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Kepler-68c

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Also known as Kepler-68Ac

Kepler-68c is an Earth-sized planet orbiting the star Kepler-68 in the constellation of Cygnus. It was discovered by planetary-transit methods by the Kepler space telescope in February 2013. It has a mass of 4.8 times that of Earth (0.015 MJ) and a radius of 0.953 Earth radii. It has an orbital period of 9.605085 days at a distance of about 0.09059 AU from its star. Relatively wide constraints on Kepler-68c's mass are the result lack of detection of the planet through radial-velocity and transit-timing-variation methods.

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Vinony's link graph records 82 inbound references to Kepler-68c, and connects out to Kepler Space Telescope, Kepler-69 and mass.

It sits within the topics Cygnus (constellation), Exoplanets discovered by the Kepler space telescope and Exoplanets discovered in 2013.

Vinony links it to 5 Wikipedia language editions.

Astronomical data · SIMBAD

Object type
Pl
Distance
471 light-years
Coordinates
RA 291.0324° · Dec 49.0403°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Wikidata facts

Instance of
star
Constellation
Cygnus
Parent body
Kepler-68
Radius
0.0827
Mass
0.00642
Orbital period
9.6051
Image
Kepler-68 c.jpg
Show 15 more facts
catalog code
Kepler-68c
discovery method
transit method
time of discovery or invention
2013-03-00
discoverer or inventor
Kepler Space Telescope
right ascension
291.03235837937075
declination
49.04025783364222
epoch
J2000.0
orbital inclination
86.93
semi-major axis of an orbit
0.09059
argument of periapsis
0.0
orbital eccentricity
0.099
right ascension component of proper motion
-7.334
declination component of proper motion
-10.430
parallax
6.9076
M sin i
2.669529507

via Wikidata · CC0

~1 min read

Encyclopedic overview

2 sections
Contents
  • See also
  • References

Kepler-68c is an Earth-sized planet orbiting the star Kepler-68 in the constellation of Cygnus. It was discovered by planetary-transit methods by the Kepler space telescope in February 2013. It has a mass of 4.8 times that of Earth (0.015 MJ) and a radius of 0.953 Earth radii. It has an orbital period of 9.605085 days at a distance of about 0.09059 AU from its star. Relatively wide constraints on Kepler-68c's mass are the result lack of detection of the planet through radial-velocity and transit-timing-variation methods.

==See also== List of planets discovered by the Kepler spacecraft

Excerpted from Wikipedia’s “Kepler-68c” article, available under the CC BY-SA 4.0 licence.

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