Search Header Logo
Nuclear instability and Light

Nuclear instability and Light

Assessment

Presentation

Chemistry

10th - 11th Grade

Medium

Created by

Stacy King

Used 9+ times

FREE Resource

27 Slides • 5 Questions

1

Nuclear instability and Light

Mrs.King

Slide image

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\lambda   ν\nu  =C

  •  λ\lambda  wavelength

  •  ν\nu  frequency

  • c the speed of light constant 3.00 x 10^8

  • amplitude

6

Wavelength

  • distance of one crest to another

Slide image

7

frequency

  • the number of waves that occur in per unit time

Slide image

8

amplitude

  • distance between origin and creat

Slide image

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

Slide image

11

Multiple Choice

what is the frequency

1

the distance of one crest to another

2

the number of waves that occur in per unit time

3

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?

1

384.6 m

2

3.846 x 103 m

3

3.846 x 108 m

13

Orbitals and electrons

Slide image

14

Multiple Choice

a photon is

1

a particle of light

2

energy released by an electron as it returns to the ground state

3

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

17

Orbitals

  • dense electron clouds where e-'s are most likely to be found

  • they increase the diameter of the atom

  • S,P,D,F

18

S orbital

  • spherical

  • 2 e-

  • 1S (1S1 1S2)

  • 2S (2S1 2S2)

19

S orbital examples

  • Hydrogen has 1e- (1S1)

  • Helium has 2e- (1S2)

  • Lithium has 3e- (2S1)

  • Beryllium has 4e- (2S2)

20

Filling orbitals

  • must fill orbitals in order from lowest ground state

  • Aufbau principle

21

Slide image

22

P orbitals

  • dumbbell shaped

  • hold 6 e-

  • 2P, 3P, 4P, 5P, 6P

Slide image

23

P orbital examples

  • boron 5 e- (1S22S22P1)

  • Carbon 6e- (1S22S22P2)

  • Nitrogen 7e- (1S22S22P3)

  • Oxygen 8e- (1S22S22P4)

  • Fluorine 9e- (1S22S22P5)

  • Neon 10 e- (1S22S22P6)

24

Slide image

25

Multiple Choice

What is the electron configuration for Neon (Ne)

1

1S22S22P6

2

1S22S22P

3

1S22S21P5

4

not enough information

26

Multiple Choice

What is the electron configuration for Aluminum (Al)

1

1S22S22P63S24P1

2

1S22S22P63S23P1

3

1S22S21P63S1

4

1S22S22P63S23P

27

D orbital

  • shapes vary a little

  • hold 10 e-

  • make great catalyst

Slide image

28

F orbitals

hold 14 e-

Slide image

29

Pauli exclusion principle

  • e- can only share an orbital if their spin is in opposite directions

Slide image

30

Hund's Rule

electrons will fall into empty orbitals of the same energy before electrons begin to pair up into the same orbital.

Slide image

31

electron configuration

unpaired- paramagnetic

paired- diamagnetic

Slide image

32

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

Slide image

Show answer

Auto Play

Slide 1 / 32

SLIDE