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Briefly about what is dark matter and dark energy?
Andy Green
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1 year ago
Briefly about what is dark matter and dark energy?
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Learning
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00:00
Dark matter and dark energy are two mysterious substances that make up most of our universe,
00:06
but their nature remains largely unknown.
00:09
Although we can't see them directly, scientists are confident they exist because of the way
00:13
they influence stars, galaxies, and the universe as a whole.
00:18
What is dark matter?
00:20
Invisible but powerful, dark matter is a mysterious type of matter that doesn't emit, absorb,
00:26
or reflect light.
00:28
This makes it invisible to our telescopes.
00:30
However, we know it exists because it affects visible objects with its gravity.
00:36
Think of it like wind.
00:37
You can't see the wind, but you can feel it and see how it moves leaves.
00:42
How was dark matter discovered?
00:44
The idea of dark matter was first proposed in the 1930s when astronomers noticed that
00:49
galaxies were rotating much faster than they should be if they were made only of visible
00:53
matter, like stars and planets.
00:56
If only visible matter existed, the galaxies would fly apart due to the centrifugal force
01:02
of their rotation.
01:03
But something invisible and very massive was holding them together.
01:07
That something was called dark matter.
01:10
Example, gravitational lensing.
01:13
One of the proofs of dark matter comes from observing a phenomenon called gravitational
01:17
lensing.
01:19
Light from distant galaxies bends as it passes through areas with a lot of invisible matter,
01:24
dark matter.
01:25
This bending of light is similar to how glasses lenses change the direction of light.
01:30
Through these effects, scientists can estimate how much dark matter is in a particular region
01:34
of space.
01:36
How much dark matter is there?
01:38
Scientists estimate that dark matter makes up about 27% of all the mass and energy in
01:43
the universe.
01:44
That's five times more than all the visible matter, stars, planets, and other objects,
01:50
which makes up only 5% of the universe.
01:53
What is dark energy?
01:55
A force stretching the universe.
01:57
Dark energy is even more mysterious than dark matter.
02:01
It was discovered in the late 1990s when scientists found out that the universe isn't just expanding
02:06
as predicted since the Big Bang, but it's expanding faster and faster.
02:11
This was surprising because it was previously thought that gravity would slow down the expansion,
02:16
not speed it up.
02:18
Dark energy is a hypothetical force that acts like anti-gravity, making space itself
02:24
expand faster.
02:25
We don't know exactly what dark energy is, but essentially, it works against gravity,
02:31
pushing galaxies away from each other.
02:33
Example, a balloon.
02:35
Imagine our universe is like a balloon with galaxies drawn on it.
02:39
If you blow up the balloon, the galaxies move apart as the balloon expands.
02:44
Dark energy is like the force causing the balloon to expand faster and faster.
02:49
How much dark energy is there?
02:52
Dark energy makes up a whopping 68% of the universe's total energy.
02:57
This means that the vast majority of the cosmos is this mysterious energy that we can't see
03:02
or measure directly.
03:04
Why is it important?
03:05
Dark matter and dark energy are crucial to understanding how our universe is structured
03:10
and how it will evolve in the future.
03:12
For example, the future of the universe.
03:15
If dark energy continues to accelerate the universe's expansion, one day galaxies could
03:20
drift so far apart that our corner of space would become completely empty.
03:25
This is called the Big Rip.
03:27
The shape and structure of the universe.
03:30
Dark matter explains why galaxies have the structure we observe today.
03:34
Without dark matter, they would have disintegrated or looked entirely different.
03:39
Existing facts and evidence.
03:42
Galaxies and star clusters.
03:43
We can observe groups of galaxies and stars behaving as though they contain much more
03:48
matter than we can see.
03:49
This means there must be something invisible inside the galaxies.
03:53
This is dark matter.
03:55
Cosmic microwave background.
03:57
This faint radiation left over from the Big Bang can be measured by scientists.
04:01
Its variations confirm the existence of dark matter, which helped shape the formation of
04:06
the first stars and galaxies.
04:08
Dark matter and dark energy are mysterious but extremely important parts of the universe,
04:14
about which we still know very little.
04:16
They play a huge role in how the universe works and are among the most exciting and
04:20
challenging questions in modern science.
04:23
Scientists continue to work on unraveling their mysteries, and perhaps in the future
04:28
we'll learn more about what makes up this vast part of the cosmos.
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