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Kepler-16
EntityQ1190765· pop 19· linked from 316 articles

Kepler-16 is an eclipsing binary star system in the constellation of Cygnus that was targeted by the Kepler spacecraft. Both stars are smaller than the Sun; the primary, Kepler-16A, is a K-type main-sequence star and the secondary, Kepler-16B, is an M-type red dwarf. They are separated by 0.23 AU, and complete an orbit around a common center of mass every 41 days. The system is host to one known extrasolar planet in circumbinary orbit: the Saturn-sized Kepler-16b.

Wikidata facts

Distance from Earth
75.298
Radius
0.65
Mass
0.8499
Image
Kepler-16.jpg
Show 14 more facts
catalog code
Kepler-16
spectral class
K7
effective temperature
4450
apparent magnitude
11.738809
parallax
13.2806
radial velocity
-30.07
metallicity
-0.13
surface gravity
30000
luminosity
0.12502325
right ascension component of proper motion
14.092
declination component of proper motion
-48.939
Commons category
Kepler-16
right ascension
289.07573265789
declination
51.75743964613999
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3 sections
Contents
  • Eclipses
  • Planetary system
  • References

Kepler-16 is an eclipsing binary star system in the constellation of Cygnus that was targeted by the Kepler spacecraft. Both stars are smaller than the Sun; the primary, Kepler-16A, is a K-type main-sequence star and the secondary, Kepler-16B, is an M-type red dwarf. They are separated by 0.23 AU, and complete an orbit around a common center of mass every 41 days. The system is host to one known extrasolar planet in circumbinary orbit: the Saturn-sized Kepler-16b.

==Eclipses== thumb|left|Light curves for the Kepler-16 system, adapted from Doyle et al. (2011) The Kepler-16 system is almost edge-on to Earth and the two stars eclipse each other as they orbit. The larger and brighter primary star is partially eclipsed by the secondary for about six hours and the brightness drops by about 0.15 magnitudes. The secondary star is completely occulted by the primary star for about two hours, but the overall brightness only drops by about 0.02 magnitudes.

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