First Image of Extrasolar Planet Confirmed
An anonymous reader writes "The year-long controversy about whether the European Southern Observatory had indeed captured the first picture of an extrasolar planet has apparently been resolved. Journal publication today of a fuzzy image of this Jupiter-sized, extrasolar planet led Christophe Dumas, a member of the discovery team, to say enthusiastically: 'The thrill of seeing this faint source of light in real-time on the instrument display was unbelievable. Although it is surely much bigger than a terrestrial-size object, it is a strange feeling that it may indeed be the first planetary system beyond our own ever imaged.'"
It's actually (according to the BBC and eso.org) 5x the size of Jupiter, or about half the size of our sun. Calling it a mere planet may be a bit harsh - Jupiter itself is a net producer of energy (radiated = 2x incident, roughly), and it's speculated that this is due to gravity forces. This gas-giant 'planet' is presumably more active gravitationally - perhaps 'proto-sun' or 'failed sun' might be a better description (except that discovering a planet is a far greater acheivement than a tiny star...
Simon.
Physicists get Hadrons!
That, and it's orbiting a brown dwarf.
I never vote for anyone. I always vote against.
-- W.C. Fields
The key issue is whether the suspected planet is at the same distance as the brown dwarf [and I assume that we know accurately enough about the distance to the brown dwarf].
Since these stars are co-moving, it is very likely that these objects are either formed out of the same primodial materials (ie., these stars are in the same association) or gravitationally bound (i.e., the suspect planet revolves around the brown dwarf). The evidence of the co-moving alone doesn't necessarily prove that the stars are bounded by gravity, but the accuracy of their measurements probably suggest that it's pretty darn likely. Further studies are necessary to derive the orbits for sure.
Anyway, once you establish the distance, one can figure out its true brightness of the suspected planetary object. That helps you narrow down the mass of that object (which is nailed down to be about 5x the mass of Jupiter). Combined with the "color" information of the object, these scientists makes a conclusion that this is indeed a planet.
By the way, these objects are separated by the whooping 0.7 arcseconds. Its apparent seperation is 5 times greater than the apparent size of Pluto or something like that. You don't really need use the Hubble for studying something like this.
I actually work at the ESO, at the Technische Universitaet Muenchen in Garching, Germany. This is a major event for them up there- (I'm surprised it made /., they usually discourage it as they discouraged me from posting about the Venus Transit last year) . Generally, they have to fight hard to get funding from the government (although Europe is nicer about astronomy (as opposed to stuff like the ISS) than the US), so something like this is great. It incites public interest in astronomy, which is always needed for scientific institutions such as this.
Wow! I must have been under a rock these past few years. I thought the only extra-solar system stellar object to be imaged with as much clarity as this photo of a Brown Dwarf (w/ companion planet) was Betelgeuse! What other stars have been resolved so that you can make out or almost make out the disk????