Destroyed — no longer habitable Magnetic Field Extreme Activity
Why is this a Rocky Terrestrial? Your planet is dominated by silicate (16.7%) and iron (38.9%) content, forming a rocky terrestrial body. Rocky terrestrial planets are primarily composed of silicate rocks and metals. They're the most common type of small planet in the universe.
✓ Silicon: 16.7% + Iron: 38.9% + Magnesium: 0.0% ✓ Mass: 8.0x Earth (terrestrial range)
Habitability Destroyed — no longer habitable Physical Properties Mass
8.00x Earth (4.78e+25 kg) Radius
2.00x Earth (12,742 km) This planet: 2.00× Earth radius Earth: 1× (baseline)
Surface Gravity
2.00x Earth (19.6 m/s²) Surface Temperature
278 K (5 °C / 41 °F) Rotation Period
24.0 hours/day This planet: 24 h/day Earth: 24 h/day Orbital Environment Star Type
NS-type (Neutron Star) Distance from Star
0.10 AU (15 million km) Time Dilation
Clocks run 6.5 seconds per year slower than deep space — about 9 minutes over a lifetime Atmosphere Thin, dusty trace-gas atmosphere
Surface Characteristics Rocky surface with impact craters, possible volcanic features Closest Real Exoplanet Orbiting Kepler-22 Yours Kepler-22 b Mass 8.00 × Earth 9.10 × Earth Radius 1.78 × Earth 2.10 × Earth Density (composition) 7.87 g/cm³ 5.41 g/cm³ Temperature 278.0 K 279.0 K Starlight received 1.00 × Earth 1.01 × Earth Star temperature — 5,596 K
Matched on physical properties only — but pulsar planets are real: the first exoplanets ever confirmed (PSR B1257+12, 1992) orbit a neutron star. Discovered 2011 via transit · 636 light-years away Source: NASA Exoplanet Archive Browse all 5,568 real exoplanets Learn more about exoplanets