OGLE-2016-BLG-1195Lb: A Sub-Neptune Beyond the Snow Line of an M-Dwarf Confirmed by Keck Adaptive Optics
Aikaterini Vandorou et al 2025 AJ 169 319 Follow-up observations of a gravitational microlensing event show the source to be a 10-Earth-mass exoplanet orbiting an M-dwarf star, consistent with the…
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Free-Floating Neptunes May Not Be So Alone: Study Reveals Complex Planetary Family Histories
The galaxy seems to be full of free-range Neptunes, but a closer look reveals some complicated family dynamics in planetary systems.
Free-Floating Neptunes May Not Be So Alone: Study Reveals Complex Planetary Family Histories
The galaxy seems to be full of free-range Neptunes, but a closer look reveals some complicated family dynamics in planetary systems.

Kmt-2023-blg-0332l b
KMT-2023-BLG-0332L b is a gas giant exoplanet that orbits a Unknown-type star. Its mass is 22 Jupiters, it takes 7.8 years to complete one o

Kmt-2023-blg-0332l b
KMT-2023-BLG-0332L b is a gas giant exoplanet that orbits a Unknown-type star. Its mass is 22 Jupiters, it takes 7.8 years to complete one o
Astronomers Directly Image Third Giant Exoplanet in β Pictoris System
We report the direct imaging discovery of a third exoplanet in the β Pictoris system.

HD 127195 b
HD 127195 b is a gas giant exoplanet that orbits a K-type star. Its mass is 0.67 Jupiters, it takes 1.5 years to complete one orbit of its s

HD 127195 b
HD 127195 b is a gas giant exoplanet that orbits a K-type star. Its mass is 0.67 Jupiters, it takes 1.5 years to complete one orbit of its s
Astronomers discover two ultra-low-density 'super-puff' exoplanets orbiting dwarf star TOI-791
"Only a handful of these super-puffy planets are known, and it is even rarer to find two in the same system."
Astronomers discover two ultra-low-density 'super-puff' exoplanets orbiting dwarf star TOI-791
"Only a handful of these super-puffy planets are known, and it is even rarer to find two in the same system."
JWST Panchromatic Study Reveals KELT-7 b is a Metal-Enriched Ultra-Hot Jupiter Orbiting a Young Star
We present the first panchromatic JWST transmission spectrum of an ultra-hot Jupiter, combining NIRISS and NIRSpec observations to constrain

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