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Kepler-6
Sign in to saveKepler-6 is a G-type star situated in the constellation Cygnus. The star lies within the field of view of the Kepler Mission, which discovered it as part of a NASA-led mission to discover Earth-like planets. The star, which is slightly larger, more metal-rich, slightly cooler, and more massive than the Sun, is orbited by at least one extrasolar planet, a Jupiter-sized planet named Kepler-6b that orbits closely to its star. thumb|Kepler-6
Astronomical data · SIMBAD
- Object type
- *
- Distance
- 1,906 light-years
- Redshift
- z = -0.00016126523679016458
- Coordinates
- RA 296.8372° · Dec 48.2399°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Distance from Earth
- 597.14
- Diameter
- 2020000
- Radius
- 1.39
- Mass
- 1.21
- Image
- Kepler-6-Sun comparison.png
Show 15 more facts
- catalog code
- KIC 10874614
- Commons category
- Kepler-6
- effective temperature
- 5647
- luminosity
- 1.4724084
- parallax
- 1.7108
- apparent magnitude
- 13.158453
- radial velocity
- -50.2
- metallicity
- 0.36
- stellar rotational velocity
- 2.1
- surface gravity
- 19500
- declination
- 48.23993306378
- right ascension component of proper motion
- 0.935
- declination component of proper motion
- 8.458
- right ascension
- 296.83724148235
- age estimated by a dating method
- 3.8
Sources (1)
via Wikidata · CC0
~3 min read
Article
5 sectionsContents
- Nomenclature and history
- Characteristics
- Planetary system
- See also
- References
Kepler-6 is a G-type star situated in the constellation Cygnus. The star lies within the field of view of the Kepler Mission, which discovered it as part of a NASA-led mission to discover Earth-like planets. The star, which is slightly larger, more metal-rich, slightly cooler, and more massive than the Sun, is orbited by at least one extrasolar planet, a Jupiter-sized planet named Kepler-6b that orbits closely to its star. thumb|Kepler-6
==Nomenclature and history== Kepler-6 was named for the Kepler Mission, a NASA project launched in 2009 that aims to discover Earth-like planets that transit, or cross in front of, their home stars with respect to Earth. Unlike stars like the Sun or Sirius, Kepler-6 does not have a common and colloquial name. The discovery of Kepler-6b was announced by the Kepler team on January 4, 2010 at the 215th meeting of the American Astronomical Society along with planets around Kepler-4, Kepler-5, Kepler-7, and Kepler-8. It was the third planet to be discovered by the Kepler spacecraft; the first three planets to be verified by data from Kepler had been previously discovered. These three planets were used to test the accuracy of Kepler's measurements.
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