For centuries, scientists imagined objects
so heavy and dense that their gravity might
be strong enough to pull anything in - including
light. They would be, quite literally, a black
hole in space. But it’s only in the past
few decades that astronomers have conclusively
proved their existence.
Today, Hubble lets scientists measure the
effects of black holes, make images of their
surroundings and glean fascinating insights
into the evolution of our cosmos.
Hi everyone, and welcome to the Hubblecast.
In science fiction, black holes are often
portrayed as some kind of menacing threat
to the safety of the whole Universe, like
giant vacuum cleaners that suck up all of
existence.
Now, in this episode, we’re going to separate
the fiction from the facts and we’re going
to look at the real science behind black holes
and how Hubble has contributed to it.
Black holes come in different sizes. We’ve
had solid evidence for the smaller ones since
the 1970s. These form when a huge star explodes
at the end of its life.
As the outer layers are blown away, the star’s
core collapses in on itself forming an incredibly
dense ball. For instance, a black hole with
the same mass as the Sun would have a radius
of only a few kilometres.
These black holes won’t suck you in unless
you get very close to them though. In fact,
contrary to popular belief, a black hole the
size of the Sun doesn’t actually exert any
more gravitational pull than the Sun does.
But these stellar black holes are just part
of the story.
Before Hubble was launched, astronomers had
noticed that the centres of many galaxies
were somehow much denser and brighter than
they were expected to be. And so they speculated
that there must be some kind of huge, massive
objects lurking in the centres of these galaxies
in order to provide the additional gravitational
attraction.
Now, could these objects be supermassive black
holes, that is, black holes which are millions
or even billions of times more massive than
the stellar ones? Or was there perhaps a simpler,
less exotic explanation, like giant star clusters?
Frustratingly, at that time, telescopes just
weren’t quite powerful enough to see enough
detail to solve the mystery.
Fortunately, Hubble was on its way, along
with a range of other high-tech telescopes.
When the space telescope was being planned,
the search for supermassive black holes was
in fact one of its main objectives.
Some of Hubble’s early observations in the
1990s were dedicated to these dense, bright
galactic centres. Where ground-based telescopes
were just seeing a sea of stars, Hubble was
able to resolve the details. In fact, around
the very centres of these galaxies, Hubble
discovered rotating discs of gas and dust.
When Hubble observed the disc at the centre
of a nearby galaxy, Messier 87, the astronomers
saw that its colour was not quite the same
on both sides. One side was shifted towards
blue and the other towards red, and this told
the scientists that it must have been rotating
very quickly.
This is because the wavelength of light is
changed by the motion of an object emitting
it. Think about how the pitch of an ambulance
siren drops as it drives past you, because
the sound waves are more spaced out as the
vehicle moves away.
Similarly, if an object is moving towards
you, the light’s wavelength is squashed,
making it bluer; if it’s moving away, it’s
stretched, making it redder. This is also
known as the Doppler effect.
So, by measuring how much the colours had
shifted on either side of the disk, astronomers
were able to determine its speed of rotation.
And it turned out that this disk was spinning
at a rate of hundreds of kilometres per second.
This in turn allowed astronomers to deduce
that, hidden at the very centre, there must
be some kind of object which was two to three
billion times the mass of our Sun – and
this was very likely a supermassive black
hole.
Now, along with a lot of other observations,
this was a key piece of evidence that led
to the notion that there is a supermassive
black hole lurking at the centre of most,
if not all, giant galaxies, including our
own Milky Way.
So far, so good. But this work was almost
20 years ago — what does it tell us about
cutting-edge science today? Well, the science
of black holes has moved along a lot since
then. The mystery now isn’t whether they
exist, but why they behave in the strange
ways they do.
For example, Hubble observations have helped
to show that the mass of a black hole is closely
related to the mass of its surrounding host
galaxy. The bigger the black hole, the bigger
the galaxy. Now the reason for this is totally
unclear.
A supermassive black hole is pretty big, and
it packs a lot of punch, but you’ve got
to remember that compared to its host galaxy
it’s actually tiny.
The region of space that is most obviously
and most immediately influenced by a supermassive
black hole is in fact about a million times
smaller than its surrounding galaxy. That’s
about the same size difference as between
this coin and a whole city.
So it’s pretty hard to think of any processes
that would link the two in a long-lasting
way.
So a big area in science just now is trying
to find out what’s going on here, and why
the two are linked. Do black holes regulate
the size of galaxies, or do galaxies regulate
the size of black holes? Or is something altogether
different happening?
Just now, astronomers don’t know, but they’re
working hard to find out. But there’s another
interesting, and probably connected black
hole mystery, that has astronomers scratching
their heads.
When matter falls into supermassive black
holes, it forms this big swirling disc that
heats up and gives off a lot of powerful radiation.
The more matter falls into the black hole,
the more powerful the radiation.
Now these active, accreting black holes are
called quasars, and they are among the most
luminous and most powerful objects in the
Universe.
The thing is, a quasar can get so greedy that
its radiation is powerful enough to actually
blow away all the gas and dust that’s feeding
it. And so it seems there’s a natural upper
limit to the rate at which a black hole can
grow.
Now, this implies that one wouldn’t expect
to see any really big and powerful quasars
in the very early Universe, because there
simply wouldn’t have been enough time to
build up the supermassive black hole that
is needed to power a quasar.
But recent discoveries have in fact shown
quasars in existence just a billion years
after the Big Bang, which is much earlier
than we had expected. And so there you have
it: another mystery for astronomers to pore
over.
So, by helping to clear up one mystery about
black holes, Hubble has opened up whole new
research areas, and these will eventually
give us a better understanding of the history
of our Universe.
This is Dr J signing off for the Hubblecast.
Once again, the Universe has surprised us
beyond our wildest imagination.
