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How much energy is in a magnet? – Standard Free Energy Change Meaning

The magnetic field from a magnet causes electrons to move up and down like this:

So the more energy a magnet has, the more electrons the magnet attracts.

We now know that when we are standing right next to a big black hole, the magnetic field looks like this:

And when we are at the edge of this big black hole, the magnetic field is like this:

Here’s a little math to give you an idea of what happens:

Let’s say you put a piece of tape between your ear and your skin, and then you apply a strong magnet to it. With the tape firmly in place, the skin won’t move. The skin moves because the tape is pulling the skin away from the magnet. What you see in the image above is the result.

But the magnet is actually pulling at the skin, drawing it in. And in its pull, it pulls on electrons, and all those electrons are moving along the tape, creating a magnetic field.

If you look at the black hole, you see what happens: the black hole pulls everything it can towards it (not just energy) and you see a bunch of stuff flying about: particles, and ions.

That magnet is making the black hole behave slightly like a star. The star can actually shine brightly and shine down on its small host of electrons.

So for the star to stay cool, it needs a lot of energy. We know that by how bright and long it shines down (because we measure the amount of light it reveals.)

But with so much energy, what happens if we just sit there and wait?

As it turns out, the answer is not much, just like the answer to the above equation. Just because the black hole is big doesn’t mean it doesn’t have much gravity or anything like that.

I mentioned that our bodies have two types of gravitational fields. One is gravity in space, and the other is gravity in time. It’s true that in space, there is no gravitational field. But there is a gravitational field in time, and that time field is what lets the stars shine in the first place.

If you take a big star and drop it in orbit around the sun, the star will slowly move around in an orbit around the sun, and the rest of the stars will follow along for the journey.
IB Chemistry on Gibbs Free Energy and Entropy

But in the future, when the star leaves the solar system, it will still be in the same place

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