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Hot Topic Deep Space Cosmic Evolution Free-floating Twins Test Theories
 
Free-floating Twins Test Theories
based on an ESO release
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Cosmic Evolution
Posted:   08/08/06

Summary: The cast of exoplanets has an extraordinary new member. Using ESO's telescopes, astronomers have discovered an approximately seven- Jupiter-mass companion to an object that is itself only twice as hefty. Both objects have masses similar to those of extra-solar giant planets.

Free-floating Twins Test Theories

Near-infrared image of the system Oph 162225-240515AB, obtained with ISAAC on ESO's Very Large Telescope. North is up and East is to the left. The apparent separation is less than 2 arcseconds, corresponding to 242 times the distance between the Earth and the Sun (242 astronomical units) at the distance of the system, 400 light-years.
Credit: ESO


The cast of exoplanets has an extraordinary new member. Using ESO's telescopes, astronomers have discovered an approximately seven- Jupiter-mass companion to an object that is itself only twice as hefty. Both objects have masses similar to those of extra-solar giant planets, but they are not in orbit around a star - instead they appear to circle each other. The existence of such a double system puts strong constraints on formation theories of free-floating planetary mass objects.

Ray Jayawardhana of the University of Toronto (Canada) and Valentin D. Ivanov of ESO report the discovery in the August 3 issue of Science Express, the rapid online publication service of the journal Science.

"This is a truly remarkable pair of twins - each having only about one percent the mass of our Sun," said Jayawardhana. "Its mere existence is a surprise, and its origin and fate a bit of a mystery."

Roughly half of all Sun-like stars come in pairs. So do about a sixth of brown dwarfs, 'failed stars' that have less than 75 Jupiter masses and are unable to sustain nuclear fusion in their cores. During the past five years, astronomers have identified a few dozen of even smaller free-floating planetary mass objects, or planemos, in nearby star forming regions. Oph 162225-240515, or Oph1622 for short, is the first planemo found to be a double.

The researchers discovered the companion candidate in an optical image taken with ESO's 3.5-m New Technology Telescope at La Silla, Chile. They decided to take optical spectra and infrared images of the pair with ESO's 8.2-m Very Large Telescope to make sure that it is a true companion, instead of a foreground or background star that happens to be in the same line of sight. These follow up observations indeed confirmed that both objects are young, at the same distance, and much too cool to be stars. This suggests the two are physically associated.

By comparing to widely used theoretical models, Jayawardhana and Ivanov estimate that the companion is about seven times the mass of Jupiter, while the more massive object comes in at about 14 times Jupiter's mass. The newborn pair, barely a million years old, is separated by about six times the distance between the Sun and Pluto, and is located in the Ophiuchus star-forming region approximately 400 light years away.

Planets are thought to form out of discs of gas and dust that surround stars, brown dwarfs, and even some free-floating planetary mass objects (see ESO 19/06). But, "it is likely that these planemo twins formed together out of a contracting gas cloud that fragmented, like a miniature stellar binary," said Jayawardhana. "We are resisting the temptation to call it a 'double planet' because this pair probably didn't form the way that planets in our Solar system did," added Ivanov.

This is an artist's impression of what a twin planemo system might look like. The two objects are still very young and are probably surrounded by a disc of material. For clarity, the image is not to scale to Oph 1622, the system just discovered as the size of the discs and the separation between the two objects would make them very tiny.
Credit: ESO


Oph1622B is only the second or third directly imaged planetary mass companion to be confirmed spectroscopically (see ESO 23/04 [1]), and the first one around a primary that is itself a planetary mass object. What's more, its existence poses a challenge to a popular theoretical scenario, which suggests that brown dwarfs and free- floating planetary mass objects are embryos ejected from multiple proto-star systems. Since the two objects in Oph1622 are so far apart, and only weakly bound to each other by gravity, they would not have survived such a chaotic birth.

"Recent discoveries have revealed an amazing diversity of worlds out there. Still, the Oph1622 pair stands out as one of the most intriguing, if not peculiar," said Jayawardhana.

"Now we're curious to find out whether such pairs are common or rare. The answer could shed light on how free-floating planetary-mass objects form," added Ivanov.

 

 


Related Web Pages

Extrasolar Planets Encyclopedia
Planet Quest (JPL)
Kepler Mission
'Planemo' Spawn
Twinkle Twinkle Little Star
Busy Brown Dwarfs
The Wolf: New Planet or Brown Dwarf Star?


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