The world, known as HD189733b, has a deep azure hue -
probably the result of silicate (glass) rain in the atmosphere, which
scatters blue light.
Details of the discovery, made with the Hubble Space Telescope, are to appear in Astrophysical Journal Letters.
Although it might resemble Earth from a distance, HD189733b is a huge gas giant which orbits close to its host star.
The temperature of the planet's atmosphere is a scorching
1,000C, and it rains glass, sideways, in howling 7,000km-per-hour winds.
Its atmosphere has been found to be dramatically changeable and exotic, with hazes and violent bursts of evaporation.
At a distance of 63 light-years from us, this turbulent alien
world is one of the nearest exoplanets to Earth that can be seen
crossing the face of its star.
It has been extensively studied by ground- and space-based telescopes. Now, astronomers have measured its visible colour.
"Measuring its colour is a real first - we can actually imagine
what this planet would look like if we were able to look at it
directly," said Prof Frederic Pont, from the University of Exeter.
In order to measure what this planet would look like to our
eyes, the astronomers measured how much light was reflected from its
surface - a property known as albedo.
HD 189733b is faint and close to its sun. But as the planet
passed behind its host star, the astronomers were able to measure
changes in the spectrum as light reflected by the planet was temporarily
blocked out.
"We saw the brightness of the whole system drop in the blue
part of the spectrum when the planet passed behind its star," explained
Tom Evans from the University of Oxford, first author of the paper.
"From this, we can gather that the planet is blue, because the signal remained constant at the other colours we measured."
Earth looks blue from space because the oceans absorb red and
green wavelengths more strongly than blue ones, and reflect the
blue-ish hue of our sky.
The exoplanet's azure colour does not come from the
reflection of an ocean, say the researchers, but is probably due to the
hazy, turbulent atmosphere being laced with silicate particles - which
scatter blue light.
HD 189733b presented a favourable case for these kinds of
measurements as it belongs to a class of planets known as "hot
Jupiters". These massive planets are similar in size to the gas giants
in our Solar System, but instead lie very close to their parent stars.
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