…and, in conclusion…

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…and, in conclusion…

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…and, in conclusion…. You will need to know the contributions of…. Bohr Planck Einstein Heisenberg de Broglie. Q: How is light produced?. Q: How is light produced?. A: An excited electron…. Q: How is light produced?. A: An excited electron… loses energy…. - PowerPoint PPT Presentation

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Page 1: …and, in conclusion…

…and, in conclusion…

Page 2: …and, in conclusion…

You will need to know the contributions of…

• Bohr

• Planck

• Einstein

• Heisenberg

• de Broglie

Page 3: …and, in conclusion…

Q: How is light produced?

Page 4: …and, in conclusion…

Q: How is light produced?

• A: An excited electron…

Page 5: …and, in conclusion…

Q: How is light produced?

• A: An excited electron…

• loses energy…

Page 6: …and, in conclusion…

Q: How is light produced?

• A: An excited electron…

• loses energy…

• as it falls…

Page 7: …and, in conclusion…

Q: How is light produced?

• A: An excited electron…

• loses energy…

• as it falls…

• from a higher to a lower energy level,…

Page 8: …and, in conclusion…

Q: How is light produced?

• A: An excited electron…

• loses energy…

• as it falls…

• from a higher to a lower energy level,…

• emitting that energy…

Page 9: …and, in conclusion…

Q: How is light produced?

• A: An excited electron…

• loses energy…

• as it falls…

• from a higher to a lower energy level,…

• emitting that energy…

• as a photon of light

Page 10: …and, in conclusion…

An electron that gains energy is excited:

moves to a higher energy level,

physically moves away from nucleus

An electron in its normal position is in its ground state

*

(gains energy)

Ground state

Excited *

Page 11: …and, in conclusion…

• Light is produced*

As it loses energy

Ground state

Excited *

Page 12: …and, in conclusion…

We use a * to mark an excited electron or atom.

• An atom can be excited by:

Page 13: …and, in conclusion…

We use a * to mark an excited electron or atom.

• An atom can be excited by:

Heat (light bulbs, stars, sparks, flames)

Electricity (sparks, fluorescent bulbs) or

Chem. rxns (lightning bugs, glow sticks)

Page 14: …and, in conclusion…

Let’s do the wave.

Page 15: …and, in conclusion…

The wave equation

Where

c is the speed of light, 3.00 x 108 m/s

is the wavelength (the symbol, lambda, is the Greek “l” for length) and

is the frequency (the symbol, nu, is the Greek “n”)

c=

Page 16: …and, in conclusion…

Please notice:

• Wavelength and frequency are inversely related.

• When wavelength increases, frequency decreases.

Page 17: …and, in conclusion…

• Q: What is the frequency of light that has a wavelength of 570 nm(5.7x10-7m)?

Page 18: …and, in conclusion…

• Q: What is the frequency of light that has a wavelength of 570 nm(5.7x10-7m)?

• c=

Page 19: …and, in conclusion…

• Q: What is the frequency of light that has a wavelength of 570 nm(5.7x10-7m)?

• c==c/

Page 20: …and, in conclusion…

• Q: What is the frequency of light that has a wavelength of 570 nm(5.7x10-7m)?

• c==c/=(3.00x108m/s) / (5.7x10-7m)

Page 21: …and, in conclusion…

• Q: What is the frequency of light that has a wavelength of 570 nm(5.7x10-7m)?

• c==c/=(3.00x108m/s) / (5.7x10-7m)

• 5.3 x 1014 /s =5.3 x 1014 Hz

Page 22: …and, in conclusion…

Next: Planck’s equation

• The energy of a photon is directly related to its frequency

E=h• where

• E is the energy (in Joules),

• is the frequency (in waves/s, or Hz), and

• h is the conversion factor, Planck’s constant.

h=6.63 x 10-34 Js

Page 23: …and, in conclusion…

The electromagnetic spectrum

Page 24: …and, in conclusion…

For any pair--

Which has greater , , E, v?

Page 25: …and, in conclusion…

The electromagnetic spectrumIncreasing wavelength

Increasing frequency

Increasing energy

and, c is the velocity of light (c for constant!)

Page 26: …and, in conclusion…

Visible light400 nm

700 nm

Short wavelength High energy High frequency

Long wavelength Low energy Low frequency

Page 27: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

450 nm

93.3 MHz

353 m

9.47 x 10-21 J

4.03 x 10-19 J

Page 28: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

3.00 x 108 m/s

450 nm 6.67 x 1014 Hz

4.42 x 10-19 J

93.3 MHz

353 m

9.47 x 10-21 J

4.03 x 10-19 J

Page 29: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

3.00 x 108 m/s

450 nm 6.67 x 1014 Hz

4.42 x 10-19 J

3.00 x 108 m/s

3.22 m 93.3 MHz 6.19 x 10-26 J

353 m

9.47 x 10-21 J

4.03 x 10-19 J

Page 30: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

3.00 x 108 m/s

450 nm 6.67 x 1014 Hz

4.42 x 10-19 J

3.00 x 108 m/s

3.22 m 93.3 MHz 6.19 x 10-26 J

3.00 x 108 m/s

353 m 8.50 x 105 Hz

5.63 x 10-28 J

9.47 x 10-21 J

4.03 x 10-19 J

Page 31: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

3.00 x 108 m/s

450 nm 6.67 x 1014 Hz

4.42 x 10-19 J

3.00 x 108 m/s

3.22 m 93.3 MHz 6.19 x 10-26 J

3.00 x 108 m/s

353 m 8.50 x 105 Hz

5.63 x 10-28 J

3.00 x 108 m/s

2.10 x 10-5 m

1.43 x 1013 Hz

9.47 x 10-21 J

4.03 x 10-19 J

Page 32: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

3.00 x 108 m/s

450 nm 6.67 x 1014 Hz

4.42 x 10-19 J

3.00 x 108 m/s

3.22 m 93.3 MHz 6.19 x 10-26 J

3.00 x 108 m/s

353 m 8.50 x 105 Hz

5.63 x 10-28 J

3.00 x 108 m/s

2.10 x 10-5 m

1.43 x 1013 Hz

9.47 x 10-21 J

3.00 x 108 m/s

4.94 x 10-7 m

6.08 x 1014 Hz

4.03 x 10-19 J

Page 33: …and, in conclusion…

Fill in the missing information

Type of photon

c=

3x108m/s

(m) (s-1) E (per photon)

Blue or indigo light

3.00 x 108 m/s

450 nm 6.67 x 1014 Hz

4.42 x 10-19 J

FM radio 3.00 x 108 m/s

3.22 m 93.3 MHz 6.19 x 10-26 J

AM radio 3.00 x 108 m/s

353 m 8.50 x 105 Hz

5.63 x 10-28 J

IR 3.00 x 108 m/s

2.10 x 10-5 m

1.43 x 1013 Hz

9.47 x 10-21 J

Blue or Green light

3.00 x 108 m/s

4.94 x 10-7 m

6.08 x 1014 Hz

4.03 x 10-19 J

Page 34: …and, in conclusion…

The Bohr Model of the atom• Bohr’s solar system model

-- shows why the H gives off only 4 wavelengths of visible light.

• He calculated the energy that the electrons did give off, and the differences in energy.

Page 35: …and, in conclusion…

Bohr drew a picture like this

Electron loses energy

Electron gains energy

Page 36: …and, in conclusion…

• These 4. No more. There is nothing between the levels– no “half-transitions”

Visible wavelengths produced by

hydrogen atoms

Page 37: …and, in conclusion…

In the hydrogen spectrum

• The wavelengths are:– 410 nm (violet)– 434 nm (blue)– 486 nm (green)– 656 nm (red)

Page 38: …and, in conclusion…

4.85x10-19J

4.58x10-19J

4.09x10-19 J

3.03x10-19J

In the hydrogen spectrum

Page 39: …and, in conclusion…

4.85x10-19J

4.58x10-19J

4.09x10-19 J

3.03x10-19J

In the hydrogen spectrum

What is the energy difference between these two levels?

Page 40: …and, in conclusion…

4.85x10-19J

4.58x10-19J

4.09x10-19 J

3.03x10-19J

In the hydrogen spectrum

What is the energy difference between these two levels?

.49 x 10-19 J

Page 41: …and, in conclusion…

• These energies represent the differences in the energy levels…

…and that’s how we know where the energy levels are.

Page 42: …and, in conclusion…

Other phenomena that teach us about electrons and light

The photoelectric effect

– Described by Einstein for his Nobel prize– Light knocks electrons off a metal– Indicates the particle nature of

light

One photon excites one electron

Page 43: …and, in conclusion…

Other phenomena that teach us about electrons and light

• Heisenberg’s Uncertainty Principle

– “You cannot determine both the location and momentum of a particle exactly.”

– If you measure one, you change the other unpredictably

– Leads to the wave and particle natures of everything

Page 44: …and, in conclusion…

Gratuitous joke

Heisenberg was pulled over on the highway. The officer asks,

“Do you know how fast you were going?”

Heisenberg replies,

Page 45: …and, in conclusion…

Gratuitous joke

Heisenberg was pulled over on the highway. The officer asks,

“Do you know how fast you were going?”

Heisenberg replies,

“No, but I do know where I am!”

Page 46: …and, in conclusion…

Other phenomena that teach us about electrons and light

• DeBroglie’s wavelength

– Describes the wave nature of particles– Considers the uncertainty in position as a

wavelength

Page 47: …and, in conclusion…

Electron Configurations

…and now, the rest of the story

Page 48: …and, in conclusion…

Fe (2,8,14,2)

• --An electron configuration (EC) shows the location of all electrons in an atom or ion.

• --In an atom, number of electrons = number of protons = atomic number

• --Electrons are found around the nucleus of an atom in specific energy levels.

Page 49: …and, in conclusion…

Levels have sublevels!

Page 50: …and, in conclusion…

Levels have sublevels!

Sublevels have orbitals!

Page 51: …and, in conclusion…

1st energy level

• -has one sublevel, 1s

• -An s sublevel (spherical) has one orbital,

• -An orbital can hold two electronsZ

XY

Page 52: …and, in conclusion…

• So the electron configuration of hydrogen and helium are more properly written

• 1H 1s1

• 2He 1s2

Page 53: …and, in conclusion…

• 1H 1s1

• 2He 1s2

• The 1 refers to the energy level

Page 54: …and, in conclusion…

• 1H 1s1

• 2He 1s2

• The s refers to the sublevel

Page 55: …and, in conclusion…

• 1H 1s1

• 2He 1s2

• The superscripts are the number of electrons in this sublevel.

Page 56: …and, in conclusion…

2nd energy level

• -has 2s (bigger, still spherical) and 2p (has 3 bi-lobed orbitals in x, y, and z directions)

• -holds up to 8 electrons total

(2 in the s and 3 x 2 in the p)

Z

XY

Z

XY

Z

XY

Page 57: …and, in conclusion…

• 3Li 1s22s1

• 4Be 1s22s2

• 5B 1s22s22p1

• 6C 1s22s22p2

• 7N 1s22s22p3 …

Page 58: …and, in conclusion…

Third energy level

has three sublevels, 3s, 3p, and 3d.

The 3s and 3p sublevels are similar in structure (but bigger) than the s and p sublevels seen before.

Page 59: …and, in conclusion…

The 3d sublevel

• (and any d) has five orbitals of varying shapes.

• These orbitals can hold two electrons each for a total of ten electrons.

• The 3d sublevel is the highest energy sublevel of energy level 3, so high, in fact, that energy level 4 begins to fill (the 4s sublevel fills) before the 3d sublevel

Page 60: …and, in conclusion…

See text

Z

XY

Z

XY

Z

XY

Z

XY

Z

XY

Page 61: …and, in conclusion…

See handout

The fourth energy level has four sublevels (notice the trend?) They are called 4s, 4p, 4d, and 4f. The s, p, and d sublevels are structured as before.

Page 62: …and, in conclusion…

See handout

The f sublevel has seven orbitals, and can hold up to fourteen electrons.

The 5s sublevel is filled before the 4d, and the 5p and 6s sublevels precede the 4f.

Let’s look at a picture instead

Page 63: …and, in conclusion…

You must remember this…

• s=1 orbital, 2 electrons

• p=3 orbitals, 6 electrons

• d=5 orbitals, 10 electrons

• f=7 orbitals, 14 electrons

Page 64: …and, in conclusion…

The Aufbau diagram

This structure is shown below. Boxes are orbitals, each can hold two electrons

1s

2s

3s

4s

5s

6s

7s

7p

6p

5p

4p

3p

2p

3d

4d

5d

6d 5f

4f

Page 65: …and, in conclusion…

1s

2s

3s

4s

5s

6s

7s

7p

6p

5p

4p

3p

2p

3d

4d

5d

6d 5f

4f

Page 66: …and, in conclusion…

Rules, rules, rules.

• Orbitals are filled according to three rules:– Aufbau (building up) principle—lower energy

sublevels are filled first– Pauli exclusion principle—electrons sharing

an orbital must have opposite spins– Hund’s Rule—when a sublevel has several

orbitals, electrons will distribute to separate orbitals with parallel spins, before sharing orbitals with opposite spins

Page 67: …and, in conclusion…

1s

2s

3s

4s

5s

6s

7s

7p

6p

5p

4p

3p

2p

3d

4d

5d

6d 5f

4f

Page 68: …and, in conclusion…

Levels have sublevels

• All Electron configurations are some subset of the order shown below. Only the last sublevel might be incomplete

• 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10

5p6 6s2 4f14 5d10 6p6 7s2 5f14 6d10 7p6…

Page 69: …and, in conclusion…

Watch out for two things

1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10 5p6 6s2 4f14 5d10 6p6 7s2 5f14 6d10 7p6 … gets old.

Ex:

87Fr 1s2 2s2 2p6 3s2 3p6 4s2 3d10 4p6 5s2 4d10 5p6 6s2 4f14 5d10 6p6 7s1

87Fr [Rn] 7s1

(Radon is a noble gas, and accounts for the first 86 electrons)

Look for the last octet and use a noble gas core

Page 70: …and, in conclusion…

• Practice:

• Write the full EC for Titanium (element 22) and write the EC with a noble gas core

Page 71: …and, in conclusion…

• Practice:

• Write the full EC for Titanium (element 22) and write the EC with a noble gas core

• A) Ti 1s2 2s2 2p6 3s2 3p6 4s2 3d2

• and Ti [Ar] 4s2 3d2

Page 72: …and, in conclusion…

…and watch out for Cu and Cr!• Chromium, copper and a few others

rearrange electrons to become more stable.

• Sublevel energies go down when a sublevel is full or half full.

• Cr 1s2 2s2 2p6 3s2 3p6 4s2 3d4 becomes• Cr 1s2 2s2 2p6 3s2 3p6 4s1 3d5 and

• Cu 1s2 2s2 2p6 3s2 3p6 4s2 3d9 becomes• Cu 1s2 2s2 2p6 3s2 3p6 4s1 3d10

Page 73: …and, in conclusion…

Problems:

1. Write the electron configurations for phosphorus and molybdenum. Then draw the aufbau diagrams for these elements.

2. Write the complete electron configurations for magnesium, sulfur, and potassium. Then write their electron configurations using the symbols for the noble gases.

3. What element is represented by [Ne]3s23p6?

4. Determine the electron configuration for the last SUBLEVEL of the following elements: S, Pt, Sr, K, and Al.

Page 74: …and, in conclusion…

5. The an unknown element has an electron configuration of 1s22s22p63s23p4.

A. What is the element?

B. What does the superscript 6 refer to?

C. What does the letter s refer to?

D. What does the coefficient 3 refer to?

6. Write the electron configuration for calcium, a nutrient essential to healthy bone growth and development.

7. Write the electron configuration for copper, which is used in pennies.

Page 75: …and, in conclusion…

8. Use the symbols for the noble gases to write the electron configurations for the following elements:

A. Zr B. U C. Rn

9. Write the electron configuration and draw the orbital diagrams for the following elements:

A. Carbon B. Silver C. Aluminum

Page 76: …and, in conclusion…

VOCABULARY

• Electron configuration• Atomic number• Energy level• Valence level• Sublevel• s,p,d,f• Orbital• Spin

• Proton• Electron• Spherical• Two-lobed• Dumbell-shaped• Aufbau principle• Pauli’s exclusion

principle• Hund’s rule

Page 77: …and, in conclusion…

Be able to:

• Describe the levels, sublevels, and orbitals.• Recreate the aufbau order from the periodic

chart• Write a complete EC and EC with a noble gas

core for any element• Determine the last sublevel, and number of

electrons there from a position on a periodic chart

• Identify a position on the chart and the element from an EC

• Fill out an aufbau diagram for any element

Page 78: …and, in conclusion…

Trends in the Periodic Chart

…since the position on the chart indicates electrons, and electrons are responsible for physical and chemical

properties…

Page 79: …and, in conclusion…

• …the position on the periodic chart indicates the physical and chemical properties of elements!

• Opposite charges attract– electrons are attracted by the protons in the nucleus

Page 80: …and, in conclusion…

Simple

• Valence electrons

– The representative (tall) columns represent the number of valence electrons

– Transition elements have only two valence electrons, but have a part-filled d sublevel

Page 81: …and, in conclusion…
Page 82: …and, in conclusion…

Simple

• Ionization pattern

• Metals

- have only a few valence electrons

-lose these electrons, empty their valence level

-form positive ions

Page 83: …and, in conclusion…

Simple

• Ionization pattern

• Non-metals have

-more valence electrons

-gain electrons to fill valence level

-form negative ions

Page 84: …and, in conclusion…
Page 85: …and, in conclusion…

Medium

• Atomic size

• In a column, a lower row indicates an extra energy level

• Outer energy levels are larger

• The largest atom in a column is the bottom element

Page 86: …and, in conclusion…

Medium

• Ionization energy —the energy required to remove an electron

X + IE X+ + e-

• Outer energy levels are farther from the nucleus• It is easier to remove an electron from a larger

energy level• The lowest ionization energy is at the bottom of the

column

Page 87: …and, in conclusion…

Medium

• Electronegativity —the attraction an atom has for a shared pair of electrons

• See IE—the highest electronegativity is at the top

Page 88: …and, in conclusion…

Medium

• Electron affinity —attraction an atom has for an electron from the outside

X + e- X- + EA

• See e-neg—the highest electron affinity is at the top

Page 89: …and, in conclusion…

One moment…

As you go across a row, you get more protons in the nucleus

• They attract the electrons better

• Each energy level gets smaller

Page 90: …and, in conclusion…

Hard

• Atoms get smaller as you go across a row

• Ionization energy gets larger

• Electronegativity gets larger

• Electron affinity gets larger

--All because there are more protons--

Page 91: …and, in conclusion…

Recap

• Atomic size

• INCREASES as you go down

and left

Page 92: …and, in conclusion…

Recap

• Electronegativity, ionization energy, and electron affinity

• INCREASE as you go up

and right

Page 93: …and, in conclusion…

Pop Quiz

• Which element on the entire periodic chart is the largest?

• Smallest?

• Which element on the entire periodic chart has the largest IE?

• Smallest?

Page 94: …and, in conclusion…

Pop Quiz

• Which element on the entire periodic chart has the largest e-negativity?

• Smallest?

• Which element on the entire periodic chart has the largest EA?

• Smallest?

Page 95: …and, in conclusion…

Pop Quiz

• Who’s your favorite pop star?

Page 96: …and, in conclusion…

• Which has the greatest / least: Size, IE, EA, e-neg?

C

Sn I

F

Page 97: …and, in conclusion…

The diagonal effect

• Of the previous four elements, the ones in the same row and column are easy, right?

• What can you say about carbon and iodine?

• They might be just about the same!

Page 98: …and, in conclusion…

The metal/nonmetal line

Diagonal effect!

(due to electronegativity or EA)

Page 99: …and, in conclusion…

Hard (cont’d)

• Ionic radius

Negative ions are (way!) larger than their atom

Positive ions are (way!) smaller than their atom

Page 100: …and, in conclusion…

• Which has the largest / smallest ion?

Li

K Ca

Be

Page 101: …and, in conclusion…

• Which has the largest / smallest ion?

S

Te I

Cl

Page 102: …and, in conclusion…

• Which has the smallest / largest ion?

Mg

Sr Te

S

Page 103: …and, in conclusion…

• Which has the smallest / largest ion?

+2 -2

+2 -2

Mg

Sr Te

S

Page 104: …and, in conclusion…

Hard (cont’d)

• Second and third ionizations

• If you ionize an atom, you make a (+) ion

• It’s harder to ionize it again

• It gets way harder after you empty the valence level

Page 105: …and, in conclusion…

Hard (cont’d)

• First, second, and third ionization energies

X + IEX+1 + e-

X+1 + IE2X+2 + e-

X+2 + IE3X+3 + e-

Page 106: …and, in conclusion…

Shielding

• Shielding –weakening of attraction due to electrons interfering with attraction of the nucleus

• Shielding increases a little as you go across a period (not as much as attraction)

• Shielding jumps tremendously as you start a new energy level

Page 107: …and, in conclusion…

Remem-mem-mem…

• Ionic radius

Negative ions are (way!) larger than their atom

Positive ions are (way!) smaller than their atom

Page 108: …and, in conclusion…

Remem-mem-mem…

• Ionic radius

Negative ions are (way!) larger than their atom

…due to shielding by the extra electrons

Positive ions are (way!) smaller than their atom

…because they have lost shielding or shielded electrons

Page 109: …and, in conclusion…

Disclaimer

• Noble gasses have no electronegativity—they don’t share electrons

• Noble gasses have no electron affinity—they don’t gain electrons

• Most metals have no electron affinity—they don’t gain electrons

Page 110: …and, in conclusion…
Page 111: …and, in conclusion…
Page 112: …and, in conclusion…
Page 113: …and, in conclusion…

• Ionization Energies in kJ/mol• 1 2 3 4 5H 1312He 23725250Li 520 7297 11810Be 899 1757 14845 21000B 800 2426 3659 25020 32820C 1086 2352 4619 6221 37820N 1402 2855 4576 7473 9442O 1314 3388 5296 7467 10987F 1680 3375 6045 8408 11020Ne 2080 3963 6130 9361 12180Na 496 4563 6913 9541 13350Mg 737 1450 7731 10545 13627

Page 114: …and, in conclusion…

• Ionization Energies in kJ/mol• 1 2 3 4 5H 1312He 23725250Li 520 7297 11810Be 899 1757 14845 21000B 800 2426 3659 25020 32820C 1086 2352 4619 6221 37820N 1402 2855 4576 7473 9442O 1314 3388 5296 7467 10987F 1680 3375 6045 8408 11020Ne 2080 3963 6130 9361 12180Na 496 4563 6913 9541 13350Mg 737 1450 7731 10545 13627

Page 115: …and, in conclusion…

Size of metal atoms

Page 116: …and, in conclusion…

Size of Atoms (radius, nm)

Page 117: …and, in conclusion…
Page 118: …and, in conclusion…
Page 119: …and, in conclusion…

Size of Anions

Page 120: …and, in conclusion…

A positive charge is

worth about three energy

levels!

Page 121: …and, in conclusion…

Size of Cations

Page 122: …and, in conclusion…

Electron Affinity*, Electronegativity*, Ionization energy

Page 123: …and, in conclusion…

Size

Page 124: …and, in conclusion…

Atomic number, shielding, diagonal effect

Page 125: …and, in conclusion…

Th-th-that’s all, folks.