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(1)

“No familiar conceptions can be woven

around the electron. Something unknown is

doing we don’t know what.”

-Sir Arthur Eddington

The Nature of the Physical World (1934)

“No familiar conceptions can be woven

around the electron. Something unknown is

doing we don’t know what.”

-Sir Arthur Eddington

The Nature of the Physical World (1934)

The ELECTRON:

(2)

The Big Bang Theory

(3)

The Dilemma of the Atom

Electrons outside the nucleus are

attracted to the protons in the nucleus

Charged particles moving in curved

paths lose energy

What keeps the atom from collapsing?

Electrons outside the nucleus are

attracted to the protons in the nucleus

Charged particles moving in curved

paths lose energy

(4)

Wave-Particle Duality

JJ Thomson won the Nobel prize for describing the

electron as a particle.

His son, George Thomson won the Nobel prize for

describing the wave-like nature of the electron.

The

electron is

a particle!

electron is

The

an energy

(5)

The Wave-like Electron

Louis deBroglie

The electron propagates

through space as an energy

wave. To understand the

atom, one must understand

the behavior of

electromagnetic waves.

The electron propagates

through space as an energy

wave. To understand the

atom, one must understand

(6)

c =



c = speed of light, a constant (3.00 x 10

8

m/s)

= frequency, in units of hertz (hz, sec

-1

)

= wavelength, in meters

(7)

E = h

E

= Energy, in units of Joules (kg·m

2

/s

2

)

h

= Planck’s constant (6.626 x 10

-34

J·s)

(8)

Long

Wavelength

=

Low Frequency

=

Low ENERGY

Short

Wavelength

=

High

Frequency

=

High ENERGY

Wavelength Table
(9)

Practice problems

Wave length (

) (

m

)

Frequency(

)

(

hz

)

NRG (E) (

J

)

Violet

400nm

Blue

475nm

Green

510nm

Yellow

570nm

Orange

590nm

Red

650nm

H-red line 656nm

1. Most show all work to receive full credit.

2. Use the speed of light eqtn (

c =



) to solve for frequency.

Wavelengths must be in m not nm.

(10)

Practice problems

Wave length (

) (

m

)

Frequency(

)

(

hz

)

NRG (E) (

J

)

Violet

400nm= 4.00 x 10

-7

= 7.5 x 10

14

= 5.01 x 10

-19

Blue

475nm= 4.75 x 10

-7

= 6.32 x 10

14

= 4.19 x 10

-19

Green

510nm= 5.10 x 10

-7

= 5.88 x 10

14

= 3.90 x 10

-19

Yellow

570nm= 5.70 x 10

-7

= 5.26 x 10

14

= 3.49 x 10

-19

Orange

590nm= 5.90 x 10

-7

= 5.08 x 10

14

= 3.37 x 10

-19

Red

650nm= 6.50 x 10

-7

= 4.62 x 10

14

= 3.06 x 10

-19

H-red line 656nm= 6.56 x 10

-7

= 4.57 x 10

14

= 3.03 x 10

-19

1. Most show all work to receive full credit.

2. Use the speed of light eqtn (

c =



) to solve for frequency.

Wavelengths must be in m not nm.

3. Then use that # to solve for NRG (

E = h

)

(11)

Answering the Dilemma of the

Atom

Treat electrons as waves

As the electron moves toward the

nucleus, the wavelength shortens

Shorter wavelength = higher energy

Higher energy = greater distance from

the nucleus

Treat electrons as waves

As the electron moves toward the

nucleus, the wavelength shortens

Shorter wavelength = higher energy

Higher energy = greater distance from

(12)
(13)

This produces bands

of light with definite

wavelengths.

Electron transitions

involve jumps of

(14)

…produces a “bright line” spectrum

(15)

Photoelectric Effect

a. Quantum – of nrg is the minimum quantity of nrg

that can be lost or gained by an atom.

b. Photon – is a particle of electromagnetic radiation

having zero mass and carrying a quantum of nrg.

c. Elements can have different levels of nrg.

i. Ground state –little to no nrg

ii. Excited state – higher potential nrg

a. when excited, then return to ground state,

certain gases give off light

(16)

Flame Tests

strontium

sodium

lithium

potassium

copper

(17)

Bohr’s model:

A. Nucleus is in the center of an atom(like the sun) and the

electrons orbit the nucleus similar to the planets.

B. Used the emission spectrum(photon) to determine nrg

levels

i. Orbits are called shells

a. 1

st

shell = 2 electrons

b.2

nd

shell = 8 electrons

c. 3

rd

shell = 8 electrons etc….

(18)

The Bohr Model of the Atom

Neils Bohr

I pictured electrons

orbiting the nucleus much

like planets orbiting the

sun.

I pictured electrons

orbiting the nucleus much

like planets orbiting the

sun.

(19)

Quantum Mechanical

Model of the Atom

Mathematical laws can identify the regions

outside of the nucleus where electrons are

most “

likely”

to be found.

(20)

Heisenberg Uncertainty Principle

You can find out where the

electron is, but not where it

is going.

OR…

You can find out where the

electron is going, but not

where it is!

“One cannot simultaneously

determine both the position

and momentum of an electron.”

“One cannot simultaneously

determine both the position

and momentum of an electron.”

(21)

Electron Energy Level (Shell)

Generally symbolized

by n, it denotes the

probable distance of

the electron from

the nucleus. “n” is

also known as the

Principle Quantum

number

Number of electrons

that can fit in a

(22)

Orbital shapes are defined as the surface

that contains 90% of the total electron

probability.

An orbital is a region within an energy level

where there is a probability of finding an

electron.

(23)

The

s

orbital has

a spherical shape

centered around

the origin of the

three axes in

space.

There is only 1

type of s orbital.

(24)

There are three dumbbell-shaped

p

orbitals in each energy level above n = 1,

each assigned to its own axis (x, y and z)

in space.

(25)
(26)
(27)

Things get a bit more

complicated with the

five

d

orbitals that are

found in the

d

sublevels

beginning with n = 3. To

remember the shapes,

think of “double

dumbells

…and a “dumbell

with a donut”!

(28)
(29)

Energy

Level

(n)

Orbital type

in the

energy level

(types = n)

Number of

orbitals

Number of

Electrons

Number of

electrons per

Energy level

(2n

2

)

1

s

1

2

2

2

s

p

1

3

2

6

8

3

s

p

d

1

3

5

2

6

10

18

4

s

p

d

f

1

3

5

7

2

6

10

14

32

(30)

A. Distribution of Electrons

i. Atoms are electronically neutral.

ii. There is an electron for every proton in the nucleus.

iii. The larger the atom, the larger the electron cloud.

1. Pauli Exclusion Principle: only two e- can occupy the

same orbital due to the opposite electronic spin .

2. Aufbau Principle: an e- occupies the lowest energy

orbital that can receive it.

3. Hund’s Rule: orbital's of equal energy are each occupied

by one e- before any orbital is occupied by a second e-.

All e- in singly occupied orbital's must have same spin.

1s 2s 2p

(31)

Electron Spin

Electron spin

describes the behavior

(direction of spin) of an electron

within a magnetic field.

Possibilities for electron spin:

1

2

1

2

(32)

7

s

2

7

p

6

6

s

2

6

p

6

6

d

10

5

s

2

5

p

6

5

d

10

5

f

14

4

s

2

4

p

6

4

d

10

4

f

14

3

s

2

3

p

6

3

d

10

2

s

2

2

p

6

(33)
(34)

7

s

2

7

p

6

6

s

2

6

p

6

6

d

10

5

s

2

5

p

6

5

d

10

5

f

14

4

s

2

4

p

6

4

d

10

4

f

14

3

s

2

3

p

6

3

d

10

2

s

2

2

p

6

(35)

Element

e- Configuration

notation

Orbital notation

Noble gas

notation

Lithium 1s22s1

____ ____ ____ ____ ____ 1s 2s 2p

[He]2s1

Beryllium 1s22s2

____ ____ ____ ____ ____ 1s 2s 2p

[He]2s2

Boron 1s22s22p1

____ ____ ____ ____ ____ 1s 2s 2p

[He]2s22p1

Carbon 1s22s22p2

____ ____ ____ ____ ____ 1s 2s 2p

[He]2s22p2

Nitrogen 1s22s22p3

____ ____ ____ ____ ____

1s 2s 2p

[He]2s22p3

Oxygen 1s22s22p4

____ ____ ____ ____ ____ 1s 2s 2p

[He]2s22p4

Fluorine 1s22s22p5

____ ____ ____ ____ ____ 1s 2s 2p

[He]2s2p5

Neon 1s22s22p6

____ ____ ____ ____ ____ 1s 2s 2p

(36)

Practice Problems #2

For Elements # 11-36 answer the following

questions

a. Write the e- ConFig (

arrows

)

b. Write the Orbital Notation (

exponents

)

c. Write the Noble Gas Config (

cheater

)

Due the next Class!!!!!

http://www.youtube.com/watch?v=EnHnzpbqE-Y

References

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