Star and planets drawn to scale (a typical star of its class), with only the star's edge in view. Orbits spaced as in the star system view.
Planet, moons and orbits drawn to one scale; the smallest moons are enlarged so they can be seen.
Surface. No solid surface - thick gaseous envelope with possible rocky core deep within
Hydrogen and helium dominated with trace methane and ammonia
Hydrogen-rich atmosphere typical of gas giants (partially stripped by slow rotation)| Yours | Kepler-167 e | |
|---|---|---|
| Mass | 335.0 × Earth | 321.0 × Earth |
| Radius | 11.2 × Earth | 10.2 × Earth |
| Density (composition) | 1.30 g/cm³ | 1.67 g/cm³ |
| Temperature | 156.6 K | 134.0 K |
| Starlight received | 0.10 × Earth | 0.10 × Earth |
| Star temperature | 3,050 K | 4,884 K |
Inside the Roche limit (1.79 planet radii): torn apart into a ring system.
Small and distant: a quiet, stable companion.
Tidal braking locked the planet to its moon: one face forever moonward.
Tidal heat sustains a subsurface ocean over a rock seafloor: a strong candidate for life (Europa-like, 45/100).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Tidal flexing melts its interior: an actively volcanic surface (Io-like).