Exoplanet · super-Earth
tau Cet f
tau Cet f is a super-Earth orbiting the star τ Cet. Its year lasts 636 Earth days. It was discovered in 2017 by the Radial Velocity method.
| Host star | τ Cet |
|---|---|
| Distance | 11.8 light-years (3.60 pc) |
| Orbital period | 636 days |
| Orbital radius | 1.33 AU |
| Eccentricity | 0.160 |
| Radius | 1.81 R⊕ · 0.161 R♃ |
| Mass (minimum) | 3.93 M⊕ · 0.0124 M♃ |
| Density | 3.64 g/cm³ |
| Equilibrium temperature | 202 K (-71 °C) |
| Stellar flux received | 0.278 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2017 |
| Discovered by | Multiple Observatories |
Habitable zone
Beyond the habitable zone: it receives only %28 of the light the Earth does, a frozen world.
Its star in the sky
In the planet's sky its star is a disc 0.33° across: 0.62 times the Sun as we see it from Earth.
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 3.49). Visible from the whole Southern Hemisphere and north to latitude 74° N. South of latitude 74° S it never sets. It stands highest at midnight in October, the best time to observe it.
Light's journey
The light you see tonight set out around the year 2014. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 208 thousand years.
Planets in the same system
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.