Plenary Abstracts Session & Oral Presentations
HemaSphere, Volume 9, Issue S1, June 2025.
wiley +1 more source
Formation of Ultra-short-period Planets in Hot Jupiter Systems: Application to WASP-47
The WASP-47 system is notable as the first known system hosting both inner and outer low-mass planetary companions around a hot Jupiter, with an ultra-short-period (USP) planet as the innermost planetary companion.
Su Wang+4 more
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Hot-atom synthesis of organic compounds on Jupiter
John S. Lewis, Bruce Fegley
openalex +1 more source
An Eccentric Hot Jupiter Orbiting the Subgiant HD 185269 [PDF]
John Asher Johnson+6 more
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Producing optimized and accurate transmission spectra of exoplanets from telescope data has traditionally been a manual and labor intensive procedure.
Reza Ashtari+6 more
doaj +1 more source