Hanny’s Voorwerp represents a snapshot in time that reveals clues about the life cycle of black holes.
While sorting through hundreds of galaxy images as part of the Galaxy Zoo citizen science project 2 years ago, Dutch schoolteacher and volunteer astronomer Hanny van Arkel stumbled upon a strange-looking object that baffled professional astronomers. Two years later, a team led by Yale University researchers has discovered that the unique object represents a snapshot in time that reveals surprising clues about the life cycle of black holes.
In a new study, the team has confirmed that the unusual object, known as Hanny's Voorwerp (Hanny's "object" in Dutch), is a large cloud of glowing gas illuminated by the light from a quasar — an extremely energetic galaxy with a supermassive black hole at its center. The twist is that the quasar lighting up the gas has since burned out almost entirely, even though the light it emitted in the past continues to travel through space, illuminating the gas cloud and producing a sort of "light echo" of the dead quasar.
"This system really is like the Rosetta Stone of quasars," said Kevin Schawinski from Yale University in New Haven, Connecticut. "The amazing thing is that if it wasn't for the Voorwerp being illuminated nearby, the galaxy never would have piqued anyone's interest."
The team calculated that the light from the dead quasar, which is the nearest known galaxy to have hosted a quasar, took up to 70,000 years to travel through space and illuminate the Voorwerp — meaning the quasar must have shut down sometime within the past 70,000 years.
Until now, it was assumed that supermassive black holes took millions of years to die down after reaching their peak energy output. However, the Voorwerp suggests that the supermassive black holes that fuel quasars shut down more quickly than previously thought. "This has huge implications for our understanding of how galaxies and black holes co-evolve," Schawinski said.
"The timescale on which quasars shut down their prodigious energy output is almost entirely unknown," said Meg Urry, director of the Yale Center for Astronomy & Astrophysics. "That's why the Voorwerp is such an intriguing — and potentially critical — case study for understanding the end of black hole growth in quasars."
Although the galaxy no longer shines brightly in X-ray light as a quasar, it is still radiating at radio wavelengths. Whether this radio jet played a role in shutting down the central black hole is just one of several possibilities Schawinski and the team will investigate next.
"We've solved the mystery of the Voorwerp," he said. "But this discovery has raised a whole bunch of new questions."