Exoplanet · super-Earth
Kepler-1932 b
Kepler-1932 b is a super-Earth orbiting the star Kepler-1932. Its year lasts 0.524 Earth days. It was discovered in 2021 by the Transit method.
| Host star | Kepler-1932 |
|---|---|
| Distance | 2,328 light-years (713.7 pc) |
| Orbital period | 12.6 hours |
| Orbital radius | 0.0123 AU |
| Eccentricity | 0.000 |
| Radius | 1.51 R⊕ · 0.135 R♃ |
| Mass | 2.91 M⊕ · 0.00916 M♃ (estimated from the radius) |
| Density | 4.6 g/cm³ |
| Equilibrium temperature | 1,891 K (1,618 °C) |
| Stellar flux received | 2,800 × Earth |
| Discovery method | Transit |
| Discovery year | 2021 |
| Discovered by | Kepler |
Habitable zone
Inside the inner edge of the habitable zone: it receives 2,800 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 34° across: 64 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 15.29. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° 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 303 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 41 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.