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What Is a Black Hole? A Fundamental Explanation

Jagatheesh is a Mechanical Engineer and interested in writing on science and technology in our life.

Black Holes are astronomical objects with intense gravity, even light can't escape.

Black Holes are astronomical objects with intense gravity, even light can't escape.

Black holes are astronomical objects in the universe that have extremely strong gravity. The gravitational pull of a black hole is so strong that even light cannot escape. Since English astronomical pioneer John Michell shared his theory about these dark stars, the scientific community's interest has grown. The existence of black holes has been confirmed by the theory of relativity and other ideas.

Space scientists recently viewed and released an image of a black hole using advanced telescopes. So, exactly what is a black hole? How does it come to be? This article will delve into the science of black holes.

What Is a Blackhole?

A black hole is an astronomical space object with extremely high gravity. When light enters a black hole, it cannot escape because the gravity is so strong. The temperature of a black hole is so high that direct observation is impossible.

Black holes are classified into three types based on their mass and size. There are three types of black holes, according to Nasa. They are:

  1. Primordial: They are the size of an atom but have the mass of a mountain. They form in the early days following the big bang event.
  2. Stellar: These are the most common medium-sized black holes. A stellar black hole will have a mass 20 times that of the sun. There are dozens of stellar black holes in our Milky Way galaxy.
  3. Supermassive: These are massive black holes with masses greater than a million suns added together. According to scientific evidence, each galaxy contains a supermassive black hole at its center. Sagittarius A is the supermassive black hole at the heart of our galaxy.

“In space, no one can hear you scream; and in a black hole, no one can see you disappear.”

— Stephen Hawking, Black Holes: The Reith Lectures

How Do Black Holes Form?

Black holes are formed by gravitational collapse, but in theory, a few other formational models exist.

Gravitational Collapse

When an object's internal pressure is insufficient to support its own gravity, it collapses. When the center of a large star collapses, the star explodes and ejects a portion of itself into space. This phenomenon is also referred to as a "supernova."

It occurs when a star's internal energy is insufficient to keep its temperature stable. As a result, a lack of temperature causes stars to collapse. If the collapsing star's mass exceeds the Tolman–Oppenheimer–Volkoff (TOV) limit, the crushing will continue until zero volume is reached, at which point a black hole will form in space.

Big Bang

Scientists thought the big bang created primordial black holes. Densities were higher in the early universe, shortly after the big bang. This could have resulted in the formation of black holes. Higher densities can currently be found only in stars. Because high density alone cannot produce black holes, the initial density perturbation after the big bang aids in forming black holes.

High Energy Collisions

A high-speed particle collision will concentrate enough mass and kinetic energy in one location to form a black hole. Theoretical high-energy collisions exist. Several particle accelerator experiments have been conducted to create black holes.

Some scientists believe that when cosmic rays enter the Earth's atmosphere, they will collide with it and create tiny black holes. CERN's Large Hadron Collider may produce small black holes. However, many experts believe these black holes will vanish soon after they form. As a result, this concept is still theoretical.

Colliding Black Holes Video

Who Discovered the First Black Hole?

John Michell, an English astronomical pioneer and clergyman, published a letter in 1784 in which he proposed dark stars, a large body from which even light cannot escape. Later, Einstein's theory of relativity demonstrated the effect of gravity on light motion. Numerous scientists contributed to the discovery of black holes after Einstein.

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Cygnus X-1, a galactic x-ray source discovered in 1964, is widely regarded as the first black hole. The Milky Way galaxy, where our planet is located, contains a supermassive black hole in its center. Two astronomers, Bruce Balick and Robert Brown, discovered Sagarritus A, a supermassive black hole in the center of our galaxy. Reinhard Genzel and Andrea Ghez received the Nobel Prize in 2020 for confirming that Sagarittus A is a black hole.

To describe black holes, John Michell coined the phrase "dark star." Physicists later used the term "gravitationally collapsed objects." Robert H. Dicke compared it to a prison in Calcutta, India, where people entered and never left alive. In December 1967, a student suggested the term "black hole" to John Wheeler during a lecture, which he popularised.

Components of a Black Hole

Various components of a black hole are as follows:

Event Horizon

A black hole's event horizon is its boundary. Anything that enters this region is trapped. Objects will be drawn into the black hole. The event horizon prevents even light from escaping. Whatever happens inside an event horizon cannot be seen by an observer outside of it, as the name implies. As a result, the inside of a black hole remains a mystery to observers from outside the black hole.


The center of the black hole is gravitational singularity or singularity. It is a place where gravity is so strong that spacetime itself breaks down. The singular region has infinite density and zero volume. The laws of physics are violated here. The Schwarzschild radius is the distance between the singularity and the event horizon's outer surface.

Photon Sphere

Photons are forced to travel in orbits around a black hole in this region. Photons revolve around the black hole due to the gravitational force of the black hole. They maintain an unstable orbit because even minor disturbances cause photons to escape from their orbit.


An ergosphere is a region outside the event horizon where objects cannot remain stationary. The ergosphere is commonly discovered in rotating black holes. Any object near the ergosphere will begin to rotate in the same direction as the black hole. If an object must come to a halt, it must move faster than the speed of light in the opposite direction. An ergosphere allows objects and radiation to escape.

Accretion Disk

An accretion disk is a hot, thin rotating disc formed by matter spiraling slowly toward a black hole. The accretion disc is visible as long as the black hole has a continuous source of matter.

Common Questions About Black Holes

Humans have always been fascinated by black holes. The following are some of the most frequently asked questions about these astronomical space objects.

Can We Survive in a Black Hole?

Nothing can escape a black hole, according to the scientific community. Even light is drawn in by gravity. Furthermore, the intense gravity compresses the human body through a process known as "spaghettification." Human bodies will be compressed like a noodle due to vertical stretching and horizontal compression.

Does a Black Hole Destroy the Earth?

The nearest black hole to Earth is located 26000 light years away. As a result, there is no threat of a black hole destroying the Earth and our solar system. Even if a black hole replaces the sun, the Earth will continue to revolve around it rather than fall into it.

Does Time Stop in a Black Hole?

Near a black hole, time slows down. Any massive body, according to Einstein's theory, is capable of doing this. As a result, the flow of time near a black hole is slower than the flow of time further away.

Do Black Holes Swallow Planets?

Anything that falls into a black hole cannot escape it. Massive black holes have already devoured many stars in the galaxy. After attracting objects, black holes expand in size. However, the galaxy is large enough to accommodate all massive objects.

Do Black Holes Die?

Black holes, according to Stephen Hawking, lose energy through thermal radiation. This is referred to as "Hawking radiation." On the other hand, a black hole takes a very long time to die.

What Is the Closest Black Hole to Earth?

Sagittarius A* is a supermassive black hole at the heart of our galaxy. The Sagittarius A* supermassive black hole is the closest to our planet. It is located at a distance of 25000 light-years from Earth. A0620-00 is a tiny black hole 3600 light years away from Earth.

How Can We See a Black Hole?

The intense gravity of a black hole pulls light into it. Even with powerful telescopes that detect electromagnetic radiation, it is impossible to see a black hole. A black hole, however, significantly impacts the stars and the gases surrounding it. When a star approaches a black hole, it emits a bright light. Scientists will use powerful telescopes to observe such light to identify a black hole.

Using the Event Horizon Telescope, scientists obtained an image of a black hole in 2019.

Using the Event Horizon Telescope, scientists obtained an image of a black hole in 2019.

Black Holes Will Help Us Understand the Universe

The Event Horizon Telescope is a global network of telescopes dedicated to studying black holes. Scientists captured an image of a black hole in the center of galaxy M87 in 2019. Scientists released the first image of Sagittarius A* in May 2022.

Understanding the evolution of galaxies and the universe's origin will be aided by research into black holes. Black holes also shed light on the effects of gravity. These suggestions will assist us in improving our space activities and gaining a better understanding of physics.


This content is accurate and true to the best of the author’s knowledge and is not meant to substitute for formal and individualized advice from a qualified professional.

© 2022 Jagatheesh Aruchami

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