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- Tau Ceti g - Science@NASA
Tau Ceti g is a super Earth exoplanet that orbits a G-type star Its mass is 1 75 Earths, it takes 20 days to complete one orbit of its star, and is 0 133 AU from its star Its discovery was announced in 2017
- System 60 - Tau Ceti - eldacur. com
Low-G, Hot, Airless, 1-Face: Distance from primary star: 5 3E+07 KM: 0 355 AU: Mass: 5 5E+22Kg: 0 009 Earth masses: Surface gravity: 201 4 cm sec 2: 0 21 Earth gees: Surface pressure: 0 millibars: 0 000 Earth atmospheres: Surface temperature: 121 8° Celcius 251 3° Fahrenheit +107 8° C Earth temperature +194 1° F Earth temperature: Normal
- Planet tau Cet g - Extrasolar Planets Encyclopaedia
Detailed information about planet tau Cet g and its parameters Feng et al (2017) : To be consistent with the names used by Tuomi et al 2013, the new signals at periods of 20 and 49d are named τ Ceti g and h Automatic model-based telluric correction for the ESPRESSO data reduction software
- System 1850770294 - Tau Ceti
Low-G, Hot, Airless, 1-Face: Distance from primary star: 4 5E+07 KM: 0 303 AU: Mass: 6 7E+23Kg: 0 112 Earth masses: Surface gravity: 463 6 cm sec 2: 0 47 Earth gees: Surface pressure: 0 millibars: 0 000 Earth atmospheres: Surface temperature: 154 0° Celcius 309 3° Fahrenheit +140 0° C Earth temperature +252 1° F Earth temperature: Normal
- tau Cet g ExoPlanet Facts - Universe Guide
tau Cet g is a Confirmed extrasolar planet (exoplanet) that orbits the star Tau Ceti in the constellation of Cetus
- Exoplanet Tau Ceti g - Stellar Catalog
Exoplanet Tau Ceti g orbits star Tau Ceti that lies 12 light years away from the Sun It weighs about 1 8 Earth masses and orbits its star closer than Earth orbits Sun
- Orions Arm - Encyclopedia Galactica - Tau Ceti
Tartarus (Tau Ceti f): Semi-major axis: 1 334 AU Orbital period: 1 741 standard years Mass: 6 852 x Earth Type: Gas Dwarf Mostly Unity affiliation; the moon Persephone was considered the sect's second home after they were exiled from Nova Beamrider booster station with links to the Deeper Covenant Ceti asteroid belt
- THE CHEMICAL COMPOSITION OF CETI AND POSSIBLE EFFECTS ON TERRESTRIAL . . .
τ Ceti (HD10700), a G8 dwarf with mass 0 78M , is a close (3 65pc) Sun-like star where five possibly terrestrial planet candidates (minimum masses of 2, 3 1, 3 5, 4 3, and 6 7M Å ) have recently been discovered
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