Nuclear Chemistry: Crash Course Chemistry #38

Summary

Nuclear chemistry is often misunderstood, painted as a power that mutates genes or causes catastrophic change. However, this Crash Course episode dives into the realities beyond the myths. Radioactivity involves the transformation of atomic nuclei, resulting in significant energy releases, fundamentally different from typical chemical reactions that involve electron exchanges. Understanding radioactivity's principles, like half-life, helps explain its persistence in nature and its potential uses. This episode also clarifies misconceptions about radioactive decay forms, such as alpha, beta, and gamma decay, and introduces the concept of spontaneous fission. With a fun and engaging format, the episode makes complex nuclear concepts accessible and interesting.

Highlights

• Radioactivity has fascinated and scared humans for over a century. 🤖
• The power of nuclear chemistry lies in its ability to transform elements and release massive energy. ⚡
• Half-life lets us predict the decay of elements, crucial for everything from archaeology to medicine. 📉
• Different decay types (alpha, beta, and gamma) behave in unique ways, affecting how we handle radioactivity. 🚀
• Spontaneous fission—it's pretty rare, but when it happens, it happens! 🤯

Key Takeaways

• Radioactivity isn't just dangerous mutations; it's also a key source of misunderstood power. ⚛️
• Nuclear chemistry transforms elements differently than traditional chemistry, focusing on protons and neutrons, not electrons. 🤔
• There's a form of radioactive decay out there called spontaneous fission—how spontaneous! 🎲
• Understanding half-life helps explain why we still have radioactive elements on Earth. 🌍
• Gamma radiation can sneak through skin, so watch out for the invisible rays! 😱

Overview

Radioactivity might conjure up images of mutants and superhero origins in sci-fi, but it’s far from just a plot device. This episode explores how nuclear chemistry, involving the interactions of protons and neutrons, can lead to dramatic transmutations with huge energy releases. These nuclear processes differ from typical chemistry, which only plays around with electron shells, showing us why this field is both fascinating and powerful!

We dive into the granular details, like what exactly happens when atoms undergo radioactive decay—whether they're ditching alpha particles, beta particles, or merely releasing energy as gamma rays. Understanding these processes lets scientists harness, control, and sometimes fear the implications of nuclear reactions. Plus, identifying half-lives helps track how long elements stick around, which is pretty darn useful for age estimations in fossils and more.

Speaking of nuclear reactions, did you know some atoms can split into smaller atoms on their own? This spontaneous fission is rare and mostly theoretical but still a thrilling component of nuclear chemistry. By demystifying these concepts, the episode makes it apparent why we should care more about radioactivity beyond just fear—it affects our energy solutions, medical advancements, and even how we understand time itself!

Chapters

• 00:00 - 00:30: Introduction to Radioactivity The chapter titled 'Introduction to Radioactivity' explores the common misconceptions and fictional representations of radioactivity in popular culture. It highlights how radioactivity is often depicted as a transformative force, capable of turning people into superheroes or mutant zombies, and serving as a central plot device in numerous sci-fi movies over the past six decades. Additionally, the chapter notes the song that describes radioactivity as ushering in a 'new age,' presumably post-apocalypse. The chapter underscores the prominence and simultaneous misunderstanding of radioactivity, emphasizing that many associate it with genetic mutations and extreme physical transformations.
• 00:30 - 01:30: Understanding Radioactivity and its Applications The chapter 'Understanding Radioactivity and its Applications' explains the need to understand radioactivity and its dual nature in offering both benefits and challenges. It highlights its ability to generate substantial electricity without exacerbating global warming, referencing the Fukushima incident as a cautionary tale. The chapter sets the stage for exploring nuclear chemistry, including nuclear fission and fusion, emphasizing radioactivity's complexity and importance.
• 01:30 - 02:00: Basics of Nuclear Chemistry This chapter introduces the concept of nuclear chemistry and attempts to demystify common fears associated with radioactivity. It begins by setting a context that radioactivity is distinct from typical chemical reactions that involve atoms' outermost electrons, implying that the internal components of the atom, such as protons and neutrons, remain unaffected during standard chemical reactions.
• 02:00 - 03:00: Transmutation and Stability in Nuclear Chemistry Nuclear chemistry focuses on reactions that involve changes to the nucleus of an atom, including protons and neutrons. Such changes can release immense energy, much greater than ordinary chemical reactions involving electron transfer. This particular study emphasizes the transformative impact that altering the nucleus can have on the nature of an atom.
• 03:00 - 04:00: Radioactive Decay and Half-Life The chapter 'Radioactive Decay and Half-Life' explores the fundamental aspects of atomic structure and identity, focusing on the role of protons and neutrons. Protons define an atom's identity, meaning any change in their number transforms an element into a different one—akin to the ancient dream of alchemists transmuting lead into gold. However, such transformations are not common in typical chemical reactions
• 04:00 - 05:00: Decay Chains and Cosmic Radiation This chapter delves into the concept of decay chains and cosmic radiation, focusing on transmutation—changing one isotope into another. It highlights that while it is technically possible to transmute lead into gold, the process is prohibitively expensive, yielding minuscule amounts of gold not worth the cost. This underscores the unique nature of nuclear chemistry, which, similar to non-nuclear chemistry, is driven by the atom's quest for stability.
• 05:00 - 08:00: Types of Radioactive Decay: Alpha, Beta, Gamma Atoms are most stable when their outer electron orbitals are full, and certain proton and neutron combinations in the nucleus also lead to stability. To reach a stable nuclear configuration, radioactive decay occurs when there is an imbalance. This process involves the nucleus releasing protons or neutrons, transforming the nucleus into a different one. Understanding nuclear reactions requires more information beyond just the reactants and products.
• 08:00 - 09:30: Spontaneous Fission and Its Applications The chapter 'Spontaneous Fission and Its Applications' covers the concept of half-life, which is crucial in understanding the rate at which a product is produced and decayed. It explains that the half-life is the time required for half of a sample to decay and varies for different nuclei. This knowledge is vital for calculating the amount of a sample that will remain over a specific time period. For instance, phosphorus-32 has a half-life of 14.3 days, meaning a 100 gram sample will reduce to 50 grams after about two weeks.
• 09:30 - 10:00: Summary and Credits The chapter titled 'Summary and Credits' delves into the concept of radioactive decay. It explains that over time, radioactive substances decay into more stable isotopes, eventually becoming non-radioactive. However, despite this ongoing decay process, radioactive elements are still present in the environment. This is primarily because radioactive elements with shorter half-lives are continuously replenished by the decay of elements with longer half-lives. The chapter also touches upon the stability of elements like bismuth, which has an exceptionally long half-life, even longer than the age of the universe.

Nuclear Chemistry: Crash Course Chemistry #38 Transcription

• 00:00 - 00:30 Apparently, it can turn you into a superhero or into a mutant zombie. It's the plot device for probably half of the sci-fi movies made in the last 60 years and it's even the name of the song that welcomes you to the new age, to the new age, welcome to the new age. Presumably this new age occurring after some kind of apocalypse. As principles of chemistry go, few figure more prominently in the popular imagination than radioactivity, but at the same time few are as completely misunderstood. Most people think of radioactivity as just some thing that mutates genes and melts faces off.
• 00:30 - 01:00 And yes, some forms of radioactivity can do those things. But all the more reason to understand it, right? And also we can harness it to produce lots of electricity to fuel our rock and roll lifestyles without contributing to global warming, though as Fukushima has taught us it comes with some of its own problems, which we'll explore more next episode. Before we get into the nuts and bolts of nuclear chemistry, like nuclear fission and why it's so awesome as well as fusion and why it's so hard to do, we'll first get to know radioactivity.
• 01:00 - 01:30 What it is, what different kinds there are, and why you don't really need to fear it. At least, you know, not all the time. [Theme Music] So, radioactivity doesn't actually have a lot to do with chemistry in the sense that we've been talking about for most of this course. Chemical reactions happen when an atom's outermost electrons do stuff, and the protons and neutrons and even the inner electron shells are usually completely unaffected.
• 01:30 - 02:00 But the protons and neutrons are still part of the atom, of course, still part of the chemicals, and their interactions are important. When protons and neutrons get directly involved in reactions and their numbers do change, huge amounts of energy can be released. Far more than by the transfer of electrons that we've learnted about in other reactions. When these changes happen to the nucleus of an atom we rather logically call their study: Nuclear Chemistry. Now it's probably occurred to you already that changing the nucleus of an atom can completely change it's nature.
• 02:00 - 02:30 Protons are the key to an atom's identity so any change that affects the number of protons will turn one element into a completely different one. An alchemist's dream, right? Lead to gold. So as you might expect, that's not something that usually happens in a typical chemical reaction. The same can be said of that other component of the nucleus, neutrons. Atoms of the same element that have the same number of protons, but different numbers of neutrons are isotopes. So changes in the number of neutrons in an atom create different isotopes of the same element. Both of these kinds of changes, changing one element to another,
• 02:30 - 03:00 or changing one isotope to another are known as transmutation. And it is, indeed, possible to transmute lead to gold. Its just so ridiculously expensive that the tiny amounts of gold produced could never pay for the process. But the very fact that it is possible, should clue you in that nuclear chemistry is an entirely different flavor of chemistry sauce. Though, as with non nuclear chemistry, the changes that take place in a nuclear reaction all come down to the atom's desire to have what we all want in life, stability.
• 03:00 - 03:30 Just as atoms are most stable when their outermost electron orbitals are full of electrons, certain combinations of protons and neutrons make the nucleus more stable. And just like when an atom gains or loses or shares electrons to stabilize it's outer shell, when the numbers of protons or neutrons aren't ideal, the nucleus releases some of them to try to reach a stable configuration. When a nucleus decomposes in this way to form a different nucleus that's radioactive decay. And just like with other chemical reactions we've talked about, we need to know more about a nuclear reaction than just what's reacting and what's being produced.
• 03:30 - 04:00 Probably the most important thing to learn is how much of the product is being made and how fast. Now you've heard of half life, it's the measurement that tells us just that. The time it takes for exactly one half of the sample to decay. Different nuclei have different half lives. By knowing the half life, we can calculate how much of a sample will be gone in a given amount of time. For example, the half life of phosphorus-32 is 14.3 days. So if you start with a 100 gram sample, after about 2 weeks you'll have 50 grams left.
• 04:00 - 04:30 After another 2 weeks, half of the remainder would decay leaving only 25 grams of undecayed phosphorus, and so on. Now you might be asking, if radioactive elements are always decaying in to more and more stable isotopes that are eventually no longer radioactive, why are they still around at all? Fascinating question, you seem to have brought your clever pants today. Well it's fairly simple, given enough time all radioactive elements would decay in to non radioactive forms. Even ultra stable bismuth, with it's half life longer than the age of the universe. But elements with short half lives are around because they were decayed in to by elements that recently decayed in to them.
• 04:30 - 05:00 The chain of decay from the element originally produced in whatever supernova created them, to the elements that exist on Earth now last billions and billions of years. Also, I should note that some radioactive isotopes like carbon-14 in the atmosphere are constantly being renewed by cosmic rays. Now radioactive decay occurs when a nucleus has a higher energy level than a potentially more stable version. Typically this difference in energy is released as what's called ionizing radiation.
• 05:00 - 05:30 Which you know as radioactivity. It's ionizing because it has enough energy to knock electrons out or add electrons to other atoms. Essentially creating ions. There are three general types of radioactive decay, each named for exactly what is released from the nucleus as it decays. Let's take a look at what may be the most famous radioactive element, uranium. By far the most common naturally occurring form of uranium is the isotope uranium-238. More than 99% of the natural uranium in the world is in this form. U-238 spontaneously decays in to thorium-234, in a process that releases something called an alpha particle.
• 05:30 - 06:00 This is called alpha decay and the particle that it emits is basically the same as a helium nucleus: two protons and two neutrons. We even describe it that way when writing it. So right away you can see that the math checks out when it comes to the protons and neutrons. 92 minus 2, is 90. And 238 minus 4, leaves you with 234. But you'll note, that we don't write the charges. The helium nucleus obviously has a plus 2 charge, and the thorium atom would have a negative charge as well.
• 06:00 - 06:30 While its not incorrect to write them, these charges are often omitted to emphasize what's going on in the nucleus. Now alpha particles have relatively low energy, they're pretty heavy as particles go. So while I try not to make a habit of walking around with a hunk of uranium in my pocket, alpha particles can be stopped by nothing more than a sheet of paper or cloth. The second type of radioactive decay is beta decay, which simply emits electrons. It has somewhat higher energy than alpha radiation, but it can still be stopped by a sheet of aluminum foil or the top layers of your skin. So that thorium-234 that formed when uranium underwent alpha decay?
• 06:30 - 07:00 It can continue to decay on its own, and when it does it undergoes beta decay. Releasing an electron and an atom of xenon. Notice that again, the way we write this is a little different. Even though the thorium emits an electron we don't use the usual symbol for electrons. Instead we write it in nuclear notation form, with the mass number at top and the atomic number at the bottom. Since its an electron, and not a proton, we put a negative 1 for the atomic number. That probably seems a little weird right now,
• 07:00 - 07:30 but next week when we talk about nuclear equations, you will see why it's useful. The third type of decay, is a little different, because it only emits energy, not a particle. Its called gamma decay, and it releases electromagnetic radiation similar to visible light, or UV radiation, but higher on the energy scale. Because it's just energy, gamma radiation has no mass and contains no protons, neutrons, or electrons. So it's written with two zeros. This form of radiation is often released when electrons transition from an unstable excited state, to a more stable state that has a lower energy. That's called the ground state.
• 07:30 - 08:00 Depending on how much energy the electron loses, the extra energy can be released in the form of visible, or ultraviolet light, x-rays, or gamma waves. Let's take the example of nickle-60. Imagine there's an atom of nickle-60 with one or more of its electrons in an excited state. That's what the little asterisks designates. Atoms can get to this state when they are themselves the products of radioactive decay, or if they get bombarded with radiation from other reactions pushing their electrons in to a higher energy level.
• 08:00 - 08:30 Now when all those electrons drop down to the ground state, that atom is going to release some gamma radiation. This kind of transition can also take place where other kinds of nuclear reactions are going on. So gamma decay often occurs along with some other form of decay too. So for example, if that uranium atom is at an excited state when it decays in to thorium, it can simultaneous release gamma waves as well as the alpha particle I already mentioned. Now you might have heard of gamma radiation more than the other kinds I've mentioned because it can actually do some serious harm. Like potentially turning you in to a giant green rage monster that doesn't obey the laws of conservation of matter.
• 08:30 - 09:00 Unlike the particles emitted by other kinds of radiation, gamma rays can penetrate your skin, your cell membranes, and ultimately the organelles within your cells. So gamma radiation can not only cause skin burns, nausea, other symptoms we associate with radiation poisoning, it can also alter your DNA causing mutations and cancer. OK, but to turn the frown upside down. There's one more type of radioactivity that I'm happy to say is really simple. It's called spontaneous fission and it occurs when an atom simply breaks in to 2 smaller atoms without any outside help.
• 09:00 - 09:30 This occurs at a ridiculously slow rate in most cases. In fact, the only substances that does it at a rate that sufficient to serve any purposes is Californium-254. And that purpose is to produce neutrons for use in other nuclear reactions. But we'll talk more about that when we go in to fission, fusion, and how scientists use and control nuclear reactions. In the meantime, thank you for watching this episode of Crash Course Chemistry. If you listened carefully, you learned what radioactivity really is. And about transmutation among elements and among isotopes.
• 09:30 - 10:00 And how to make calculations based on an elements half life. You also learned about different types of radioactive decay: alpha, beta, and gamma. And about spontaneous fission. This episode was written by Edi González and Blake de Pastino. It was edited by Blake de Pastino. And our chemistry consultant is Dr. Heiko Langner. It was filmed, edited, and directed by Nicholas Jenkins. The script supervisor was Michael Aranda, who is also our sound designer. And our graphics team is Thought Café.