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Jon-Richfield says:

The way you it put that makes it sound as though you are confusing two things. For a start, gravity does not push away the outer layers.

Try to imagine this analogy: You have a pot on the stove with a closely fitting lid, and it contains boiling water with steam forcing its way out between the lid and the pot. Let us assume that it is boiling at a temperature of 100°C. This does not suit you, so you press down on the lid to prevent the steam from escaping by forcing its way out.

However, by pressing down, although you keep the steam inside, you cause the temperature to rise and you press the bottom of the pot into closer connection with the stovetop, thereby inproving the heat conduction into the bottom of the pot and increasing the rate of heat flow. Pretty soon the steam is forcing its way out and escaping faster than ever, and this process continues until the pot boils dry.

Notice that the pressure that you apply does not remove steam any faster. You could demonstrate this at any time by suddenly letting go and removing the pressure that you had applied. Instead of the escape of the steam slowing down when you remove the pressure, at that point the steam really starts to escape at a great rate, possibly even explosively, and it continues to do so until things settle down again.

Now, without going into too much detail, think of the star. The heavier the pressure with which gravity presses the outer layers of gas against the core of the star, the hotter the core becomes, and the faster the nuclear reactions run inside the core, producing yet more heat, and faster than before. The hotter the particles in the core, the more vigorously they in turn apply pressure against the outer layers.  Depending on the kind of sun, and how large it is, their outward pressure  actually may force it to expand into a giant of one kind or another. For example we expect our Sun to become a red giant in perhaps another billion years or so.

However, this can go on only for so long. Sooner or later the star must run out of nuclear fuel and then the "nuclear burning" simply must stop. After that the star begins to cool, and because it cools it must shrink. If it is big enough and its outer layers shrink fast enough and symmetrically enough, they fall onto the central core with an almighty bang, and partly from their own momentum and partly from the nuclear reactions resulting from that crunch, they rebound into space. That is what we call a supernova.

Notice that gravity did not throw anything out into space. In fact, rather like when you press down on the lid of your pot of boiling water, gravity actually resisted any tendency for anything to move away from the core of the star. What actually threw all the stuff out was the combination of the bounce and the sudden flood of heat and particles (particularly neutrinos, amazingly enough!) that were released by that final gravitational and inertial squeeze.  

I hope that helps. If not, then please ask again.    

sssss
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Tags: gravity, stars.

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posted on 2010-10-22 13:13:05 | Report abuse


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