A long, long time ago, a pair of black holes collided with such power that they created ripples in spacetime, which emanated through the universe. All the while, molecules on a tiny rock in a fairly irrelevant nook of the Milky Way galaxy arranged themselves into living things, which evolved into self-aware apes. Those apes eventually realized they could actually measure those spacetime wobbles, and built several kilometer-long machines (tiny if you really think about it) in order to do so. When they flipped the switch, they caught the wobbles just in time.
But then they spotted another set of wobbles, and hints of yet another (though they weren’t sure). Now they’ve confirmed a third event, and it made the apes wonder: What does it all mean? And where do we go from here?
Today, the pair of Laser Interferometer Gravitational Wave Observatories (LIGO) are confirming the detection of a third set of these gravitational waves, first predicted by Albert Einstein over a hundred years ago. While the third discovery is still almost as exciting as the first and second, scientists are now starting to think about what these waves can tell them about our universe, and what they can do once they’ve seen a lot of them.
“This is just the beginning,” Gabriela Gonzalez, the last spokesperson for the LIGO Scientific Collaboration and professor from Louisiana State University, told Gizmodo. “There’s a lot more coming.”
Scientists have tasked two LIGOs with observing gravitational waves, one in Washington State and the other in Louisiana. They’re essentially a pair of perpendicular rulers made out of light, where optics systems split a laser, send the beams down long pipes, then unite them at a detector. If a gravitational wave rolls by, the amount of space the light has to traverse changes, moving the two beams in and out of alignment and creating a waveform on a graph. Scientists need two LIGOs to confirm that the observation wasn’t just a truck rolling by. And a similar observatory, called Virgo, is now turned on in Italy and will join the LIGOs soon to better determine the origin and behavior of gravitational waves.
The LIGOs spotted the most the most recent wave event, GW170104, on January 4 of this year. They used the waveform to determine that it came from a pair of colliding black holes three billion lightyears away, approximately 31 and 19 times the mass of our Sun, turning into a single black hole around 49 times the mass, and published their results today in the journal Physical Review Letters. The mass of this black hole fits quite nicely between the mass of the black holes inferred from heavier and lighter waves measured previously. The waveform also supplied some tantalizing hints of an answer to the question of how a pair of black holes end up orbiting each other in the first place.
A black hole binary could either form from a pair of orbiting stars that both collapsed, or if one black hole passed by another and got tangled up in its gravity. If the first case were true, the spins of the black holes would align with their orbits. But if the spins were in the opposite direction of the orbits, the second scenario would be more likely. The latest gravitational wave observation is starting to point scientists towards the second case. It’s certainly not conclusive yet, but it implies that in the distant (and therefore younger) universe, there could places concentrated with coalescing black holes, Imre Bartos, associate research scientist from Columbia University, told Gizmodo.
“This event is not a smoking gun, but it’s the first event for which we more seriously prefer one scenario over another,” Salvatore Vitale, assistant professor at MIT, told Gizmodo. “If you ask me I think it’s too early to say anything conclusive,” he said.
Gravitational wave astronomy is still in its infancy, but we’re soon going to get to a point where each individual detection of waves isn’t news. We’re not there yet, but soon you should expect to start hearing more about what scientists can pick out of trends among lots of colliding black holes, and about follow-up observations from the networks of satellites and telescopes looking for an electromagnetic or neutrino counterpart to the gravitational waves.
“If you want to get some kind of optical or electromagnetic follow up observation, you’ll need something that doesn’t just have two black holes,” Scott Hughes, professor of physics at MIT, told Gizmodo. Picking out such a signature would likely require two neutron stars, incredibly massive balls not quite dense enough to collapse into black holes. LIGO probably needs its sensitivity increased before it can spot neutron star mergers, something the detectors will work on when this year’s run is over. “The hope is that we will start those observations,” those with the two LIGO detectors plus Virgo, and improved sensitivities, “mid summer 2018 or so,” said Gonzalez. “Having the sensitivity, perhaps we’ll begin seeing neutron stars with a few months of data.”
All the while, scientists will continue using gravitational waves to test various theories about our universe, from the more exotic, to whether gravitational fields have a particle associated with them the way that electricity does, to Einstein’s theory of relativity. “You can never prove that a theory is correct—you can only prove it wrong,” said Vitale. “Einstein is not yet wrong.”
That is amazing, by the way. Gravitational waves, a prediction made by general relativity dreamed up a hundred years ago to explain strange kinks in the theory of gravity, like the weirdness of Mercury’s orbit, can also describe powerful events taking place on the other end of the universe. “It’s a human being compared to Usain Bolt,” he said. “That same theory without any modifications also explains the motion of objects incredibly massive moving incredibly fast, velocities comparable to the speed of light.” To be fair, it would be very exciting to a lot of people if someone did find a deviation from Einstein’s theory.
Further down the road after Virgo is hooked up, other detectors, including one in India and another in Japan, will help pinpoint the location of gravitational waves—right now, there’s a huge swath of the sky from which they can originate. Eventually, scientists will also be able to determine the waves’ polarization, the way they actually deform space as they travel.
Scientists are crossing their fingers for something unexpected. “To tell you the truth, what I’m most exited about is discovering the unknown,” said Gonzalez. “Like finding a signal strong like the first one that doesn’t follow a model that we know of.”