Exoplanets
Worlds Beyond Our Solar System: Exploring the diverse and fascinating planets orbiting distant stars
What Are Exoplanets?
An exoplanet is any planet beyond our solar system. Most orbit other stars, but some free-floating exoplanets, called rogue planets, drift through the galaxy untethered to any star. We've confirmed more than 6,000 exoplanets out of the billions we believe exist.
Most discovered exoplanets are in a relatively small region of our galaxy, the Milky Way. Even the closest known exoplanet, Proxima Centauri b, is still about 4 light-years away. Scientists now know there are more planets than stars in the galaxy.
By measuring exoplanets' sizes and masses, we can determine compositions ranging from rocky (like Earth) to gas-rich (like Jupiter). We've identified lava worlds covered in molten seas, puffy planets with the density of Styrofoam, and super-Earths that might harbor conditions suitable for life.
Fascinating Exoplanet DiscoveriesClick cards to explore more
How We Discover Exoplanets
Transit Method
~75%Detecting dips in starlight as planets pass in front of their stars
Radial Velocity
~20%Measuring star wobbles caused by gravitational tugs from orbiting planets
Direct Imaging
~2%Capturing actual images of planets by blocking out starlight
Microlensing
~3%Using gravity to magnify light from background stars
Key Exoplanet Missions
Kepler (2009-2018)
Discovered over 2,600 exoplanets by monitoring 150,000 stars for transit events.
TESS (2018-Present)
Surveying 200,000 nearby stars to find transiting exoplanets around bright stars.
James Webb (2021-Present)
Analyzing exoplanet atmospheres using advanced spectroscopy to search for biosignatures.
Data source: NASA Exoplanet Archive | Updated October 2025