What happens when a black hole
falls on hard times? An international team of astronomers have found a
black hole that’s rapidly getting dimmer, and they think it’s starving.
The idea makes sense. Black holes often lie at
the core of galaxies. When a black hole forms you can’t see it, but
whatever falls into the black hole heats up as it falls, throwing off
detectable radiation all over the EM spectrum. This leaves galactic
centers aglow with spinning debris. But after a certain point, a
black hole
should clear its surroundings, having already accreted everything that
was close enough to fall in. And after that, after the glow of gases
falling into the black hole has faded, what remains would be just the
black hole itself, bereft of its incandescent accretion disc.
Scientists are thrilled to have caught this
fading phenomenon in action, right after it started to happen to a
supermassive black hole at the core of Markarian 1018, a galaxy in the
Cetus constellation. This is the first such thing we’ve ever studied.
Bernd Husemann, CARS project leader and lead author of a
paper
discussing their observations and hypotheses, explained: “We were lucky
that we detected the event just 3-4 years after the decline started, so
we could begin monitoring campaigns to study details of the accretion
physics of active galaxies that cannot be studied otherwise.”
Black holes don’t just hover in space glowing
at a constant brightness. As they accrete material of varying densities
and amounts, they flicker, with a frequency on the order of tens of
thousands of years — almost like a candle guttering and flaring in a
breeze. But that’s not what’s going on here. Ten years is such a short
little blip on cosmic timescales, but 10 years is all it’s taken for the
brightness of this supermassive black hole to dim by an order of
magnitude. Scientists have actually been watching this particular black
hole off and on for thirty years. Every instrument they looked with has
showed a five- to ten-fold decrease in brightness over the last ten
years.
Ingesting a star causes a brief, sharp flare
that trails off slowly as the black hole finishes its “meal.” But the
team of astronomers who have been watching this black hole have seen it
do exactly none of that, either. Geometry and spectral lines have ruled
out debris along the line of sight. No, the dimming the astronomers have
seen suggests something else entirely.
There’s a huge ring of ingestable debris at a
radius of about 24 light-days, at which distance it would take about
five years to fall into the black hole. But the ring isn’t being sucked
in, even though it’s within range. Why? “It’s possible that this
starvation is because the inflow of fuel is being disrupted,” said
Rebecca McElroy, lead author of the paper
outlining the discovery.
“An intriguing possibility is that this could be due to interactions
with a second supermassive black hole.” Such a black hole binary system
is a distinct possibility in Markarian 1018, since it’s the product of a
major merger of two galaxies — each of which probably had a
supermassive black hole at its core.
How far does the metaphor extend? Can a black hole starve to death?
The astronomers intend on finding out. Their discovery of this
phenomenon got them discretionary time on the VLA, Hubble and Chandra
all, and they’ll be making continuing observations across the whole EM
band to figure out just exactly what is going on at Markarian 1018.
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