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Nuclear Chemistry Ch.18

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Nuclear Chemistry. Ch.18. (18-1) Nuclear Stability. Nucleons : p + & n 0 Nuclide : any combo of p + & n 0 in a nucleus Isotope : same at.#, but different mass Te-122, Te-124, Te-128 Isobar : same mass, but different at.# Xe-124, Te-124, Sn-124. Binding Forces. - PowerPoint PPT Presentation

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Page 1: Nuclear Chemistry

Nuclear Chemistry

Ch.18

Page 2: Nuclear Chemistry

(18-1) Nuclear Stability

• Nucleons: p+ & n0

• Nuclide: any combo of p+ & n0 in a nucleus– Isotope: same at.#, but different mass• Te-122, Te-124, Te-128

– Isobar: same mass, but different at.#• Xe-124, Te-124, Sn-124

Page 3: Nuclear Chemistry

Binding Forces

• Strong nuclear force: attraction that holds nuclear particles together– Overcomes repulsive forces

Page 4: Nuclear Chemistry

Mass Defect

• Mass converted to E when a nucleus forms

Page 5: Nuclear Chemistry

Nuclear Binding E• E emitted when nucleons come together (E

needed to break a nucleus apart)

Page 6: Nuclear Chemistry

Band of Stability

• Area on a graph of n0 # v. p+ # in which all stable nuclei lie

Page 7: Nuclear Chemistry

Nuclei are more stable if they…

• Contain n0 ≥ p+

• Do not have too many or too few n0

• Have even #’s of nucleons• Have “magic #’s” of p+ or n0

– 2, 8, 20, 28, 50, 82, 126• Are not a neighboring isobar

Page 8: Nuclear Chemistry

(18-2) Types of Nuclear Change

• Spontaneous1. Radioactivity

– Artificial Transmutations2. Fission3. Fusion

• Nonspontaneous4. Transmutation

Page 9: Nuclear Chemistry

Radioactivity

• A nucleus decays & emits particles & electromagnetic waves

Page 10: Nuclear Chemistry

Converting n0 to p+

• Beta (β) decay: nuclei w/ too many n0 for the at.# become more stable by decaying & emitting radiation

• β particle: e- emitted from a nucleus when a n0 changes to a p+

• Ex:

Page 11: Nuclear Chemistry

Converting p+ to n0

• e- capture: nucleus has too few n0, so it absorbs an e-, which changes a p+ into a n0

• Gamma rays (γ): E produced by decaying nuclei

• Ex:

Page 12: Nuclear Chemistry

Converting p+ to n0 (cont.)

• Positron emission: nuclei emit postitrons (antiparticles of e-)

• Ex:

Page 13: Nuclear Chemistry

Annihilation of Matter

• Event when a particle collides w/ its anitparticle & both are changed into E

Page 14: Nuclear Chemistry

Losing Alpha Particles

• Alpha (α) decay: very large nuclei w/ too few n0 can decay by emitting α particles

• α particles: Helium-4 made when a n0 decays• Ex:

• Decay series: many heavy nuclei must decay several times before reaching a stable state

Page 15: Nuclear Chemistry

Balancing Nuclear Eq.’s

• Total mass #’s & nuclear charges must balance on both sides of the eq.

• Ex: Masses = 234, Charges = 90

• Ex: Masses = 238, Charges = 92

Page 17: Nuclear Chemistry

Nuclear Fusion

• 2 small nuclei combine to form 1 more stable nucleus & lots of E

• Reactants are plasmas (mixture of + nuclei & e-)

• Need very high T’s & P’s

Page 18: Nuclear Chemistry

Transmutation

• Creating new nuclei by bombarding a nucleus w/ α particles

• Produces an unstable cmpd that stabilizes by emitting a p+

Page 19: Nuclear Chemistry

(18-3) How Nuclear Chem is Used

• Radioactive dating: using radioactive isotopes to determine an object’s age

• Half-life: time required for half of a radioactive material to decay

Page 20: Nuclear Chemistry

Smoke Detectors

• Have an α emitter, which attract e- from the gas, changing them to ions which conduct electricity

• When smoke particles mix w/ the gas, they reduce current flow & the detector’s circuits are set off

Page 21: Nuclear Chemistry

Neutron Analysis

• Used to determine composition of objects– Meteorite composition– Forensic science (gun residue)

Page 22: Nuclear Chemistry

Radiation Exposure

• rem: biological effect of exposure to nuclear radiation– Limit of 5 rems/yr