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Q3195372
EntityQ3195372· pop 10· linked from 181 articles

Kepler-14b is an extrasolar planet in orbit around the primary star of the binary Kepler-14 system. It is currently the only planet known to exist in this star system. Kepler-14b is 8.4 times the mass of Jupiter and has a radius 1.14 times that of Jupiter, and it orbits its host star every 6.79 days. It was discovered by NASA-led Kepler mission, which noted the planet as a planetary candidate as early as March 2009, around the same time as the discovery of the first five planets discovered by Kepler (Kepler-4b to Kepler-8b). However, the team was unable to confirm the planet until extensive fo

Astronomical data · SIMBAD

Object type
Pl
Coordinates
RA 287.7088° · Dec 47.3330°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Planet.name
Kepler-14b
Planet.discoverer
L. Buchhave et al.
Planet.discovery_site
Kepler spacecraft
Planet.discovered
Paper submitted 27 June 2011
Planet.discovery_method
Transit method
Planet.apsis
astron
Planet.eccentricity
0.035 (± 0.02)
Planet.period
d
Planet.inclination
90.0
Planet.star
Kepler-14A (KOI-98)
Planet.mean_radius
1.136
Planet.mass
8.40
Planet.density
7.1 (± 1.1) g cm−3

via Wikipedia infobox

~7 min read

Encyclopedic overview

4 sections
Contents
  • Discovery
  • Host star system
  • Characteristics
  • References

Kepler-14b is an extrasolar planet in orbit around the primary star of the binary Kepler-14 system. It is currently the only planet known to exist in this star system. Kepler-14b is 8.4 times the mass of Jupiter and has a radius 1.14 times that of Jupiter, and it orbits its host star every 6.79 days. It was discovered by NASA-led Kepler mission, which noted the planet as a planetary candidate as early as March 2009, around the same time as the discovery of the first five planets discovered by Kepler (Kepler-4b to Kepler-8b). However, the team was unable to confirm the planet until extensive follow-up observations, as high-resolution imaging resolved the star Kepler-14 as a closely orbiting binary system. The Kepler team would have not noticed that Kepler-14 was a binary star based solely on initial radial velocity measurements (a standard method for confirming a planet's existence), and found that if they had not realized this, their data on Kepler-14b would have been very inaccurate.

==Discovery==

Excerpted from Wikipedia’s “Q3195372” article, available under the CC BY-SA 4.0 licence.