Exoplanet · super-Earth
GJ 625 b
GJ 625 b is a super-Earth orbiting the star GJ 625. Its year lasts 14.6 Earth days. It was discovered in 2017 by the Radial Velocity method.
| Host star | GJ 625 |
|---|---|
| Distance | 21.1 light-years (6.47 pc) |
| Orbital period | 14.6 days |
| Orbital radius | 0.0784 AU |
| Eccentricity | 0.130 |
| Radius | 1.49 R⊕ · 0.133 R♃ |
| Mass (minimum) | 2.82 M⊕ · 0.00887 M♃ |
| Density | 4.68 g/cm³ |
| Equilibrium temperature | 336 K (62 °C) |
| Stellar flux received | 2.08 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2017 |
| Discovered by | Multiple Observatories |
Habitable zone
Inside the inner edge of the habitable zone: it receives 2.08 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 2.1° across: 4 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 10.13. Visible from the whole Northern Hemisphere and south to latitude 36° S. North of latitude 36° N it never sets. It stands highest at midnight in May, the best time to observe it.
Light's journey
The light you see tonight set out around the year 2005. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 374 thousand years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.