Not to be outdone, a French team today released their image of a tiny but definitely real speck glowing in the infrared 0.4 arcsecond from Beta Pictoris, a young star 63 light-years away. The speck is just inside the inner edge of Beta Pic's enormous, famous debris disk a wide platter of dust that we see nearly edge-on.
The astronomers, led by Anne-Marie Lagrange (University of Grenoble), used one of the 8.2-meter reflectors of the Very Large Telescope array run by the European Southern Observatory at Paranal in Chile. The speck, glowing in infrared light 1,000 times fainter than Beta Pic itself, was resolved by means of severe image processing to eliminate almost all of the star's dazzling glare. Beta Pic is a naked-eye star shining at 4th magnitude in the far-southern sky near Canopus. It is a hot, white, type-A3 star eight times as luminous as the Sun.
Beta Pic b lies about 8 astronomical units from the star, roughly Saturn's distance from the Sun. This puts it much closer to its star than last week's directly-imaged exoplanets. Gravitational effects perturbing the debris disk had already suggested that a giant planet ought to be there.
Given Beta Pic's very young age (10 or 20 million years) and the new object's apparent high temperature (about 1,500 kelvins), it should have a mass of about 8 Jupiters, which puts it within the planetary category.
Unlike the four planets in last week's images, "Beta Pictoris b" has not been observed long enough for it to show any sign of orbital motion around its star or even to show that it is traveling with the star across the sky ("common proper motion"). Even so, the chance that it could be a background object unrelated to Beta Pic is extremely slim.
Read the full (and very informative) ESO press release.
And here is the team's discovery paper.