Kepler-419 c
Sign in to saveKepler-419c (also known by its Kepler Object of Interest designation KOI-1474.02) is a super-Jupiter exoplanet orbiting within the habitable zone of the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years (1040 parsecs )from Earth in the constellation Cygnus. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion.
In the Vinony graph
Vinony's link graph records 65 inbound references to Kepler-419 c, and connects out to list of planet types, outer space and Kepler Space Telescope.
It sits within the topics Cygnus (constellation), Exoplanets discovered by the Kepler space telescope and Exoplanets discovered in 2014.
Vinony links it to 8 Wikipedia language editions.
Wikidata facts
- Constellation
- Cygnus
- Parent body
- Kepler-419
- Mass
- 7.3
- Orbital period
- 675.47
Show 14 more facts
- time of discovery or invention
- 2014-08-00
- discoverer or inventor
- Kepler Space Telescope
- right ascension
- 295.41791299680370
- declination
- 51.18476834617250
- epoch
- J2000.0
- discovery method
- transit-timing variation
- semi-major axis of an orbit
- 1.68
- orbital eccentricity
- 0.184
- right ascension component of proper motion
- -0.072
- declination component of proper motion
- -1.271
- parallax
- 0.9603
- catalog code
- TIC 27454084c
- argument of periapsis
- 275.3
- orbital inclination
- 88
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Encyclopedic overview
9 sectionsContents
- Physical characteristics
- Mass, radius and temperature
- Host star
- Orbit
- Habitability
- Discovery
- See also
- References
- External links
Kepler-419c (also known by its Kepler Object of Interest designation KOI-1474.02) is a super-Jupiter exoplanet orbiting within the habitable zone of the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years (1040 parsecs )from Earth in the constellation Cygnus. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion.
==Physical characteristics==
Excerpted from Wikipedia’s “Kepler-419 c” article, available under the CC BY-SA 4.0 licence.
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