Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) telescope in northern Chile have today announced the discovery of an unexpected clump of carbon monoxide gas in the dusty disk around the star Beta Pictoris. This is a surprise, as such gas is expected to be rapidly destroyed by starlight. Something—probably frequent collisions between small, icy objects such as comets—must be causing the gas to be continuously replenished. The new results are published today in the journal Science.
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 harbor a planet that orbits some 1.2 billion kilometers from the star, and it was one of the first stars found to be surrounded by a large disk of dusty debris [1].
New observations from ALMA now show that the disk 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 be a good habitat for life. If there is carbon monoxide in the comets, then there is likely also water ice, meaning that the cometary bombardment that its planets are currently undergoing could also be providing them with life-giving water.
But carbon monoxide is easily and rapidly broken up by starlight—it can only last about 100 years. Seeing it in a disk of this age 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 William R.F. 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.”
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—complete destruction of a large comet once 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 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 disk 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.
Figure 1. The ALMA image of carbon monoxide around Beta Pictoris (above) can be deprojected (below) to simulate a view looking down on the system, revealing the large concentration of gas in its outer reaches. For comparison, orbits within the Solar System are shown for scale.
Credit: ALMA (ESO/NAOJ/NRAO) and NASA’s Goddard Space Flight Center/F. Reddy
Click to enlarge (JPEG/ 774KB)
“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 many 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 understand what conditions were like during the formation of our own Solar System.
This research was presented in a paper entitled “Molecular Gas Clumps from the Destruction of Icy Bodies in the Pictoris Debris Disk” to appear in the journal Science on 6 March 2014.
Note
[1] Many stars harbor such dust, known as debris disks. They are the remains of a collisional cascade of the rocks in orbit around the star, much like the collisional breakup of the space station depicted in the movie Gravity (but on a much larger scale).
Figure 2. Artist’s impression of the preferred model for explaining ALMA observations of Beta Pictoris. 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.
Credit: NASA’s Goddard Space Flight Center/F. Reddy
Click to enlarge (JPG/ 2.6MB)
