Kepler-452b: What It Would Be Like to Live On Earth’s ‘Cousin’
Kepler-452b may be Earth’s close cousin, but living on the newfound world would still be an alien experience.
A group of pioneers magically transported to the surface of —which is the closest thing to an “Earth twin” yet discovered, researchers announced yesterday (July 23) — would instantly realize they weren’t on their home planet anymore. (And magic, or some sort of warp drive, must be invoked for such a journey, since Kepler-452b lies 1,400 light-years away.)
Kepler-452 is 60 percent wider than Earth and probably about five times more massive, so its surface gravity is considerably stronger than the pull people are used to here. Any hypothetical explorers would thus feel about twice as heavy on the alien world as they do on Earth, researchers said. []
“It might be quite challenging at first,” Jon Jenkins, of NASA’s Ames Research Center in Moffett Field, California, said during a news conference yesterday. Jenkins is data analysis lead for the space agency’s , which discovered Kepler-452b.
Other features of life on Kepler-452b would be more familiar. For example, the orbits a solar-type star at about the same distance at which Earth circles the sun. []
Models also suggest that Kepler-452b might soon experience a runaway greenhouse effect, similar to the one that changed from a potentially habitable world billions of years ago to the sweltering hothouse it is today, researchers said.
Kepler-452b’s star is apparently older than the sun—6 billion years, compared to 4.5 billion years. It’s thus in a more energetic phase of its life cycle than is; indeed, the star is about 10 percent larger and 20 percent brighter than Earth’s sun. (That means the sunlight on Kepler-452b, while familiar to explorers from Earth, would not be exactly equivalent.)
“But, you know, we don’t know exactly,” Jenkins said.
So he and other members of the discovery team helped devise an artist’s concept that imagines how Kepler-452b would look if a runaway were beginning to unfold.
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