NASA
DISCOVERS FIRST EARTH-SIZE PLANETS BEYOND OUR SOLAR SYSTEM
From
NASA
Dec.
20, 2011
The
discovery marks the next important milestone in the ultimate search for planets
like Earth. The new planets are thought to be rocky. Kepler-20e is slightly
smaller than Venus, measuring 0.87 times the radius of Earth. Kepler-20f is
slightly larger than Earth, measuring 1.03 times its radius. Both planets
reside in a five-planet system called Kepler-20, approximately 1,000
light-years away in the constellation Lyra. Kepler-20e orbits its parent star
every 6.1 days and Kepler-20f every 19.6 days. These short orbital periods mean
very hot, inhospitable worlds. Kepler-20f, at 800 degrees Fahrenheit, is
similar to an average day on the planet Mercury. The surface temperature of
Kepler-20e, at more than 1,400 degrees Fahrenheit, would melt glass.
"The
primary goal of the Kepler mission is to find Earth-sized planets in the
habitable zone," said Francois Fressin of the Harvard-Smithsonian Center
for Astrophysics in Cambridge, Mass., lead author of a new study published in
the journal Nature. "This discovery demonstrates for the first time that
Earth-size planets exist around other stars, and that we are able to detect
them." The Kepler-20 system includes three other planets that are larger
than Earth but smaller than Neptune .
Kepler-20b, the closest planet, Kepler-20c, the third planet, and Kepler-20d,
the fifth planet, orbit their star every 3.7, 10.9 and 77.6 days. All five
planets have orbits lying roughly within Mercury's orbit in our solar system.
The host star belongs to the same G-type class as our sun, although it is
slightly smaller and cooler.
The
system has an unexpected arrangement. In our solar system, small, rocky worlds
orbit close to the sun and large, gaseous worlds orbit farther out. In
comparison, the planets of Kepler-20 are organized in alternating size: large,
small, large, small and large. "The Kepler data are showing us some
planetary systems have arrangements of planets very different from that seen in
our solar system," said Jack Lissauer, planetary scientist and Kepler
science team member at NASA's Ames Research Center
in Moffett Field , Calif. "The analysis of Kepler data
continue to reveal new insights about the diversity of planets and planetary
systems within our galaxy."
Scientists
are not certain how the system evolved but they do not think the planets formed
in their existing locations. They theorize the planets formed farther from
their star and then migrated inward, likely through interactions with the disk
of material from which they originated. This allowed the worlds to maintain
their regular spacing despite alternating sizes. The Kepler space telescope
detects planets and planet candidates by measuring dips in the brightness of
more than 150,000 stars to search for planets crossing in front, or transiting,
their stars. The Kepler science team requires at least three transits to verify
a signal as a planet.
The
Kepler science team uses ground-based telescopes and the Spitzer Space
Telescope to review observations on planet candidates the spacecraft finds. The
star field Kepler observes in the constellations Cygnus and Lyra can be seen
only from ground-based observatories in spring through early fall. The data
from these other observations help determine which candidates can be validated
as planets. To validate Kepler-20e and Kepler-20f, astronomers used a computer
program called Blender, which runs simulations to help rule out other
astrophysical phenomena masquerading as a planet.
On
Dec. 5 the team announced the discovery of Kepler-22b in the habitable zone of
its parent star. It is likely to be too large to have a rocky surface. While
Kepler-20e and Kepler-20f are Earth-size, they are too close to their parent
star to have liquid water on the surface. "In the cosmic game of hide and
seek, finding planets with just the right size and just the right temperature
seems only a matter of time," said Natalie Batalha, Kepler deputy science
team lead and professor of astronomy and physics at San Jose State
University . "We are
on the edge of our seats knowing that Kepler's most anticipated discoveries are
still to come."
[Every
planet we find – and we find planets almost everywhere we look – increases
substantially the number of environments where extra-terrestrial life can
emerge, evolve and flourish just as it did here on Earth. The odds against life
elsewhere and the odds that we are the only planet with life decrease every
time we find another world orbiting another star. Those who still think that we
are alone in the Universe can only see the weight of circumstantial evidence
mounting against them and must realise that it is only a matter of time before
definitive evidence for life is found. I personally look forward to their howls
of anguish as we lose yet another of our ‘special’ attributes!]
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