September 29, 2026

Kepler-442 b

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Kepler-442 b is one of the most remarkable planets in Lisa Kaltenegger’s research, often cited as being potentially “super-habitable”—even more life-friendly than Earth itself. It is located approximately 1,200 light-years away in the constellation Lyra.

Key Physical Characteristics

  • Planet Type: Terrestrial (rocky) Super-Earth.
  • Size: It is about 1.34 times the radius of Earth.
  • Orbit: It completes one orbit around its star every 112.3 Earth days.
  • The Star: It orbits a K-type orange dwarf. These stars are considered “Goldilocks stars” because they are more stable and longer-lived than our Sun, but warmer and less violent than red dwarfs.

Habitability & Environment

In Kaltenegger’s work, Kepler-442 b is a top-tier candidate for a life-sustaining world:

  • Energy Intake: It receives about 70% of the starlight that Earth gets from the Sun. This puts it in a very temperate range—slightly cooler than Earth, but potentially very comfortable if it has a stable atmosphere.
  • Super-Habitability: Scientific models suggest this planet could be more life-friendly than Earth. Its star lasts billions of years longer than our Sun, and its slightly larger size could provide more land/sea area and a stronger magnetic field to protect the atmosphere.
  • Temperature: If it has an Earth-like atmosphere, its average surface temperature is estimated to be around -2.5 °C, which is cold but easily warm enough for liquid water if there is a modest greenhouse effect.

Scientific Significance

  • No Tidal Locking: Unlike many red dwarf planets, Kepler-442 b is far enough from its star that it is likely not tidally locked. This means it should have a normal day-night cycle, which helps distribute heat evenly and creates more stable weather patterns.
  • Rocky Confirmation: Its size and the energy it receives make it highly likely to be a solid rocky world with the potential for diverse continents or a global ocean.
  • A Gold Standard: Because it orbits a stable orange dwarf, it is considered one of the best long-term prospects for the search for complex life in the galaxy.