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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.
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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.
NASA
Guillermo Gonzalo Sánchez Achutegui
FELICIDADES, A ESOS CIENTIFICOS, TONY.
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