Magnetic Field Low Activity
Why is this a Rocky Terrestrial? Your planet is dominated by silicate (41.1%) and iron (13.7%) 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: 41.1% + Iron: 13.7% + Magnesium: 13.7% ✓ Mass: 0.7x Earth (terrestrial range)
Habitability Score Uninhabitable
Contributing Factors water 4
Very dry - minimal water - frozen solid, no liquid phase at this temperature geology 60
Some geological activity provides slow nutrient cycling rotation 100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution Organic Chemistry 50
Carbon and hydrogen present - organic chemistry possible atmosphere 50
CO₂ atmosphere with moderate greenhouse effect temperature 20
Very cold - water frozen, challenging for life magnetic Field 100
Magnetic field provides radiation protection 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
137 K (-136 °C / -213 °F) Rotation Period
25.0 hours/day (slower than Earth) This planet: 25 h/day Earth: 24 h/day Orbital Environment Star Type
NS-type (Neutron Star) Distance from Star
0.41 AU (61.3 million km) Atmosphere Thin, dusty CO₂ atmosphere
Surface Characteristics Rocky surface with impact craters, possible volcanic features Closest Real Exoplanet Orbiting Teegarden's Star Yours Teegarden's Star d Mass 0.70 × Earth 0.82 × Earth Radius 0.92 × Earth 0.95 × Earth Density (composition) 4.95 g/cm³ 5.20 g/cm³ Temperature 137.3 K 159.0 K Starlight received 0.06 × Earth 0.12 × 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 2024 via radial velocity · 12 light-years away Source: NASA Exoplanet Archive Browse all 5,568 real exoplanets Learn more about exoplanets Moons
Moon 1 rings 0.00010% - 1.5 radii
Inside the Roche limit (2.80 planet radii): torn apart into a ring system.
Moon 2 merged 0.00010% - 1.5 radii
Merged with an adjacent moon: too close for both to hold a stable orbit.
Moon 3 rings 0.00010% - 2.1 radii
Inside the Roche limit (2.80 planet radii): torn apart into a ring system.