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Nuclear Chemistry

Nuclear Chemistry. Nuclear Reactions. Chemical reactions What can NOT change in a chemical reaction? Nuclear Reactions: changes that occur in the nucleus of an atom The nucleus is unstable!! Most atoms have unstable nuclei. Why are some stable, while others are not?. Primary Reason:

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Nuclear Chemistry

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  1. Nuclear Chemistry

  2. Nuclear Reactions • Chemical reactions • What can NOT change in a chemical reaction? • Nuclear Reactions: changes that occur in the nucleus of an atom • The nucleus is unstable!! • Most atoms have unstable nuclei.

  3. Why are some stable, while others are not? • Primary Reason: • ratio of the neutrons to the protons (n/p) • An atom is most stable when ratio is 1:1 • The maximum ratio of stability is around 1.5 : 1

  4. Radioactivity • An unstable nucleus emits rays and particles, called radiation, to become stable • The process is called radioactivity • Gain stability by LOSING energy • Discovery dealt a deathblow to Dalton’s theory of indivisible atoms

  5. Types of Radiation • Alpha particle () • helium nucleus paper 2+ • Beta particle (-) • electron 1- • Gamma () • high-energy photon lead 0

  6. 3 Radioactive Particles • 1. Alpha Particle (+) • It travels about 1/10 the speed of light (slowest) • It is the largest, most massive particle • It is the most dangerous if ingested • It has the least penetrating ability - paper can stop this particle

  7. 3 Radioactive Particles • 2. Beta Particle (-) • Fast accelerated electron • Ejected when a neutron is converted to a proton in the nucleus • Travels 1/4 the speed of light. • It is lighter and faster than the alpha particle. • Average penetrating ability - can be stopped by heavy clothing

  8. 3 Radioactive Particles • 3. Gamma Ray • Not a particle; it is high energy electromagnetic radiation • Has no mass and no charge. • Always accompanies either beta or alpha radiation. • Travels at the speed of light. • Highest penetrating ability - can be stopped by heavy shielding such as lead.

  9. Radioactive Particles Summary

  10. parent nuclide daughter nuclide alpha particle Nuclear Decay • Alpha Emission Numbers must balance!!

  11. Nuclear Decay • Beta Emission • A neutron is converted in the nucleus of an atom • A new atom is formed whose atomic number is increased by 1

  12. Nuclear Decay • Gamma Emission • Always accompanies alpha and beta emissions. • Transmutation • One element becomes another.

  13. Half-life • Half-life (t½) • Time required for half the atoms of a radioactive nuclide to decay. • Shorter half-life = less stable.

  14. So, what does this mean? • Let’s say you have 100 g of radioactive C-14. The half-life of C-14 is 5730 years. • How many grams are left after one half-life? • How many grams are left after two half-lives? 50 g 25 g

  15. Common Radioisotopes

  16. To find the remaining amount… Half-life r :final mass i :initial mass n :# of half-lives

  17. More Half-Life Equations • Total time passed (p) = n x t1/2 • To find the half-life • t1/2 = • To find the # of half lives that have passed… • n =

  18. Half-life • Fluorine-21 has a half-life of 5.0 seconds. If you start with 25 g of fluorine-21, how many grams would remain after 60.0 s? GIVEN: t½ = 5.0 s i = 25 g r = ? p = 60.0 s n = 60.0s ÷ 5.0s =12 WORK: r = i (0.5)n r = (25 g)(0.5)12 r = 0.0061 g

  19. You try it! • If the half life element A is 3 hours and you have 90 grams of it, how many grams would be left after 9 hours?

  20. Fission • splitting a nucleus into two or more smaller nuclei • 1 g of 235U = 3 tons of coal

  21. Fission • chain reaction - self-propagating reaction

  22. Fusion • combining of two nuclei to form one nucleus of larger mass • thermonuclear reaction – requires temp of 40,000,000 K to sustain • 1 g of fusion fuel = 20 tons of coal • occurs naturally in stars

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