Aero-V
0
Gas Giant
Magnetic FieldExtreme Activity
Why is this a Gas Giant?Your planet has 87.0% hydrogen and helium, combined with a mass of 60.0x Earth, which exceeds the gas giant threshold.
Gas giants form when massive cores capture enormous atmospheres of light gases. They typically form beyond the 'frost line' where volatiles can condense.
Classification Criteria:
✓ Hydrogen + Helium: 87.0% (>60% required)✓ Mass: 60.0x Earth (>10x required)
Habitability ScoreExtremely Harsh
Contributing Factors
water15
No solid surface — any water is locked in a supercritical mantle and hot ice, not oceans
geology50
Extreme volcanic activity may be hazardous (tidal flexing sustains geologic activity)
rotation10
Near tidally locked - one hemisphere perpetually scorched, other frozen, narrow habitable twilight zone only
Organic Chemistry80
Core organic elements (CHNO) present
atmosphere12
Hydrogen-rich atmosphere typical of gas giants (partially stripped by slow rotation)
temperature20
Very cold - water frozen, challenging for life
magnetic Field100
Magnetic field provides radiation protection
Physical Properties
Mass
60.00x Earth (3.58e+26 kg)Radius
3.91x Earth (24,942 km)Surface Gravity
3.91x Earth (38.4 m/s²)Surface Temperature
122 K (-151 °C / -240 °F)Rotation Period
9.0 hours/day (faster than Earth)Orbital Environment
Star Type
G-type (Yellow (Sun-like))Distance from Star
5.20 AU (778 million km)Orbital Period
11.9 yearsAtmosphere
Hydrogen and helium dominated with trace methane and ammonia
Elemental Composition
H - Hydrogen
55.0%
He - Helium
32.0%
O - Oxygen
5.0%
Surface Characteristics
No solid surface - thick gaseous envelope with possible rocky core deep withinClosest Real Exoplanet
GJ 414 A c74% similar
Orbiting GJ 414 A| Yours | GJ 414 A c | |
|---|---|---|
| Mass | 60.0 × Earth | 53.8 × Earth |
| Radius | 6.34 × Earth | 8.40 × Earth |
| Density (composition) | 1.30 g/cm³ | 0.50 g/cm³ |
| Temperature | 121.9 K | 125.0 K |
| Starlight received | 0.04 × Earth | 0.06 × Earth |
| Star temperature | 5,600 K | 4,120 K |
MoonsLife may exist on a moon
Moon 1recedingOcean world0.080% - 6.0 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Tidal braking locked the planet to its moon: one face forever moonward.
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (22/100).
Moon 2recedingOcean world - life0.10% - 9.5 radii
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, 96/100).
Moon 3recedingOcean world0.10% - 14.5 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
A thin tidal-warmed subsurface ocean may exist, but conditions are marginal (7/100).
Moon 4receding0.10% - 27.2 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).