

Nuclear instability and Light
Presentation
•
Chemistry
•
10th - 11th Grade
•
Medium
Stacy King
Used 9+ times
FREE Resource
27 Slides • 5 Questions
1
Nuclear instability and Light
Mrs.King

2
Nuclear decay
Alpha decay- loss of alpha particle
beta decay- neutron and loss of e-
gamma decay- nuclear fission and excess energy
Alpha and beta are nuclear changes
gamma is caused by alpha and energy
3
Light
c=the speed of light
4
Light are wave particles
Photons
electromagnetic wave particles-electric field and magnetic field
quantum
5
Components of light waves
λ ν =C
λ wavelength
ν frequency
c the speed of light constant 3.00 x 10^8
amplitude
6
Wavelength
distance of one crest to another
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frequency
the number of waves that occur in per unit time
8
amplitude
distance between origin and creat
9
Speed of light
the constant speed that light travels in a vacuum
3.00 x 108
10
electromagnetic spectrum
increase frequency=increase in energy
wavelengths increase as energy increases
11
Multiple Choice
what is the frequency
the distance of one crest to another
the number of waves that occur in per unit time
the distance between the origin and crest
12
Multiple Choice
A news broadcast on a statin that transmits at 780.0 kHz (convert to Hz) what is the wavelength?
384.6 m
3.846 x 103 m
3.846 x 108 m
13
Orbitals and electrons
14
Multiple Choice
a photon is
a particle of light
energy released by an electron as it returns to the ground state
all of the above
15
Electrons
the gain loss or sharing of electrons create chemical bonding
are found in orbitals around the nucleus
16
Valence shells
outermost energy shell
the reactive e- 's
the bonding force
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Orbitals
dense electron clouds where e-'s are most likely to be found
they increase the diameter of the atom
S,P,D,F
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S orbital
spherical
2 e-
1S (1S1 1S2)
2S (2S1 2S2)
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S orbital examples
Hydrogen has 1e- (1S1)
Helium has 2e- (1S2)
Lithium has 3e- (2S1)
Beryllium has 4e- (2S2)
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Filling orbitals
must fill orbitals in order from lowest ground state
Aufbau principle
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P orbitals
dumbbell shaped
hold 6 e-
2P, 3P, 4P, 5P, 6P
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P orbital examples
boron 5 e- (1S22S22P1)
Carbon 6e- (1S22S22P2)
Nitrogen 7e- (1S22S22P3)
Oxygen 8e- (1S22S22P4)
Fluorine 9e- (1S22S22P5)
Neon 10 e- (1S22S22P6)
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25
Multiple Choice
What is the electron configuration for Neon (Ne)
1S22S22P6
1S22S22P
1S22S21P5
not enough information
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Multiple Choice
What is the electron configuration for Aluminum (Al)
1S22S22P63S24P1
1S22S22P63S23P1
1S22S21P63S1
1S22S22P63S23P
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D orbital
shapes vary a little
hold 10 e-
make great catalyst
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F orbitals
hold 14 e-
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Pauli exclusion principle
e- can only share an orbital if their spin is in opposite directions
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Hund's Rule
electrons will fall into empty orbitals of the same energy before electrons begin to pair up into the same orbital.
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electron configuration
unpaired- paramagnetic
paired- diamagnetic
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Quantum numbers
Principle- size of energy level
angular momentum- shape of the orbital
spin- spin of e-
magnetic- orbital orientation
Nuclear instability and Light
Mrs.King

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