Magnetic Field High Activity
Why is this a Venus Like? Your planet has a thick CO₂ atmosphere creating a runaway greenhouse effect, with surface temperatures of 712K. Venus-like planets experience runaway greenhouse warming where CO₂ traps heat, evaporating oceans and creating hostile conditions despite being in the habitable zone.
✓ Temperature: 712K (500-800K range) ✓ CO₂-rich atmosphere creating greenhouse effect
Habitability Score Uninhabitable
Contributing Factors water 15
Abundant water - boiling away, little would be retained geology 90
Active geology recycles nutrients and drives carbon cycle rotation 60
Fast rotation - strong global wind patterns and weather systems, but manageable Organic Chemistry 50
Carbon and hydrogen present - organic chemistry possible atmosphere 35
Dense CO₂ atmosphere with extreme greenhouse effect 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
2.60x Earth (1.55e+25 kg) Radius
1.38x Earth (8,761 km) This planet: 1.38× Earth radius Earth: 1× (baseline)
Surface Gravity
1.38x Earth (13.5 m/s²) Surface Temperature
712 K (439 °C / 822 °F) Rotation Period
13.0 hours/day (faster than Earth) This planet: 13 h/day Earth: 24 h/day Orbital Environment Star Type
M-type (Red Dwarf) Distance from Star
0.11 AU (16.5 million km) Atmosphere Dense CO₂ atmosphere with sulfuric acid clouds, extreme greenhouse effect
Surface Characteristics Rocky surface with volcanic plains, extreme pressure and heat