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Exoplanet Detection: The Radial Velocity Method

Using the radial velocity method and the Doppler effect.

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Exoplanet Detection: The Radial Velocity Method is a Photo & Image software developed by Mario Belloni. After our trial and test, the software is proved to be official, secure and free. Here is the official description for Exoplanet Detection: The Radial Velocity Method:

The Exoplanet Detection: radiaL Velocity Method model simulates the detection of exoplanets by using the radial velocity method and the Doppler effect. In this simulation the exoplanet orbits the Star (Sun-sized) in circular motion via Kepler's third law. The radial velocity of the star is determined from the velocity of the exoplanet. This velocity is then used to calculate the Doppler shift of the Fraunhofer lines of the star.
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