Kepler-22
Kepler-22 is a star, located in the northern constellation of Cygnus. The star is orbited by a planet that is located within the star's habitable zone. The estimated distance of Kepler-22 is approximately 620 light-years away from our solar system.Kepler-22 is slightly smaller and cooler then the Sun.


Kepler-22b's first transit in front of its host sun was observed on Kepler's third day of scientific operations in mid-2009. Kepler-22b's third transit was detected in late 2010. The Spitzer Space Telescope provided more data that confirmed Kepler-22b's transits. On December, 2011, the confirmation of the existence of Kepler-22b was announced.
On December 5th, 2011, scientists from the Kepler mission announced that a possible Earthlike planet - Kelper-22b. It’s super-Earth (size of 9 Earths) that could be covered in super ocean.
The habitable zone is the region in which liquid water could exist on a planet's surface. Liquid water is a key ingredient to life, so planets found within this zone are more likely to be habitable worlds. However, planets must also be the right size, and Kepler-22b is too big. Planet’s orbital period is around 300 days which is similar to our environment.
credits:
https://exoplanets.nasa.gov/exoplanet-catalog/1599/kepler-22b/
https://sos.noaa.gov/catalog/datasets/exoplanet-kepler-22b/sg=AOvVaw0_CTeNEePHssViAHdQWLXa&opi=89978449
Why does the size of the planet matter in whether it's habitable or not?
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