Exoplanet · super-Earth
Kepler-1335 b
Kepler-1335 b is a super-Earth orbiting the star Kepler-1335. Its year lasts 6.26 Earth days. It was discovered in 2016 by the Transit method.
| Host star | Kepler-1335 |
|---|---|
| Distance | 2,028 light-years (621.9 pc) |
| Orbital period | 6.26 days |
| Orbital radius | 0.0615 AU |
| Eccentricity | 0.000 |
| Radius | 1.45 R⊕ · 0.129 R♃ |
| Mass | 2.7 M⊕ · 0.0085 M♃ (estimated from the radius) |
| Density | 4.87 g/cm³ |
| Equilibrium temperature | 809 K (536 °C) |
| Stellar flux received | 80.7 × Earth |
| Discovery method | Transit |
| Discovery year | 2016 |
| Discovered by | Kepler |
Habitable zone
Inside the inner edge of the habitable zone: it receives 80.7 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 6.4° across: 12 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 15.25. Visible from the whole Northern Hemisphere and south to latitude 48° S. North of latitude 48° 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 3 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 36 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.