Exoplanets
Exoplanets are planets that orbit stars outside our own solar system, with thousands now confirmed since the first discovery in the early 1990s, significantly expanding understanding of planetary diversity.
Confirmed for the first time only a few decades ago, these planets orbiting distant stars have since been discovered by the thousands, revealing a staggering diversity of worlds beyond our own solar system.
Planets Beyond Our Solar System
Exoplanets are planets that orbit stars other than our Sun, existing throughout the broader galaxy in numbers that continue to be revised upward.
Thousands Now Confirmed
Since the first confirmed discovery in 1992, astronomers have identified thousands of exoplanets, revealing extraordinary diversity in planetary size, composition, and orbital characteristics.
The Search for Habitable Worlds
A significant focus of exoplanet research involves identifying planets within a star's "habitable zone," where conditions might potentially support liquid water and life.
Advanced Detection Technology
Exoplanet discovery has been significantly enabled by advanced space telescopes and detection techniques, including the transit method measuring stars' brightness changes.
