Magnetic Field Low Activity
Why is this a Venus Like? Your planet has a thick CO₂ atmosphere creating a runaway greenhouse effect, with surface temperatures of 536K. Venus-like planets experience runaway greenhouse warming where CO₂ traps heat, evaporating oceans and creating hostile conditions despite being in the habitable zone.
✓ Temperature: 536K (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 60
Some geological activity provides slow nutrient cycling rotation 100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution Organic Chemistry 0
Limited organic chemistry potential - chlorine-laced environment attacks organic molecules atmosphere 35
Dense CO₂ atmosphere with extreme greenhouse effect temperature 15
Extremely hot - hostile to known life forms magnetic Field 100
Magnetic field provides radiation protection Physical Properties Mass
0.80x Earth (4.78e+24 kg) Radius
0.93x Earth (5,914 km) This planet: 0.93× Earth radius Earth: 1× (baseline)
Surface Gravity
0.93x Earth (9.1 m/s²) Surface Temperature
536 K (263 °C / 505 °F) Rotation Period
19.0 hours/day (faster than Earth) This planet: 19 h/day Earth: 24 h/day Orbital Environment Star Type
G-type (Yellow (Sun-like)) Distance from Star
0.48 AU (71.8 million km) Atmosphere Dense CO₂ atmosphere with sulfuric acid clouds, extreme greenhouse effect
Surface Characteristics Rocky surface with volcanic plains, extreme pressure and heat