Kepler-419 b
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Kepler-419b (also known by its Kepler Object of Interest designation KOI-1474.01) is a hot Jupiter exoplanet orbiting 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.
In the Vinony graph
Vinony's link graph records 368 inbound references to Kepler-419 b, 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 6 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- Pl
- Distance
- 3,284 light-years
- Coordinates
- RA 295.4179° · Dec 51.1848°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Constellation
- Cygnus
- Parent body
- Kepler-419
- Radius
- 34.09
- Mass
- 2.5
- Orbital period
- 69.7546
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 method
- argument of periapsis
- 95.2
- orbital inclination
- 88.95
- semi-major axis of an orbit
- 0.37
- orbital eccentricity
- 0.8
- right ascension component of proper motion
- -0.072
- declination component of proper motion
- -1.271
- parallax
- 0.9603
- catalog code
- TIC 27454084b
via Wikidata · CC0
~2 min read
Encyclopedic overview
7 sectionsContents
- Characteristics
- Mass, radius and temperature
- Host star
- Orbit
- Discovery
- References
- External links
Kepler-419b (also known by its Kepler Object of Interest designation KOI-1474.01) is a hot Jupiter exoplanet orbiting 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.
==Characteristics==
Excerpted from Wikipedia’s “Kepler-419 b” article, available under the CC BY-SA 4.0 licence.