| 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.