Exoplanet · super-Earth
Kepler-1300 b
Kepler-1300 b is a super-Earth orbiting the star Kepler-1300. Its year lasts 22.2 Earth days. It was discovered in 2016 by the Transit method.
| Host star | Kepler-1300 |
|---|---|
| Distance | 2,534 light-years (777.0 pc) |
| Orbital period | 22.2 days |
| Orbital radius | 0.16 AU |
| Eccentricity | 0.000 |
| Radius | 1.37 R⊕ · 0.122 R♃ |
| Mass | 2.45 M⊕ · 0.00771 M♃ (estimated from the radius) |
| Density | 5.24 g/cm³ |
| Equilibrium temperature | 954 K (681 °C) |
| Stellar flux received | 149 × Earth |
| Discovery method | Transit |
| Discovery year | 2016 |
| Discovered by | Kepler |
Habitable zone
Inside the inner edge of the habitable zone: it receives 149 times the light the Earth does, too hot to keep liquid water on its surface.
Its star in the sky
In the planet's sky its star is a disc 6° across: 11 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 12.86. Visible from the whole Northern Hemisphere and south to latitude 50° S. North of latitude 50° N it never sets. It stands highest at midnight in July, the best time to observe it.
Light's journey
The light you see tonight set out around 509 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 45 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.