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 | psi1 Dra B b | |
|---|---|---|
| Mass | 300.0 × Earth | 486.0 × Earth |
| Radius | 10.1 × Earth | 13.5 × Earth |
| Density (composition) | 1.60 g/cm³ | 1.09 g/cm³ |
| Temperature | 183.8 K | 159.0 K |
| Starlight received | 0.06 × Earth | 0.11 × Earth |
| Star temperature | 35,000 K | 6,212 K |
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Tidal braking locked the planet to its moon: one face forever moonward.
Tidal flexing melts its interior: an actively volcanic surface (Io-like).
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Cold and massive enough to hold its nitrogen and methane as a thick haze (Titan-like).