Astronomers Just Zoomed Stunningly Close to The Event Horizon of Our Galaxy's Black Hole

around the world have joined forces to try to provide us with our first
photograph of a black hole. That's still a few months off, at least, but all
that staring at a black hole is already starting to produce results.

In 2013, the
Atacama Pathfinder Experiment (APEX) radio telescope in Chile joined the global
telescope collective that makes up the Event Horizon Telescope (EHT), to take
observations of Sagittarius A*, the supermassive black hole at the centre of
our galaxy.

And it
almost doubled the longest baseline length in the array, leading to observation
of the finest details yet of the space right around the event horizon of this
black hole.

Now, we
can't actually see black holes. They're thought to be incredibly dense
collapsed stars with a gravitational pull so strong that nothing, not even
light, can escape - and if there's nothing coming out of them, we can't detect

What we can
detect is the space around them, along with matter as it falls into the black
hole's gravitational tug, forming a swirling accretion disc that glows with the
intense heat of friction. However, at a certain distance from the black hole,
there is no escape, and everything falls in. Even light. This point of no
return, where the escape velocity is higher than light speed, is called the
event horizon, and this is what the Event Horizon Telescope is trying to

Some black
holes are absolutely immense, like Sagittarius A*, which is millions of times
the mass of the Sun. These are way bigger than any stars that we know of, and
astronomers are not quite sure how they form. But a bigger object means it's
easier to see - and that's why the EHT is looking at the closest one we know.

The 2013
observations of Sagittarius A* narrowed down the resolution to just three
Schwarzschild radii - one of which equals the radius of the event horizon, or
the hypothetical size of the black hole - revealing details as small as 36
million km (kilometers).

This may
seem huge - after all, Earth is 150 million kilometers from the Sun - but it's
smaller than the expected size of the accretion disc, and has allowed
astronomers to start figuring out the event horizon's structure by working out
models and applying them to the data.

started to figure out what the horizon- scale structure may look like, rather
than just draw generic conclusions from the visibilities that we sampled
explained astronomer Ru-Sen Lu of the Max Planck Institute for Radio Astronomy (MPIRA).

"It is
very encouraging to see that the fitting of a ring-like structure agrees very
well with the data, though we cannot exclude other models, e.g., a composition
of bright spots

So it's
looking like the structure of the space around the event horizon of Sagittarius
A* could be shaped like a giant doughnut around the black hole. Which could
explain why it gets so hungry. Of course, the data isn't detailed enough yet to
draw any firm conclusions. Future observations by the EHT will get more data in
order to build up a more comprehensive picture. But, so far, this is pretty
exciting stuff.

results are an important step to ongoing development of the Event Horizon
," said Sheperd Doeleman from the Harvard-Smithsonian Center for
Astrophysics and director of the EHT.

analysis of new observations, which since 2017 also include ALMA, will bring us
another step closer to imaging the black hole in the centre of our

The research
has been published in The Astrophysical Journal.