Exoplanetary Weather Watchers Find Strong Evidence of Magnetic Fields
Astronomers studying wind speeds on distant exoplanets have discovered weather systems driven by magnetic fields, rather than the largely hydrodynamic weather p...
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Astronomers studying wind speeds on distant exoplanets have discovered weather systems driven by magnetic fields, rather than the largely hydrodynamic weather p...
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Abstract page for arXiv paper 2606.02648: Quantitative Nonequilibrium Pathway from Fundamental Physics to the Emergence and Persistence of Exoplanetary Biospher...
Abstract page for arXiv paper 2606.02705: A Massive Hot-Jupiter Companion that Disfavors Giant Planet Formation Beyond the Water-Ice Line
Abstract page for arXiv paper 2510.27386: Stacking transmission spectra of different exoplanets
By tracking fierce winds racing through the atmospheres of seven ultra-hot Jupiters, astronomers have uncovered the strongest evidence yet that magnetic fields ...
The hottest giant planets in the galaxy should, in theory, have the fastest winds.
How do you weigh a planet you can't see? Astronomers may have the answer and it involves
It’s 2234, you’re on your annual class field trip touring exoplanets, and your teacher informs everyone they can pick one more exoplanetary system to explor...
Abstract page for arXiv paper 2605.31523: Mind the Companion : Demographics of Transiting S-type Exoplanets
Abstract page for arXiv paper 2511.03045: Quantifying the Impact of Starspot-Crossing Events on Retrieved Parameters from Transit Lightcurves
Astronomers have recently discovered red dwarfs absorbing matter from Earth-like planets. While this highlights the destructive behavior of red dwarfs, it also ...
We know that stars can engulf planets because stars that swell up to become red giants overwhelm any close-in planets. The Sun will do this to Venus, Mercury, a...
Abstract page for arXiv paper 2605.28635: Comparing telluric removal methods in their capability to recover injected exoplanet atmosphere signals with high reso...
Abstract page for arXiv paper 2605.28719: A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$λ$ Trends in Three Gas-Giant Mass Regimes
Abstract page for arXiv paper 2605.28755: Hidden worlds: a non-transiting candidate planet in the Neptunian desert around the solar-type pulsator KIC 9139163
Abstract page for arXiv paper 2605.28768: The unique ability of the Hubble Space Telescope to characterize young exoplanet environments
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