13 June 2012

Introducing Black Holes



The question “Is travelling to distant galaxies possible?” has fascinated many teenage minds. I confess I was one of them when I first read about fictional, intergalactic travel. I was mesmerised by the sheer magnitudes Space Science encompasses; the farthest of stars, the most violent of events, the brightest of explosions and the densest of objects. I have been fascinated by Black Holes ever since I saw a documentary in 6th grade. What followed was a sudden and determinedly incessant reading up session comprising several encyclopaediae. It is for this reason that I’ve decided to write about the most mysterious objects in the universe. Here’s hoping that you find them as fascinating as I did and still do. Happy reading!

Introduction:

The subject of what constitutes light has long been a topic of debate among scientists. This relentless tug-of-war spawned two groups of scientists- one group supported the Particle Theory of Light and theorised that light is composed of particles just like any other matter. The other supported the Wave Theory of Light, and stated that light comprises waves, and not particulate matter.
With the advent of quantum mechanics, we now know that really both theories are correct.
Under the theory that light is made up of waves, it was not clear how it would respond to gravity. But if one accepts that light is composed of particles, then one might expect these particles to be affected by gravity in the same way as any matter is affected. That said, it is possible to extrapolate this idea to a star that is sufficiently massive to have a gravitational field so strong that even light can’t escape from it.
The light from such a star would be pulled back inside before it got very far. This obviously means that we will not be able to see the star. This is exactly what a black hole is; a black void in space that is invisible and which can only be “felt” by means of gravitational attraction. The term black hole was coined by John Wheeler, an American scientist, in the year 1969.
                                                                                        


Death of a Star

We know that there are three possible results when a stellar death occurs. One, the star shrinks into a white dwarf. Two, the star shrinks into a neutron star and three, it collapses under its own gravity and explodes into a supernova thereby forming a black hole. This is governed by the Chandrasekhar limit (which is a mass equal to 1.4 times the mass of the Sun) of the star. A star having mass more than this limit explodes into a supernova. A supernova is a cataclysmic explosion in space whose brightness outshines even supergiants (a category of stars) sometimes. The magnitude of this explosion can’t be imagined by the human mind. The energy released in a supernova explosion far exceeds the energy that will be emitted by our sun in its entire lifetime.

White dwarves and neutron stars are incredibly dense objects found in space. A cubic centimetre of matter from a neutron star would have a mass equivalent to several football stadiums.

However, it’s the third category of stellar death that is of paramount importance to us. The Chandrasekhar limit determines whether a star would eventually collapse into a black hole. This limit is merely a mass which was calculated by Dr. Chandrasekhar to be 1.4 times the mass of our sun. (So no, our sun will not form a black hole when its fuel runs out.)

Thus, a black hole is a region of space with a gravity field so strong that nothing, including light, can escape from it, i.e. it has an escape velocity greater than the speed of light.

 A black hole is thought to be a result of the gravitational collapse of a massive star at the end of its life. Black holes may also be created in the
centres of young galaxies.

 Imagine a star in space as a ball on a rubber sheet. A massive object like a star will “bend” space and anything close to it will fall in towards it. If the ball were so heavy that the sheet stretched into a long, deep tube, the result would be a black hole.

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