Venus Like 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 633K. Venus-like planets experience runaway greenhouse warming where CO₂ traps heat, evaporating oceans and creating hostile conditions despite being in the habitable zone.
✓ Temperature: 633K (500-800K range) ✓ CO₂-rich atmosphere creating greenhouse effect
Habitability Score Uninhabitable
Contributing Factors water 50
Water present but likely as steam — shielded under ice and rock, a subsurface refuge could outlast the blast geology 90
Active geology recycles nutrients and drives carbon cycle rotation 100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution Organic Chemistry 80
Core organic elements (CHNO) present 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 — but the remnant's shock fronts flood this orbit with cosmic rays Physical Properties Mass
0.90x Earth (5.37e+24 kg) Radius
0.97x Earth (6,151 km) This planet: 0.97× Earth radius Earth: 1× (baseline)
Surface Gravity
0.97x Earth (9.5 m/s²) Surface Temperature
633 K (360 °C / 680 °F) Rotation Period
25.0 hours/day (slower than Earth) This planet: 25 h/day Earth: 24 h/day Orbital Environment Star Type
SNR-type (Supernova Remnant) Distance from Star
0.31 AU (46.4 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 0.00063% - 26.0 radii
Small and distant: a quiet, stable companion.