Kepler 102

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Star
Kepler-102
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation lyre
Right ascension 18 h 45 m 55.86 s
declination + 47 ° 12 ′ 28.8 ″
Apparent brightness 12.07 ± 0.19 mag
Typing
Known exoplanets 5
B − V color index (0.51) 
Spectral class K3 V
Astrometry
Radial velocity (-27.67 ± 0.61) km / s
parallax (9.25 ± 0.02)  mas
distance (352 ± 1)  ly
(108)  pc
Proper movement 
Rec. Share: (−41.14 ± 0.04)  mas / a
Dec. portion: (−43.14 ± 0.04)  mas / a
Physical Properties
Dimensions 0.81   +0.04−0.09 M
radius 0.76 ± 0.07  R
Luminosity

0.3 ± 0.1  L

Effective temperature 4,909 ± 41  K
Metallicity [Fe / H] 0.18   +0.42−0.47
Age 1.41 billion  a
Other names
and catalog entries
Tycho catalog TYC 3544-1383-1 [1]Template: Infobox star / maintenance / specification of the TYC catalog
2MASS catalog 2MASS J18455585 + 4712289 [2]
Other names KIC 10187017, KOI-82, Kepler-102

Kepler-102 is a star in the constellation Lyra . The star in a main sequence star of the spectral class K. Its mass and radius as well as its luminosity are aösp lower than those of the sun . The system is approximately 350 LJ from the sun. Kepler-102 has a planetary system made up of five known exoplanets .

Planetary system

The discovery of 49 exoplanet candidates around 22 stars, including Kepler-102, was published in January 2014 based on observations from the Kepler Space Telescope . The two innermost planets and the outermost planet have a smaller radius than the earth . The largest planet is Kepler-102d, whose mass could be determined from measurements of the radial velocity to be a little less than 9 Earth masses . All planets need far less time to orbit their central star than Mercury does to orbit the sun.

Planetary system from Kepler-102
Planet
(by distance from the star)
Discovery
(year)
Radius
(in )
Mass
(in M )
Cycle time
(in days)
Major semi-axis
(in AU )
eccentricity
Kepler-102b 2014 0.47 ± 0.02 0.41 ± 1.6 5,28696 - -
Kepler-102c 2014 0.58 ± 0.02 <3.0 7.07142 - -
Kepler-102d 2014 1.18 ± 0.04 3.80 ± 1.8 10.3117 - -
Kepler-102e 2014 2.22 ± 0.07 8.93 ± 2.0 16.1457 - -
Kepler-102f 2014 0.88 ± 0.03 0.62 ± 3.3 27.4536 - -

Individual evidence

  1. a b c d e f g KOI-82. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed on September 3, 2018 .
  2. a b c d e f g h i j k NASA Exoplanet Archive: Kepler 102.Retrieved September 3, 2018 .
  3. ^ A b Marcy, Geoffrey W. et al .: Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets . arxiv : 1401.4195 .