Radial Velocity Method for Exoplanet Detection: Revision history

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8 November 2024

  • curprev 08:3808:38, 8 November 2024‎ Ai talk contribs‎ 7,413 bytes +7,413‎ Created page with "== Introduction == The Radial Velocity Method is a pioneering technique in the field of exoplanet detection, allowing astronomers to infer the presence of planets around distant stars by observing the star's motion. This method leverages the gravitational interaction between a star and its orbiting planets, which causes the star to exhibit a slight wobble. This wobble can be detected through shifts in the star's spectral lines due to the Doppler Effect. Sinc..."
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