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Kepler-19 b

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Kepler-19b is a planet orbiting around the star Kepler-19. The planet has an orbital period of 9.3 days, with an estimated radius of roughly 2.2 times that of the Earth, with a mass around 8.4 times that of the Earth. It is one of three planets orbiting Kepler-19.

In the Vinony graph

Within Vinony's link graph, Kepler-19 b is referenced by 11 other articles, and connects out to method of detecting extrasolar planets, Earth and day.

It is catalogued under topics including Exoplanets discovered by the Kepler space telescope and Exoplanets discovered in 2011.

Its subject is documented across 9 Wikipedia language editions.

Astronomical data · SIMBAD

Object type
Pl
Distance
720 light-years
Coordinates
RA 290.4208° · Dec 37.8518°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Wikidata facts

Instance of
exoplanet
Constellation
Lyra
Parent body
Kepler-19
Diameter
31500
Radius
0.198
Mass
0.02643
Orbital period
9.28716
Image
Kepler-19 b.jpg
Show 15 more facts
catalog code
Kepler-19b
right ascension
290.42083156988997
discovery method
transit method
time of discovery or invention
2011-12-00
discoverer or inventor
Kepler Space Telescope
declination
37.85178785031417
epoch
J2000.0
orbital eccentricity
0.41
orbital inclination
89.94
semi-major axis of an orbit
0.085
right ascension component of proper motion
25.284
declination component of proper motion
-30.711
parallax
4.5465
M sin i
0.02327759556
argument of periapsis
59.1
Sources (1)

via Wikidata · CC0

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Encyclopedic overview

3 sections
Contents
  • See also
  • Other planets in the Kepler-19 system
  • References

Kepler-19b is a planet orbiting around the star Kepler-19. The planet has an orbital period of 9.3 days, with an estimated radius of roughly 2.2 times that of the Earth, with a mass around 8.4 times that of the Earth. It is one of three planets orbiting Kepler-19.

==See also== List of planets discovered by the Kepler spacecraft Exoplanet Planetary System

Excerpted from Wikipedia’s “Kepler-19 b” article, available under the CC BY-SA 4.0 licence.

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