Magnetic Field Moderate Activity
Why is this a Venus Like? Your planet has a thick CO₂ atmosphere creating a runaway greenhouse effect, with surface temperatures of 674K. Venus-like planets experience runaway greenhouse warming where CO₂ traps heat, evaporating oceans and creating hostile conditions despite being in the habitable zone.
✓ Temperature: 674K (500-800K range) ✓ CO₂-rich atmosphere creating greenhouse effect
Habitability Score Uninhabitable
Contributing Factors water 0
No water - the recipe has no hydrogen and oxygen to form it geology 90
Active geology recycles nutrients and drives carbon cycle rotation 30
Very slow rotation - extreme temperature swings between eternal day and night sides Organic Chemistry 20
Limited organic chemistry potential atmosphere 21
Dense CO₂ atmosphere with extreme greenhouse effect (partially stripped by slow rotation) temperature 5
Scorching - hot enough to melt lead, though rock stays solid; no chance for life magnetic Field 100
Magnetic field provides radiation protection Physical Properties Mass
1.00x Earth (5.97e+24 kg) Radius
1.00x Earth (6,371 km) This planet: 1.00× Earth radius Earth: 1× (baseline)
Surface Gravity
1.00x Earth (9.8 m/s²) Surface Temperature
674 K (401 °C / 754 °F) Rotation Period
12.0 hours/day (faster than Earth) This planet: 12 h/day Earth: 24 h/day Orbital Environment Star Type
G-type (Yellow (Sun-like)) Distance from Star
0.61 AU (91.3 million km) Atmosphere Dense CO₂ atmosphere with sulfuric acid clouds, extreme greenhouse effect
Surface Characteristics Rocky surface with volcanic plains, extreme pressure and heat Moons
Moon 1 stable 0.0032% - 5.0 radii
Small and distant: a quiet, stable companion.
Moon 2 stable 0.00025% - 6.2 radii
Small and distant: a quiet, stable companion.
Moon 3 stable 0.00014% - 45.9 radii
Small and distant: a quiet, stable companion.
+4 chemistry: tidal pools cycle wet and dry - a boost for prebiotic chemistry