- Billions of habitable worlds in Milky Way
- Astronomers hunting for rocky planets with the right temperature to support life estimate there may be tens of billions of them in our galaxy alone. A European team said that about 40 percent of red dwarf stars - the most common type in the Milky Way - have a so-called "super-Earth" planet orbiting in a habitable zone that would allow water to flow on the surface. Since there are around 160 billion red dwarfs in the Milky Way, the number of worlds that are potentially warm enough and wet enough to support life is enormous. Here's a look at artistic samplings of some far-away worlds:
- This artist's impression shows a sunset seen from the super-Earth Gliese 667 Cc. The brightest star in the sky is the red dwarf Gliese 667 C, which is part of a triple star system. The other two more distant stars, Gliese 667 A and B appear in the sky also to the right. Astronomers have estimated that there are tens of billions of such rocky worlds orbiting faint red dwarf stars in the Milky Way alone.
- An artist rendering illustrates the newly discovered world (HAT-P-1) that has baffled astronomers, since the planet is much larger than theory predicts, scientists said September 14, 2006. HAT-P-1 has a radius about 1.38 times Jupiter's but contains only half Jupiter's mass.
- An artist's illustration of Kepler-22b, a planet known to comfortably circle in the habitable zone of a sun-like star, is seen in this undated handout picture released by NASA, December 5, 2011. Kepler-22b, the most Earth-like planet ever discovered is circling a star 600 light years away, a key finding in an ongoing quest to learn if life exists beyond Earth, scientists said.
- An artist's impression shows a unique type of exoplanet discovered with the Hubble Space Telescope. The planet is so close it to its star that it completes an orbit in 10.5 hours. The planet is only 750,000 miles from the star, or 1/130th the distance between Earth and the Sun. The Jupiter-sized planet orbits an unnamed red dwarf star that lies in the direction of the Galactic Centre; the exact stellar distance is unknown.
An artist's
rendering image released to Reuters on October 19, 2009 shows an exoplanet 6
times the Earth-size circulating around its low-mass host star at a distance
equal to 1/20th of the Earth-Sun distance. The host star is a companion to two
other low-mass stars, which are seen here in the distance (L). European
astronomers announced they had found 32 new planets orbiting stars outside our
solar system and said on Monday they believe their find means that 40 percent
or more of Sun-like stars have such planets.
In this artist's
conception released by NASA February 2, 2011, Kepler-11 is a sun-like star
around which six planets orbit. At times, two or more planets pass in front of
the star at once, as shown in a simultaneous transit of three planets observed
by NASA's Kepler spacecraft on August 26, 2010.
Scientists using
NASA's Spitzer Space Telescope observed a fledgling solar system like the one
depicted in this artist's concept, finding deep within it enough water vapor to
fill all the oceans on Earth five times. The scientists peered at an embryonic star
called IRAS 4B located in our Milky Way galaxy about 1,000 light years from
Earth in the constellation Perseus.
An artist's
impression shows a Jupiter-sized planet passing in front of its parent star.
Such events are called transits. When the planet transits the star, the star's
apparent brightness drops by a few percent for a short period. Through this
technique, astronomers can use the Hubble Space Telescope to search for planets
across the galaxy by measuring periodic changes in a star's luminosity. The
first class of exoplanets found by this technique are the so-called "hot
Jupiters," which are so close to their stars they complete an orbit within
days, or even hours.
NASA
handout image shows an artist's concept of the circumbinary planet Kepler-16b -
the first planet known to definitively orbit two stars. The cold planet, with
its gaseous surface, is not thought to be habitable. The largest of the two
stars, a K dwarf, is about 69 percent the mass of our sun, and the smallest, a
red dwarf, is about 20 percent the sun's mass. These star pairs are called
eclipsing binaries
Astronomers
searching the skies for distant planets have detected two Saturn-sized worlds
orbiting distant suns, the smallest planets found thus far outside our solar
system. The discovery boosted the likelihood that even smaller planets -
perhaps the size of Earth - exist elsewhere in the universe, Professor Steve
Vogt of the University of California-Santa Cruz said. This artists concept
shows a view of the discovered planet orbiting 79 Ceti.
NASA handout image shows an artist's
concept of the circumbinary planet
Kepler-16b - the first planet known to
definitively orbit two stars. The cold
planet, with its gaseous surface, is not
thought to be habitable. The largest of
the two stars, a K dwarf, is about 69
percent the mass of our sun, and the
smallest, a red dwarf, is about 20 percent
the sun's mass. These star pairs are
called eclipsing binaries.
NASA handout image
of an artist's concept illustrating an icy planet-forming disk around a young
star called TW Hydrae, located about 175 light-years away in the Hydra, or Sea
Serpent, constellation. Astronomers using the Herschel Space Observatory detected
copious amounts of cool water vapor, illustrated in blue, emanating from the
star's planet-forming disk of dust and gas. The water vapor, which probably
comes from icy grains in the disk, is located in the frigid outer regions of
the star system, where comets will take shape.
A newly discovered planet, designated by the
unglamorous identifier of OGLE-2005-BLG-390Lb, orbits a red star five
times less massive than the Sun and located at a distance of about 20,000
light years, in this undated artist's impression. A new planet-hunting
technique has detected the most Earth-like planet yet around a star other
than our sun, raising hopes of finding a space rock that might support
life, astronomers reported on January 25, 2006.
A handout photo from
the European Space Agency released December 10, 2008 shows an artist's
impression of the Jupiter-size extrasolar planet, HD 189733b, being eclipsed by
its parent star. Astronomers using the Hubble Space Telescope have measured
carbon dioxide and carbon monoxide in the planet's atmosphere. The planet is a
?hot Jupiter?, so close to its parent star that it completes an orbit in only
2.2 days.
Handout picture released June 14, 2005 shows an
artist's conception of a newly discovered planet being shown as a hot,
rocky, geologically active world glowing in the deep red light of its
nearby parent star, the M dwarf Gliese 876. The heat and the reddish light
are among the few things about the new planet that are certain, depending
on the thickness and composition of its atmosphere - if any - it could
range from being a barren, cratered ball of rock like Mercury or the Moon,
to being a featureless, cloud-shrouded cue-ball like Venus.
A rich starry sky fills the view from an ancient
gas-giant planet in the core of the globular star cluster M4, as imagined
in this artist's concept. The 13-billion-year-old planet orbits a helium
white-dwarf star and the millisecond pulsar B1620-26, seen at lower left.
The globular cluster is deficient in heavier elements for making planets,
so the existence of such a world implies that planet formation may have
been quite efficient in the early universe.
NASA's Hubble Space
Telescope has taken the first visible-light snapshot of a planet circling
another star in this image released by NASA November 13, 2008. Estimated to be
no more than three times Jupiter's mass, the planet, called Fomalhaut b, orbits
the bright southern star Fomalhaut, located 25 light-years away in the
constellation Piscis Australis, or the "Southern Fish."
Image shows
composite image of Elephant's Trunk Nebula, an elongated dark globule within
the emission nebula IC 1396 in the constellation of Cepheus, one of the first
images from the new Spitzer Space Telescope released by NASA on December 18,
2003. The new Spitzer Space Telescope, that looks at the cosmos with infrared
detectors, has lifted the dust veils from newborn stars and a bumptious comet,
and revealed the detail in the spiral arms of a neighboring galaxy.
A handout image
received April 5, 2005 from the University of Jena and the European Space
Observatory ( ESO) shows the first photograph of a planet (B) beyond our solar
system and the star, GQ Lupi (A) around which it orbits. The planet is thought
to be one to two times as massive as Jupiter, according to the scientists who
imaged it. It orbits a star similar to a young version of our Sun.
A new view of the Whirlpool Galaxy, one of the two
largest and sharpest images Hubble Space Telescope has ever taken, is
released by NASA on Hubble's 15th anniversary April 25, 2005. The new
Whirlpool Galaxy image showcases the spiral galaxy's curving arms where
newborn stars reside and its yellowish central core that serves as home
for older stars. During the 15 years Hubble has orbited the Earth, it has
taken more than 700,000 photos of the cosmos.
A California astronomer has discovered what he
believes is the 10th planet in our solar system, a group of NASA-funded
researchers said on July 29, 2005. The new planet, known as 2003UB313, has
been identified as the most distant object ever detected orbiting the sun,
California Institute of Technology astronomer Michael Brown said. This
artist's concept shows planet 2003UB313 at the lonely outer fringes of our
solar system. Our sun can be seen in the distance. The new planet, which
is yet to be formally named, is at least as big as Pluto and about three
times farther away from the Sun than Pluto.