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Chapter Two …continued

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1 Chapter Two …continued
Electrons in Atoms

2 Bohr’s Model Why don’t the electrons fall into the nucleus?
Move like planets around the sun. Circular orbits at different levels. Amounts of energy separate one level from another.

3 Bohr’s Model Nucleus Electron Orbit Energy Levels

4 } Bohr’s Model Further away from the nucleus means higher energy.
There is no “in between” energy Energy Levels Fifth Fourth Third Increasing energy Second First Nucleus

5 The Quantum Mechanical Model
The atom is found inside a blurry “electron cloud” area where there is a chance of finding an electron.

6 Evidence of Quantum Mechanical Model
The study of light led to the development of the quantum mechanical model. Light is a kind of electromagnetic radiation. Electromagnetic radiation includes many kinds of waves All move at 3.00 x 108 m/s ( c)

7 Parts of a wave Crest Wavelength Amplitude Orgin Trough

8 Parts of Wave Orgin - the base line of the energy.
Crest - high point on a wave Trough - Low point on a wave Amplitude - distance from origin to crest Wavelength - distance from crest to crest abbreviated l (Greek letter lambda).

9 Frequency The number of waves that pass a given point per second. Units are cycles/sec, or hertz (hz) Abbreviated n the Greek letter nu c = ln

10 Frequency and wavelength
Are inversely related As one goes up, the other goes down. Different frequencies of light are different colors of light. Wide variety of frequencies The whole range is called a spectrum

11 Low Energy High Energy Radiowaves Microwaves Infrared . Ultra-violet X-Rays GammaRays Low Frequency High Frequency Long Wavelength Short Wavelength Visible Light

12 How color tells us about atoms
Atomic Spectrum How color tells us about atoms

13 Prism White light is made up of all the colors of the visible spectrum. Passing it through a prism separates it.

14 If the light is not white
By heating a gas with electricity we can get it to give off colors. Passing this light through a prism does something different...

15 Atomic Spectrum Each element gives off its own characteristic colors.
Can be used to identify the atom. Composition of stars.

16 Emission Spectra These are called discontinuous spectra, or line spectra unique to each element. Light is given off, or emitted.

17 Energy and frequency (Honors)
E = hn E is the energy of the photon n is the frequency h is Planck’s constant h = x Joules sec. Joule is the metric unit of Energy

18 Equations for Light Only 2 equations c = ln E = hn Plug and chug.

19 Examples What is the wavelength of blue light with a frequency of 8.3 x 1015 hz? What is the frequency of red light with a wavelength of 4.2 x 10-5 m? What is the energy of a photon of each of the above?

20 An Explanation of Atomic Spectra

21 Where the Electron Starts
The energy level an electron starts from is called its ground state.

22 Changing the energy Let’s look at a hydrogen atom

23 Changing the energy Heat, electricity, or light can move the electron up energy levels

24 Changing the energy As the electron falls back to ground state it gives the energy back as light

25 Changing the energy May fall down in steps
Each with a different energy

26 { { {

27 Ultraviolet Visible Infrared Further they fall, more energy, higher frequency. This is simplified the orbitals also have different energies inside energy levels All the electrons can move around.

28 Heisenberg Uncertainty Principle
It is impossible to know exactly the speed and velocity of a particle. The better we know one, the less we know the other. The act of measuring changes the properties.

29 More obvious with the very small
To measure where a electron is, we use light. But the light moves the electron And hitting the electron changes the frequency of the light.

30 After Before Photon changes wavelength Photon Moving Electron
Electron Changes velocity Moving Electron

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