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REMINDER: STUDY GROUP ASSIGNMENT THIS WEEK LAB THIS WEEK ELECTRON ORBITALS October 26, 2009

October 26, 2009

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October 26, 2009. REMINDER: STUDY GROUP ASSIGNMENT THIS WEEK LAB THIS WEEK ELECTRON ORBITALS. Visible Spectroscopy. Heisenberg Uncertainty Principle. We can’t know both the exact location and the energy of a particle - PowerPoint PPT Presentation

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Page 1: October 26, 2009

•REMINDER: STUDY GROUP ASSIGNMENT THIS WEEK

•LAB THIS WEEK

•ELECTRON ORBITALS

October 26, 2009

Page 2: October 26, 2009

Visible Spectroscopy

Page 3: October 26, 2009

Heisenberg Uncertainty Principle

We can’t know both the exact location and the energy of a particle

For electrons => We know the energy, so we don’t know the location very well

Page 4: October 26, 2009

Schrödinger’s Model of Hydrogen

Electrons act as standing waves

Wave behavior is described by a wave function: ψ Certain wave functions are allowed ψ2 describes the probability of finding the electron in

a particular spot (aka, electron density)

Page 5: October 26, 2009

Here’s what a probability density looks like…

(A bit simplified)

…but what does it mean?

o-r/a2 2 = x e

Page 6: October 26, 2009

Orbitals

Each wave function describes a shape = Orbital Where an electron can be found/exist Organized into main shells and subshells

Number of orbitals is different for each subshell type: s = 1 orbital p = 3 orbitals d = 5 orbitals f = 7 orbitals

Size and Energy(n=1, 2, 3, … )

Shape(s, p, d, f, … )

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Page 8: October 26, 2009

1s ___11

2p ___ ___ ___2s ___22

3d ___ ___ ___ ___ ___

3p ___ ___ ___3s ___

33

ENERGY

•1, 2, and 3 correspond to the major energy levels (main shells)

•At the same main shell level, a p orbital will be at a higher energy than an s orbital

4f ___ ___ ___ ___ ___ ___ ___ 4d ___ ___ ___ ___ ___ 4p ___ ___ ___

4s ___

44

Page 9: October 26, 2009

What type of orbital is this?

1 2 3 4

25% 25%25%25%1. s2. pz

3. dxy

4. dxz

10

Page 10: October 26, 2009

Which type of orbital can’t exist?

1 2 3 4

25% 25%25%25%1. 1px

2. 2px

3. 2s4. 3dxy

10

Page 11: October 26, 2009

NODES- Where electrons don’t go

Spherical Nodes

Page 12: October 26, 2009

Hydrogen

Page 13: October 26, 2009

You too can play with hydrogen…

http://homepages.ius.edu/kforinas/physlets/quantum/hydrogen.html

Page 14: October 26, 2009

Quantum # Rules

There are four different quantum numbers: n, l, ml, and ms

n, l, and ml are integers n cannot be zero l can be 0 to n-1 ml can be anything from –l to l Ms can be +½ or -½

Page 15: October 26, 2009

Quantum Numbers and Orbitals

Page 16: October 26, 2009

Rules for filling orbitals

1. Pauli Exclusion PrincipleNo two electrons can have the same 4 quantum numbersAn orbital has a maximum of 2 electrons of opposite spin

2. Aufbau/Build-up PrincipleLower energy levels fill before higher energy levels

3. Hund’s RuleElectrons only pair after all orbitals at an energy level have

1 electron

4. Madelung’s RuleOrbitals fill in the order of the value of n + l

Page 17: October 26, 2009

Orbital Filling Order