Exoplanet · super-Earth
K2-72 e
K2-72 e is a super-Earth orbiting the star K2-72. Its year lasts 24.2 Earth days. It was discovered in 2016 by the Transit method.
| Host star | K2-72 |
|---|---|
| Distance | 216.7 light-years (66.4 pc) |
| Orbital period | 24.2 days |
| Orbital radius | 0.106 AU |
| Eccentricity | 0.110 |
| Radius | 1.29 R⊕ · 0.115 R♃ |
| Mass | 2.21 M⊕ · 0.00695 M♃ (estimated from the radius) |
| Density | 5.66 g/cm³ |
| Equilibrium temperature | 286 K (13 °C) |
| Stellar flux received | 1.2 × Earth |
| Discovery method | Transit |
| Discovery year | 2016 |
| Discovered by | K2 |
Habitable zone
At the edge of the habitable zone (within the optimistic limits): liquid water would be possible only with a favourable atmosphere.
Its star in the sky
In the planet's sky its star is a disc 1.7° across: 3.1 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 15.28. Visible from the whole Southern Hemisphere and north to latitude 80° N. It stands highest at midnight in August, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1809. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.8 million 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.