The galactic train wreck of dark matter
When physicists want to understand the deep constituents of fundamental particles, they have the luxury of smashing them together in super-powerful accelerators like the Large Hadron Collider. The subatomic shrapnel that flies out of those collisions can be highly informative about whether the physicists’ theories match reality. Alas, astrophysicists hoping to learn more about the makeup of galaxies don’t have quite the same latitude: galaxies are notoriously hard to push around on command.
Sometimes, however, nature does scientists a favor and delivers the experiment they could never do on their own. Recently, through the Hubble Space Telescope and other instruments, astronomers have been able to check the wreckage of accidental collisions between distant clusters of galaxies for hints about one of the greatest unsolved mysteries in science: dark matter.
To their frustration and surprise, however, the new data may only leave dark matter as more mysterious than ever. Not only do results from a Hubble survey of the galaxy cluster Abell 520 announced this past week contradict physicists’ theories about how dark matter should behave, but they also directly conflict with observations of a similar collision from five years ago.
Dark matter deduced
Back in the 1930s, the astronomer Fritz Zwicky of the California Institute of Technology first noticed something odd about the rotations of galaxies: they were moving as though they had about six times as much mass as all their stars could account for. He and other astronomers would have expected the stars to orbit the centers of their galaxies more or less like particles loosely swirling around a drain. Instead, the stars seemed to revolve in a more rigid formation, like specks on a spinning disk.
Astronomers’ best explanation was that the galaxies’ missing mass must exist as some form of invisible “dark matter” that didn’t reflect light or interact with conventional matter in any way except gravitationally.
The scientists have batted around various ideas about the nature of dark matter and the current favorite is that it consists of what they call weakly interacting massive particles, or WIMPs. Vast, football shaped halos of WIMPs may extend out beyond the swirling spirals and other configurations of stars in galaxies.
The irony, then, was that everything in the universe visible to us as ordinary matter (or baryonic matter, in the jargon of physics) — all the stars, planets, moons, chairs, trees, and so on — was an exception on a cosmic scale. It represented only 5 percent of all the mass in the university[typo: ha!] universe, whereas dark matter was 25 percent. (The remaining 70 percent is tied up in dark energy, a repulsive force that makes the universe expand and is not to be confused with dark matter.)
For obvious reasons, astronomers have desperately wanted to observe dark matter directly to verify their theories, to little or no avail. Huge subterranean instruments in Italy and Minnesota constructed to detect WIMPs passing through the earth have sometimes reported seeing signals that might betray them, but the general consensus among physicists at the moment is that dark matter has still only ever been seen on a cosmic scale by inferring its presence from its gravitational effects. Dark matter appeared too elusive and too hard to strip away from galaxies’ baryonic matter to see on its own.
Putting galactic collisions to work
Astronomers realized, however, that collisions between clusters of galaxies — which move at millions of miles an hour and are the largest structures in the universe — might succeed in stripping dark matter away from ordinary matter and leaving it relatively exposed (even if it would still be invisible). Even in an ever-expanding universe, the lumpy distribution of galaxies throughout the heavens guarantees that sometimes their trajectories will intersect. When that happens, gravity will make the stars, gas clouds and other baryonic masses in each galaxy cluster mutually interact. They may not actually slam together like cars in a demolition derby (galaxy clusters are mostly empty space, after al) but they can slow one another’s motions and disrupt the galaxies’ shapes.
Not so the galaxies’ dark matter halos, however. Because the dark matter does not interact with much of anything, the slippery, invisible halos should pass right through one another even while their visible matter accompaniments scrape together and tear free.
In 2006 astronomers thought they had discovered proof of their ideas about dark matter. Researchers at the Kavli Institute for Particle Astrophysics and Cosmology turned the Hubble Space Telescope, the Magellan and Very Large Telescopes in Chile, and the orbiting Chandra X-ray Observatory toward the Bullet Cluster, which marks a collision between two galaxies three billion light-years away. As predicted, the mass in the cluster resolved into four clumps: two small ones made of luminous matter in close proximity flanked by two much heavier clumps speeding away from the collision that lacked any visible stars.
Astronomers’ sense of vindication lasted only about a year, however. By 2007, astronomers at the University of Victoria in Canada had attempted a similar examination of another gigantic galaxy cluster called Abell 520, about 2.4 billion light-years away. Their results were jarringly different from those for the Bullet Cluster. In fact, they showed very nearly the exact opposite pattern: small, disrupted clumps of luminous baryonic matter were sailing away from the collision site, but most of the mass was still sitting at the center in a relatively starless void.
With some hope that further observations might somehow eliminate the discrepancy, astronomers began examining Abell 520 again in more detail with the Hubble Space Telescope and other instruments. James Jee of the University of California in Davis and his colleagues in California and Canada published the results of those studies last week in The Astrophysical Journal. Disconcertingly, they only confirmed the earlier observations.
As NASA’s press release on the research notes:
“This result is a puzzle,” said astronomer James Jee of the University of California in Davis [...]. “Dark matter is not behaving as predicted, and it’s not obviously clear what is going on. It is difficult to explain this Hubble observation with the current theories of galaxy formation and dark matter.”
What explanations could there be for the differences between how the dark matter has behaved in Abell 520 and in the Bullet Cluster? Several possibilities exist, as Jee and his colleagues have enumerated, but each is rather less savory than the next.
One obvious way to wish away the Abell 520 observations is simply to say that they might be wrong or incomplete. Perhaps the “dark core” of the collision contains more galaxies than the Hubble detected because for some reason, those galaxies contain unusually few stars. The special pleading and odd coincidences involved in making that explanation stand up seem rather far-fetched, however.
Similarly, astronomers could be wrong about the dynamics of the galaxy cluster collisions. The Bullet Cluster was the product of a merger between just two galaxy systems; if Abell 520 emerged from the merger of three, then maybe that difference is enough to explain the discrepancy between the two. Further computer simulations may help to illuminate the problem but it is not immediately clear why a three-cluster collision would end up with so much dark matter at its center.
Physicists also can’t rule out the possibility that dark matter exists in different forms, one of which is “stickier” than the other. That solution might seem like the easiest to embrace: why not simply tack on one more property to such a mysterious substance? The problem is that for the stickiness to exist, then at least some dark matter must be capable of interactions other than the weak ones ascribed to hypothetical WIMPs. And if that is so, it might undermine the standard model of cosmology — a change so disruptive that it would pose more questions than it solved.
The most unsettling of all explanations would be that dark matter doesn’t behave as expected because dark matter doesn’t exist. For almost 30 years, a small minority of physicists inspired by Mordehai Milgrom of the Weizmann Institute have argued that it was wrong to deduce dark matter’s existence from gravitational anomalies in galactic rotations. The more straightforward possibility, they say, is that gravity behaves a little differently on the scale of a galaxy than it does here on earth. They favor a reformulation of gravitational theory called modified Newtonian dynamics (MOND) that tweaks the equations established by Isaac Newton and Albert Einstein.
MOND, too, might disrupt more of physics than it saves, but even putting that objection aside, Abell 520 may not offer much support for the theory. Astrophysicist Arif Babul of the University of Victoria, who was involved in both the previous study and the current one, has been quoted by New Scientist as saying that he and his colleagues tried to fit the observational data into a MOND framework before they wrote up their 2007 paper and couldn’t do it.
So the mystery of dark matter seems to be as profound as ever. Collisions between galactic clusters were supposed to help bring the invisible to light. Instead, they seem to be making a train wreck of the available theories.