Detecting the thin rings would reaffirm Einstein’s theory of gravity
Faint rings of light surrounding
enormous black holes could be spotted with the help of a future generation of telescopes
The doughnut-shaped glow spotted in the first image of a black hole, released in April 2019 by the Event Horizon
Telescope collaboration (SN: 4/10/19),
is more complex than the worldwide network of radio telescopes could discern. The
black hole’s gravity is so intense that some particles of light, called
photons, can circle the black hole partway — or once, twice or multiple times —
before escaping to be picked up by telescopes. Those orbiting photons produce a
“photon ring,” made up of a series of subrings — circles of light that appear
successively thinner and harder for telescopes to pick out.
“It’s sort of like a hall of mirrors,
where we’re getting an infinite series of images,” says astrophysicist Michael
Johnson of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass.
Now, Johnson and colleagues calculate
that, with the help of new telescopes in space, the photon subrings theoretically
could be observed around the supermassive black hole at the center of the
galaxy M87, the subject of that first black hole snapshot.
The Event Horizon Telescope, or EHT, combines
the powers of telescopes across the world, via a technique called very long baseline interferometry, so that they operate like one, larger telescope (SN: 4/10/19). But to tease out more
details, such as black hole subrings, researchers would need to add telescopes
separated by even larger distances.
A radio telescope orbiting Earth could capture the first subring, the team reports March 18 in Science Advances. But observing the second subring would require an even more distant telescope — on the moon. The third subring could be detected with a telescope even farther out, 1.5 million kilometers from Earth.
Scientists previously have proposed such
telescopes, but the plans haven’t yet gotten off the ground. Johnson says that
the new study provides new motivation for adding a space-based telescope to the
Although the EHT wouldn’t directly
photograph the subrings, it could detect their existence. That detection would
reaffirm Einstein’s theory of gravity, the general theory of relativity, which
predicts the rings’ existence. It also could allow for better measurements of
the black hole’s mass and how fast it is spinning.
The idea “will be challenging, but it’s
something to look forward to,” says astrophysicist Avi Loeb at Harvard
University, who was not involved with the research. “It is an exciting goal for
the next generation.”