This was released a couple of days ago but I just ran across it. The European Corot satellite observatory has discovered an extrasolar planet which seems to have a temperature in the liquid-water range.
This is rare because of the way astronomers look for exoplanets: they search for visible fluctuations in the star's output -- which are usually caused by massive objects passing in front of the star's disk, blocking some of the light. It's easiest to detect when the object is really close to the target star. Not only does that mean it's blocking more light, it also means the planet's orbital period is nice and short, so it can turn up in a relatively small sample of observations. For example, if you're on a planet of another star and you're watching our Sun to see if it has planets, you're much more likely to spot Mercury crossing the face of the Sun than Earth, because Mercury makes seven orbits around the Sun for each one that Earth does. (It's also possible to look for Doppler shift fluctuations caused by the motion of a massive body around the star, but that also favors large, close-in, fast-moving planets.)
But the Corot team have been watching long enough to spot a giant planet orbiting at the right distance from its parent star to have temperatures in the liquid water range. Now despite the headlines on the pop-science articles, it's more than unlikely for a gas giant -- no matter what its temperatures -- to have life. That's not really the important thing about this find. What is important is that it's the first large exoplanet which doesn't have insanely high temperatures, and that means scientists can compare it to the giants of our own Solar system, and thus learn more about how planets form and develop.
Astronomy is one of those sciences which don't allow experiments. You're limited to one set of data, which happens to be the observable universe. Any new data point, especially about planets, is valuable.
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