Exoplanet Candidates
Exoplanet candidates are celestial bodies that are suspected to be planets orbiting stars outside of our solar system. These candidates are identified through various methods, including the transit method, radial velocity method, and direct imaging. The transit method involves observing a star's brightness and looking for periodic dips that could indicate a planet passing in front of it. The radial velocity method involves measuring the star's wobble caused by the gravitational pull of an orbiting planet. Direct imaging involves taking pictures of the exoplanet itself. However, exoplanet candidates are not confirmed planets until they have been observed and studied extensively to rule out other possible explanations for the observed data. This confirmation process can involve follow-up observations with other telescopes and instruments, as well as data analysis and modeling.
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