Follow - up observations of planetary candidates identified by detection of transit - like events are needed both for identification of astrophysical phenomena that
mimic planetary transits and for characterization of the true planets and planetary systems found by Kepler.
Follow - up observations of planetary candidates identified by detection of transit - like events are needed both for identification of astrophysical phenomena that
mimic planetary transits and for characterization of the... ▽ More The Kepler Mission was launched on March 6, 2009 to perform a photometric survey of more than 100,000 dwarf stars to search for terrestrial - size planets with the transit technique.
Not exact matches
Giant
transiting exoplanets are easily
mimicked by false positives, so spectroscopic follow - up observations are needed to establish the
planetary nature of the
transit detections, and easily reveal blended multiple stellar systems.