Tuesday 25 October 2016

Life of a star.

The life of a star is something I already know and I would like to teach other people who want to know about the life of a star. 

A star is born from a nebula, (a cloud dust and gases including hydrogen and helium in space) That cloud eventually collapses under it's own gravitational pull. During that collapse the cloud gets hotter and hotter because of friction. Then eventually BOOM! The hydrogen and helium collide together and create nuclear fusion. That will continue to happen for millions of years. And whilst that is happening you have a star. But sadly your star will die. 

The star will run out of nuclear energy and collapse becoming hotter because of gravity. Now even through the star has run out of helium there will still be hydrogen so on the out side there will be hydrogen fusion forming a sphere around the core and the very hot inside will push that sphere out where it cools and forms a red giant.

Stars like our sun will continue ejecting their sphere until the core is exposed. Those stars are called white dwarfs. And if there is another star close by to that star it might pull hydrogen from the other star therefor turning into a new star. Sometimes, mostly massive white dwarfs (those near the 1.4 solar masses) may accumulat so much mass that they collapse and explode entirely, creating a supernova.

In the biggest stars, nuclear reactions create iron in the core. Having created this iron when it collapses it squishes that iron into an extremely small area and the outer layers of the star start to collapse along with the core, they then rebound releasing an enormous amount energy that explodes outward. Supernova release so much energy that for days, sometimes weeks that they can outshine galaxys!

If the collapsing core contains between around 1.4 and 3 solar masses, the collapse continues until electrons and protons combine to create neutrons and produce a neutron star. Neutron stars are extremely dense, like the density of an atomic nucleus. and because it contains so much mass squished into such a small area, the gravitational pull at the surface of a neutron star is immense. An like the white dwarfs, if a neutron star forms in a multiple star system it can accumulat gas by pulling it off nearby stars.

If the collapsed star is larger than three solar masses it completely collapses falling into an infinity small  area so it has a gravitational pull so strong that nothing can pull away not even light! The fasted thing in the universe!

Thank you for reading.
The End.



Nebula
Star
 Red giant
 White dwarf
                                         
Black hole


Thank you NASA for teaching me on https://science.nasa.gov/astrophysics/focus-areas/how-do-stars-form-and-evolve

Saturday 22 October 2016

Gravitational energy Theory

This is my most logical and best theory that I have ever created (yet). It is the theory of  "Gravitational energy".

As you probably know, the universe has one amount of energy never more, never less. In my theory of gravitational energy I propose that constant amount of energy that it uses to maintain it's size.

As you probably know, when something is compressed or has more matter in a smaller area it has a more powerful gravitational pull. Why?

What I propose is that when a object is compressed  or has more matter in a smaller area it no longer needs that energy that keeps it's size so that is transferred into gravitational energy. Therefore that object has more gravitational energy. Just like a star turning into a black hole.

First the star is really big and has strong gravitational pull then it turns into black hole. The black hole is indefinitely small but has impossibly strong gravitational pull.

And that is my theory of gravitational energy. I hope you like it.

The End


Star


Black hole