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Chemical Ideas 6.1

Light and the electron.

Sometimes we use the wave model for light …

• λ (lambda)= wavelength

Wavelength increases, Frequency ?

decreases

C

c = speed of light = 3.00 x

10 8 m s -1 c = λ ν λ = wavelength m lambda

ν = frequency Hz

( or s -1 ) nu

λ c

ν

c

 

λ  c

υ

  c

Use m for λ

C = λν problems….

c = 3.00x10

8 m s -1

Work out λ:

1. If ν is 3.00 m

2. If ν is 30.0 cm

3. If ν is 3.00 mm

Work out λ:

4. If ν

Sometimes we use the particle

E

 h

 model …  

4 .

5 x 10

14 Hz h = 6.63 x 10 -34 J Hz -1

Planck constant

• Packages of energy are called photons

• Light is a stream of photons

• E = 6.63 x10 -34 x 4.5 x 10 14 = 3.0 x 10 -19 J

h

Rearranging again….

E

E

 h

 

E h

E = h ν problems …

• h = 6.63 x 10-34 J Hz -1

• Planck constant

5. If the frequency is 1.089 x 10 6 Hz, what is the energy of each photon?

6. If E = 3.65 x 10 -20 J per photon, what is the frequency ( ν) of the radiation?

Emission Spectrum of hydrogen.

• Black background

• Coloured lines.

• Prism

Spectroscopy

• Sample of hydrogen

• High voltage

 

E h

ΔE

• Electrons can only exist in fixed energy levels.

• Electrons absorb energy and move to a higher energy level.

• The electrons drop back to a lower energy level and emit energy.

• The frequency of the radiation emitted depends on ΔE.

3  2

4  2

?

7 etc

6

5

4

3

2

1

Why no

• 7  2

• 8  2

• 9  2?

visible ultra violet

E increases

E increasing

Balmer  2

Lyman  ?

1

6

4

3

2

1

4

3

2

1

Absorption Spectrum of hydrogen.

• Continuous spectrum

• Black lines.

How do the 2 compare?

What happens to electrons?

• Electrons absorb energy

• Electrons are excited

• Electrons move to higher energy level

• E = h v

4

3

2

1

Back to the Storyline….

• Particles in the chromosphere absorb some of the light

• Photosphere of hot stars emit visible or

UV light

• Every element has a different absorption spectrum

H

He

Fe

• Have a look at assignment 5

Ionisation energy

X (g)

X

+

(g) + e

-

Ground state electron?

4

3

2

1

Energy needed to remove one e from 1 mole of atoms of a gaseous element

Convergence limit = 3.27 x 10 15 Hz

7. Use ΔE = hν to calculate the energy per photon corresponding to this frequency (in J). h = 6.63 x 10-34 J Hz -1 .

8. Ionisation energy has units of kJ mol -1 . You have calculated the energy required to ionise a single atom. Work out the ionisation energy for hydrogen.

L = 6.02 x 10 23 mol -1 .

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