Scientists have recently discovered ripples in space-time caused by the collision of two gigantic black holes located billions of light-years away. Each black hole has more than 100 times the mass of our sun. They danced around each other for eons before merging into an even larger black hole.
This merger is the largest of its kind ever detected by gravitational wave observatories. The event is pushing physicists to rethink how these enormous black holes form. The observatories on Earth picked up a faint signal from the merging black holes, which was smaller than the width of a proton.
According to Professor Mark Hannam from Cardiff University, “These are the most violent events we can observe in the universe, but they are incredibly weak by the time they reach us.” The ripples were detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO) at precisely 2 PM UK time on November 23, 2023. Two detectors in Washington and Louisiana picked up simultaneous signals.
During the merger, space-time experienced a brief stretch and squeeze lasting just one-tenth of a second. This moment captured the “ringdown phase” as the two black holes settled into a new, larger one. Experts analyzed the signal and found that the black holes weighed in at 103 and 137 times the mass of the sun. They were spinning at nearly 400,000 times the speed of Earth, approaching the limits of what we thought was possible for black holes.
“It’s surprising because this mass range is where we didn’t expect black holes to form,” Hannam noted. Most black holes develop when massive stars exhaust their nuclear fuel and collapse, creating an event horizon beyond which nothing, not even light, can escape.
Interestingly, scientists believe these black holes may have originated from earlier mergers themselves, helping to explain their immense size and rapid spin. This merger is especially significant because it produced a black hole up to 265 times the mass of the sun, surpassing the previous record of 140 solar masses.
About 300 black hole mergers have been identified through gravitational waves. The details of this remarkable finding will be unveiled at the upcoming GR-Amaldi meeting in Glasgow.
Before the 1990s, when the first gravitational wave detectors came online, scientists had limited ways to explore the universe—mostly through visible light and other electromagnetic waves. Gravitational wave observatories like LIGO have opened up a new dimension in cosmic observation, revealing events previously hidden from view.
Hannam highlights a transformative aspect of scientific discovery: “When you explore the universe in new ways, unexpected revelations often emerge. Upcoming detectors will allow us to see all black hole mergers in the universe, plus some surprises we can’t predict.”
The rapid advancements in gravitational wave astronomy signal a new era in our understanding of the universe. The potential to spot more black holes and unveil their mysteries excites researchers across the globe. As technology evolves, the scientific community eagerly anticipates what lies ahead in this fascinating field.
For more detailed insights, you can visit the LIGO website.