No life — too hot for liquid water High Activity
Why is this a Venus Like? Your planet has a thick CO₂ atmosphere creating a runaway greenhouse effect, with surface temperatures of 571K. Venus-like planets experience runaway greenhouse warming where CO₂ traps heat, evaporating oceans and creating hostile conditions despite being in the habitable zone.
✓ Temperature: 571K (500-800K range) ✓ CO₂-rich atmosphere creating greenhouse effect
Habitability Score Uninhabitable
Contributing Factors water 5
Very dry - minimal water - boiling away, little would be retained geology 90
Active geology recycles nutrients and drives carbon cycle rotation 10
Near tidally locked - one hemisphere perpetually scorched, other frozen, narrow habitable twilight zone only Organic Chemistry 50
Carbon and hydrogen present - organic chemistry possible atmosphere 14
Dense CO₂ atmosphere with extreme greenhouse effect (partially stripped by slow rotation) temperature 15
Extremely hot - hostile to known life forms magnetic Field 30
No magnetic field - vulnerable to solar radiation Physical Properties Mass
0.70x Earth (4.18e+24 kg) Radius
0.89x Earth (5,657 km) This planet: 0.89× Earth radius Earth: 1× (baseline)
Surface Gravity
0.89x Earth (8.7 m/s²) Surface Temperature
571 K (298 °C / 568 °F) Rotation Period
567.0 hours/day (slower than Earth) This planet: 567 h/day Earth: 24 h/day Orbital Environment Star Type
M-type (Red Dwarf) Distance from Star
0.10 AU (15 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 rings 0.079% - 2.1 radii
Inside the Roche limit (2.80 planet radii): torn apart into a ring system.