As the stars spiraled into each other, they sent gravitational waves through the universe and released tremendous amounts of light when they finally collided. Scientist call the phenomenon a "kilonova."
"We don't actually know what happened to the objects at the end," David Shoemaker, a senior research scientist at MIT and a spokesman for the LIGO Scientific Collaboration, said at a news conferenceOct. 16 at the National Press Club in Washington, DC "We don't know whether it's a black hole, a neutron star, or something else."
From neutron stars to black hole?
Such a massive object could collapse under its own weight, forming a black hole. A black hole is essentially a point of infinite density surrounded by a region of no return — the event horizon, inside which not even light can escape.
If the new object did collapse into a black hole, "it's the lightest one that we know about," Harvard astronomer Edo Berger said at the news conference. Berger's team analyzed the light from the kilonova and found evidence of superheavy elements, like gold and platinum, forged in the violent event. [What Neutron Stars Are Made Of (Infographic)]
Eleonora Troja, a high-energy astrophysicist at the University of Maryland and NASA's Goddard Space Flight Center, expressed a bit more confidence in what the new object may be. "[It's] very likely the collision of two neutron stars resulted in a new black hole," she said at the news conference.
Troja has good reason to believe the stars did form a black hole. Right after the gamma-rays and gravitational waves were detected on Earth, NASA's Swift Gamma-Ray Burst observatory, which orbits high above Earth, returned some interesting results: a bright source of ultraviolet light, but no X-rays. This was the first time in the Swift observatory's 13 years of working on the mission that it had come up empty-handed, according to Troja. NASA's Chandra X-ray Observatory, and Nuclear Spectroscopic Telescope Array (NuSTAR), also saw nothing in the X-ray spectrum.
A signal! But from what?
Nine days after the gravitational waves were detected by LIGO and Virgo, Troja's team finally picked up a faint X-ray signal — one so weak only the space-based Chandra X-ray Observatory could detect it.
For Troja, the faint signal suggests the presence something far more powerful: jets of matter and radiation spewing the same amount of energy in a few days that the sun radiates over millions of years.
The paltry signal was an effect of the viewing angle, Raffaella Margutti, an astrophysicist at Northwestern University, told Space.com. It took nine days for the jet to spread out enough for the spray of X-rays to begin hitting Earth, she said. Margutti is the lead author on one of the Chandra X-ray Observatory studies that resulted from the discovery, and a coauthor on at least eight related studies.