Imaginary Picture of Kepler-195 c
/
Exoplanet Name : Kepler-195 c
Alternate Name :
Radius (Rjup / Re): 0.1380 (Rjup) 1.5468 (Rearth)
Mass (Mjup / Me): 0.0124 (Mjup) 3.9582 (Mearth)
Semi Major Axis / Orbital Distance Calculated 0.1970 (AU) 0.1970 (AU Est.)
Eccentricity : 0.0000
Orbital Period(Yrs) 0.0933
Orbital Period(Observed/Estimated) 34.10 (Days Obs.) 31.62 (Days Est.)
Star Radiation at Atmospheric Boundary: 15504.0 (W/m2)
Measured Temperature (K) 0.0 (K)
Blackbody T 0.1(K) 498.0 (K)
Blackbody T 0.3(K) 467.7 (K)
Blackbody T 0.7(K) 378.4 (K)
Tidally Locked Blackbody T 0.1(K) 592.3 (K)
Tidally Locked Blackbody T 0.3(K) 556.2 (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-195
Alternate Name :
Star Distance(LY) : 0.0
Stellar Radius(Rsun) : 0.8 (Rsun Measured)
Stellar Mass(Msun) : 1.0 (Msun Measured) 0.9 (Msun Estimated)
Star Age : 0.0 (GY)
Temperature : 5329 (K)
Spectral type : K0
Metalicity : -0.1
Absolute Magnitude: 25.0
Apparent Magnitude: 13.5
Right Ascension(RA) 288.1210
Declination (DEC) 47.9667
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-195%20c/
Kepler-195 c
Kepler-195 c

  • Kepler-195 c is an exoplanet orbiting the star Kepler-195. Its discovery was publicly announced on 2014.
  • The host star Kepler-195 has apparent magnitude of 13.5, with absolute magnitude of 25.0.
  • It is 1.0 times more massive and 0.8 times bigger compared with our Sun. The surface temperature is 5329 with its spectral types of K0
  • In this planetary system, the extrasolar planet Kepler-195 c orbits around the star Kepler-195 every 34.1 days with its orbital distance of 0.20 AU ( 29470780.5 km)
  • (Projected orbit of Kepler-195 c around its host star Kepler-195)


  • The Star Kepler-195 's habitable zone is located at the following distance
  • Inner Boundary (the orbital distance at Venus's Equivalent Radiation ) : 0.480 AU ( 71786727.5 km)
  • Earth Boundary (the orbital distance at Earth's Equivalent Radiation) : 0.663 AU ( 99228017.5 km)
  • Outer Boundary (the orbital distance at Mars's Equivalent Radiation) : 1.011 AU ( 151201539.5 km)
  • Snow Line (the orbital distance at Snow Line Equivalent Radiation) : 1.487 AU ( 222499689.1 km)
  • Radiation at Planetary Boundary of Kepler-195 c : 15504.02 W/m2

    (Habitable zone calculated based on SEAU(Solar Equivalent Astronomical Unit) around the star Kepler-195)



  • Kopparapu Recent Venus for Star Kepler-195 distance : 0.510 AU
  • Kopparapu Runaway Greenhouse for Earth-sized planet for Star Kepler-195 distance : 0.646 AU
  • Kopparapu Runaway Greenhouse for Super-Earth-sized planet for Star Kepler-195 distance : 0.624 AU
  • Kopparapu Runaway Greenhouse for Mars-sized planet for Star Kepler-195 distance : 0.685 AU
  • Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-195 distance : 1.157 AU
  • Kopparapu Outer Boundary for Early Mars for Star Kepler-195 distance : 1.220 AU

    (Habitable zone calculated based on Kopparapu et al.(2013) around the star Kepler-195)



  • Original Kopparapu Recent Venus for Star Kepler-195 distance : 0.507 AU
  • Original Kopparapu Runaway Greenhouse for Star Kepler-195 distance : 0.665 AU
  • Original Kopparapu Moist Greenhouse for Star Kepler-195 distance : 0.671 AU
  • Original Kopparapu Outer Boundary for Maximum Greenhouse for Star Kepler-195 distance : 1.177 AU
  • Original Kopparapu Outer Boundary for Early Mars for Star Kepler-195 distance : 1.224 AU

    (Habitable zone calculated based on Kopparapu et al.(Original) around the star Kepler-195)



    (Position in Stellar Map of star Kepler-195 and its Exoplanet Kepler-195 c)



    (Zoomed position in Stellar Map of star Kepler-195 and its Exoplanet Kepler-195 c (zoom level 3))