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Kepler-442b

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Template:Planetbox begin Template:Planetbox image Template:Planetbox star Template:Planetbox character Template:Planetbox orbit Template:Planetbox discovery Template:Planetbox catalog Template:Planetbox end Kepler-442b (also known by its Kepler Object of Interest designation KOI-4742.01) is a confirmed near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of a sun-like star Kepler-442, about 1,120 light-years (342 pc) from the Earth in the constellation Lyra. The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. NASA announced the discovery of the exoplanet on 6 January 2015.

Confirmed exoplanet

Kepler-442b, a near-Earth-sized exoplanet, has a radius 1.34 times that of Earth. The planet orbits a sun-like star, named Kepler-442, once every 112.3 days.

Habitability

The planet was announced as being located within the star's "habitable zone", a region where liquid water could exist on the surface of the planet. It was described as being one of the most Earth-like planets, in terms of size and temperature, yet found.

See also

References

  1. ^ Cite error: The named reference NASA-20150106 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference TG-20150107-IS was invoked but never defined (see the help page).

External links

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