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Kepler-78 (formerly known as KIC 8435766) is a 12th magnitude star away in the constellation Cygnus. Initially classified as an eclipsing binary with orbital period 0.710015 days, it was later re-classified as a single star with significant interaction between star magnetosphere and close-in planet. The radius of the star is of about 74% of the Sun, and the effective temperature is about .

Astronomical data · SIMBAD

Object type
EB*
Spectral type
K2.5V
Distance
407 light-years
Redshift
z = -0.00000827235534495152
Coordinates
RA 293.7417° · Dec 44.4483°
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Wikidata facts

Distance from Earth
124.376
Diameter
1090000
Radius
0.7475
Mass
0.779
Image
Kepler-78b.png
Show 15 more facts
effective temperature
5058
apparent magnitude
11.525862
spectral class
K0V
radial velocity
-4.21
parallax
8.0085
metallicity
0
catalog code
TYC 3147-188-1
surface gravity
36000
stellar rotational velocity
2.0
luminosity
0.31175715
right ascension component of proper motion
38.195
declination component of proper motion
-16.309
right ascension
293.74172391967
declination
44.44832227415
age estimated by a dating method
0.625

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Article

2 sections
Contents
  • Planetary system
  • References

Kepler-78 (formerly known as KIC 8435766) is a 12th magnitude star away in the constellation Cygnus. Initially classified as an eclipsing binary with orbital period 0.710015 days, it was later re-classified as a single star with significant interaction between star magnetosphere and close-in planet. The radius of the star is of about 74% of the Sun, and the effective temperature is about .

==Planetary system== The Kepler-78 planetary system is composed of one known planet called Kepler-78b, a planet slightly bigger than Earth with an extremely close orbit to the parent star. The orbital period of this planet is about 8.5 hours because of its proximity to its star. While it has a similar density to the Earth (at 5.57 g/cm3), its surface temperature is about 1300 to 1500 K.

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