This image, created using computer models, shows how the extreme
gravity of the black hole in M87 distorts the appearance of the jet near
the event horizon. Part of the radiation from the jet is bent by
gravity into a ring that is known as the 'shadow' of the black hole.
(Sep. 27, 2012) — The point of no return: In
astronomy, it's known as a black hole -- a region in space where the
pull of gravity is so strong that nothing, not even light, can escape.
Black holes that can be billions of times more massive than our sun may
reside at the heart of most galaxies. Such supermassive black holes are
so powerful that activity at their boundaries can ripple throughout
their host galaxies.
Now, an international team, led by researchers at MIT's Haystack
Observatory, has for the first time measured the radius of a black hole
at the center of a distant galaxy -- the closest distance at which
matter can approach before being irretrievably pulled into the black
hole.
The scientists linked together radio dishes in Hawaii, Arizona and
California to create a telescope array called the "Event Horizon
Telescope" (EHT) that can see details 2,000 times finer than what's
visible to the Hubble Space Telescope. These radio dishes were trained
on M87, a galaxy some 50 million light years from the Milky Way. M87
harbors a black hole 6 billion times more massive than our sun; using
this array, the team observed the glow of matter near the edge of this
black hole -- a region known as the "event horizon."
"Once objects fall through the event horizon, they're lost forever,"
says Shep Doeleman, assistant director at the MIT Haystack Observatory
and research associate at the Smithsonian Astrophysical Observatory.
"It's an exit door from our universe. You walk through that door, you're
not coming back."
Doeleman and his colleagues have published the results of their study this week in the journal Science.
Jets at the edge of a black hole
Supermassive black holes are the most extreme objects predicted by
Albert Einstein's theory of gravity -- where, according to Doeleman,
"gravity completely goes haywire and crushes an enormous mass into an
incredibly close space." At the edge of a black hole, the gravitational
force is so strong that it pulls in everything from its surroundings.
However, not everything can cross the event horizon to squeeze into a
black hole. The result is a "cosmic traffic jam" in which gas and dust
build up, creating a flat pancake of matter known as an accretion disk.
This disk of matter orbits the black hole at nearly the speed of light,
feeding the black hole a steady diet of superheated material. Over time,
this disk can cause the black hole to spin in the same direction as the
orbiting material.
Caught up in this spiraling flow are magnetic fields, which
accelerate hot material along powerful beams above the accretion disk
The resulting high-speed jet, launched by the black hole and the disk,
shoots out across the galaxy, extending for hundreds of thousands of
light-years. These jets can influence many galactic processes, including
how fast stars form. 'Is Einstein right?'
A jet's trajectory may help scientists understand the dynamics of
black holes in the region where their gravity is the dominant force.
Doeleman says such an extreme environment is perfect for confirming
Einstein's theory of general relativity -- today's definitive
description of gravitation.
"Einstein's theories have been verified in low-gravitational field
cases, like on Earth or in the solar system," Doeleman says. "But they
have not been verified precisely in the only place in the universe where
Einstein's theories might break down -- which is right at the edge of a
black hole."
According to Einstein's theory, a black hole's mass and its spin
determine how closely material can orbit before becoming unstable and
falling in toward the event horizon. Because M87's jet is magnetically
launched from this smallest orbit, astronomers can estimate the black
hole's spin through careful measurement of the jet's size as it leaves
the black hole. Until now, no telescope has had the magnifying power
required for this kind of observation.
"We are now in a position to ask the question, 'Is Einstein right?'"
Doeleman says. "We can identify features and signatures predicted by his
theories, in this very strong gravitational field."
The team used a technique called Very Long Baseline Interferometry,
or VLBI, which links data from radio dishes located thousands of miles
apart. Signals from the various dishes, taken together, create a
"virtual telescope" with the resolving power of a single telescope as
big as the space between the disparate dishes. The technique enables
scientists to view extremely precise details in faraway galaxies.
Using the technique, Doeleman and his team measured the innermost
orbit of the accretion disk to be only 5.5 times the size of the black
hole event horizon. According to the laws of physics, this size suggests
that the accretion disk is spinning in the same direction as the black
hole -- the first direct observation to confirm theories of how black
holes power jets from the centers of galaxies.
The team plans to expand its telescope array, adding radio dishes in
Chile, Europe, Mexico, Greenland and Antarctica, in order to obtain even
more detailed pictures of black holes in the future.
Christopher Reynolds, a professor of astronomy at the University of
Maryland, says the group's results provide the first observational data
that will help scientists understand how a black hole's jets behave.
"The basic nature of jets is still mysterious," Reynolds says. "Many
astrophysicists suspect that jets are powered by black hole spin ... but
right now, these ideas are still entirely in the realm of theory. This
measurement is the first step in putting these ideas on a firm
observational basis."
This research was supported by the National Science Foundation.




