|Exoplanet||List of exoplanets|
|Right ascension||(α)||19h 47m 20.9s|
|Declination||(δ)||+48° 14′ 23.8″|
|Mass||(m)||1.209 ± 0.04  M☉|
|Radius||(r)||1.391 ± 0.024  R☉|
|Temperature||(T)||5647 ± 44  K|
|Metallicity||[Fe/H]||0.34 ± 0.06 |
|Age||3.8 ± 1.0  Gyr|
|Mass||(m)||0.669 ± 0.027 MJ|
|Radius||(r)||1.323 ± 0.026 RJ|
|Density||(ρ)||0.352 ± 0.019 kg m−3|
|Temperature||(T)||1660 ± 100|
|Semi-major axis||(a)||0.04567 ±0.00050  AU|
|Orbital period||(P)||3.234723 ± 0.000017  d|
|Inclination||(i)||86.8 ± 0.3 °|
|Discovery method||Transit (Kepler Mission)|
|Other detection methods||Radial velocity,
|Discovery status||Conference announcement|
Kepler-6b is an extrasolar planet in the orbit of the unusually metal-rich Kepler-6, a star in the field of view of the NASA-operated Kepler spacecraft, which searches for planets that cross directly in front of, or transit, their host stars. It was the third planet to be discovered by Kepler. Kepler-6 orbits its host star every three days from a distance of .046 AU. Its proximity to Kepler-6 inflated the planet, about two-thirds the mass of Jupiter, to slightly larger than Jupiter's size and greatly heated its atmosphere.
Follow-up observations led to the planet's confirmation, which was announced at a meeting of the American Astronomical Society on January 4, 2010 along with four other Kepler-discovered planets.
Discovery and naming
NASA's Kepler satellite trails the Earth and continually observes a portion of the sky between the constellations Cygnus and Lyra. It is devised to search for and discover planets that transit, or cross in front of, their host stars with respect to Earth by measuring small and generally periodic variations in a star's brightness. Kepler recognized a potential transit event around a star that was designated KOI-017, which was named Kepler-6 after the confirmation of Kepler-6b. The star was designated "6" because it was the sixth planet to be observed (but the third planet to be discovered) by the Kepler satellite.
After the initial detection of a transit signal by Kepler, follow-up observations were taken to confirm the planetary nature of the candidate. Speckle imaging by the WIYN Telescope was used to determine the amount of light from nearby, background stars that was present. If not accounted for, this light would have made Kepler-6 appear brighter than it actually was. Consequently, the size of Kepler-6b would have been underestimated. Radial velocity data was taken by HIRES at the Keck I telescope in order to determine the mass of the planet. Independently, observations were made with the Spitzer Space Telescope at infrared wavelengths of 3.6 and 4.5 micrometres. Along with additional data taken by Kepler, these observations detected the occultation and phase curves of Kepler-6b behind its star.
The confirmation of Kepler-6b was announced at the 215th meeting of the American Astronomical Society with the discoveries of planets Kepler-4b, Kepler-5b, Kepler-7b, and Kepler-8b on January 4, 2010.
Kepler-6 is a sunlike star in the Cygnus constellation. It is approximately 20.9% more massive than and 39.1% larger than the Sun. With an effective temperature of 5647 K, Kepler-6 is cooler than the Sun. It is predicted to be 3.8 billion years old, compared to the Sun's age of 4.6 billion years. It is most notable for its unusually high metallicity for an exoplanet-bearing star; with an [Fe/H] = 0.34, Kepler-6 has 2.18 times more iron than the Sun does. Kepler-6b is the only planet that has been discovered in the orbit of Kepler-6.
Kepler-6b is a hot Jupiter, having a mass 0.669 times that of Jupiter, but an average distance of only 0.046 AU from its star and, thus, an orbital period of 3.23 days. It is almost 10 times closer to its star than Mercury is from our Sun. As a result, Kepler-6b is strongly irradiated by its star, heating its atmosphere to a temperature of 1660 K and puffing it up to a size 1.3 times that of Jupiter. It may also be the case that Kepler-6b has a thermal inversion of its atmosphere, where temperature increases with increasing distance from the center of the planet. However, additional observations are required to confirm or refute this possibility.
- Borucki, William J.; et al. (2010-01-07). "Kepler Planet-Detection Mission: Introduction and First Results". sciencemag.org. Retrieved 2011-04-14.
- Dunham, Edward W.; et al. (2010-04-20). "Kepler-6b: A Transiting Hot Jupiter Orbiting a Metal-rich Star". Astrophysical Journal. Retrieved 2011-04-14.
- Desert, Jean-Michael; et al. (2011-02-03). "The atmospheres of the hot-Jupiters Kepler-5b and Kepler-6b observed during occultations with Warm-Spitzer and Kepler". arXiv: .
- "Kepler: About the Mission". Kepler Mission. NASA. 2011. Retrieved 29 April 2011.
- "Summary Table of Kepler Discoveries". NASA. 2010-03-15. Retrieved 2010-03-18.
- Rich Talcott (5 January 2010). "215th AAS meeting update: Kepler discoveries the talk of the town". Astronomy.com. Astronomy magazine. Retrieved 30 April 2011.
- Jean Schneider (2010). "Notes for star Kepler-6". Extrasolar Planets Encyclopaedia. Retrieved 30 April 2011.
Media related to Kepler-6 b at Wikimedia Commons