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 - a deep volatile envelope over a supercritical water mantle and hot-ice interior
Hydrogen and helium with water, methane, and ammonia ices
Hydrogen-rich atmosphere typical of gas giants (partially stripped by slow rotation)| Yours | MOA-2010-BLG-477L b | |
|---|---|---|
| Mass | 325.0 × Earth | 480.0 × Earth |
| Radius | 10.4 × Earth | 13.6 × Earth |
| Density (composition) | 1.60 g/cm³ | 1.05 g/cm³ |
| Temperature | 2.79 K | — |
| Starlight received | 0.00 × Earth | — |
| Star temperature | 6,750 K | 5,950 K |
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 (21/100).
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, 51/100).
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, 91/100).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Inside the synchronous orbit: it spiraled inward and was torn apart at the Roche limit (Phobos's fate).