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List of directly imaged exoplanets

This is a list of extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit infrared light and are far from the glare of the star. Currently, this list includes both directly imaged planets and imaged planetary-mass companions. This list does not include free-floating planetary-mass objects in star-forming regions or young associations, which are also referred to as rogue planets.

Key
Exoplanets have been discovered using several different methods for collecting or combining direct images to isolate planets from the background light of their star. Non-Redundant Aperture Masking Interferometry is a method of combining the views of multiple telescopes into a single image, while the other methods are algorithms for combining multiple direct images taken from the same telescope. • ADI = Angular Differential Imaging • KLIP = Karhunen–Loève Image Processing • LOCI = Locally Optimized Combination of Images • NRM = Non-Redundant Aperture Masking InterferometryRSDI = Reference Star Differential Imaging • SDI = Spectral Differential Imaging • TLOCI = Template Locally Optimized Combination of Images == Exoplanets ==
Exoplanets
Although listed in the table below, the identities of Alpha Centauri candidate 1, FW Tau b, 2MASS J044144 b, CVSO 30 c and HD 100546 b are disputed. They may not actually be true exoplanets.   †   There is no consensus whether these companions of stars should be considered sub-brown dwarfs or planets Check https://exoplanetarchive.ipac.caltech.edu/docs/imaging.html to see more directly imaged planets. It contains an updated table of all of them. == See also ==
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