And so it's going to depend on Coulomb's Law, how big that ionization energy is going to be.

所这取决于库仑定律，即电离能有多大。

And then ionization energy remember is the amount of energy required to remove an electron.

然后电离能记住是去除一个电子所需的能量。

Now in chemistry it's important because we can use Coulomb's Law to predict ionization energy.

现化学中它很重要，因为我们可库仑定律来预测电离能。

One theory is that this is caused by a quasar ionization echo.

一种理论认为这是由类星体电离回波起的。

Today, point-of-use processes usually involve ionization to lower mineral content.

如今，点处理工艺通常包括离子化降低矿物质含量。

In this tube, we have an ionization chamber.

这个管子里，我们有一个电离室。

This energy is called " ionization energy."

这种能量称为“电离能” 。

Yeah, so ionization is the process of removing electrons from something.

是的，电离就是从某个物体中移除电子的过程。

It's getting really super hot, and they call it ionization.

它变得非常热，人们称之为电离。

That ionization made the gas glow in colors our eyes can see.

电离气体发出人眼可见的颜色光芒。

But on Apollo 13, this ionization goes on longer than normal.

但阿波罗13号任务中，这种电离过程持续的时间比正常情况下要长。

In other words why would the ionization increase and then drop down again?

换句话说, 为什么电离会增加然后再次下降?

Ionization energy is the amount of energy required to create an ion.

电离能是产生一个离子所需的能量。

Second, in our explanation we simplified the circuitry of the smoke detector's ionization chamber.

其次，我们的解释中，我们简化了烟雾探测器电离室的电路。

And as these protons and electrons hit our atmosphere they are giving off ionization of colors.

当这些质子和电子撞击我们的大气层时，它们会发出离子化的色彩。

1920. Indian physicist Meghnad Saha demonstrates how temperature, pressure and ionization are linked in a star.

1920年，印度物理学家梅格纳德·萨哈展示了恒星中温度、压力与电离作之间的关联。

Ionization energy should be like this.

离子化能量应该是这样的。

Just like with the ionization energy there's a discrete energy jump involved with the adding of an electron.

就像电离能一样， 有一个离散的能量跃迁涉及到一个电子的添加。

Now, when we talked about ionization energy, I think, we talked about when oxygen and water bond, right?

现，当我们谈到电离能时，我认为我们提到过氧和水结合的情况，对吧？

And so ionization is the energy required to remove an electron.

所电离是移除一个电子所需的能量。