An instrument that blocks a star's light to reveal nearby faint objects like planets or dust.A coronagraph is an instrument designed to block out the bright light from a star, allowing astronomers to see faint objects nearby, such as exoplanets, dust disks, or stellar coronae. The name comes from the solar corona, which was the first target of such instruments. By artificially creating an eclipse, a coronagraph reveals the otherwise hidden environment around a star, making it a cornerstone of direct imaging in astronomy.
The coronagraph was invented by French astronomer Bernard Lyot in 1931 to observe the solar corona without waiting for a total solar eclipse. It was later adapted for stellar observations in the 1980s and 1990s.
A coronagraph uses an opaque disk (or a more complex mask) placed in the focal plane of a telescope to block the star's light. However, light diffracts around the edges of the disk, so additional components — such as a Lyot stop and apodizing masks — are used to suppress this diffracted light. Modern coronagraphs use advanced phase masks or deformable mirrors to cancel out the starlight while preserving the light from nearby faint objects. The result is a dark region where planets or dust can be detected.
Coronagraphs are used on ground-based telescopes and space observatories like the Hubble Space Telescope and the James Webb Space Telescope to directly image exoplanets and study circumstellar disks.
The first exoplanet directly imaged with a coronagraph was 2M1207b in 2004, using the Very Large Telescope in Chile.






