What is a black hole? Do they really exist? How do they form? How are they related to stars? What would happen if you fell into one? How do you see a black hole if they emit no light? What’s the difference between a black hole and a really dark star? Could a particle accelerator create a black hole? Can a black hole also be a worm hole or a time machine? In Astro 101: Black Holes, you will explore the concepts behind black holes. Using the theme of black holes, you will learn the basic ideas of astronomy, relativity, and quantum physics. After completing this course, you will be able to: • Describe the essential properties of black holes. • Explain recent black hole research using plain language and appropriate analogies. • Compare black holes in popular culture to modern physics to distinguish science fact from science fiction. • Describe the application of fundamental physical concepts including gravity, special and general relativity, and quantum mechanics to reported scientific observations. • Recognize different types of stars and distinguish which stars can potentially become black holes. • Differentiate types of black holes and classify each type as observed or theoretical. • Characterize formation theories associated with each type of black hole. • Identify different ways of detecting black holes, and appropriate technologies associated with each detection method. • Summarize the puzzles facing black hole researchers in modern science.
01.10 – What is a Black Hole?
Loading...
Do curso por University of Alberta
Astro 101: Black Holes
4 ratings
Na lição
Introduction to Black Holes
Hello and welcome to the first module of Astro 101! In this module, you will become familiar with the basic structure of a black hole, learn the terminology used to describe them, and explore the history of black hole physics.
Conheça os instrutores
Sharon MorsinkAssociate Professor
Department of Physics, University of Alberta
The basic idea behind a dark star only requires knowledge of 18th century physics.
If a star is dense enough,
its escape velocity will be the speed of light,
making it impossible for light emitted by the star to escape the stars gravity.
The idea of a dark star,
as proposed by John Michell is not correct,
but it is still important since it introduces
some ideas that apply to black holes even in modern theories.
The problem is, that the concept of a dark star uses
Newton's older theory of gravity instead of Einstein's newer theory.
That being said, Newton's theory of gravity
is a pretty good approximation to Einstein's theory of gravity,
when gravity is weak.
It was good enough for us to plan a mission to the moon, for instance.
When I mean by weak is this,
calculate the escape velocity from a planet or star,
and compare the value of its escape velocity to the speed of light.
If the escape velocity is tiny compared to the speed of light,
then we say that gravity is weak,
and Newton's theory of gravity is a good enough approximation.
For example, the escape velocity from the Earth is 11.2 kilometers per second,
but the speed of light is approximately 27,000 times larger.
Since the escape velocity from Earth is so small compared to the speed of light,
Newton's gravity is good enough for most calculations near the surface of the Earth.
But if the escape velocity is larger,
say 10 percent of the speed of light or larger,
that means that Newton's theory of gravity is no
longer sufficient to calculate the strength of gravity.
Since Albert Einstein's equations correctly describe relativistic effects at high speeds,
they improved on Newton's theory of gravity.
This means that we can predict what happens in situations with strong gravity.
Einstein's theory of gravity is called The Theory of General Relativity.
In general relativity, mass, energy,
and angular momentum are all responsible for creating curvature in space time.
The curvature of space time then causes planets,
stars, and light to travel on curved paths.
To create a dark star,
we might start with a large star and compress it
inwards to make it smaller and denser while keeping the amount of mass unchanged.
As the star shrinks in size,
the escape velocity from the surface becomes faster
and faster until it becomes equal to the speed of light.
At this point, Newton's theory of gravity just
predicts that light won't be able to escape from the star,
and it will appear dark.
However, the predictions from Einstein's theory of
gravity demonstrate a so called dark star,
would exert a much stronger force due to gravity than predicted by Newton.
This additional inwards gravitational force
makes it impossible for a start to have a stable size.
In order for stars to exist,
there is a delicate balance between its gas molecules,
which exert a net outwards pressure
that is exactly balanced by the attraction of gravity,
allowing stars to stay the same size over time.
When a star gets so small,
that it's escape velocity is the speed of light,
then the required outward gas pressure is infinite.
There is no way to create infinite gas pressure,
so the star is unstable and begins collapsing inwards.
A black hole is what remains after stars unable to resist gravity and collapses inwards.
A black hole does not have a surface but there is
a special boundary that surrounds a black hole called an event horizon.
In the case of the simplest black hole,
the event horizon is a sphere with a radius called
the Schwarzschild radius with the value,
event horizon radius equals 2 times G,
times the mass of the black hole,
divided by the speed of light squared.
The amazing thing about the formula for
the event horizon radius is that it is
exactly the same equation that Michell derive for the radius of a dark star.
The event horizon radius is a boundary for light rays.
If an astronaut shines a flashlight outside of the event horizon,
the light rays can escape and be seen by astronomers far away from the black hole
but if the flashlight is at or inside of the event horizon,
all light emitted will be trapped inside of a black hole and it's not just light,
massive objects like cakes,
or rockets, or astronauts,
can escape as long as they are outside of
the event horizon radius and their rocket is good enough
but if a cake eating astronaut crosses the boundary defined by black holes event horizon,
no escape is possible.
The name black hole didn't enter a common usage until 1967,
where it was popularized by John Wheeler.
Before then, astronomers used the name
Totally Gravitationally Collapsed Objects to describe black holes.
This is an accurate phrase,
but difficult to say.
So it's not surprising that the name black hole caught on
so quickly with scientists and science fiction writers alike.
The distinguishing difference between Michell's dark stars and black holes,
as they are described in general relativity,
is whether or not the star within the dark boundary maintains a surface.
Michell didn't consider what would happen to the surfaces of
a star when its escape velocity reaches the speed of light.
Scientists now believe that the creation of an event horizon causes all the material
hidden behind it to continue collapsing inwards with no chance of a stable surface.
There are other dark objects that astronomers make reference to,
but they aren't black holes.
For instance, there are dark nebula which consist of
clouds of cool molecules and dust that block out passing light.
These types of nebula can be observed
if they lie between us and a bright source of light,
since we will see that sunlight is blocked out by the nebula.
One famous example is the horsehead nebula.
The Horsehead is a dense,
cool cloud that blocks out the red light that has admitted behind it,
allowing us to see it.
In addition, dust emits infrared light so we can
detect dust clouds if we use an infrared telescope.
Dark Matter is a hypothesized type of matter that was
introduced to explain the motions of stars and gas and galaxies.
Dark Matter is a type of matter that doesn't emit light,
which means it can't be observed directly.
However, dark matter does have mass,
so there is a mutual gravitational attraction between dark matter,
and the stars, and gas, in the galaxy.
The gravitational attraction of the dark matter affects how the stars in the galaxy move,
allowing scientists to infer the existence of
dark matter by their observations with theoretical models.
In the 1970s, Vera Rubin,
observes spiral galaxies and measured the speeds of the stars.
She showed that the fast speeds of these stars implies the existence of dark matter.
A tiny amount of the dark matter could
be black holes but most of the Dark Matter is a type of particle called a WIMP,
which means weakly interacting massive particle.
Physicists are trying to detect WIMPs using the Large Hadron Collider in Geneva,
Switzerland, and SNOLAB in Sudbury,
Canada, as well as other laboratories.
So far, the dark matter WIMPs have not been detected.
The main thing that dark matter and black holes have in common is that they are
both detected by observing their gravitational interactions with luminous objects.
Dark energy is the name for
another mysterious force which appears to act in opposition to the force of gravity.
When astronomers measure galaxies far, far away,
they measure that the most distant galaxies appear to
move away from us more quickly than galaxies that are close.
This is one of the pieces of evidence that our universe is expanding
from a moment in history referred to as The Big Bang.
Since all these galaxies have mass,
they are gravitationally attracted to each other,
and we might expect that the rate of the universe's expansion should slow down over time.
Instead, there is evidence that the expansion is speeding up,
as if there were a repulsive force like a very large scale kind of anti-gravity.
This force called dark energy has nothing to do with black holes.
However, there are some theorist who have considered types of stars that have
some dark energy in them to help combat gravitational collapse.
Black holes may give some people melanoheliophobia,
but in most ways,
they are no more dangerous than any other star in the sky.
For example, entering into a black hole is dangerous,
once you pass through the event horizon,
you can't get out but if you enter into a star,
the hot gas would burn you up too.
I would say they are both equally dangerous.
There are safe ways to visit a star or a black hole.
Instead of traveling directly towards a black hole,
you could instead, orbit the black hole just as you can orbit around a star.
For example, the Earth orbits around the sun in a safe stable orbit.
Similarly, the Earth could orbit a black hole with
the same mass as the sun and at the same distance,
making the orbit just as safe and stable as it is now.
Unfortunately, it would be very cold around
a black hole since the sunlight that warms us would no longer be present.
There is nothing about the black hole's gravity that would suck in the Earth.
Black holes can become dangerous if they are surrounded by an orbiting disc of hot gas,
that looks similar to the rings of Saturn.
The disc of gas could emit high energy X-rays.
So if you were to approach the black hole's disc,
you could receive an unhealthy dose of radiation.
For this reason, in the movie Interstellar,
the script writers decided to make the disc of
gas orbiting their black hole be relatively cool,
so that it only emits visible light and no harmful X-rays.
The tidal force, which is a difference in the strength of gravity at different locations,
can become very strong around a black hole.
In fact, when it comes to the tidal force,
the smaller a black hole is,
the more dangerous it becomes.
An astronaut venturing too close to a small black hole
would be stretched by gravity into long thin spaghetti-like strands.
Out of all the types of black holes,
the most dangerous are thought to be the isolated black holes.
In isolation, a black hole does not have a companion star or an orbiting disc of gas,
making them extremely difficult to see due to their difficulty of detection,
it's possible that you could accidentally stumble across one,
and inadvertently cross into it's event horizon while you are exploring the universe.
Gravitational lensing by the black hole's mass
will distort the images of background stars.
So, the presence of an isolated black hole could still be deduced,
if you are careful.
Explore nosso catálogo
Registre-se gratuitamente e obtenha recomendações, atualizações e ofertas personalizadas.
O Coursera proporciona acesso universal à melhor educação do mundo fazendo parcerias com as melhores universidades e organizações para oferecer cursos on-line.
© 2018 Coursera Inc. Todos os direitos reservados.
