Although well over 500 planets orbiting other stars are known to exist — and we know of many, many more awaiting confirmation — direct images of the planets are very rare. That’s because stars are billions of times brighter than planets, and the planets tend to huddle so closely to their star that their feeble light gets overwhelmed.
But it’s possible, and we have several images of such exoplanets. One of them is Beta Pictoris b, a super-Jupiter orbiting the star Beta Pic (as we in the know call it) about as far out as Saturn orbits the Sun. Its existence was confirmed in 2009, but it was also seen in earlier images in 2003 and 2008. The motion of the planet from one side of the star was obvious, and now observations from March 2010 again show it has moved as it orbits the star:
Pretty cool! These infrared images from the Very Large Telescope all have the starlight removed to show the faint planet (the faint rings and other blobs are optical effects and can be ignored). The upper left picture is from 2003; the upper ...
"
