Most exoplanets detected by radial velocity methods are gas giants orbiting close to the host star
Transit method is the predominant technique for detecting exoplanets orbiting stars. Based on detecting the small dip in starlight as an exoplanet pass in front of the host star, development of sensitive detectors has afforded the detection of a large number of exoplanets hitherto thought not to exist. But, there exists other methods for the … More Most exoplanets detected by radial velocity methods are gas giants orbiting close to the host star