Lavayus
0
Lava World
Magnetic FieldExtreme Activity
Why is this a Lava World?Runaway tidal heating from its moons keeps the surface molten - the planet is kneaded like Io, only far harder.
Resonant, close-in moons pump orbital eccentricity, and the resulting tidal flexing dissipates enormous heat in the interior. Past a threshold the crust cannot cool: volcanism resurfaces the world continuously.
Classification Criteria:
✓ Close-in moons in a resonant configuration✓ Tidal heat flux beyond the runaway threshold- Orbit itself was fine: 0.10 AU, 739K equilibrium
Habitability ScoreUninhabitable
Contributing Factors
water0
No water - the recipe has no hydrogen and oxygen to form it
geology40
Extreme volcanic activity may be hazardous
rotation10
Near tidally locked - one hemisphere perpetually scorched, other frozen, narrow habitable twilight zone only
Organic Chemistry20
Limited organic chemistry potential
atmosphere16
Atmosphere present but composition not ideal for life (partially stripped by slow rotation)
temperature0
Scorching - hot enough to melt lead, though rock stays solid; no chance for life (large moon stabilizes the axial tilt - steady seasons) (runaway tidal heating keeps the surface molten regardless of orbit)
magnetic Field100
Magnetic field provides radiation protection (a large close moon may help stir the core dynamo (speculative))
Physical Properties
Mass
5.20x Earth (3.11e+25 kg)Radius
1.73x Earth (11,038 km)Surface Gravity
1.73x Earth (17.0 m/s²)Surface Temperature
739 K (466 °C / 871 °F)Rotation Period
12.0 hours/day (faster than Earth)Orbital Environment
Star Type
SNR-type (Supernova Remnant)Distance from Star
0.10 AU (15 million km)Orbital Period
10 daysTime Dilation
Clocks run 6.5 seconds per year slower than deep space — about 9 minutes over a lifetimeAtmosphere
Volcanic outgassing - sulfur compounds and vaporized rock
Elemental Composition
Fe - Iron
26.7%
Si - Silicon
26.7%
Mg - Magnesium
20.0%
Surface Characteristics
Runaway tidal heating keeps the surface molten - volcanic activity everywhereClosest Real Exoplanet
HD 219134 c92% similar
Orbiting HD 219134| Yours | HD 219134 c | |
|---|---|---|
| Mass | 5.20 × Earth | 4.36 × Earth |
| Radius | 1.56 × Earth | 1.51 × Earth |
| Density (composition) | 7.52 g/cm³ | 6.98 g/cm³ |
| Temperature | 739.2 K | 782.0 K |
| Starlight received | 50.0 × Earth | 62.1 × Earth |
| Star temperature | — | 4,699 K |
Moons
Moon 1receding5.6% - 7.7 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Tidal braking locked the planet to its moon: one face forever moonward.