Host star — Kepler-452
- Spectral type
- G2
- Temperature
- 5,757 K
- Radius
- 1.11 R☉
- Mass
- 1.04 M☉
- Luminosity
- 1.215 L☉
- Distance
- 551.7 pc (1,799 ly)
Yellow star — the same class as our Sun.
Similar to our Sun (5,778 K).
Orbits Kepler-452 · 1,799 light-years from Earth
Kepler-452 b orbits a sun-like star just 1,800 light-years away, making it one of astronomy's most famous exoplanet discoveries. At 1.63 times Earth's radius and 3.29 times Earth's mass, it is a super-Earth with a density of 4.17 grams per cubic centimeter, suggesting a rocky composition. Its equilibrium temperature of 265 Kelvin (minus 8 degrees Celsius) places it near the cold edge of the habitable zone, comparable to Earth's polar regions. The planet orbits every 385 days at 1.05 astronomical units from its host star, nearly matching Earth's year and distance, and a perfectly circular orbit means stable, predictable conditions. Whether 265 Kelvin permits surface liquid water depends on atmospheric composition—a thick greenhouse blanket could warm the surface, while a thin one would leave it frozen. The planet's exact atmospheric properties remain unknown, and its larger mass raises questions about geological activity and volatile retention that ground-based observations cannot yet answer. Kepler-452 b's 2015 discovery by the Kepler space telescope and its resemblance to Earth have made it a touchstone for the search for habitable worlds beyond our solar system.
Kepler-452 b is a super-Earth — larger than our planet but likely still rocky or ice-rich. Whether it has a thin atmosphere like Mars or a crushing one like Venus remains unknown.
Surface gravity is about 1.2g — noticeably heavier what you're used to on Earth.
With an equilibrium temperature around -8°C, this planet sits in the temperature range where liquid water could potentially exist on the surface — a key ingredient for life as we know it.
One orbit takes 384.84 days — a year here is 1.1× longer than Earth's.
Logarithmic bars so Jupiter-class planets fit the same scale as Earth-size worlds.
Yellow star — the same class as our Sun.
Similar to our Sun (5,778 K).
Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.
Nearly circular orbit.
Rocky composition likely. Earth is 5.51 g/cm³.
A transit photometer watches a star nonstop and measures its brightness to ~0.01%. When a planet passes between us and the star, the star dims briefly — the deeper the dip, the bigger the planet. This is how Kepler and TESS found most known exoplanets.
Where this host star sits among … exoplanet host stars. The main sequence band runs diagonally — giants and supergiants sit above, white dwarfs below.
ESI combines radius similarity and equilibrium temperature similarity. Earth = 100. Mars ≈ 73. Venus ≈ 44. This score reflects two physical parameters only — not atmosphere, water, or magnetic field.