So there's a bunch of hydrogen molecules around, and some of these iodine gas molecules around.

Surpass the kinetic so they have enough kinetic energy to get into the activation state, and then they can go to the

So right now, we have H2 plus I2 yielding 2 hydrogen iodides.

I want to draw iodide and then the hydrogen.

They both feel like they've completed their 1s shell.

So hydrogen has a covalent bond with another hydrogen.

Your brain needs iodine to make myelin the insulation for the wiring.

You can smell me. INAUDIBLE .

Here. On one side, you have mercuric oxide and graphite from your brake pads.

So essentially, we start off here, and this is the H2 plus I2.

Silver bullets. Do I look like the Lone Ranger to you?

B12 which is cobalamin.

If you have 2 moles of hydrogen, 2 moles of iodine, so it's going to form 2 moles of hydrogen iodide.

We're filling this 1s shell, but look at this.

Whoops!

Away from the, Euclideas slope to further up we go. Now, let's look what galaxy evolution does.

And it's clearly in the area of finance.

It's not like you can just take some hydrogen and put it with some iodine and it just magically turns into hydrogen iodide.

Studies have shown that 80 of Americans have a relatively low iodine.

Same thing on the iodine side where you have two iodines.

And so, there were no re ally standard candles or standard rulers.

There is one important distinction though, the early type galaxies, ellipticals and S0s tend to concentrate in clusters more than in general field and there is relatively few spiral galaxies in clusters.

There is certain stripping of gas which removes few of our star formation and so on.

You have both of them separate.

The banking sector has undergone tremendous transformation, from over 80 banks to 25 banks.

There is a good mutual agreement and the counts are above the new evolution prediction.

Because of the dense environment both proximity of many other galaxies to zip by or merge with and the dense intergalactic medium of x ray gas.

Another approach to this is by considering all of the quasar light ever emitted.

They have these electrons in between that are keeping them bonded.

Next time we will talk about phenomenon of biasing and how is clustering evolving in time.

Then further shifting focus, not on cluster appearance, but on their galaxy population, Oemler also classfied them according to the Amont of spiral versus elliptical galaxies in them.

And this energy, the difference between the energy we were at when we were just hydrogen molecules and iodine molecules, and the energy we have to get to get this activated state this distance right here this is the activation energy.

The, what's shown here is a snapshot from one such survey called COSMOS, and what's show on the left is the smoother distribution of light that's observing galaxies.

We can see the same processes at work in terms of the Commerce Bank its dependence on natural ventilation, the way that you can model those gardens, the way they spiral around.

Silver

Galaxies

What bank?

Bank?

Gold, silver...

Start differentiating into effector and memory cells.

And that's because the bluer bands are more sus, more susceptible.

I'm in banking. In banking? How'd you get into that?

And adequate iodine lowers your risk of breast cancer and prostate cancer.

Galaxy

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