|
Astronomers
Find First Earth-like Planet in Habitable Zone
The Dwarf Carried Other
Worlds Too!
|
|
|
|
The
star Gliese 581
Source:
Digital Sky Survey
Video
The
Dwarf Carried Other Worlds Too!
MOV
Format 63.7MB
Credit:
ESO
|
Astronomers have discovered
the most Earth-like planet outside our Solar System to date, an
exoplanet with a radius only 50% larger than the Earth and
capable of having liquid water. Using the ESO 3.6-m telescope, a
team of Swiss, French and Portuguese scientists discovered a
super-Earth about 5 times the mass of the Earth that orbits a red
dwarf, already known to harbor a Neptune-mass planet. The
astronomers have also strong evidence for the presence of a third
planet with a mass about 8 Earth masses.
This
exoplanet - as astronomers call planets around a star other than
the Sun - is the smallest ever found up to now and it completes a
full orbit in 13 days. It is 14 times closer to its star than the
Earth is from the Sun. However, given that its host star, the red
dwarf Gliese 581, is smaller and colder than the Sun - and thus
less luminous - the planet nevertheless lies in the habitable
zone, the region around a star where water could be liquid! The
planet's name is Gliese 581 c.
"We
have estimated that the mean temperature of this super-Earth lies
between 0 and 40 degrees Celsius, and water would thus be
liquid," explains Stéphane Udry, from the Geneva
Observatory (Switzerland) and lead-author of the paper reporting
the result. "Moreover, its radius should be only 1.5 times
the Earth's radius, and models predict that the planet should be
either rocky - like our Earth - or fully covered with oceans,"
he adds.
"Liquid
water is critical to life as we know it," avows Xavier
Delfosse, a member of the team from Grenoble University (France).
"Because of its temperature and relative proximity, this
planet will most probably be a very important target of the
future space missions dedicated to the search for
extra-terrestrial life. On the treasure map of the Universe, one
would be tempted to mark this planet with an X."
The
host star, Gliese 581, is among the 100 closest stars to us,
located only 20.5 light-years away in the constellation Libra
("the Scales"). It has a mass of only one third the
mass of the Sun. Such red dwarfs are intrinsically at least 50
times fainter than the Sun and are the most common stars in our
Galaxy: among the 100 closest stars to the Sun, 80 belong to this
class.
Artist's
impression of the planetary system around the red dwarf
Gliese 581. Using the instrument HARPS on the ESO 3.6-m
telescope, astronomers have uncovered 3 planets, all of
relative low-mass: 5, 8 and 15 Earth masses. The five
Earth-mass planet (seen in foreground - Gliese 581 c) makes
a full orbit around the star in 13 days, the other two in 5
(the blue, Neptunian-like planet - Gliese 581 b) and 84 days
(the most remote one, Gliese 581 d).
Credit:
ESO
|
"Red dwarfs are ideal
targets for the search for low-mass planets where water could be
liquid. Because such dwarfs emit less light, the habitable zone
is much closer to them than it is around the Sun,"
emphasizes Xavier Bonfils, a co-worker from Lisbon University.
Planets lying in this zone are then more easily detected with the
radial-velocity method, the most successful in detecting
exoplanets.
Two
years ago, the same team of astronomers already found a planet
around Gliese 581. With a mass of 15 Earth-masses, i.e. similar
to that of Neptune, it orbits its host star in 5.4 days. At the
time, the astronomers had already seen hints of another planet.
They therefore obtained a new set of measurements and found the
new super-Earth, but also clear indications for another one, an 8
Earth-mass planet completing an orbit in 84 days. The planetary
system surrounding Gliese 581 contains thus no fewer than 3
planets of 15 Earth masses or less, and as such is a quite
remarkable system.
The
discovery was made thanks to HARPS (High Accuracy Radial Velocity
for Planetary Searcher), perhaps the most precise spectrograph in
the world. Located on the ESO 3.6-m telescope at La Silla, Chile,
HARPS is able to measure velocities with a precision better than
one meter per second (or 3.6 km/h)! HARPS is one of the most
successful instruments for detecting exoplanets and holds already
several recent records, including the discovery of another 'Trio
of Neptunes'
The
detected velocity variations are between 2 and 3 meters per
second, corresponding to about 9 km/h! That's the speed of a
person walking briskly. Such tiny signals could not have been
distinguished from 'simple noise' by most of today's available
spectrograph's.
"HARPS
is a unique planet hunting machine," says Michel Mayor, from
Geneva Observatory, and HARPS Principal Investigator. "Given
the incredible precision of HARPS, we have focused our effort on
low-mass planets. And we can say without doubt that HARPS has
been very successful: out of the 13 known planets with a mass
below 20 Earth masses, 11 were discovered with HARPS!"
HARPS
is also very efficient in finding planetary systems, where tiny
signals have to be uncovered. The two systems known to have three
low mass planets - HD 69830 and Gl 581 - were discovered by
HARPS.
"And
we are confident that, given the results obtained so far, finding
a planet with the mass of the Earth around a red dwarf is within
reach," affirms Mayor.
Source:
ESO

|
Scientific
Frontline®
The
Comm Center
Space
Weather Alerts
Stellar
Nights®
Imagineers
The
E.A.R.®
The
Delta Quadrant
Photo,
Sketches, & Video Gallery
|