32
Chapter 13 Notes Electron Models

Chapter 13 Notes

  • Upload
    dalia

  • View
    33

  • Download
    0

Embed Size (px)

DESCRIPTION

Chapter 13 Notes. Electron Models. Evolution of Electron Models. The first model of the electron was given by J.J. Thompson—the electron’s discoverer. His was the “plum pudding” model. The Rutherford Model. With Rutherford’s discovery of the nucleus of an atom, the atomic model changed. - PowerPoint PPT Presentation

Citation preview

Page 1: Chapter 13 Notes

Chapter 13 NotesElectron Models

Page 2: Chapter 13 Notes

Evolution of Electron Models• The first model of the electron was given

by J.J. Thompson—the electron’s discoverer. His was the “plum pudding” model.

Page 3: Chapter 13 Notes

The Rutherford Model• With Rutherford’s discovery of the

nucleus of an atom, the atomic model changed.

Page 4: Chapter 13 Notes

The Bohr Model• Niels Bohr introduced his model, which

answered why electrons do not fall into the nucleus.

• He introduced the concept of energy levels, where the electrons orbited similar to the way the planets orbit the sun.

Page 5: Chapter 13 Notes

Bohr Model and Energy Levels• In the Bohr model, electrons are in energy

levels, or regions where they most probably are orbiting around the nucleus.

• The analogy is that energy levels are like the rungs of a ladder—you cannot be between rungs, just like an electron cannot be between energy levels.

• A quantum of energy is the amount of energy it takes to move from one energy level to the next.

Page 6: Chapter 13 Notes

Bohr Model and Energy Levels

• The Bohr model worked well for explaining the behavior of electrons in hydrogen, but for all other elements, the equations he used to predict the electron location did not work.

Page 7: Chapter 13 Notes

Quantum Mechanical Model• In 1926, Erwin Schrodinger used the new

quantum theory to write and solve mathematical equations to describe electron location.

Page 8: Chapter 13 Notes

The Quantum Mechanical Model, cont.• Today’s model comes from the solutions to

Schrodinger’s equations.

• Previous models were based on physical models of the motion of large objects.

• This model does not predict the path of electrons, but estimates the probability of finding an electron in a certain position.

• There is no physical analogy for this model!

Page 9: Chapter 13 Notes

Where are the electrons?• In an atom, principal energy levels (n) can

hold electrons. These principal energy levels are assigned values in order of increasing energy (n=1,2,3,4...).

• Within each principal energy level, electrons occupy energy sublevels. There are as many sublevels as the number of the energy level (i.e., level 1 has 1 sublevel, level 2 has 2 sublevels, etc.)

Page 10: Chapter 13 Notes

Where are the electrons?• There are four types of sublevels we will talk

about—s,p,d and f. Inside the sublevel are atomic orbitals that hold the electrons. Every atomic orbital can hold two electrons.

• S has one orbital, P has three, D has five and F has seven. How many electrons can each one hold?

Page 11: Chapter 13 Notes

Orbital Shapes

s orbital = s sublevel

+ +

px orbital py orbital pz orbital

= p sublevel

Page 12: Chapter 13 Notes

• http://winter.group.shef.ac.uk/orbitron/AOs/1s/index.html

Page 13: Chapter 13 Notes

Where are the electrons?• So how many electrons can each energy level

hold?

– Level 1 has an s sublevel=2 e-

– Level 2 has an s and a p sublevel=8e-

– Level 3 has an s, p and d sublevel=18e-

– Level 4 has an s, p, d and f sublevel=32e-

Page 14: Chapter 13 Notes

Electron Configuration

Page 15: Chapter 13 Notes

Electron Configuration• In the atom, electrons and the

nucleus interact to make the most stable arrangement possible.

• The ways that electrons are arranged around the nucleus of an atom is called the electron configuration.

Page 16: Chapter 13 Notes

Aufbau Principal• Electrons enter orbitals of the lowest energy

first.

Pauli’s Exclusion Principal• An atomic orbital may describe at most two

electrons.

Hund’s Rule• When electrons occupy orbitals of equal

energy, one electron enters each orbital until all orbitals contain one electron with parallelwith parallel spins.

Page 17: Chapter 13 Notes

He1s

2s

3s

4s

5s

6s

7s

2p

3p

4p

5p

6p

7p

3d

4d

5d

6d

4f

5f

Page 18: Chapter 13 Notes

EMR and Quantum Theory

Page 19: Chapter 13 Notes

What does a wave look like?

• With your partner, label all the parts of a wave you can remember.

Page 20: Chapter 13 Notes

A Quick Look at Waves—Parts of Waves

Page 21: Chapter 13 Notes

A Quick Look at Waves

• The number of waves to pass a point in a given time is called frequency () and is measured in 1/s or Hertz (Hz).

Page 22: Chapter 13 Notes

Electromagnetic Radiation (EMR)

• According to the wave model, visible light consists of electromagnetic waves and is just a small fraction of waves classified as electromagnetic radiation.

• Other EMR includes radio waves, microwaves, infrared, ultraviolet, X-rays, gamma rays and cosmic rays.

Page 23: Chapter 13 Notes

Electromagnetic Radiation (EMR)

• All of these waves travel at the same speed, 3.0x108m/s!

• The waves differ in their frequencies and wavelengths, and obey the equation: c =

• This is an inverse relationship—as the frequency increases, the wavelength decreases.

Page 24: Chapter 13 Notes

Practice Problems

• What is the wavelength of an electromagnetic wave with a frequency of 4.45x1015Hz?

• What is the frequency of a light wave with a wavelength of 497nm?

• What is the wavelength in nanometers of an electromagnetic wave with a frequency of 2.97x1014Hz?

Page 25: Chapter 13 Notes

Atomic Emission Spectra

• When sunlight is broken down into the waves it is made of, it creates a continuous spectrum

• Scientists used a hydrogen lamp to produce light, they expected a continuous spectrum but it wasn’t! They had an atomic emission spectrum.

Page 26: Chapter 13 Notes

• When we previously found the electron configuration for elements, it was for electrons at ground state (the lowest energy possible).

• As energy is added to atoms, they absorb the energy by electrons going from ground state to an excited state, where electrons are no longer in the lowest energy orbitals.

Page 27: Chapter 13 Notes

• Electrons can then only go back to ground state by releasing the energy, usually in the form of light in discreet packets called photons.

• These packets defied classical physics, that said electrons would go back to ground state continuously.

Page 28: Chapter 13 Notes

Max Planck• To understand why this points towards

the concept of energy levels, we need to know about Max Planck’s discovery:

•E = h • Planck’s constant (h=6.6262x10-34Js)

Page 29: Chapter 13 Notes

Practice Problems

• How much energy is associated with a wave with a frequency of 4.4x1014Hz?

• An electromagnetic wave is found to have 1.18x10-19J of energy. What is its frequency?

• How much energy is associated with a wave of red light with a wavelength of 697nm?

Page 30: Chapter 13 Notes

Putting It Together• So, if only specific frequencies of So, if only specific frequencies of

light are emitted when electrons fall light are emitted when electrons fall back to ground state from being back to ground state from being excited, then there are only certain excited, then there are only certain energies that electrons can have. energies that electrons can have. This explains atomic emission This explains atomic emission spectra!spectra!

Page 31: Chapter 13 Notes

Even Stranger…• Louis de Broglie predicts yet another Louis de Broglie predicts yet another

property of electrons—that they have property of electrons—that they have both a wave nature and a particle both a wave nature and a particle nature. nature.

• Any moving particle can be described Any moving particle can be described to have a wave nature described by to have a wave nature described by de Broglies equation:de Broglies equation:

• = h / mv = h / mv

Page 32: Chapter 13 Notes

• Even stranger still is the Even stranger still is the Heisenberg Heisenberg Uncertainty PrincipleUncertainty Principle..

• It states that you cannot know both a It states that you cannot know both a particles exact position and exact particles exact position and exact velocity (the more you know about velocity (the more you know about one the less you know about the one the less you know about the other).other).