Imaginary Picture of Kepler-365 c
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Exoplanet Name : Kepler-365 c
Alternate Name :
Radius (Rjup / Re): 0.1460 (Rjup) 1.6365 (Rearth)
Mass (Mjup / Me): 0.0131 (Mjup) 4.1712 (Mearth)
Semi Major Axis / Orbital Distance Calculated 0.1370 (AU) 0.1370 (AU Est.)
Eccentricity : 0.0000
Orbital Period(Yrs) 0.0487
Orbital Period(Observed/Estimated) 17.78 (Days Obs.) 18.61 (Days Est.)
Star Radiation at Atmospheric Boundary: 94106.2 (W/m2)
Measured Temperature (K) 0.0 (K)
Blackbody T 0.1(K) 781.7 (K)
Blackbody T 0.3(K) 734.1 (K)
Blackbody T 0.7(K) 594.0 (K)
Tidally Locked Blackbody T 0.1(K) 929.6 (K)
Tidally Locked Blackbody T 0.3(K) 873.0 (K)
Size Class: super-Earth-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-365
Alternate Name :
Star Distance(LY) : 0.0
Stellar Radius(Rsun) : 1.1 (Rsun Measured)
Stellar Mass(Msun) : 1.0 (Msun Measured) 1.1 (Msun Estimated)
Star Age : 0.0 (GY)
Temperature : 6012 (K)
Spectral type : G0
Metalicity : -0.0
Absolute Magnitude: 25.0
Apparent Magnitude: 13.5
Right Ascension(RA) 295.6266
Declination (DEC) 49.1304
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-365%20c/
Kepler-365 c
Kepler-365 c

  • Kepler-365 c is an exoplanet orbiting the star Kepler-365. Its discovery was publicly announced on 2014.
  • The host star Kepler-365 has apparent magnitude of 13.5, with absolute magnitude of 25.0.
  • It is 1.0 times more massive and 1.1 times bigger compared with our Sun. The surface temperature is 6012 with its spectral types of G0
  • In this planetary system, the extrasolar planet Kepler-365 c orbits around the star Kepler-365 every 17.8 days with its orbital distance of 0.14 AU ( 20494908.3 km)
  • (Projected orbit of Kepler-365 c around its host star Kepler-365)


  • The Star Kepler-365 's habitable zone is located at the following distance
  • Inner Boundary (the orbital distance at Venus's Equivalent Radiation ) : 0.822 AU ( 122994404.9 km)
  • Earth Boundary (the orbital distance at Earth's Equivalent Radiation) : 1.136 AU ( 170010409.8 km)
  • Outer Boundary (the orbital distance at Mars's Equivalent Radiation) : 1.732 AU ( 259058241.3 km)
  • Snow Line (the orbital distance at Snow Line Equivalent Radiation) : 2.548 AU ( 381215550.7 km)
  • Radiation at Planetary Boundary of Kepler-365 c : 94106.18 W/m2

    (Habitable zone calculated based on SEAU(Solar Equivalent Astronomical Unit) around the star Kepler-365)



  • Kopparapu Recent Venus for Star Kepler-365 distance : 0.840 AU
  • Kopparapu Runaway Greenhouse for Earth-sized planet for Star Kepler-365 distance : 1.064 AU
  • Kopparapu Runaway Greenhouse for Super-Earth-sized planet for Star Kepler-365 distance : 1.028 AU
  • Kopparapu Runaway Greenhouse for Mars-sized planet for Star Kepler-365 distance : 1.126 AU
  • Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-365 distance : 1.868 AU
  • Kopparapu Outer Boundary for Early Mars for Star Kepler-365 distance : 1.970 AU

    (Habitable zone calculated based on Kopparapu et al.(2013) around the star Kepler-365)



  • Original Kopparapu Recent Venus for Star Kepler-365 distance : 0.845 AU
  • Original Kopparapu Runaway Greenhouse for Star Kepler-365 distance : 1.092 AU
  • Original Kopparapu Moist Greenhouse for Star Kepler-365 distance : 1.118 AU
  • Original Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-365 distance : 1.901 AU
  • Original Kopparapu Outer Boundary for Early Mars for Star Kepler-365 distance : 1.977 AU

    (Habitable zone calculated based on Kopparapu et al.(Original) around the star Kepler-365)



    (Position in Stellar Map of star Kepler-365 and its Exoplanet Kepler-365 c)



    (Zoomed position in Stellar Map of star Kepler-365 and its Exoplanet Kepler-365 c (zoom level 3))