Of all the physical sciences, one of the most
popular is astronomy.
I mean, who hasn’t looked up at the night
sky, wondering about the twinkling stars and
the occasional meteor that flashes across
the upper atmosphere?
Since mankind invented the telescope, our
wonder has only increased.
With the Hubble telescope, we can look deep
into the cosmos, seeing the birth of the very
first galaxies in the universe.
Looking at objects a little nearer, we see
lovely spiral galaxies, majestic pinwheels,
slowly twirling over the eons.
It is by looking at spiral galaxies that this
video’s big mystery was first discovered.
In the 1920s, astronomers first realized that
the smudges that had long been seen on their
photographic plates were actually collections
of stars held together by gravity that we
now call galaxies.
Immediately, they began to apply Newton’s
law of gravity and inertia to predict the
rate at which the galaxies rotated.
The idea is simple.
Just like planets orbit the sun, stars orbit
the galaxy.
These orbits are basically circular and in
order for a star to move in a circular path,
it needs to feel a force.
The force that causes this orbital motion
is gravity.
By measuring how the mass of the galaxy is
distributed, you can calculate how much the
galaxy tugs at each particular star.
The equation we see here highlights the most
important points.
The force needed for circular motion is the
force of gravity.
The equal sign just says that they have equal
value.
The force it takes for an object to move in
a circular path depends on the object’s
velocity, just like an object tied to a string
and spun in a circle pulls more strongly on
the string the faster it goes.
The force felt on the star due to gravity
depends on the mass of the galaxy.
More mass means a stronger force.
Finally, both forces depend on the distance
from the center of the galaxy to the center
of the star.
These effects are well known and anyone who
has taken an introductory physics class will
have seen them.
Since we see that one side of the equation
involves the velocity of the star, and the
other involves the mass of the galaxy, with
a little effort, it’s pretty easy to calculate
what the known laws of physics predict for
the velocity of a star for different distances
from the center of the galaxy.
This relationship is shown here.
Stars near the center of the galaxy orbit
slowly, and the speed at which they orbit
increases as the star’s distance from the
galactic center increases.
Once you get far from the center of the galaxy,
the star’s velocity is predicted to again
be slower.
This is an easy calculation for astronomers
to do and there is no controversy about this
prediction.
So what is observed?
Do the stars move as expected or do they have
a surprise for us?
Well, stars near the center of the galaxy
move with exactly the predicted velocity,
with stars near the center of the galaxy moving
slowly and those further away moving more
quickly.
So far, so good.
However, stars very far from the center of
the galaxy do not move slower and slower as
predicted from the theory.
Instead, the measured orbital velocity of
stars is nearly independent of the radius
of the orbit.
This result is shocking.
When you see a discrepancy of this magnitude,
something is very, very wrong.
No small tweak of your equations will explain
the differences between calculation and observation.
And since the calculation is so simple, it
forces scientists to return to the very basics.
So let’s just take another look at the equation
we just saw.
The equation says that the force required
to make a star move in a circle is equal to
the force of gravity.
Thus we are required to conclude that either
we don’t understand the equations that govern
circular motion or we don’t understand gravity
or these two forces aren’t equal.
There is no other possibility.
Rather than using this equation, I’d like
to use this image of a tree which says the
same thing, but in a way that's easier to
understand.
The roots of the tree are the various observations
that show us we don’t understand the motions
of the heavens.
There are many such observations, the rotation
of galaxies is just one.
The branch in the trunk shows the two big
possibilities, that we don’t understand
motion or gravity.
Each subsequent branching is a different hypothesis.
Over the last 90 years or so, all possible
explanations have been tested.
We don’t have time in a short video to explain
all of the tests but, in 2013, one final hypothesis
seems to explain all of the data.
This hypothesis is that surrounding most galaxies
is a huge amount of matter that is invisible.
We call this matter “dark matter.”
So what does “invisible” mean?
Well it obviously means that we can’t see
it with our eyes, but it also means that this
matter doesn’t emit heat, radio waves or
any other form of electromagnetic radiation.
Perhaps even weirder, our best guess is that
there is five times as much of this dark matter
as there is the ordinary matter that makes
up you and me.
Five times!
Do we have any evidence for dark matter beyond
our astronomical observations?
Well… no.
The hypothesis of dark matter does a pretty
good job of explaining these cosmic anomalies,
but it would be good to detect this dark matter
in a more direct way.
Because the identity of dark matter is one
of the big mysteries of modern physics, there
are many experiments trying to find it.
Experiments located a kilometer or more underground
in abandoned mines search for dark matter
that should be passing through the Earth.
Experiments on satellites probe the heavens
looking for the signature of dark matter particles
occasionally interacting with each other.
And scientists at particle accelerators are
trying to actually create dark matter in the
laboratory.
Several of the experiments have seen hints
that suggest that they’ve seen dark matter,
but others haven’t.
Until several experiments begin to tell a
common story, nobody should believe the dark
matter hypothesis has been proven.
Still, the evidence is very strong and a big
push is on to solve this mystery once and
for all.
