Beta Pictoris, a nearby star easily visible to the naked eye in the southern sky, is already hailed as the archetypal young planetary system. It is known to harbour a planet that orbits some 1.2 billion kilometres from the star, and it was one of the first stars found to be surrounded by a large disc of dusty debris [1].
New observations from ALMA now show that the disc is permeated by carbon monoxide gas.
Paradoxically the presence of carbon monoxide, which is so harmful to humans on Earth, could indicate that the Beta Pictoris planetary system may eventually become a good habitat for life. The cometary bombardment that its planets are currently undergoing is likely providing them with life-enabling water [2].
But carbon monoxide is easily and rapidly broken up by starlight — it can only last about 100 years where it is observed in the Beta Pictoris disc. Seeing it in the 20-million year old Beta Pictoris disc is a complete surprise. So where did it come from, and why is it still there?
"Unless we are observing Beta Pictoris at a very unusual time, the carbon monoxide must be continuously replenished," said Bill Dent, an ESO astronomer at the Joint ALMA Office in Santiago, Chile, and lead author on a paper published today in the journal Science. "The most abundant source of carbon monoxide in a young solar system is collisions between icy bodies, from comets up to larger planet-sized objects."
This artist's concept illustrates the preferred model for explaining Atacama Large Millimeter/submillimeter Array observations of Beta Pictoris. The new observations from Atacama Large Millimeter/submillimeter Array now show that the disc around the star is permeated by carbon monoxide gas. The presence of carbon monoxide could indicate that the Beta Pictoris planetary system may eventually become a good habitat for life. At the outer fringes of the system, the gravitational influence of a hypothetical giant planet (bottom left) captures comets into a dense, massive swarm (right) where frequent collisions occur.
(Photo Credit: NASA's Goddard Space Flight Center/Francis Reddy)
But the rate of destruction must be very high: "To get the amount of carbon monoxide we observe, the rate of collisions would be truly startling — one large comet collision every five minutes," noted Aki Roberge, an astronomer at NASA's Goddard Research Center in Greenbelt, USA, and coauthor of the paper. "To get this number of collisions, this would have to be a very tight, massive comet swarm."
But there was another surprise in the ALMA observations, which did not just discover the carbon monoxide, but also mapped its location in the disc, through ALMA's unique ability to simultaneously measure both position and velocity: the gas is concentrated in a single compact clump. This concentration lies 13 billion kilometres from the star, which is about three times the distance of Neptune from the Sun. Why the gas is in this small clump so far from the star is a mystery.
"This clump is an important clue to what is going on in the outer reaches of this young planetary system," says Mark Wyatt, an astronomer at the University of Cambridge, UK, and a co-author on the paper. He goes on to explain that there are two ways such a clump can form: "Either the gravitational pull of an as yet unseen planet similar in mass to Saturn is concentrating the cometary collisions into a small area, or what we are seeing are the remnants of a single catastrophic collision between two icy Mars-mass planets".
Both of these possibilities give astronomers reason to be optimistic that there are several more planets waiting to be found around Beta Pictoris. "Carbon monoxide is just the beginning — there may be other more complex pre-organic molecules released from these icy bodies,"adds Roberge.
Further observations are planned with ALMA, which is still ramping up to its full capabilities, to shed more light on this intriguing planetary system, and so help us to understand what conditions were like during the formation of the Solar System.
Source: ESO