Barren Life possible Magnetic Field High Activity
Your planet has an unusual composition that doesn't fit standard classifications, or lacks the elements needed for complex geological processes. Barren worlds can form from uncommon element combinations or may be remnants of larger bodies that lost their atmospheres and volatile materials.
Composition doesn't match standard planet types Mass: 4.6x Earth Temperature: 336K
Reading your planet’s atmosphere Dominant elements: H, O, P, C, Mg This is what a telescope would measure while your planet crosses in front of its star: starlight passes through the atmosphere and spreads into a rainbow band. Each dark line marks a wavelength the atmosphere absorbed. Every element absorbs its own signature wavelengths — hydrogen always darkens the same two spots, calcium another pair, and so on. Astronomers match the lines in a real spectrum against a library of these signatures to say what an atmosphere is made of, light-years away, without ever visiting. A deeper line generally means more of that element is present. For a real planet, distance is usually measured by parallax: as Earth orbits the Sun, a nearby star appears to shift very slightly against the distant background stars, and the size of that shift gives its distance directly — the same geometry surveyors use, at an interstellar scale. Close
Habitability Score Uninhabitable
Contributing Factors water 30
Abundant water (water stripped by extreme rotation) geology 90
Active geology recycles nutrients and drives carbon cycle rotation 5
Extreme rotation (< 4 hrs) - winds exceeding 1000 mph, constant category 5 hurricanes, uninhabitable surface Organic Chemistry 25
Carbon and hydrogen present - organic chemistry possible - chlorine-laced environment attacks organic molecules atmosphere 15
CO₂ atmosphere with moderate greenhouse effect (severely compromised by extreme rotation) temperature 70
Challenging but potentially habitable temperature magnetic Field 100
Magnetic field provides radiation protection — but the pulsar's beams bathe this orbit in hard X-rays Physical Properties Mass
4.60x Earth (2.75e+25 kg) Radius
1.66x Earth (10,596 km) This planet: 1.66× Earth radius Earth: 1× (baseline)
Surface Gravity
1.66x Earth (16.3 m/s²) Surface Temperature
336 K (62 °C / 144 °F) Rotation Period
2.0 hours/day (faster than Earth) This planet: 2 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 CO₂ atmosphere
Surface Characteristics Barren rocky surface with unusual elemental composition Closest Real Exoplanet Orbiting TOI-1452 Yours TOI-1452 b Mass 4.60 × Earth 4.82 × Earth Radius 1.53 × Earth 1.67 × Earth Density (composition) 7.08 g/cm³ 5.70 g/cm³ Temperature 335.5 K 326.0 K Starlight received 1.00 × Earth 1.80 × Earth Star temperature — 3,185 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 2022 via transit · 99 light-years away Source: NASA Exoplanet Archive Browse all 5,893 real exoplanets Learn more about exoplanets Moons
Moon 1 stable Ice lost: bare rock 0.00010% - 8.4 radii Stand on this moonSmall and distant: a quiet, stable companion.
Too warm for ice and too small to hold an atmosphere: the ice sublimated, leaving bare rock.
Habitability ✓ Conditions could support life This planet’s modelled conditions could support biological processes: stable temperatures, liquid water and the chemistry life as we know it needs. That makes life possible, not present.