# Can We Compress Stars **URL:** https://davidaw.ad/posts/09-01-can-we-compress-stars **LLM version:** https://davidaw.ad/posts/09-01-can-we-compress-stars/llms.txt **Author:** David Awad **Published:** 2015-09-01 **Tags:** docs **Description:** How many times have you looked at the stars? Often I hope! Well its not unrealistic to assume you haven’t. As most people don’t. Especially... --- How many times have you looked at the stars? Often I hope! Well its not unrealistic to assume you haven’t. As most people don’t. It wasn't until after college that I myself finally started taking the time to look up. So why don’t you take one… _with_ you? We all have smartphones which make it easier to manage work related things as well as a convenient way to see lolcats on the go. Why not have a star too? Its also been shown that looking at the sun can help improve a person’s psychological health and even physical health. And sunlight, is technically starlight, since, as we all know the sun is a star. So it would indeed be beneficial to us, if we were to have a star with us at all times. It could be a MUCH more effective flashlight than an LED for starters. But the more important benefit is that it could improve people’s lives. Making people happier on the go. And with every will, there’s a way (sort-of)! So to understand how we would be able to keep a star around with us all the time we have to understand how they work. So now think of a star, what gives it it’s heat? It’s not magic. It’s hydrogen Fusion. So here’s where we get quantum, or perhaps, nuclear is a better term for it. So, an atom of hydrogen is one of the most common things in the universe as you already know; because it is only one proton and one electron. Let’s look at this diagram. Don’t get intimidated by the confusing particles and explosions.  Look on the left, we can see that there are 4 protons going into a series of reactions, and on the far right, we see that there are only 2 protons left, and a helium-4 atom. So whats happening? Well, in short, hydrogen is becoming helium and less hydrogen. So lets look. 2 protons collide. And out comes a deuteron, a positron and a neutrino. A deuteron is simply a proton attached to a neutron. In the graph we see that the deuteron hits another deuteron created by the same reactions. Once those deuterons hit other protons they become helium-3. (two protons and that bland neutron from before). If you’ve been following along in the diagram, you should be able to tell that two helium-3's become a helium-4. So now you can officially tell people you understand hydrogen fusion! Hooray. We don’t really need to focus on the other two right now but if you’re interested here’s a fun video on what a neutrino is.
Positrons, not to be confused with Decepticons, are the anti particles of electrons. If a particle were ever to make contact with it’s anti-particle the two would both turn into energy and they would create a subatomic explosion-like reaction that would give off photons in opposite directions. Which means it would be dangerous to throw your box into a highly dense field of electrons! But enough about that. Lets get back to Deuterons! This is how almost all low-mass stars produce energy. So usually, this happens on a MASSIVE scale, which takes billions of hydrogen atoms.So the sun, is in essence a huge ball of incredibly hot burning molecules; and it can get VERY hot. That’s the only way nuclear fusion can happen. When it’s incredibly hot. But how hot can it get? This is a bit off topic but here’s an interesting video on how hot it really can be.Shrink it.
Well… **how**? for that matter, how do stars get their spherical shape anyway? When you think about it there’s no reason for a star to be a… circle. Well, here’s how it works, when a star is created, it is essentially a conglomeration of very hot gas. This gas continues to get hotter and hotter. If you watched the video above you know that the more heat is applied to a particle the more energy it releases. So then if that’s the case then shouldn’t a star be constantly expanding in random directions determined by where particles happen to conglomerate? Well, yes. However were forgetting something; gravity. Look at this picture. All the material falls inward in the star and a sphere is the most stable shape at equilibrium.