Imaginary Picture of AE 1 b

Display orbital revolution of AE 1 b around the hoststar AE 1
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Exoplanet Name : AE 1 b
Alternate Name :
Status : Confirmed
Radius (Rjup / Re): 0.9078 (Rjup) 10.1759 (Rearth)
Mass (Mjup / Me): 21.0000 (Mjup) 6676.6980 (Mearth)
Semi Major Axis / Orbital Distance Calculated 0.0002 (AU) 0.0002 (AU Est.)
Eccentricity : 0.0000
Orbital Period(Yrs) 0.0000
Orbital Period(Observed/Estimated) 0.00 (Days Obs.) 0.00 (Days Est.)
Surface Gravity (G Earth) 64.4791
Star Radiation at Atmospheric Boundary: 0.0 (W/m2)
Measured Temperature (K) 0.0 (K)
Blackbody T 0.1(K) 0.0 (K)
Blackbody T 0.3(K) 0.0 (K)
Blackbody T 0.7(K) 0.0 (K)
Tidally Locked Blackbody T 0.1(K) 0.0 (K)
Tidally Locked Blackbody T 0.3(K) 0.0 (K)
Size Class: Jupiter-size
Mass Class:
Detection Type : "Timing, Other"
Mass Detection :
Radius Detection :
Habitability by Solar Eq. Astronomical Unit: Not habitable
Habitability by Kopparapu: Not habitable
Star Name : AE 1
Alternate Name : GCVS V803 Cen
Star Distance(LY) : 1131.8
Stellar Radius(Rsun) : 0.0 (Rsun Measured)
Stellar Mass(Msun) : 1.3 (Msun Measured) 0.0 (Msun Estimated)
Star Age : 0.0 (GY)
Temperature : 14000 (K)
Spectral type : DA
UV portion[%]: 0.3
Visible portion[%]: 1.5
IR portion[%]: 98.2
Metalicity : 0.0
Absolute Magnitude: 6.7
Apparent Magnitude: 14.4
Right Ascension(RA) 200.9356
Declination (DEC) -41.7415
Hubble Space Telescope Guide Star Catalog (GSC) ID
Discovered by
Discovery Paper - Authors
Discovery Paper - Title
Discovery Paper - Journal
Discovery Paper - URL
SIMBAD LINK
Open Exoplanet Database Link
AE 1 b
AE 1 b

  • AE 1 b is an exoplanet orbiting the star AE 1, located about 1131.8 light-years (347.0 pc) away from Solar System. Its discovery was publicly announced on 2011.
  • The host star AE 1 has apparent magnitude of 14.4, with absolute magnitude of 6.7.
  • It is 1.3 times more massive compared with our Sun. The surface temperature is 14000 with its spectral types of DA
  • (Projected orbit of AE 1 b around its host star AE 1)


  • The Star AE 1 's habitable zone is located at the following distance
  • Inner Boundary (the orbital distance at Venus's Equivalent Radiation ) : 0.042 AU ( 6352054.0 km)
  • Earth Boundary (the orbital distance at Earth's Equivalent Radiation) : 0.059 AU ( 8780198.7 km)
  • Outer Boundary (the orbital distance at Mars's Equivalent Radiation) : 0.089 AU ( 13379079.7 km)
  • Snow Line (the orbital distance at Snow Line Equivalent Radiation) : 0.132 AU ( 19687901.9 km)
  • Radiation at Planetary Boundary of AE 1 b : 0.00 W/m2

    (Habitable zone calculated based on SEAU(Solar Equivalent Astronomical Unit) around the star AE 1)



  • Kopparapu Recent Venus for Star AE 1 distance : nan AU
  • Kopparapu Runaway Greenhouse for Earth-sized planet for Star AE 1 distance : nan AU
  • Kopparapu Runaway Greenhouse for Super-Earth-sized planet for Star AE 1 distance : nan AU
  • Kopparapu Runaway Greenhouse for Mars-sized planet for Star AE 1 distance : nan AU
  • Kopparapu Outer Boundary for Maximum Greenhouse for Star AE 1 distance : nan AU
  • Kopparapu Outer Boundary for Early Mars for Star AE 1 distance : nan AU

    (Habitable zone calculated based on Kopparapu et al.(2013) around the star AE 1)



  • Original Kopparapu Recent Venus for Star AE 1 distance : nan AU
  • Original Kopparapu Runaway Greenhouse for Star AE 1 distance : nan AU
  • Original Kopparapu Moist Greenhouse for Star AE 1 distance : nan AU
  • Original Kopparapu Outer Boundary for Maximum Greenhouse for Star AE 1 distance : nan AU
  • Original Kopparapu Outer Boundary for Early Mars for Star AE 1 distance : nan AU

    (Habitable zone calculated based on Kopparapu et al.(Original) around the star AE 1)



    (Position in Stellar Map of star AE 1 and its Exoplanet AE 1 b)



    (Zoomed position in Stellar Map of star AE 1 and its Exoplanet AE 1 b (zoom level 3))

    (Synthetic Spectrum of star AE 1*)
    *Yamashiki YA et al. 2019 ApJ 881 114
    MUSCLES Paper I - France et al. 2016 ApJ 820 89
    MUSCLES Paper II- Youngblood et al. 2016 ApJ 824 101
    MUSCLES Paper III- Loyd et al. 2016 ApJ 824 102