Astronomers discovered
the smallest planet outside our solar system. This is the first that is certainly
rocky like Earth. Measurements of extraordinary precision-called Kepler showed
that 10b is 1.4 times the diameter of Earth and a mass 4.6 times greater than
he. However, because it orbits very close to its star, the exoplanet could not
support life. The discovery has been hailed as "one of the deepest in the
history of mankind."
The result was announced
at the 217th annual meeting of the American Astronomical Society in Seattle, by
the Kepler telescope team space agency NASA. The Kepler is designed to search
for signs of distant planets, first sighted the exoplanet at a distance of 560
light years, along with hundreds of other candidate planets.
Technique
The Kepler space
telescope uses a technique known as transiting in English, which is the search
for planets that pass between the sun and Earth guest. This report will be
considered as one of the most profound scientific discoveries in the history of
mankind Geoffrey Marcy, University of California, Berkeley.
A small fraction of the
star's light is blocked periodically, giving an indication that the star has a
planet orbiting. The radius of exoplanet correlates with the exact amount of
light that is blocked when passing.
The review of the
measures, this time by a telescope at the Keck Observatory in Hawaii, confirmed
the discovery of Kepler 10b, after measuring how the planet moves away from one
side to another of its parent star as it continues its orbit. These
measurements also confirmed that the star has approximately 8,000 million
years, a sort of grandfather among the stars of its type.
Basically, this means
that the sun is free of optical and magnetic activities, which have introduced
some uncertainty in the calculations of previous candidates to rocky exoplanets
like Corot-7b, whose discovery was announced in early 2009.
Constantly expanding
The cosmic dance causes
small changes in the color of the starlight that is measured by telescopes. However,
completing the set of measurements Kepler team was the use of asteroseismology,
a study of distant stars that is similar to the analysis of earthquakes on
Earth. The oscillation occurs within a star-like in the interior of our planet,
affecting the frequencies of light emitted by the star in a telling sign of its
size.
We have determined the
characteristics of this planet with a precision so fantastic that we can say
without doubt that this is a rocky world in which one could stand Natalie
Batalha, San Jose State University. With data as the mass of the parent star,
the details of the mutual dance of the planet and the star, and the radius of
the exoplanet can calculate the density of the planet.
"All our best
capabilities have come together to form an image of Kepler 10b," said
Natalie Batalha, a professor of astrophysics at San Jose State University, who
helps run the Kepler science mission for NASA. Batalha told the BBC that the
only result was a widening field of exoplanet discoveries, in which heavenly
bodies are getting smaller, while improving experimental methods. "We have
determined the characteristics of this planet with a precision so fantastic
that we can say without doubt that this is a rocky world in which one could
stand," he added.
Are we alone?
The Kepler 10b is very
close to its sun, while its daytime temperature exceeds 1300 ° C. Therefore,
the exoplanet is not a reasonable candidate for harboring life. However, as
explained Professor Batalha, the finding is an important step for the Kepler
mission. An artist's impression shows how the face would look Kepler 10b
watching his star.
"We want to know
whether we are alone in the galaxy and this discovery is a link in the chain to
reach that goal," he said. "First we have to know if planets that
could potentially harbor life are common, something we do not know. That's what
Kepler aims," he added.
The pioneer of the
"hunt" for exoplanets Geoffrey Marcy of the University of California
at Berkeley, said the Kepler 10b is "a global link lost".
"It is a bridge
between the gas giant planets we've been finding and the Earth itself, a
transition from what I have been finding and what we hope to find." "This
report will be considered as one of the most profound scientific discoveries in
human history," he concluded.
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