Exoplanetary Science
The discovery, characterization, and study of planets and planetary systems orbiting stars other than our Sun.
Explore by Exoplanetary Science

February 12, 2026
Webb Finds Diamond-Rain Planet Around Neutron Star

February 4, 2026
HD 137010b: Earth-Sized Exoplanet in Habitable Zone Discovered

January 22, 2026
Metallic Winds Reveal Planetary Impact in Distant Star System

January 20, 2026
Fastest Spinning Asteroid: 2025 MN45 Record-Breaking Rotation Discovery

January 7, 2026
First Direct Mass Measurement of a Rogue Planet

January 2, 2026
JWST Exoplanet Breakthrough Discoveries 2025

December 30, 2025
Dimethyl Sulfide Detection on K2-18b

December 21, 2025
JWST Eccentric Exoplanet Orbits

December 18, 2025
Atmospheric Biosignatures on Habitable Exoplanets
FAQs about Exoplanetary Science
It is the search for and study of planets orbiting stars other than our Sun. These distant worlds are called exoplanets.
The most common method is called the transit method, where we watch for a star's light to dip slightly. This dimming tells us a planet may have passed in front of it.
Yes. When an exoplanet transits its star, we can study the starlight that filters through its atmosphere. This light tells us what gases, like oxygen or methane, might be present.
A primary goal is to find planets that exist in the "habitable zone"—the right distance from a star where liquid water could exist on the surface, which is a key ingredient for life as we know it.