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  • Hello, I'm Hank Green and I want to teach you chemistry. But please,

  • do not run away screaming. If you give me five minutes to try to convince you that

  • chemistry is not torture, but instead

  • the amazing and beautiful science of stuff. And if you give it a chance

  • it will not only blow your mind but also give you a deeper understanding of

  • your world. This is just my opinion here,

  • but I think that understanding the world leads to greater ability to enjoy the

  • world and there's nothing that helps you understand the world better than chemistry.

  • Chemistry holds the secrets to how life first formed, how cancers are cured, how

  • iPhones have bigger hard drives than 5 year old laptops

  • and how life on this planet might just be able to continue thriving,

  • even ours, if we play our cards right. Chemistry is the science of how three

  • tiny particles, the proton, the neutron and the electron

  • came together in trillions of combinations to form,

  • get this, everything. Now chemistry is a peculiar science, sometimes talked

  • about as a bridge between the ultra abstract world of particle physics and

  • the more visible sciences like biology.

  • But calling chemistry a bridge is like calling Eurasia an island.

  • Chemistry has it all, mad scientists, world changing revelations, the practical,

  • the impractical, medicine, bombs, food, beauty, destruction, life and death,

  • answers to questions you never knew you had.

  • I love chemistry, and I hope I can give you a glimpse into why.

  • So today, let's start out with maybe the biggest idea of all time, and move on

  • from there: stuff is made from atoms.

  • [Intro]

  • I know, you aren't shocked, you aren't awed, you might not even be paying attention any more,

  • but when atomic theory was first proposed, it sounded

  • pretty crazy. And yes, we call it 'Atomic Theory', using the scientific definition of theory,

  • which is "a well-tested set of ideas that explains many disparate

  • observations", not the colloquial definition of theory, which is

  • "a guess." But luckily there's no-one running around any more saying

  • "atoms are just a theory." But it wasn't that long ago that people were running around

  • saying that. You wanna know who settled it for good?

  • Einstein! Atoms had been postulated for a long time by the 20th century, but it

  • wasn't until Einstein mathematically proved the existence

  • of atoms and molecules in 1905 that the matter was truly settled.

  • And you thought Einstein was all about relativity and E=mc2, he also

  • proved atoms exist! Here's how it happened. In 1827,

  • a botanist named Robert Brown was looking at pollen grains in water

  • through a microscope and he noticed

  • that they jiggled randomly even when there was no movement to cause the jiggling.

  • It was a mystery for a long time, until 1905 when Einstein theorized that

  • this phenomenon was caused by as-yet-unproven

  • atomic particles actually smacking into the grains of pollen.

  • He wrote up some fancy math, showing that his theory predicted this motion almost perfectly,

  • and everyone had to concede that yes, tiny

  • discrete bits of matter were indeed smacking into the pollen,

  • and thus molecules, and by extension atoms, must exist.

  • Today, we remember this botanist and his discovery by calling the motion he observed

  • Brownian motion. It's kinda crazy that every physical thing you've ever

  • interacted with is made up of little

  • ball thingies. It started with people wondering what would happen if you just

  • kept slicing something in half forever.

  • Eventually, and of course it turns out that there's no knife sharp enough to do

  • this, you end up with one,

  • pure, unbreakable bit of that substance. The word "atom",

  • indeed, is from the Greek for "indivisible", though, of course, as we learned in World War II,

  • atoms can be broken as well. So all the stuff that we think of as stuff

  • is made of atoms, tiny discrete particles that have specific properties depending

  • on the arrangement

  • of three simple subatomic particles. There's the proton, heavy and positively

  • charged, the neutron, about the same size as the proton but neutral,

  • and the electron, which has the same amount of charge as the proton,

  • just opposite, and very nearly has no mass at all, about

  • 1800 times less massive than the proton or neutron. Protons and

  • neutrons hang out in the nucleus, and thus are the nuclear components or nucleons;

  • electrons hang out around the nucleus and are the parts of the atom that do all

  • the interesting chemical stuff. But before we get to the chemistry of the

  • electrons, we first

  • have got to understand the properties of the nucleus. Okay, this is pretty important,

  • so pay attention here. The number of protons in an atom

  • determines what element it is. 79 protons:

  • always gold. 59 protons: always praseodymium. The number of protons in an element

  • is its atomic number,

  • it sits right on top of the box in the periodic table because that is the

  • element's defining trait.

  • So an atom of silver with 47 protons in its nucleus is always an atom of silver.

  • Depending on what its electrons are doing and what it's bonded to, it might be

  • part of a chemical that's silver-colored or black or blue or shiny or poisonous

  • or a cure for disease,

  • but whatever it is, that atom is still silver

  • and will remain an atom of silver probably forever,

  • because that core number is very, very difficult to change. Now you might have noticed something

  • weird about silver here: its chemical symbol, the one or two-letter short code

  • that tells you what it is,

  • is Ag, not Si, which is silicon, or

  • Sv which is perfectly available, but Ag.

  • Why? To torture you? No.

  • Silver, of course, because we've known about it for a long time, was one of the first

  • elements added to the periodic table, and back then

  • it was called "argentum", Latin for "shiny gray stuff",

  • also, the root of the word "Argentina", where Spanish explorers heard rumors

  • of mountains made of silver, which of course did not exist.

  • The name "Argentina", just like the chemical symbol

  • "Ag", stuck, despite neither of them being particularly representative

  • of reality. Now, back to science.

  • Nuclei, which is the plural of nucleus, are boring. They're thousands of times smaller than

  • the atom as a whole, and they mostly just sit around being exactly the same as

  • they were when they were first created billions of years ago,

  • held together by the strongest of the four fundamental forces of physics,

  • the strong nuclear force. The fact that nuclei are so boring is the very reason they are the

  • defining characteristic of elements.

  • While electrons can jump from atom to atom whenever it's convenient, the number of protons

  • is almost always extremely stable. So that core of the atom, the nucleus, always

  • comes out of chemical reactions unscathed.

  • It's the bit that we can bump around from reaction to reaction but always

  • remains pure and behaves the same way as any other atom with that number of protons.

  • The atomic number is the soul of the atom. It's what makes

  • it it. Neutrons are important too, of course, in their own way,

  • but they don't change what element an atom is. One of the two keys to all things chemical is

  • charge, we'll discuss that in another episode, and since neutrons don't have any

  • charge, they mostly don't change the properties of an atom. But they are,

  • nonetheless, vital.

  • We all know that like charges repel each other. Neutrons serve as a kind of buffer

  • between the protons. You couldn't pack silver's 47 protons together in the

  • nucleus by themselves.

  • They couldn't handle it; they'd rip themselves apart. So nuclei only clump

  • together permanently

  • when the right number of protons and neutrons get together. Silver

  • needs about 60 neutrons to space out the 47 protons correctly.

  • But it doesn't have to be 60. In fact, silver nuclei are also very stable with 62 neutrons.

  • 61 though, that doesn't work, and the reasons for that,

  • I don't know, you would have to talk to a nuclear physicist. The atomic number of

  • silver doesn't change as the number of neutrons changes because the number of

  • protons stays the same.

  • But the relative atomic mass does change. Relative atomic mass, which used to be

  • called atomic weight back when I was in school, is basically the number of

  • protons plus the number of neutrons

  • averaged across all the silver on Earth. Because silver has two different stable

  • isotopes, each with a different number of neutrons,

  • its relative atomic mass ends up not being a whole number.

  • About 52% of silver has 60 neutrons and about 48% has 62.

  • The relative atomic mass, then, ends up being about halfway between 107 and 109, 107.8682.

  • You'll note that I said these two different sorts of silver are called

  • isotopes, they have different masses but the same chemical properties, and are

  • the same element and so belong in the same place on the periodic table.

  • In fact, the word "isotope" means "same place".

  • And different isotopes have different mass numbers. The mass number is just the

  • total number of nucleons in the nucleus,

  • which is different from atomic mass; it's simple addition

  • for a single atom, rather than an average of all the relative atomic masses of all

  • the silver atoms on Earth. So silver

  • has two stable isotopes, one with a mass number of 107,

  • which we'd call silver-107, and one with a mass number of 109,

  • silver-109. There's an easy way to write all this out, of course, to keep your information

  • straight. The chemical symbol, with the atomic number or number of protons here,

  • the mass number, or number of protons and neutrons here,

  • and the charge out here, which tells you by simple addition or subtraction how

  • many electrons there are. Finally, before we conclude this first episode of Crash

  • Course Chemistry, and thus,

  • our discussion of the atomic nucleus, a note on the pronunciation

  • of "nucleus". You are welcome to say "nuculus"; it is an accepted pronunciation

  • of that word, but if you can find it in you,

  • it's probably best to switch over to "nucleus", which is, after all,

  • how it's spelled. And that is all for today's episode of Crash Course Chemistry,

  • if you were paying attention, you now know: More about atoms than anyone did in 1900,

  • like that they were finally confirmed when Einstein mathematically defined

  • Brownian motion; That

  • elements are chemically pure substances, and the type

  • of element an atom is is defined by how many protons it has in its nucleus,

  • or its atomic number; That neutrons stabilize nuclei for their proton

  • friends; That different isotopes of the same

  • element are the reason relative atomic masses are never whole numbers;

  • and you know that nuclei are the uninteresting, boring bits of the atom,

  • and the electrons are where all the interesting chemical-ly stuff happens. Crash Course

  • Chemistry is filmed, edited, and directed by

  • Nick Jenkins, Dr. Heiko Langner is our chemistry consultant,

  • sound design is done by Michael Aranda, and our graphics team

  • is Thought Bubble. If you have any questions, comments, or ideas on any of this stuff, we will

  • endeavor to answer them in the comments below.

  • Thank you for watching Crash Course Chemistry.

Hello, I'm Hank Green and I want to teach you chemistry. But please,

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