Water
Found On Planet Outside Solar System
Water
has been found on a planet outside our solar system for the first time - giving
scientists a tantalising hint of life beyond Earth.
The
planet, known as HD189733b, is a Jupiter like gas giant which is about 60 light
years away in the constellation of Vulpeca the Fox.
Using
NASA's infrared Spitzer space telescope, astronomers discovered that as the planet
orbits its sun it absorbs starlight in a way that can only be explained by the
presence of water vapour, or steam, in its atmosphere.
The
same side of HD 189733b always faces the host star. It was only discovered in
2005 and appears to have winds that rage around it up to 6,000 mph, which would
make it completely inhospitable for life. The jet streams on Earth travel at 200
mph.
Astrophysicist
Dr Giovanna Tinetti, of the European Space Agency, said the dramatic discovery
increases the chances of life being found among the stars - but probably not on
this exotic world. The planet orbits so close to its parent star that its surface
reaches a scorching 1,700 F.
Dr
Tinetti said: "Although HD189733b is far from being habitable, and actually
provides a rather hostile environment, our discovery shows that water might be
more common out there than previously thought, and our method can be used in the
future to study more 'life friendly' environments."
Her
team's findings, published in Nature, have given scientists their first sniffs
of air from an alien world and Dr Tinetti, who has just taken up a prestigious
Aurora Fellowship at University College London, hopes it is the start of even
more exciting discoveries.
She
added: "The 'holy grail' for today's planet hunters is to find an Earth like
planet that also has water in its atmosphere.
"When
it happens, that discovery will provide real evidence that planets outside our
Solar System might harbour life. Finding the existence of water on an extra solar
gas giant is a vital milestone along that road of discovery."
The
mysterious HD189733b belongs to a type of extrasolar planet known as "hot
Jupiters". These planets orbit precariously close to their stars and are
extremely hot.
The
cloudy planet races around its star every 2.2 days. It is more than 30 times closer
to its star than the Earth is to the Sun which means temperatures on this balmy
world range from 1,200 F on the dark side to a broiling 1,700 F on the sunlit
side.
Dr
Tinetti said it is possible for water vapour to survive in even hotter temperatures
although the existence of any sort of life form would be impossible.
Previous
studies of the same planet and of another hot Jupiter HD 209458b, located about
150 light years away in the constellation Pegasus, both found no evidence for
water.
More
than 200 "extra-solar" planets like HD189733b have been discovered but
their close proximity to their own star has made detecting water and other compounds
difficult.
Dr
Tinetti and colleagues measured the radius of HD189733b at different wavelengths
by tracking how much starlight is blocked by the planet as it crosses in front
of its parent star.
The
planet looked bigger at the wavelength bands that correspond to water, suggesting
that water is present in the atmosphere where it absorbs the radiation at these
wavelengths.
The
researchers took advantage of the fact that HD189733b is a "transiting planet"
which means it passes directly in front of its star, as seen from Earth.
When
this happens water vapour in the planet's atmosphere causes the planet to appear
slightly larger in the infrared part of the starlight than in the visible portion.
A
painstaking analysis of measurements at different wavelengths and a calculation
of highly accurate water data was able to detect the tell-tale "fingerprints"
of water molecules on the planet.
The
researchers found the light blocking area of HD189733b is slightly larger when
measured at a longer wavelength because the water vapour in the atmosphere absorbs
more light. At a shorter wavelength it transmits more light.
Astronomer
Heather Knutson, of Harvard University, Massachusetts, said: "Is the presence
of water a feature common to all gas giant planets?
"The
first convincing detection of water vapour in the atmosphere of such a planet
from outside our Solar System indicates that the answer is yes."
Telescope
technologies are being developed that will probe the very faint light from other
solar systems for tell-tale signs of biology. These are the same "life markers"
known to be present in light reflected off the Earth, known as "earthshine".
They
include signatures for water, and gases such as oxygen and methane and perhaps
more complex molecules such as chlorophyll - the pigment which makes the process
of photosynthesis possible.
Dr
Tinetti said: "At the moment we are searching for water, and with it the
possible existence of alien life, in a very indirect way.
"But
space science is moving very fast and the next generation of telescopes over the
coming decade should be able to carry out more direct investigations because they
will be much more powerful."