Destroyed — no longer habitable Magnetic Field Moderate Activity
Why is this a Rocky Terrestrial? Your planet is dominated by silicate (28.6%) and iron (28.6%) 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: 28.6% + Iron: 28.6% + Magnesium: 0.0% ✓ Mass: 1.0x Earth (terrestrial range)
Habitability Destroyed — no longer habitable Physical Properties Mass
1.00x Earth (5.97e+24 kg) Radius
1.00x Earth (6,371 km) This planet: 1.00× Earth radius Earth: 1× (baseline)
Surface Gravity
1.00x Earth (9.8 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 Minimal or none
Surface Characteristics Rocky surface with impact craters, possible volcanic features Closest Real Exoplanet Orbiting Teegarden's Star Yours Teegarden's Star b Mass 1.00 × Earth 1.16 × Earth Radius 1.01 × Earth 1.05 × Earth Density (composition) 5.30 g/cm³ 5.52 g/cm³ Temperature 278.0 K 277.0 K Starlight received 1.00 × Earth 1.08 × Earth Star temperature — 3,034 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 2019 via radial velocity · 12 light-years away Source: NASA Exoplanet Archive Browse all 5,568 real exoplanets Learn more about exoplanets