Astronomers have discovered the first Earth-sized planet outside the
solar system that has a rocky composition like that of Earth. Kepler-78b
whizzes around its host star every 8.5 hours, making it a blazing
inferno and not suitable for life as we know it. The results are
published in two papers in the journal Nature.
"The news arrived in grand style with the message: 'Kepler-10b has a
baby brother,'" said Natalie Batalha, Kepler mission scientist at NASA's
Ames Research Center in Moffett Field, Calif. Batalha led the team
that discovered Kepler-10b, a larger but also rocky planet identified by
the Kepler spacecraft.
"The message expresses the joy of knowing that Kepler's family of
exoplanets is growing," Batalha reflects. "It also speaks of progress.
The Doppler teams are attaining higher precision, measuring masses of
smaller planets at each turn. This bodes well for the broader goal of
one day finding evidence of life beyond Earth."
Kepler-78b was discovered using data from NASA’s Kepler space
telescope, which for four years simultaneously and continuously
monitored more than 150,000 stars looking for telltale dips in their
brightness caused by crossing, or transiting, planets.
Two independent research teams then used ground-based telescopes to
confirm and characterize Kepler-78b. To determine the planet's mass, the
teams employed the radial velocity method to measure how much the
gravitation tug of an orbiting planet causes its star to wobble. Kepler,
on the other hand, determines the size or radius of a planet by the
amount of starlight blocked when it passes in front of its host star.
A handful of planets the size or mass of Earth have been discovered.
Kepler-78b is the first to have both a measured mass and size. With both
quantities known, scientists can calculate a density and determine what
the planet is made of.
Kepler-78b is 1.2 times the size of Earth and 1.7 times more massive,
resulting in a density that is the same as Earth's. This suggests that
Kepler-78b is also made primarily of rock and iron. Its star is slightly
smaller and less massive than the sun and is located about 400
light-years from Earth in the constellation Cygnus.
One team led by Andrew Howard from the University of Hawaii in
Honolulu, made follow-up observations using the W. M. Keck Observatory
atop Mauna Kea in Hawaii. More information on their research can be
found here.
The other team led by Francesco Pepe from the University of Geneva,
Switzerland, did their ground-base work at the Roque de los Muchachos
Observatory on La Palma in the Canary Islands. More information on their
research can be found here.
This result will be one of many discussed next week at the second
Kepler science conference Nov. 4-8 at Ames. More than 400
astrophysicists from Australia, China, Europe, Latin America and the US
will convene to present their latest results using publicly accessible
data from Kepler. To learn more about the conference, please visit the website.
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