Exoplanet · gas giant
Kepler-1656 c
Kepler-1656 c is a gas giant orbiting the star Kepler-1656. Its year lasts 1,920 Earth days. It was discovered in 2022 by the Radial Velocity method.
| Host star | Kepler-1656 |
|---|---|
| Distance | 606.2 light-years (185.9 pc) |
| Orbital period | 5.25 years |
| Orbital radius | 3.05 AU |
| Eccentricity | 0.527 |
| Radius | 14 R⊕ · 1.25 R♃ |
| Mass | 126 M⊕ · 0.398 M♃ |
| Density | 0.253 g/cm³ |
| Surface gravity | 0.645 × Earth |
| Equilibrium temperature | 161 K (-112 °C) |
| Stellar flux received | 0.113 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2022 |
| Discovered by | W. M. Keck Observatory |
Habitable zone
Beyond the habitable zone: it receives only %11 of the light the Earth does, a frozen world.
Its star in the sky
In the planet's sky its star is a disc 0.19° across: 0.36 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 11.67. 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 the year 1420. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 11 million years.
Planets in the same system
- Kepler-1656 b 31.6-day orbit · 4.57 R⊕
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.