Exoplanet · super-Earth
GJ 3323 c
GJ 3323 c is a super-Earth orbiting the star GJ 3323. Its year lasts 40.5 Earth days. It was discovered in 2017 by the Radial Velocity method.
| Host star | GJ 3323 |
|---|---|
| Distance | 17.5 light-years (5.37 pc) |
| Orbital period | 40.5 days |
| Orbital radius | 0.126 AU |
| Eccentricity | 0.170 |
| Radius | 1.32 R⊕ · 0.118 R♃ |
| Mass (minimum) | 2.31 M⊕ · 0.00727 M♃ |
| Density | 5.52 g/cm³ |
| Equilibrium temperature | 148 K (-125 °C) |
| Stellar flux received | 0.17 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2017 |
| Discovered by | La Silla Observatory |
Habitable zone
Beyond the habitable zone: it receives only %17 of the light the Earth does, a frozen world.
Its star in the sky
In the planet's sky its star is a disc 0.5° across: 0.94 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 12.10. Visible from the whole Southern Hemisphere and north to latitude 83° N. It stands highest at midnight in December, the best time to observe it.
Light's journey
The light you see tonight set out around the year 2008. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 311 thousand years.
Planets in the same system
- GJ 3323 b 5.36-day orbit · 1.23 R⊕
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.