Exoplanets are born by circumstellar disks of gas and dust around young stars.
Exoplanets are made out of similar elements that make up the planets in the solar system. They may be made of water, ice, carbon, iron, or others.
The 5 ways astronauts find exoplanets consists of:
Radial velocity
Transit
Direct imaging
Gravitational microlensing
Astrometry
Radial velocity measures the star's wobble as it's pulled down by gravity.
Transit measures the decrease in a star's brightness when a planet moves in front of it.
Direct imaging uses the light emitted by the planets to find them.
Gravitational microlensing depends on the gravitational lens effect. It uses gravity lens. It relies on the bending of light by a massive object.
Astrometry track and measure the tiny movements of the planet.
Discovering exoplanets helps us understand the processes and evolutions of planets all around.
There are more than 5,000 exoplanets discovered.
4 types of exoplanets consists of:
Gas giant
Neptunian
Super earth
Terrestrial
Planet Psr B1620-26 B is the oldest exoplanet at 12.7 billion years old.
Gas giant exoplanets are very big and made up of gas. They possess thick atmospheres and extreme weather conditions.
Neptunian exoplanets have helium and hydrogen atmospheres. They are also called mini-neptunes.
Mini-neptunes are smaller than neptune but larger than earth.
Super-earths are made up of gas, rocks, or both. They are rockier and more massive than earth but lighter than neptune. They may or may not have atmospheres.
Terrestrial exoplanets have rocky surfaces mostly made of rock and metal. Some might have oceans or atmospheres. They might be habitable.