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Kepler-22

Kepler-22
Kepler-22b System Diagram.jpg
A diagram of the Kepler-22b System, compared to our Inner Solar System.
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 16m 52.2s
Declination +47° 53′ 4.2″
Apparent magnitude (V) 11.664
Characteristics
Spectral type G5V
Astrometry
Parallax (π) ~5.26 mas
Distance 620ly
(190 pc)
Absolute magnitude (MV) ~5.27
Absolute bolometric
magnitude
 (Mbol)
~4.98
Details
Mass 0.970 ± 0.060 M
Radius 0.979 ± 0.020 R
Luminosity (bolometric) 0.8 L
Luminosity (visual, LV) ~0.67 L
Temperature 5518 ± 44 K
Metallicity [Fe/H] –0.29 ± 0.06 dex
Rotational velocity (v sin i) 0.6 ± 1.0 km/s
Other designations
KOI-087,KIC 10593626, 2MASS J19165219+4753040
Database references
SIMBAD data
KIC data

Kepler-22 is a star in the northern constellation of Cygnus, the swan, that is orbited by a planet found to be unequivocally within the star's habitable zone. It is located at the celestial coordinates: Right Ascension 19h 16m 52.2s, Declination +47° 53′ 4.2″. With an apparent visual magnitude of 11.7, this star is too faint to be seen with the naked eye. It can be viewed with a telescope having an aperture of at least 4 in (10 cm). The estimated distance to Kepler-22 is 620 light-years (190 parsecs).

Kepler-22 is slightly smaller and cooler than the Sun, with a lower abundance of elements having more mass than helium. It has a spectral type of G5V, while the luminosity class remains undetermined. This star is radiating 79% of the Sun's luminosity from its outer atmosphere at an effective temperature of 5,518 K, giving it the yellow-hued glow of a G-type star. A projected rotational velocity of 0.6 km/s suggests it has a low period of rotation.

On December 5, 2011, scientists from the Kepler mission announced that a possible Earthlike world (Kepler-22b) had been discovered orbiting in the star's habitable zone by NASA's Kepler spacecraft. This was significant in that it was the first relatively Earth-sized extrasolar planet (about twice as big) confirmed to be orbiting within a star's habitable zone.


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