Imaginary Picture of Kepler-192 c
/
Exoplanet Name : Kepler-192 c
Alternate Name :
Radius (Rjup / Re): 0.2490 (Rjup) 2.7910 (Rearth)
Mass (Mjup / Me): 0.0216 (Mjup) 6.8529 (Mearth)
Semi Major Axis / Orbital Distance Calculated 0.1500 (AU) 0.1500 (AU Est.)
Eccentricity : 0.0000
Orbital Period(Yrs) 0.0581
Orbital Period(Observed/Estimated) 21.22 (Days Obs.) 21.17 (Days Est.)
Star Radiation at Atmospheric Boundary: 50103.8 (W/m2)
Measured Temperature (K) 0.0 (K)
Blackbody T 0.1(K) 667.7 (K)
Blackbody T 0.3(K) 627.1 (K)
Blackbody T 0.7(K) 507.4 (K)
Tidally Locked Blackbody T 0.1(K) 794.1 (K)
Tidally Locked Blackbody T 0.3(K) 745.7 (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-192
Alternate Name :
Star Distance(LY) : 0.0
Stellar Radius(Rsun) : 1.0 (Rsun Measured)
Stellar Mass(Msun) : 1.0 (Msun Measured) 1.0 (Msun Estimated)
Star Age : 0.0 (GY)
Temperature : 5479 (K)
Spectral type : G7
Metalicity : -0.2
Absolute Magnitude: 25.0
Apparent Magnitude: 12.9
Right Ascension(RA) 287.9179
Declination (DEC) 45.5929
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-192%20c/
Kepler-192 c
Kepler-192 c

  • Kepler-192 c is an exoplanet orbiting the star Kepler-192. Its discovery was publicly announced on 2014.
  • The host star Kepler-192 has apparent magnitude of 12.9, with absolute magnitude of 25.0.
  • It is 1.0 times more massive and 1.0 times bigger compared with our Sun. The surface temperature is 5479 with its spectral types of G7
  • In this planetary system, the extrasolar planet Kepler-192 c orbits around the star Kepler-192 every 21.2 days with its orbital distance of 0.15 AU ( 22439680.6 km)
  • (Projected orbit of Kepler-192 c around its host star Kepler-192)


  • The Star Kepler-192 's habitable zone is located at the following distance
  • Inner Boundary (the orbital distance at Venus's Equivalent Radiation ) : 0.657 AU ( 98261205.3 km)
  • Earth Boundary (the orbital distance at Earth's Equivalent Radiation) : 0.908 AU ( 135822664.5 km)
  • Outer Boundary (the orbital distance at Mars's Equivalent Radiation) : 1.383 AU ( 206963683.2 km)
  • Snow Line (the orbital distance at Snow Line Equivalent Radiation) : 2.036 AU ( 304556126.3 km)
  • Radiation at Planetary Boundary of Kepler-192 c : 50103.75 W/m2

    (Habitable zone calculated based on SEAU(Solar Equivalent Astronomical Unit) around the star Kepler-192)



  • Kopparapu Recent Venus for Star Kepler-192 distance : 0.693 AU
  • Kopparapu Runaway Greenhouse for Earth-sized planet for Star Kepler-192 distance : 0.877 AU
  • Kopparapu Runaway Greenhouse for Super-Earth-sized planet for Star Kepler-192 distance : 0.847 AU
  • Kopparapu Runaway Greenhouse for Mars-sized planet for Star Kepler-192 distance : 0.929 AU
  • Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-192 distance : 1.563 AU
  • Kopparapu Outer Boundary for Early Mars for Star Kepler-192 distance : 1.648 AU

    (Habitable zone calculated based on Kopparapu et al.(2013) around the star Kepler-192)



  • Original Kopparapu Recent Venus for Star Kepler-192 distance : 0.690 AU
  • Original Kopparapu Runaway Greenhouse for Star Kepler-192 distance : 0.902 AU
  • Original Kopparapu Moist Greenhouse for Star Kepler-192 distance : 0.913 AU
  • Original Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-192 distance : 1.590 AU
  • Original Kopparapu Outer Boundary for Early Mars for Star Kepler-192 distance : 1.653 AU

    (Habitable zone calculated based on Kopparapu et al.(Original) around the star Kepler-192)



    (Position in Stellar Map of star Kepler-192 and its Exoplanet Kepler-192 c)



    (Zoomed position in Stellar Map of star Kepler-192 and its Exoplanet Kepler-192 c (zoom level 3))