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Nuclear Chemistry Chapter 18.

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Presentation on theme: "Nuclear Chemistry Chapter 18."— Presentation transcript:

1 Nuclear Chemistry Chapter 18

2 Quick Review Mass # Symbol Element Name or symbol – Mass #
Parts of a Reaction Reactants  Products

3 Types of Radiation Alpha emission or decay (a) –helium atom 42He
23892U  42He Th Beta emission or decay (b)– 0-1e in the products 23490Th  23491Pa + 0-1e Gamma emission or decay (g) - 00g 23892U  42He Th + 00g

4 Types of Radiation & Particles
Positron emission or decay e 2211Na  0+1e Ne Electron capture – beta particle in the reactants 20180Hg e  Au Neutron emission or decay– 10n 20984Po  10n Po Proton – 11H or 11p

5 Balancing Nuclear Equations
Mass # and the atomic # totals must be the same for reactants and the products. 3919K  3517Cl + ___ 20682Pb  0-1e + ___ 23894Pu + ___ 42He U

6 Writing Balanced Nuclear Equations
Alpha decay of Cu-68 Gamma emission of Thorium-235 Positron emission of P-18 Astatine-210 releasing 3 neutrons Electron capture of Ti-45

7 Half-Life and Nuclear Stability
Radioactive isotopes or nuclides all decay because they are unstable, some just breakdown much faster than others Half-life – amount of time for half of the original sample to decay For two samples of the same isotope, regardless of the sample size, after one half- life, only half of the original amount of sample remains.

8 Sample Half-lives Isotopes Half-Live Carbon – 14 5730 years
Sodium – hours Bismuth – seconds Polonium – seconds Thorium – years Thorium – days Uranium – x 108 years Uranium – x 109 years

9 Half-life sample problems
Barium – 139 has a half-life of 86 minutes. If you originally have a 10 gram sample of Barium-139, how much will be left after 258 minutes?

10 Half-life sample problems
How many days will it take 50 grams of Radon – 222 (half-life of 3.82 days) to decay to grams?

11 Half-life sample problems
If a sample of Cesium-135 decays from 10 grams to 2.5 grams over a period of 84 days, what is the half-life of Cesium-135?

12 Predicting radiation types from Reaction Products
238U  234Th  234Pa  234U α β β 234U  230Th  226Ra  222Rn  218Po  214Pb α α α α α 214Pb 214Bi 214Po 210Pb 210Bi 210Po206Pb β β α β β α

13 Scientists who shaped Nuclear Chemistry
Henri Becquerel Discovered Natural Radioactivity - Nobel Prize (physics) 1903 Wilhem Roentgen Discovered X- rays (1895) - Nobel Prize (physics) 1901 Marie (Sklowdowska) Curie 1867 – 1934 Discovered Radium and Polonium - (2) Nobel Prizes (physics) 1903, Chemistry (1911) – first woman to teach at the Sorbonne in its 650 yr history, first person to receive two Nobel prizes, only person to receive 2 Nobels in Sciences

14 Scientists who shaped Nuclear Chemistry
Pierre Curie Nobel Prize (physics) 1903 Ernest Rutherford Demonstrated the existence of the nucleus Nobel Prize (chemistry) 1908

15 Medical Applications of Nuclear Chem.
Cancer Radiation Treatment Computer Imaging techniques Radiocarbon dating Smoke detectors Food irradiation Radioactive tracers – Iodine 131 used to treat thyroid illnesses and Thallium -201 can be used determine the damage done to someone’s heart by a heart attack

16 Fission Nuclear fission was discovered in late 1930’s when U-235 was bombarded with neutrons and observed to split into two lighter elements. 10n U  9236Kr Ba + 310n Energy from combustion of 1 mole of U-235 produces 26 million times as much energy as the combustion of 1 mole of methane.

17 Fission The neutrons are produced from fission reactions, will then react with other radioactive atoms, which will produce more neutrons and so on, potentially creating an uncontrollable chain reaction.

18 Sample fission reaction

19 Nuclear Fusion Fusion – combining two smaller nuclei into one heavier, more stable nucleus. 32He + 11H  42He + 01e Fusion reaction produce more energy than fission reactions. Fusion reactions are most commonly seen in stars.

20 Nuclear Fusion We have many potential sources for fusion reactions, but the problem lies in trying to slam two positively charged nuclei together with enough force to make them combine. It is thought that the temperature must be over 40 million Kelvin for this to occur, which is where the speed of the particles could potentially overcome the repulsive forces.

21 Sample fusion reaction

22 Effects of Radiation Somatic damage – done to the organism itself, resulting in either sickness or death. Effect of somatic damage may be immediate or take years to show their effects, such as radiation treatment for cancer patients. Genetic damage – damages cells which can be passed on to afflict offspring of initially effecting organism.

23 Effects of Radiation Energy of radiation – higher energy = more damage (big surprise) Penetrating ability of the radiation – gamma particles are high penetrating, beta can penetrate 1 cm and alpha particles can be stopped by the skin.


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