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Modern Atomic Theory (a.k.a. the electron chapter!)

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1 Modern Atomic Theory (a.k.a. the electron chapter!)
Chemistry 1: Chapters 5, 6, and 7 Chemistry 1 Honors: Chapter 11 SAVE PAPER AND INK!!! When you print out the notes on PowerPoint, print "Handouts" instead of "Slides" in the print setup. Also, turn off the backgrounds (Tools>Options>Print>UNcheck "Background Printing")!

2 ELECTROMAGNETIC RADIATION

3 Electromagnetic radiation.

4 Electromagnetic Radiation
Most subatomic particles behave as PARTICLES and obey the physics of waves.

5 Electromagnetic Radiation
wavelength Visible light Ultaviolet radiation Amplitude Node

6 Electromagnetic Radiation
Waves have a frequency Use the Greek letter “nu”, , for frequency, and units are “cycles per sec” All radiation:  •  = c where c = velocity of light = 3.00 x 108 m/sec

7 Electromagnetic Spectrum
Long wavelength --> small frequency Short wavelength --> high frequency increasing frequency increasing wavelength

8 Electromagnetic Spectrum
In increasing energy, ROY G BIV

9 Excited Gases & Atomic Structure

10 Atomic Line Emission Spectra and Niels Bohr
Bohr’s greatest contribution to science was in building a simple model of the atom. It was based on an understanding of the LINE EMISSION SPECTRA of excited atoms. Problem is that the model only works for H Niels Bohr ( )

11 Spectrum of White Light

12 Line Emission Spectra of Excited Atoms
Excited atoms emit light of only certain wavelengths The wavelengths of emitted light depend on the element.

13 Spectrum of Excited Hydrogen Gas

14 Line Spectra of Other Elements

15 The Electric Pickle Excited atoms can emit light.
Here the solution in a pickle is excited electrically. The Na+ ions in the pickle juice give off light characteristic of that element.

16 Light Spectrum Lab! Slit that allows light inside Scale
Line up the slit so that it is parallel with the spectrum tube (light bulb) Scale

17 Light Spectrum Lab! Slit that allows light inside Scale Eyepiece
Run electricity through various gases, creating light Look at the light using a spectroscope to separate the light into its component colors Using colored pencils, draw the line spectra (all of the lines) and determine the wavelength of the three brightest lines Once you line up the slit with the light, then look to the scale on the right. You should see the colored lines under the scale. Eyepiece

18 Light Spectrum Lab!

19 An excited lithium atom emitting a photon of red light to drop to a lower energy state.

20 An excited H atom returns to a lower energy level.

21 Atomic Spectra One view of atomic structure in early 20th century was that an electron (e-) traveled about the nucleus in an orbit.

22 Atomic Spectra and Bohr
Bohr said classical view is wrong. Need a new theory — now called QUANTUM or WAVE MECHANICS. e- can only exist in certain discrete orbits e- is restricted to QUANTIZED energy state (quanta = bundles of energy)

23 Quantum or Wave Mechanics
Schrodinger applied idea of e- behaving as a wave to the problem of electrons in atoms. He developed the WAVE EQUATION Solution gives set of math expressions called WAVE FUNCTIONS,  Each describes an allowed energy state of an e- E. Schrodinger

24 Heisenberg Uncertainty Principle
Problem of defining nature of electrons in atoms solved by W. Heisenberg. Cannot simultaneously define the position and momentum (= m•v) of an electron. We define e- energy exactly but accept limitation that we do not know exact position. W. Heisenberg

25 Arrangement of Electrons in Atoms
Electrons in atoms are arranged as LEVELS (n) SUBLEVELS (l) ORBITALS (ml)

26 QUANTUM NUMBERS n (principal) ---> energy level
The shape, size, and energy of each orbital is a function of 3 quantum numbers which describe the location of an electron within an atom or ion n (principal) ---> energy level l (orbital) ---> shape of orbital ml (magnetic) ---> designates a particular suborbital The fourth quantum number is not derived from the wave function s (spin) ---> spin of the electron (clockwise or counterclockwise: ½ or – ½)

27 QUANTUM NUMBERS So… if two electrons are in the same place at the same time, they must be repelling, so at least the spin quantum number is different! The Pauli Exclusion Principle says that no two electrons within an atom (or ion) can have the same four quantum numbers. If two electrons are in the same energy level, the same sublevel, and the same orbital, they must repel. Think of the 4 quantum numbers as the address of an electron… Country > State > City > Street

28 Energy Levels Each energy level has a number called the PRINCIPAL QUANTUM NUMBER, n Currently n can be 1 thru 7, because there are 7 periods on the periodic table

29 Energy Levels n = 1 n = 2 n = 3 n = 4

30 Relative sizes of the spherical 1s, 2s, and 3s orbitals of hydrogen.

31 Types of Orbitals The most probable area to find these electrons takes on a shape So far, we have 4 shapes. They are named s, p, d, and f. No more than 2 e- assigned to an orbital – one spins clockwise, one spins counterclockwise

32 Types of Orbitals (l) s orbital p orbital d orbital

33 p Orbitals this is a p sublevel with 3 orbitals These are called x, y, and z There is a PLANAR NODE thru the nucleus, which is an area of zero probability of finding an electron 3py orbital

34 p Orbitals The three p orbitals lie 90o apart in space

35 d Orbitals d sublevel has 5 orbitals

36 The shapes and labels of the five 3d orbitals.

37 f Orbitals For l = 3, ---> f sublevel with 7 orbitals

38 Diagonal Rule The diagonal rule is a memory device that helps you remember the order of the filling of the orbitals from lowest energy to highest energy

39 Diagonal Rule 1 2 3 4 5 6 7 s s 2p s 3p 3d s 4p 4d 4f s 5p 5d 5f 5g?
Steps: Write the energy levels top to bottom. Write the orbitals in s, p, d, f order. Write the same number of orbitals as the energy level. Draw diagonal lines from the top right to the bottom left. To get the correct order, follow the arrows! 1 2 3 4 5 6 7 s s 2p s 3p 3d s 4p 4d 4f By this point, we are past the current periodic table so we can stop. s 5p 5d 5f 5g? s 6p 6d 6f 6g? 6h? s 7p 7d 7f 7g? 7h? 7i?

40 Why are d and f orbitals always in lower energy levels?
d and f orbitals require LARGE amounts of energy It’s better (lower in energy) to skip a sublevel that requires a large amount of energy (d and f orbtials) for one in a higher level but lower energy This is the reason for the diagonal rule! BE SURE TO FOLLOW THE ARROWS IN ORDER!

41 Periodic Patterns s p d (n-1) f (n-2) 1 2 3 4 5 6 7 6 7 1s 2s 3s 4s 5s

42 How many electrons can be in a sublevel?
Remember: A maximum of two electrons can be placed in an orbital. s orbitals p orbitals d orbitals f orbitals Number of orbitals Number of electrons

43 Sublevels 4f 4d 4p 4s n = 4 3d 3p 3s n = 3 Energy 2p 2s n = 2 1s n = 1
The energy of an electron is determined by its average distance from the nucleus. Each atomic orbital with a given set of quantum numbers has a particular energy associated with it, the orbital energy. In atoms or ions that contain only a single electron, all orbitals with the same value of n have the same energy (they are degenerate). Energies of the principal shells increase smoothly as n increases. An atom or ion with the electron(s) in the lowest-energy orbital(s) is said to be in the ground state; an atom or ion in which one or more electrons occupy higher-energy orbitals is said to be in the excited state. 3s 3p 2p 2s n = 2 3s 2p 2s 2p 2s 1s 1s 1s n = 1

44 Electron capacities Electron capacities
Copyright © 2006 Pearson Benjamin Cummings. All rights reserved.

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51 Electron capacities Copyright © 2006 Pearson Benjamin Cummings. All rights reserved.

52 Atoms don’t really look like this.
32 18 8 2 Atoms don’t really look like this. We know that the model is incorrect but it is good enough to help us understand important concepts. Copyright © 2007 Pearson Benjamin Cummings. All rights reserved.

53 Copyright © 2007 Pearson Benjamin Cummings. All rights reserved.

54 Sublevels 1s22s22p63s23p64s23d104p65s24d10… 4f 4d 4p 4s n = 4 3d 3p 3s
Energy 1s22s22p63s23p64s23d104p65s24d10… Electron configuration of an element is the arrangement of its electrons in its atomic orbitals One can obtain and explain a great deal of the chemistry of the element by knowing its electron configuration 2p 2s n = 2 1s n = 1

55 Electron Configurations
A list of all the electrons in an atom (or ion) Must go in order (Aufbau principle) 2 electrons per orbital, maximum We need electron configurations so that we can determine the number of electrons in the outermost energy level. These are called valence electrons. The number of valence electrons determines how many and what this atom (or ion) can bond to in order to make a molecule 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10 5p6 6s2 4f14… etc.

56 Electron Configurations
2p4 Number of electrons in the sublevel Energy Level Sublevel 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10 5p6 6s2 4f14… etc.

57 Periodic Patterns s p d (n-1) f (n-2) 1 2 3 4 5 6 7 6 7 1s 2s 3s 4s 5s

58 Order in which subshells are filled with electrons
2p 3p 4p 5p 6p 3d 4d 5d 6d 4f 5f 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d …

59 Sublevels 4f 4d 4p 4s n = 4 3d 3p 3s n = 3 Energy 2p 2s n = 2 1s n = 1
The energy of an electron is determined by its average distance from the nucleus. Each atomic orbital with a given set of quantum numbers has a particular energy associated with it, the orbital energy. In atoms or ions that contain only a single electron, all orbitals with the same value of n have the same energy (they are degenerate). Energies of the principal shells increase smoothly as n increases. An atom or ion with the electron(s) in the lowest-energy orbital(s) is said to be in the ground state; an atom or ion in which one or more electrons occupy higher-energy orbitals is said to be in the excited state. 3s 3p 2p 2s n = 2 3s 2p 2s 2p 2s 1s 1s 1s n = 1

60 Let’s Try It! Write the electron configuration for the following elements: H Li N Ne K Zn Pb

61 Orbitals and the Periodic Table
Orbitals grouped in s, p, d, and f orbitals (sharp, proximal, diffuse, and fundamental) s orbitals d orbitals p orbitals f orbitals

62 Shorthand Notation A way of abbreviating long electron configurations
Since we are only concerned about the outermost electrons, we can skip to places we know are completely full (noble gases), and then finish the configuration

63 Shorthand Notation Step 1: It’s the Showcase Showdown!
Find the closest noble gas to the atom (or ion), WITHOUT GOING OVER the number of electrons in the atom (or ion). Write the noble gas in brackets [ ]. Step 2: Find where to resume by finding the next energy level. Step 3: Resume the configuration until it’s finished.

64 Shorthand Configuration
neon's electron configuration (1s22s22p6) B third energy level [Ne] 3s1 one electron in the s orbital C D orbital shape Valence electrons – Tedious to keep copying the configurations of the filled inner subshells – Simplify the notation by using a bracketed noble gas symbol to represent the configuration of the noble gas from the preceding row – Example: [Ne] represents the 1s22s22p6 electron configuration of neon (Z = 10) so the electron configuration of sodium (Z = 11), which is 1s22s22p63s1, is written as [Ne]3s1 – Electrons in filled inner orbitals are closer and are more tightly bound to the nucleus and are rarely involved in chemical reactions Na = [1s22s22p6] 3s1 electron configuration

65 Practice Shorthand Notation
Write the shorthand notation for each of the following atoms: Cl K Ca I Bi

66 Valence Electrons Electrons are divided between core and valence electrons B 1s2 2s2 2p1 Core = [He] , valence = 2s2 2p1 Br [Ar] 3d10 4s2 4p5 Core = [Ar] 3d10 , valence = 4s2 4p5

67 Rules of the Game No. of valence electrons of a main group atom = Group number (for A groups) Atoms like to either empty or fill their outermost level. Since the outer level contains two s electrons and six p electrons (d & f are always in lower levels), the optimum number of electrons is eight. This is called the octet rule.

68 Keep an Eye On Those Ions!
Electrons are lost or gained like they always are with ions… negative ions have gained electrons, positive ions have lost electrons The electrons that are lost or gained should be added/removed from the highest energy level (not the highest orbital in energy!)

69 Keep an Eye On Those Ions!
Tin Atom: [Kr] 5s2 4d10 5p2 Sn+4 ion: [Kr] 4d10 Sn+2 ion: [Kr] 5s2 4d10 Note that the electrons came out of the highest energy level, not the highest energy orbital!

70 Keep an Eye On Those Ions!
Bromine Atom: [Ar] 4s2 3d10 4p5 Br- ion: [Ar] 4s2 3d10 4p6 Note that the electrons went into the highest energy level, not the highest energy orbital!

71 Try Some Ions! Write the longhand notation for these: F- Li+ Mg+2
Write the shorthand notation for these: Br- Ba+2 Al+3

72 General Rules Aufbau Principle
Electrons fill the lowest energy orbitals first. “Lazy Tenant Rule” 6d 5f 7s 6d 5f 6p 7s 5d 4f 6p 6s 5d 5p 4f 6s 4d 5s 5p 4d 4p 5s 3d 4s 4p 3d 3p 4s Energy 3p 3s 3s 2p 2s 2p 2s 1s 1s

73 Exceptions to the Aufbau Principle
Remember d and f orbitals require LARGE amounts of energy If we can’t fill these sublevels, then the next best thing is to be HALF full (one electron in each orbital in the sublevel) There are many exceptions, but the most common ones are d4 and d9 For the purposes of this class, we are going to assume that ALL atoms (or ions) that end in d4 or d9 are exceptions to the rule. This may or may not be true, it just depends on the atom.

74 Exceptions to the Aufbau Principle
(HONORS only) Exceptions to the Aufbau Principle d4 is one electron short of being HALF full In order to become more stable (require less energy), one of the closest s electrons will actually go into the d, making it d5 instead of d4. For example: Cr would be [Ar] 4s2 3d4, but since this ends exactly with a d4 it is an exception to the rule. Thus, Cr should be [Ar] 4s1 3d5. Procedure: Find the closest s orbital. Steal one electron from it, and add it to the d.

75 Exceptions to the Aufbau Principle
(HONORS only) Exceptions to the Aufbau Principle OK, so this helps the d, but what about the poor s orbital that loses an electron? Remember, half full is good… and when an s loses 1, it too becomes half full! So… having the s half full and the d half full is usually lower in energy than having the s full and the d to have one empty orbital.

76 Exceptions to the Aufbau Principle
d9 is one electron short of being full Just like d4, one of the closest s electrons will go into the d, this time making it d10 instead of d9. For example: Au would be [Xe] 6s2 4f14 5d9, but since this ends exactly with a d9 it is an exception to the rule. Thus, Au should be [Xe] 6s1 4f14 5d10. Procedure: Same as before! Find the closest s orbital. Steal one electron from it, and add it to the d.

77 Write the shorthand notation for: Cu W Au
(HONORS only) Try These! Write the shorthand notation for: Cu W Au

78 General Rules Pauli Exclusion Principle
Each orbital can hold TWO electrons with opposite spins. Wolfgang Pauli

79 Electron aligned against
Spin Quantum Number, ms North South S N - Electron aligned with magnetic field, ms = + ½ Electron aligned against magnetic field, ms = - ½ The electron behaves as if it were spinning about an axis through its center. This electron spin generates a magnetic field, the direction of which depends on the direction of the spin.

80 Orbital Diagrams Graphical representation of an electron configuration
One arrow represents one electron Shows spin and which orbital within a sublevel Same rules as before (Aufbau principle, d4 and d9 exceptions, two electrons in each orbital, etc. etc.)

81 WRONG RIGHT General Rules Hund’s Rule
Within a sublevel, place one electron per orbital before pairing them. “Empty Bus Seat Rule” WRONG RIGHT

82 Orbital Diagrams One additional rule: Hund’s Rule
In orbitals of EQUAL ENERGY (p, d, and f), place one electron in each orbital before making any pairs All single electrons must spin the same way I nickname this rule the “Monopoly Rule” In Monopoly, you have to build houses EVENLY. You can not put 2 houses on a property until all the properties have at least 1 house.

83 H He Li C N Al Ar F Fe La Energy Level Diagram Bohr Model
6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N 2s p 1s Electron Configuration NUCLEUS H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

84 Hydrogen H = 1s1 H He Li C N Al Ar F Fe La Energy Level Diagram
6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N 2s p 1s Electron Configuration NUCLEUS H = 1s1 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

85 Helium He = 1s2 H He Li C N Al Ar F Fe La Energy Level Diagram
6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N 2s p 1s Electron Configuration NUCLEUS He = 1s2 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

86 Lithium Group 1A Atomic number = 3 1s22s1 ---> 3 total electrons

87 Carbon Group 4A Atomic number = 6 1s2 2s2 2p2 --->
6 total electrons Here we see for the first time HUND’S RULE. When placing electrons in a set of orbitals having the same energy, we place them singly as long as possible.

88 Nitrogen N = 1s22s22p3 H He Li C N Al Ar F Fe La Energy Level Diagram
6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N Hund’s Rule “maximum number of unpaired orbitals”. 2s p 1s Electron Configuration NUCLEUS N = 1s22s22p3 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

89 Fluorine F = 1s22s22p5 H He Li C N Al Ar F Fe La Energy Level Diagram
6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N 2s p 1s Electron Configuration NUCLEUS F = 1s22s22p5 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

90 Aluminum Al = 1s22s22p63s23p1 H He Li C N Al Ar F Fe La
Energy Level Diagram Aluminum 6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N 2s p 1s Electron Configuration NUCLEUS Al = 1s22s22p63s23p1 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

91 Argon Ar = 1s22s22p63s23p6 H He Li C N Al Ar F Fe La
Energy Level Diagram Argon 6s p d f Bohr Model 5s p d 4s p d Arbitrary Energy Scale 3s p N 2s p 1s Electron Configuration NUCLEUS Ar = 1s22s22p63s23p6 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

92 Iron H He Li C N Al Ar F Fe La Energy Level Diagram Bohr Model
6s p d f Bohr Model 5s p d N 4s p d Arbitrary Energy Scale 3s p 2s p 1s Electron Configuration NUCLEUS Fe = 1s22s22p63s23p64s23d6 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

93 Lanthanum H He Li C N Al Ar F Fe La Energy Level Diagram Bohr Model
6s p d f Bohr Model 5s p d N 4s p d Arbitrary Energy Scale 3s p 2s p 1s Electron Configuration NUCLEUS La = 1s22s22p63s23p64s23d10 4s23d104p65s24d105p66s25d1 H He Li C N Al Ar F Fe La CLICK ON ELEMENT TO FILL IN CHARTS

94 Lanthanide Element Configurations
4f orbitals used for Ce - Lu and 5f for Th - Lr

95 Draw these orbital diagrams!
Oxygen (O) Chromium (Cr) Mercury (Hg)

96 Ion Configurations To form anions from elements, add 1 or more e- from the highest sublevel. P [Ne] 3s2 3p3 + 3e- ---> P3- [Ne] 3s2 3p6 or [Ar]

97 The End !!!!!!!!!!!!!!!!!!!


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