1.  UNIT 3: Nuclear Chemistry CP Chemistry Grafton High School

2. UNIT OBJECTIVES:  SWBAT:

3. Key Questions  How do nuclear reactions differ from chemical reactions?  What are the three types of nuclear radiation?  How is nuclear power used to generate electricity?  How much of a radioactive sample remains after each half life?  How is radiation detected?  What are some practical uses of radioisotopes?

4. Radioactivity  One of the pieces of evidence for the fact that atoms are made of smaller particles came from the work of Marie Curie (1876- 1934) and her husband, Antoine Henri Becquerel.  She created the term radioactivity, the spontaneous disintegration of some elements into smaller pieces by emission of particles or rays  WATCH: https://goo.gl/IyuRj4 https://goo.gl/IyuRj4

5. Nuclear Reactions vs. Normal Chemical Changes  Radioisotopes are isotopes with unstable nuclei and undergo radioactive decay  Nuclear reactions involve the nucleus  The nucleus opens, and protons and neutrons are rearranged  The opening of the nucleus releases a tremendous amount of energy that holds the nucleus together – called binding energy  “Normal” Chemical Reactions involve electrons, not protons and neutrons  Nuclear decay is NOT affected by temperature, pressure or presence of catalysts (as chemical reactions ARE).  Spontaneous nuclear decay cannot be sped up or slowed down.

6. Energy From Nuclear Decay  Nuclear decay produces ENERGY  That energy is released as electromagnetic radiation (gamma rays) or kinetic energy (carried by alpha and beta particles)

7. Types of Radiation Alpha (ά) – a positively charged helium isotope - we usually ignore the charge because it involves electrons, not protons and neutrons Alpha (ά) – a positively charged helium isotope - we usually ignore the charge because it involves electrons, not protons and neutrons Beta (β) – an electronBeta (β) – an electron Gamma (γ) – pure energy; called a ray rather than a particleGamma (γ) – pure energy; called a ray rather than a particle

8.  Characteristics of Radiation

9. Penetrating Ability

10. Alpha, Beta, and Gamma Radiation  Atoms are not all stable.  Excess energy in an unstable atom is released in a basic particle or wave  Radioactive isotopes have undergone nuclear decay to become MORE stable  Greek alphabet is used to name particles (in order of their discovery)

11. REMEMBER!  The nuclear structure changes with radioactive decay, but radioisotopes are NOT chemically different!

12. Alpha Particles  Heaviest particle  Rays, NOT waves –made of high-energy particles that are expelled from unstable nuclei  Alpha particle is a helium nucleus (ion)  Not very penetrating; easily absorbed  SPEED: 16,000km/sec (1/10 th speed of light!)

13. Balancing Nuclear Reactions In the reactants (starting materials – on the left side of an equation) and products (final products – on the right side of an equation) Atomic numbers must balance and Mass numbers must balance Use a particle or isotope to fill in the missing protons and neutrons

14. Nuclear Reactions  Alpha emission Note that mass number (A) goes down by 4 and atomic number (Z) goes down by 2. Nucleons (nuclear particles… protons and neutrons) are rearranged but conserved

15. Beta Particles  LIGHTER energy particles  Energetic electron given off by unstable nuclei to restore energy balance  Stopped by aluminum (few mm thick) or 3 meters of air  8,000 times smaller than alpha particle  SPEED: 270,000 km/sec  Can cause cellular damage

16. Nuclear Reactions  Beta emission Note that mass number (A) is unchanged and atomic number (Z) goes up by 1. This is because it is caused by a neutron that breaks apart into a proton and electron (electron is emitted).

17. Gamma Ray  HIGH-ENERGY photon (light wave)  Same family as X-rays and light  MORE energetic and harmful  Damaging to living cells  Slows down energy by transferring it to cell components

18. Artificial Nuclear Reactions New elements or new isotopes of known elements are produced by bombarding an atom with a subatomic particle such as a proton or neutron -- or even a much heavier particle such as 4 He and 11 B. Reactions using neutrons are called  reactions because a  ray is usually emitted. Radioisotopes used in medicine are often made by  reactions.

19. Transuranium Elements Elements beyond 92 (transuranium) made starting with an  reaction 238 92 U + 1 0 n ---> 239 92 U +  239 92 U ---> 239 93 Np + 0 -1  239 93 Np ---> 239 94 Pu + 0 -1  239 93 Np ---> 239 94 Pu + 0 -1 

20. Nuclear Fission

21.  Fission is the splitting of atoms caused by bombarding nuclei of isotopes with neutrons  Controlled reaction; produces ENERGY  Example: Fission of Uranium-235 nucleus

22. Nuclear Fission  Chain reaction: More neutrons are released, which strike nuclei of other isotopes  These are usually very large, so that they are not as stable  Nuclear Power stations use heat released by nuclear reaction (nuclear fission) to boil water to make steam

23. Fission Process - MODEL

24. Nuclear Fission & POWER  Currently about 103 nuclear power plants in the U.S. and about 435 worldwide.  17% of the world’s energy comes from nuclear.

25. Diagram of a nuclear power plant

26. Nuclear Explosion  Explosion occurs when reaction is allowed to run out of control  Large amounts of ENERGY released QUICKLY  WATCH:  Nuclear reactor controls rate of energy release  Uranium oxide held in fuel rods  Rods lowered into reactor core  Coolant (CO2) circulated to remove heat  Control rods in core absorb neutrons and control rate of chain reaction  Raised to speed up; lowered to slow down

27. Nuclear Fusion  Fusion occurs when small nuclei combine to create nucleus of greater mass.  Releases more energy than fission  Occur only at VERY high temperatures (40,000,000 °C)  Hydrogen bomb is uncontrolled-fusion device  Occurs naturally in the sun and other stars

28. Half-Life  HALF-LIFE is the time that it takes for 1/2 a sample to decompose.  The rate of a nuclear transformation depends only on the “reactant” concentration.

29. Half-Life Decay of 20.0 mg of 15 O. What remains after 3 half-lives? After 5 half-lives?

30. Kinetics of Radioactive Decay For each duration (half-life), one half of the substance decomposes. For example: Ra-234 has a half-life of 3.6 days If you start with 50 grams of Ra-234 After 3.6 days > 25 grams After 7.2 days > 12.5 grams After 10.8 days > 6.25 grams

31. Learning Check! The half life of I-123 is 13 hr. How much of a 64 mg sample of I-123 is left after 39 hours?

32. Effects of Radiation

33. Geiger Counter  Used to detect radioactive substances

34. Radiocarbon Dating Radioactive C-14 is formed in the upper atmosphere by nuclear reactions initiated by neutrons in cosmic radiation 14 N + 1 o n ---> 14 C + 1 H The C-14 is oxidized to CO 2, which circulates through the biosphere. When a plant dies, the C-14 is not replenished. But the C-14 continues to decay with t 1/2 = 5730 years. Activity of a sample can be used to date the sample.

35. Nuclear Medicine: Imaging Thyroid imaging using Tc-99m

36. Food Irradiation Food can be irradiated with  rays from 60 Co or 137 Cs.Food can be irradiated with  rays from 60 Co or 137 Cs. Irradiated milk has a shelf life of 3 mo. without refrigeration.Irradiated milk has a shelf life of 3 mo. without refrigeration. USDA has approved irradiation of meats and eggs.USDA has approved irradiation of meats and eggs.