The transit method involves observing a star as an exoplanet passes in front of it, causing a slight dimming of the star's light.

The habitable zone is the region around a star where the temperature is suitable for liquid water to exist on the surface of a planet.

The Kepler Space Telescope was specifically designed to search for and characterize exoplanets using the transit method.

Radial Velocity Variation refers to the slight wobble of a star caused by the gravitational pull of an orbiting exoplanet.

Hot Jupiters are characterized by their large size and high mass, short orbital periods and close proximity to their host stars, and thick atmospheres with strong winds.

Microlensing is the phenomenon where a star's light is amplified and distorted as it passes through the gravitational field of a massive object, such as an exoplanet.

The search for Earth-like exoplanets is challenging due to their small size and low mass, the distance between Earth and other stars, and the faintness of Earth-like planets compared to their host stars.

Spectroscopy is the process of studying the atmospheres of exoplanets by analyzing the light that passes through them.

Kepler-452b, 55 Cancri e, and GJ 1214b are all examples of super-Earths, which are planets that are larger than Earth but smaller than Neptune.

A Lagrangian Point is the region around a star where the gravitational pull of the star and the centrifugal force of an orbiting planet cancel each other out.

HD 209458b is an example of a hot Jupiter, which is a gas giant planet that orbits very close to its host star.

Transit is the phenomenon where an exoplanet blocks a portion of its host star's light as it passes in front of it.

C/2019 Q4 (Borisov) is an example of a rogue planet, which is a planet that is not gravitationally bound to any star.

The Transit Method is the process of detecting exoplanets by observing the slight dimming of a star's light as an exoplanet passes in front of it.

Kepler-16b, Kepler-34b, and Kepler-47c are all examples of circumbinary planets, which are planets that orbit two stars instead of one.