Black Holes
Today, we will talk about one of the most mysterious bodies of our Universe – The Black Hole. Yes, The Black Hole! The place where a singularity
comes into the picture, laws of physics break, time stops, the space-time warps and
what not!
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Black Hole - Just look at this magnificence! |
But such is the binding by the word limit and the need to keep it short and simple, we cannot discuss as much as we would wish to. Thus, we would talk very briefly about black holes in this article, mainly their formation and some of their properties. Topics related to it, such as its parts, nature of particles around it, the fate of us if we fall into one, its death, etc. would come following. So, let’s start!
To understand a black hole, to define it, we have to
look at its origin.
As we know, stars keep on burning and releasing enormous amounts
of energy due to nuclear fusion which takes place in its core. Hydrogen fuses
to form helium giving a huge amount of energy. The energy in the form of radiation
pushes against gravity. Thus, preventing the massive crust from collapsing into
the core. This maintains a delicate balance between the two forces.
But what happens when
all the fuel is consumed?
For a star that has about one half the mass of the sun is
too small and too cool to fuse helium to carbon. Thus, it ends up becoming a
white dwarf made of helium. Stars between one half to four times the mass of the sun are massive and hot enough to fuse carbon to oxygen. Carbon and oxygen fuse
more or less at the same time and a white dwarf made of carbon and oxygen is
obtained. Due to a large amount of heat and pressure, we may have a white dwarf
made of diamonds! Stars with masses greater than four times the mass of the sun
are massive and hot enough to fuse oxygen to silicon. Stars that have earned
the title of “supergiant” are so
massive and hot that they begin fusing silicon into a solid core of iron.
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White Dwarf |
Fusing silicon to iron takes more energy than it gives off.
Thus, the balance between radiation energy and gravity is broken. The star
begins to shrink under its own gravity. If the iron core builds up to 1.4 times the mass of the sun,
it cannot survive the pressure and collapse. In some cases, matter slams into
the core resulting in shock waves that trace back and blow the star apart,
ending it in a supernova. A supernova releases incredible amounts of energy and is responsible for the formation of
heavier elements in our Universe.
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Supernova |
When a large star implodes, its weight is enough to squash atoms in its core, down to its nuclei. This results in an ultra-dense neutron star. We can imagine the density of neutron stars to be that of a mountain being crushed into the size of a marble! Neutron stars due to their ultra-density can withstand enormous amounts of pressure. But if enough matter falls upon it, above a critical threshold, they will collapse into absolute nothingness! And when that happens, a black hole is born. Mass is packed into a single point known as a singularity. (Singularity is a point with infinite density and our general understanding of physics fail here.)
A decent-sized black hole is called a stellar-mass black
hole with a diameter of an asteroid. There are also super-massive black holes
with mass millions to billions of times the mass of the sun. We have one at the
centre of every galaxy, including our Milky Way! It offers a great insight into the formation of these galaxies as they must have been interdependent.
An artist's depiction of the black hole at the centre of the Milky Way Galaxy |
A common idea about a black hole is that it is made up of matter very compact. But this is wrong! The matter gets completely destroyed. It no longer exists. Yet it leaves behind one of its most powerful legacies – The Gravity!
According to Albert Einstein, gravity is not the force that
attracts two objects but it is the warping of space-time around a massive
object. A black hole is a deep puncture in space-time. The energy of matter is converted
into energy of warped space-time.
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Gravity as described by General Theory of Relativity |
One more misconception that is widely held is about the size of a black hole. A black hole has no actual size. It is a singularity. The black boundary that you often see in the pictures, represents the part of the black hole, where the gravitational pull is so strong even light cannot escape (And as light is necessary for an object to be visible the region appears black). The boundary of the black part is called the event horizon. But, the radius of the event horizon does depend upon the mass of the black hole. To give it a name, this radius is the Schwarzschild radius. It can be calculated for any mass as
Radius = 2GM/c2
Where G is the Gravitational constant.
M the mass
And, c
is the speed of light.
Thus, r = 1.48*10-30 M meter.
Or, we can say that if we crush a body into its
Schwarzschild radius, we will obtain a black hole!
Well, that was all for the day. I hope you liked the article. Don't forget to calculate your Schwarzschild radius!
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