CHAPTER 25 Nuclear Chemistry - PowerPoint PPT Presentation

1 / 23
About This Presentation
Title:

CHAPTER 25 Nuclear Chemistry

Description:

Nuclear Chemistry I I. The Nucleus -Terms (p. 798-820) II III IV Ionizing Radiation Radiation is a form of energy transferred by waves or atomic particles Ionizing ... – PowerPoint PPT presentation

Number of Views:114
Avg rating:3.0/5.0
Slides: 24
Provided by: Mrs131
Category:

less

Transcript and Presenter's Notes

Title: CHAPTER 25 Nuclear Chemistry


1
CHAPTER 25 Nuclear Chemistry
I
  • I. The Nucleus -Terms
  • (p. 798-820)

II
III
IV
2
Ionizing Radiation
  • Radiation is a form of energy transferred by
    waves or atomic particles
  • Ionizing Radiation is any radiation with high
    enough energy to create ions (by knocking
    electrons out of atoms)
  • like UV, X, gamma, and cosmic rays
  • There are both natural sources of radiation
    (unstable nuclei and stars) and human created
    sources

3
Zone of Stability
  • Stable nuclei exist within the zone of
    stability seen on the graphnot always a 11
    ratio of p to no
  • Outside this range, nuclei are unstable and will
    decay (disintegrate) into new nuclei

4
Definitions
  • Nucleons particles in nucleus (p and n0)
  • Nuclide refers to the nucleus of an atom
  • Nuclear Reactions involve transmutation where one
    element become another.
  • Radioactive Decay is the when unstable nuclei
    spontaneous lose energy by emitting ionizing
    particles as this changes the nucleus of the
    atom, this also changes the type of element

5
Alpha Decay Process
Daughter Nuclide Np-237 Th-234 Ra-228 Rn-222
???????
Parent Nuclide Am-241 U-238 Th-232 Ra-226
Alpha Particle (Helium Nucleus) (4.00147 amu)
6
A. Mass Defect
  • The mass defect describes the mass lost during
    the formation of nuclei
  • Difference between the mass of an atom and the
    mass of its individual particles.

4.00260 amu Mass of atom
4.03298 amu Mass of particles
7
B. Nuclear Binding Energy
  • Energy released when a nucleus is formed from
    nucleons. This contributes to the loss in mass of
    nucleus, described by E mc2.
  • High binding energy stable nucleus.

E mc2
E energy (J) m mass defect (kg) c speed of
light (3.00108 m/s)
8
B. Nuclear Binding Energy
Iron (Fe) is the most stable nucleus!!
Unstable nuclides are radioactive and undergo
radioactive decay.
9
CHAPTER 25 Nuclear Chemistry
I
  • II. Radioactive Decay
  • (p. 798-820)

II
III
IV
10
Types of Spontaneous Radiation
stopped by
Greek symbol
charge
  • Alpha particle (?)
  • helium nucleus

paper
2
  • Beta particle ? or ?-
  • electron

1-
wood
  • Positron ?
  • positron

1
Lead or concrete
  • Gamma (?)
  • high-energy photon

0
11
Other Radiation particles
Greek symbol
charge
  • proton p

1
  • neutron n0

0
12
How does an electron get emitted from the nucleus?
  • Basically a neutron splits into a proton which
    stays in the nucleus and an electron is emitted
    (? decay)

-


-



n converted to a proton and an e is emitted
n p in nucleus
n is really like a p and e together
13
Transmutation Reactions
  • I Alpha Emission

Numbers must balance on both sides of
arrow!! 238amu on left (234 4amu) 92 is nucl
chrg on left 90 2 on right
14
B. Nuclear Decay
  • II Beta Emission
  • III Positron Emission

a proton 1p is not the same as a positron 0e
15
B. Nuclear Decay
  • IV Electron Capture

16
B. Nuclear Decay
  • V Alpha Capture followed by neutron emission
  • Gamma Emission causes no change in mass or charge
    and
  • Usually follows the previous
  • types of decay.

17
Beta (Negatron) Decay Process
Daughter Nucleus Osmium-187 Calcium-40
???
Antineutrino
Parent Nucleus Rhenium-187 Potassium-40
?????
Beta Particle (electron)
18
Beta Particles
  • Same as an electron with kinetic energy
  • Positive or negative charge of 1
  • May be positively or negatively charged
  • Can normally be stopped by 1 cm of plastic, wood,
    paper
  • Exception for positron emitters

19
B. Nuclear Decay
  • Why nuclides decaypg. 803
  • need stable ratio of neutrons to protons

DECAY SERIES TRANSPARENCY
20
C. Half-life
  • Half-life (t½)
  • Time required for half the atoms of a radioactive
    nuclide to decay.
  • Shorter half-life less stable.

21
C. Half-life
mf final mass mi initial mass n of half-lives
22
C. 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 mi 25 g mf ? total time
60.0 s n 60.0s 5.0s 12
WORK mf mi (½)n mf (25 g)(0.5)12 mf 0.0061
g
23
Decay Series
  • Many heavy elements are unstable and so they will
    continue to decay (be radioactive) until they
    finally transmute into a stable nucleus.
  • Here is an example of the Th-232 decay series
  • Thorium oxide is used to in camping lanterns to
    intensify the brightness when on fire.

Stable isotope
Write a Comment
User Comments (0)
About PowerShow.com