Imaginary Picture of Kepler-110 c
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Exoplanet Name : Kepler-110 c
Alternate Name :
Radius (Rjup / Re): 0.1970 (Rjup) 2.2082 (Rearth)
Mass (Mjup / Me): 0.0173 (Mjup) 5.5114 (Mearth)
Semi Major Axis / Orbital Distance Calculated 0.1980 (AU) 0.1980 (AU Est.)
Eccentricity : 0.0000
Orbital Period(Yrs) 0.0868
Orbital Period(Observed/Estimated) 31.72 (Days Obs.) 36.44 (Days Est.)
Star Radiation at Atmospheric Boundary: 52198.2 (W/m2)
Measured Temperature (K) 0.0 (K)
Blackbody T 0.1(K) 674.6 (K)
Blackbody T 0.3(K) 633.5 (K)
Blackbody T 0.7(K) 512.6 (K)
Tidally Locked Blackbody T 0.1(K) 802.3 (K)
Tidally Locked Blackbody T 0.3(K) 753.4 (K)
Size Class: sub-Neptune-size
Mass Class:
Detection Type : Primary Transit
Mass Detection :
Radius Detection :
Habitability by Solar Eq. Astronomical Unit: Not habitable
Habitability by Kopparapu: Not habitable
Star Name : Kepler-110
Alternate Name :
Star Distance(LY) : 0.0
Stellar Radius(Rsun) : 1.1 (Rsun Measured)
Stellar Mass(Msun) : 0.8 (Msun Measured) 1.0 (Msun Estimated)
Star Age : 0.0 (GY)
Temperature : 5960 (K)
Spectral type : G1
Metalicity : -0.2
Absolute Magnitude: 25.0
Apparent Magnitude: 11.9
Right Ascension(RA) 292.9291
Declination (DEC) 48.6028
Hubble Space Telescope Guide Star Catalog (GSC) ID 0
Discovered by
Discovery Paper - Authors 0
Discovery Paper - Title
Discovery Paper - Journal 0
Discovery Paper - URL 0
SIMBAD LINK 0
Open Exoplanet Database Link http://www.openexoplanetcatalogue.com/planet/Kepler-110%20c/
Kepler-110 c
Kepler-110 c

  • Kepler-110 c is an exoplanet orbiting the star Kepler-110. Its discovery was publicly announced on 2014.
  • The host star Kepler-110 has apparent magnitude of 11.9, with absolute magnitude of 25.0.
  • It is 0.8 times more massive and 1.1 times bigger compared with our Sun. The surface temperature is 5960 with its spectral types of G1
  • In this planetary system, the extrasolar planet Kepler-110 c orbits around the star Kepler-110 every 31.7 days with its orbital distance of 0.20 AU ( 29620378.4 km)
  • (Projected orbit of Kepler-110 c around its host star Kepler-110)


  • The Star Kepler-110 's habitable zone is located at the following distance
  • Inner Boundary (the orbital distance at Venus's Equivalent Radiation ) : 0.885 AU ( 132387954.6 km)
  • Earth Boundary (the orbital distance at Earth's Equivalent Radiation) : 1.223 AU ( 182994750.3 km)
  • Outer Boundary (the orbital distance at Mars's Equivalent Radiation) : 1.864 AU ( 278843502.9 km)
  • Snow Line (the orbital distance at Snow Line Equivalent Radiation) : 2.743 AU ( 410330429.8 km)
  • Radiation at Planetary Boundary of Kepler-110 c : 52198.15 W/m2

    (Habitable zone calculated based on SEAU(Solar Equivalent Astronomical Unit) around the star Kepler-110)



  • Kopparapu Recent Venus for Star Kepler-110 distance : 0.907 AU
  • Kopparapu Runaway Greenhouse for Earth-sized planet for Star Kepler-110 distance : 1.149 AU
  • Kopparapu Runaway Greenhouse for Super-Earth-sized planet for Star Kepler-110 distance : 1.109 AU
  • Kopparapu Runaway Greenhouse for Mars-sized planet for Star Kepler-110 distance : 1.216 AU
  • Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-110 distance : 2.019 AU
  • Kopparapu Outer Boundary for Early Mars for Star Kepler-110 distance : 2.130 AU

    (Habitable zone calculated based on Kopparapu et al.(2013) around the star Kepler-110)



  • Original Kopparapu Recent Venus for Star Kepler-110 distance : 0.912 AU
  • Original Kopparapu Runaway Greenhouse for Star Kepler-110 distance : 1.180 AU
  • Original Kopparapu Moist Greenhouse for Star Kepler-110 distance : 1.206 AU
  • Original Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-110 distance : 2.055 AU
  • Original Kopparapu Outer Boundary for Early Mars for Star Kepler-110 distance : 2.137 AU

    (Habitable zone calculated based on Kopparapu et al.(Original) around the star Kepler-110)



    (Position in Stellar Map of star Kepler-110 and its Exoplanet Kepler-110 c)



    (Zoomed position in Stellar Map of star Kepler-110 and its Exoplanet Kepler-110 c (zoom level 3))