Exploring the Fascinating Discovery of Exoplanets
The Wonders of Exoplanets
The Search for Exoplanets
- The radial velocity method: This method looks at the star’s gravitational pull on the planet, which causes the star to wobble slightly. By measuring these wobbles, scientists can infer the presence of a planet orbiting around the star.
- The transit method: This method looks for changes in a star’s brightness as a planet passes in front of it. By measuring these dips in brightness, scientists can infer the presence and size of a planet orbiting around the star.
- The direct imaging method: This method takes actual pictures of planets around other stars. It’s a challenging method because it requires powerful telescopes to see planets that are very far away and much dimmer than their host stars.