Spectronicus
Ice Giant
Physical Properties
Orbital Environment
Atmosphere
Elemental Composition
Surface Characteristics
Icy mantle surrounding rocky core, with hydrogen-helium atmosphereClosest Real Exoplanet
| Yours | G 192-15 c | |
|---|---|---|
| Mass | 17.0 × Earth | 14.3 × Earth |
| Radius | 2.57 × Earth | 3.87 × Earth |
| Temperature | 78.1 K | 56.0 K |
| Starlight received | 0.00 × Earth | 0.00 × Earth |
| Star temperature | 6,750 K | 2,999 K |
Inside the synchronous orbit: it spiraled inward and was torn apart at the Roche limit (Phobos's fate).
Small and distant: a quiet, stable companion.
Tidal braking locked the planet to its moon: one face forever moonward.
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (9/100).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
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 heat sustains a subsurface ocean over a rock seafloor: a strong candidate for life (Europa-like, 48/100).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (5/100).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).