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Kepler-7
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Kepler-7 is a star located in the constellation Lyra in the field of view of the Kepler Mission, a NASA operation in search of Earth-like planets. It is home to the fourth of the first five planets that Kepler discovered; this planet, a Jupiter-size gas giant named Kepler-7b, is as light as styrofoam. The star itself is more massive than the Sun, and is nearly twice the Sun's radius. It is also slightly metal-rich, a major factor in the formation of planetary systems. Kepler-7's planet was presented on January 4, 2010 at a meeting of the American Astronomical Society.

Wikidata facts

Distance from Earth
947.46
Diameter
2730000
Radius
1.97
Mass
1.36
Image
Kepler-7-Sun comparison.png
Show 16 more facts
Commons category
Kepler-7
spectral class
F9
catalog code
TIC 121660904
effective temperature
5933
parallax
1.0319
metallicity
0.13
stellar rotational velocity
0
surface gravity
11000
luminosity
4.7402935
right ascension component of proper motion
-2.937
declination component of proper motion
-21.084
right ascension
288.5815096274
declination
41.08982427198
radial velocity
1.5
apparent magnitude
11.535
age estimated by a dating method
3.5
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Article

6 sections
Contents
  • Nomenclature and discovery
  • Characteristics
  • Planetary system
  • See also
  • References
  • External links

Kepler-7 is a star located in the constellation Lyra in the field of view of the Kepler Mission, a NASA operation in search of Earth-like planets. It is home to the fourth of the first five planets that Kepler discovered; this planet, a Jupiter-size gas giant named Kepler-7b, is as light as styrofoam. The star itself is more massive than the Sun, and is nearly twice the Sun's radius. It is also slightly metal-rich, a major factor in the formation of planetary systems. Kepler-7's planet was presented on January 4, 2010 at a meeting of the American Astronomical Society.

==Nomenclature and discovery== Kepler-7 received its name because it was the home to the seventh planetary system discovered by the NASA-led Kepler Mission, a project aimed at detecting terrestrial planets that transit, or pass in front of, their host stars as seen from Earth. The planet orbiting Kepler-7 was the fourth planet to be discovered by the Kepler spacecraft; the first three planets combed from Kepler's data had been previously discovered, and were used to verify the accuracy of Kepler's measurements. Kepler-7b was announced to the public on January 4, 2010 at the 215th meeting of the American Astronomical Society in Washington, D.C. along with Kepler-4b, Kepler-5b, Kepler-6b, and Kepler-8b. Kepler-7b was noted for its unusually and extremely low density.

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