Using the Kepler space telescope, NASA astronomers have found the first
planet that they believe to be made of rock, roughly equivalent in size
to Earth and potentially capable of supporting life.
The planet, Kepler-186f, orbits the star Kepler-186 some 490 light
years away in the constellation Cygnus. It has a diameter of 8,700
miles, making it larger than Earth, and its orbit lies within the
"Goldilocks zone" where temperatures could allow for liquid water to
flow on its surface. Kepler-186f likely even boasts similar
gravity. It's the first such planet to ever be discovered outside of our
solar system.
"It's Earth-size," Elisa V. Quintana of the SETI Institute and NASA's Ames Research Center told the New York Times. "It's in the habitable zone. So we now know these planets do exist."
The Bay Area Environmental Research Institute's Thomas S. Barclay says "It's a progression. ... This
is a
very, very exciting milestone discovery. It has a much higher
probability of being habitable. This planet really reminds us of Earth."
Kepler-186f
is on the outer edge of its star's habitable zone, meaning it could be
cool enough that any liquid water on its surface would freeze. But it
orbits a dwarf star, which is among the oldest stars in the universe,
meaning any life will have had billions of years to develop. And since
dwarf stars are plentiful (more than 70%
of the hundreds of billions of known stars are main-sequence M-dwarfs),
the discovery of Kepler-186f implies there may be many more such
planets scattered throughout known space. Furthermore, being at the edge
of the habitable zone may protect
Kepler-186f from the harmful solar flares and damaging radiation such
dwarf stars emit at higher rates than G-type stars like our own sun.
The Kepler telescope launched in 2009, but precision gyroscopic wheels on the craft failed
in 2013, ending its life as a planet-hunter. But it discovered
thousands of candidates during its three-year operational history. The
remaining Kepler data to be analyzed includes more than 2,800 planet
candidates, meaning that many more Earth-like bodies could remain to be
discovered.
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