ExoplanetAtlas

Exoplanet Glossary

Key terms and definitions used in exoplanet science. Click linked terms to explore related content on Exoplanet Atlas.

Astronomical Unit (AU)
The average distance from Earth to the Sun, approximately 149.6 million kilometers (93 million miles). Used as a standard unit for measuring distances within planetary systems.
Astrometry
An exoplanet detection method that measures the precise positional wobble of a star caused by orbiting planets.
Coronagraph
An instrument that blocks the light of a star to reveal faint objects orbiting nearby, such as exoplanets. Essential for direct imaging of exoplanets.
Direct Imaging
A method of detecting exoplanets by taking actual photographs of them, using coronagraphs to block the host star's overwhelming light.
Earth Mass (M⊕)
A unit of mass equal to the mass of Earth (5.97 × 10²⁴ kg). Exoplanet masses are often expressed relative to Earth's mass for easier comparison.
Earth Radius (R⊕)
A unit of length equal to Earth's radius (6,371 km). Exoplanet sizes are commonly expressed as multiples of Earth's radius.
Eccentricity
A measure of how elliptical (non-circular) an orbit is. A value of 0 means perfectly circular, while values closer to 1 indicate increasingly elongated orbits.
Equilibrium Temperature
The theoretical surface temperature of a planet based on the amount of stellar radiation it receives, assuming no atmosphere. Measured in Kelvin (K).
Exoplanet
A planet that orbits a star outside our solar system. Over 6,000 exoplanets have been confirmed since the first discovery in 1992.
Gas Giant
A large planet composed primarily of hydrogen and helium gas, similar to Jupiter and Saturn. Gas giant exoplanets have radii greater than 6 Earth radii.
Habitable Zone
The region around a star where temperatures allow liquid water to exist on a planet's surface. Also known as the Goldilocks zone.
Host Star
The star that an exoplanet orbits. The properties of the host star (temperature, mass, size) directly affect conditions on its planets.
Hot Jupiter
A gas giant exoplanet that orbits very close to its star, typically completing an orbit in just a few days. These planets have extremely high surface temperatures.
Inclination
The angle between a planet's orbital plane and our line of sight. A 90-degree inclination means the orbit is viewed edge-on, which is required for transit detection.
Insolation Flux
The amount of stellar energy a planet receives per unit area, usually expressed relative to what Earth receives from the Sun. Used to assess habitability.
Jupiter Mass (Mⱼ)
A unit of mass equal to the mass of Jupiter (1.898 × 10²⁷ kg), approximately 318 times Earth's mass. Used for measuring massive exoplanets.
Light-Year
The distance light travels in one year, approximately 9.46 trillion kilometers (5.88 trillion miles). One parsec equals about 3.26 light-years.
Microlensing
An exoplanet detection method that uses the gravitational bending of light by a foreground star to detect planets around it.
Neptune-like
An exoplanet with a size between a Super-Earth and a Gas Giant (radius 2.0 to 6.0 Earth radii), similar to Neptune and Uranus.
Orbital Period
The time it takes for a planet to complete one full orbit around its star. Earth's orbital period is 365.25 days (one year).
Parsec (pc)
A unit of distance equal to approximately 3.26 light-years (30.9 trillion kilometers). Stellar distances in exoplanet catalogs are typically given in parsecs.
Radial Velocity
An exoplanet detection method that measures the Doppler shift in a star's light caused by the gravitational tug of an orbiting planet.
Rocky Planet
A small, dense exoplanet with a solid surface, composed primarily of silicate rocks and metals. Rocky planets have radii of 1.25 Earth radii or less.
Semi-Major Axis
Half the longest diameter of an elliptical orbit. For nearly circular orbits, it approximates the average distance between the planet and its star, usually measured in AU.
Spectral Type
A classification of stars based on their surface temperature, labeled O, B, A, F, G, K, M from hottest to coolest. Our Sun is a G-type star.
Super-Earth
An exoplanet larger than Earth but smaller than Neptune (radius 1.25 to 2.0 Earth radii). A planet type with no equivalent in our solar system.
Tidal Locking
When a planet's rotation period equals its orbital period, causing one side to permanently face the star. Common for planets orbiting close to red dwarf stars.
Transit
The event when a planet passes between its star and the observer, causing a measurable dip in the star's brightness. The transit method is the most successful exoplanet detection technique.

How do planets text each other?