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Kepler-11, also designated as 2MASS J19482762+4154328, is a Sun-like star slightly larger than the Sun in the constellation Cygnus, located some 2,110 light years from Earth. It is located within the field of vision of the Kepler space telescope, the satellite that NASA's Kepler Mission uses to detect planets that may be transiting their stars. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger one

Wikidata facts

Distance from Earth
658.59
Radius
1.06
Mass
0.96
Image
Kepler11.png
Show 16 more facts
Commons category
Kepler-11
effective temperature
5663
parallax
1.5476
radial velocity
-60.17
spectral class
G3
metallicity
0
surface gravity
20000
stellar rotational velocity
0.9
luminosity
1.13
right ascension component of proper motion
0.106
declination component of proper motion
-7.103
right ascension
297.11509425782
declination
41.90913976764
catalog code
Gaia DR3 2076960598545789824
apparent magnitude
13.455
age estimated by a dating method
8.5
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6 sections
Contents
  • Nomenclature and history
  • Characteristics
  • Planetary system
  • See also
  • References
  • External links

Kepler-11, also designated as 2MASS J19482762+4154328, is a Sun-like star slightly larger than the Sun in the constellation Cygnus, located some 2,110 light years from Earth. It is located within the field of vision of the Kepler space telescope, the satellite that NASA's Kepler Mission uses to detect planets that may be transiting their stars. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size.

==Nomenclature and history== Kepler-11 and its planets were discovered by NASA's Kepler Mission, a mission tasked with discovering planets in transit around their stars. The transit method that Kepler uses involves detecting dips in brightness in stars. These dips in brightness can be interpreted as planets whose orbits move in front of their stars from the perspective of Earth. Kepler-11 is the first discovered exoplanetary system with more than three transiting planets.

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