1 Chapter 5 Section 5.1 Electromagnetic Radiation Section 5.2 Atomic Spectra and Energy Levels
2 Problems with the Rutherford Nuclear Model: Where are the electrons?Why don’t the electrons get pulled into the nucleus?No explanation for spectral lines.*Light behaves as both a wave and a particle.
3 Sometimes light behaves like a wave. Visible light is only a small part of the electromagnetic spectrum.
4 Electromagnetic Spectrum: All the forms of energy that exhibits wavelike behavior as it travels through space.Examples:Gamma rays (short wavelength, high frequency)X-raysUltra violetVisible (from short to long wavelength - Violet,I,B,G,Y,O,Red)InfraredMicrowaveTVRadio (long wavelength, low frequency)Speed of all electromagnetic radiation (light): c = 3.0 x 108m/s)
9 Speed of Light (c): c = λv Speed of light = wavelength x frequency What is the relationship between the wavelength and frequency?Inverse relationship!- the shorter the wavelength the higher the frequency (as λ ↑ , v ↓)- the longer the wavelength the lower the frequency (as λ ↓, v ↑)
10 What is the frequency of a light wave with a wavelength of 106 nm? Solution:1. Convert nm to m:106 nm x (1m/1,000,000,000nm) = 1.06 x 10-7m2. Solve the light equation for v.c = λvv = c / λ= 3.0 x 108 m/s / 1.06 x 10-7m= 2.83 x 1015 Hz
11 Sometimes light behaves like a particle. Photoelectric effect: the emission of electrons from a metal when light shines on the metal.
13 Max PlanckLight energy exists in specific small amounts called quanta (quantum – singular)quantum: the minimum quantity of energy that can be lost or gained by an atom.E = h vPlanck’s constant, h = x J•s
14 Determine the energy in joules of a photon whose frequency is 3 Determine the energy in joules of a photon whose frequency is 3.55 x 1017 Hz.Solution:E = hvE = (6.626 x J•s) (3.55 x 1017 Hz)= 2.35 x J
15 Einstein: Won the Nobel Prize for explanation of photoelectric effect. Einstein explained the photoelectric effect by proposing that electromagnetic radiation is absorbed by matter only in whole numbers of photons.
16 Photon: Massless particle of light with a quantum of energy. The energy of the photon depends on the frequency of radiation. Only certain frequencies are energetic enough to knock electrons off the surface of metals.
17 Flame Test: Metal ions produce characteristic colors in a flame. NaCl SrCl2 BaSO4
18 Line Emission Spectrum: Produced when the light given off by an element is separated into a set of colored lines that are a unique “finger print” of the element.
20 Niels Bohr applied quantum theory to the Rutherford model. Bohr Model of the AtomNiels Bohr applied quantum theory to the Rutherford model.Electrons exist only in definite orbits. Each orbit has a definite fixed energy. Labeled n = 1,2,3,…etc. Lowest energy level is called the ground state, closest to the nucleus.As long as electrons stay in one energy level they don’t gain or lose energy.
21 Bohr Cont.3. Adding energy can put atoms in an excited state, the electrons move to a higher energy level, farther from the nucleus.4. Electrons can “fall” back from higher (excited) to lower energy levels. The difference in energy is released as electromagnetic radiation (light).Explains the color of the lines in the hydrogen spectrum.