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. Runaway tidal heating drives volcanism across a cold crust - lava lakes and sulfur plains between frozen plains
Volcanic outgassing - sulfur compounds and vaporized rock
Atmosphere present but composition not ideal for life (partially stripped by slow rotation)| Yours | Kepler-167 e | |
|---|---|---|
| Mass | 92.0 × Earth | 321.0 × Earth |
| Radius | 3.41 × Earth | 10.2 × Earth |
| Density (composition) | 12.8 g/cm³ | 1.67 g/cm³ |
| Temperature | 132.9 K | 134.0 K |
| Starlight received | 0.04 × Earth | 0.10 × Earth |
| Star temperature | 5,600 K | 4,884 K |
Small and distant: a quiet, stable companion.
Tidal braking locked the planet to its moon: one face forever moonward.
Inside the Roche limit (1.79 planet radii): torn apart into a ring system.
Small and distant: a quiet, stable companion.
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (24/100).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (35/100).
Merged with an adjacent moon: too close for both to hold a stable orbit.
Merged with an adjacent moon: too close for both to hold a stable orbit.
Merged with an adjacent moon: too close for both to hold a stable orbit.
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (27/100).
Merged with an adjacent moon: too close for both to hold a stable orbit.