1. Back ©Bires, 2002 Slide 1 Bires, 2009 Chapter 4 Electron Configurations and Quantum Chemistry Electron configurations determine how an atom behaves in bonding with other atoms! Topics rearranged from your text, pages 90-116. Atomic Emissions/Abortions removed Anyone who says that they can contemplate quantum mechanics without becoming dizzy has not understood the concept in the least. -Niels Bohr

2. Back ©Bires, 2002 Slide 2 Bires, 2009 The Bohr Model Niels Bohr –rebuilt the model of the atom placing the electrons in energy levels. Quantum chemistry –a discipline that states that energy can be given off in small packets or quanta of specific size. What would happen to an electron if the right sized quanta of energy was added to it? What would happen when the electron came back down to its ground state? EXCITED STATE Ground state

3. Back ©Bires, 2002 Slide 3 Bires, 2009 Atomic Absorption / Emission Atomic Absorption –Electron is given a specific amount of energy, it “quantum jumps” to a higher energy level (excited state). Atomic Emission –Electron returns to its ground state, it emits energy equal to the amount of energy required to raise it to the higher level. –The difference in energy of the levels produces photons of differing energy –(blue = higher energy, red = lower energy) Internet Animation of Atomic Absorption / Emission

4. Back ©Bires, 2002 Slide 4 Bires, 2009 Atomic Absorption / Emission White light is composed of all visible wavelengths (colors) of light. (Electromagnetic Radiation) The continuous spectrum –having all wavelengths / colors of visible light (white)

5. Back ©Bires, 2002 Slide 5 Bires, 2009 Emissions Spectrum When electrons in a gas are charged with energy –those electrons make their quantum jumps… –Then return to their ground states… –resulting (unique) pattern of light given off is called an emission spectrum. Each element has a different emission spectrum, a sort of quantum fingerprint, that we can use to identify elements in unknown samples. What happens next?

6. Back ©Bires, 2002 Slide 6 Bires, 2009 Some bright-line emission spectra: Some emission spectra of elements –from www.webelements.com:www.webelements.com Sodium, 11 electrons in 3 ground-shells: Mercury, 80 electrons in 6 ground-shells:

7. Back ©Bires, 2002 Slide 7 Bires, 2009 Absorption Spectrum Absorption spectrum –Given off when white light is shined through a gas –electrons in the gas absorb some wavelengths of the light Viewing light from distant stars through the gasses of our planets allows us to know what chemicals make up those planets.

8. Back ©Bires, 2002 Slide 8 Bires, 2009 Bright-Line Spectra Max Planck, German physicist –calculated that energy required to make a quantum jump for specific energy levels and colors. Planck’s Constant, 6.6262x10 -27 –multiplied by the frequency of the desired emission color equals energy required to produce that jump.

9. Back ©Bires, 2002 Slide 9 Bires, 2009 Electron Configurations - overview Bohr model –electrons exist in specific energy levels. Electron orbitals (shapes) –Within each energy level, the orbits the electrons can occupy. Within each orbital –electrons can be set “spin up” or “spin down” Electron configuration –The configuration of electrons in their levels, orbitals, and spins. Modern Quantum Model –Electron exists in electron configurations

10. Back ©Bires, 2002 Slide 10 Bires, 2009 Energy Levels (n) The electrons exist in energy levels or shells. The first energy shell can hold only 2 electrons. –Hydrogen and Helium in their ground state have electrons that occupy this shell. The second shell can hold 8 electrons. The third can hold 18 electrons. 28 32 18 Shells All shells after three can hold 32 electrons. Old School: “KLM notation”

11. Back ©Bires, 2002 Slide 11 Bires, 2009 Orbitals (Shapes) Orbitals –electrons travel in set paths. –These paths form shapes, called orbitals. Each “shape” can hold 2 electrons The smallest orbital is the “s” orbital. The “s” orbital: –Has only 1 shape (holds 2 e - ) –Is spherical in shape –Is the lowest energy orbital s-2

12. Back ©Bires, 2002 Slide 12 Bires, 2009 p-Orbitals The 2 nd orbital shape is the “p” orbital shape. There are 3 “p” shapes, each holding 2 electrons, for a total of 6 electrons in the “p” orbitals. The “p” orbitals are: –Dumbbell-shaped –Higher in energy than the “s” p-6 s-2

13. Back ©Bires, 2002 Slide 13 Bires, 2009 d-Orbitals The 3 rd orbital shape is the “d” orbital shape. There are 5 “d” orbital shapes, for a total of 10 electrons in the “d” orbitals. “d” orbitals are higher in energy than “p” orbitals. s-2 d-10 p-6

14. Back ©Bires, 2002 Slide 14 Bires, 2009 f-Orbitals The last orbital shape is the “ f ” orbital shape. –“ f ” orbitals have irregular shapes due to quantum tunneling. –There are 7 “ f ” shapes, for a total of 14 electrons. Electrons in f orbitals are very high in energy s-2 f-14 d-10p-6

15. Back ©Bires, 2002 Slide 15 Bires, 2009 “Blocks” of the periodic table… The periodic table tells us in which orbital the last electron should be found. –The last electron in an atom is found in the… s orbitals p orbitals d orbitals f orbitals

16. Back ©Bires, 2002 Slide 16 Bires, 2009 Electron “Spin” Electrons can be “spin up” or “spin down.” –(by convention, an electron that is alone is “spin up”) Hund’s Rule –As electrons fill orbitals, they first fill each shape available with one electron before spin pairing. Pauli’s Exclusion Principle –If two electrons share a shape, they must be spin- paired (one up and one down). For instance: take a “p” orbital…it has three orbital-shapes that can hold 2 e - each. It would fill like this:

17. Back ©Bires, 2002 Slide 17 Bires, 2009 Writing Electron Configurations The Aufbau principleThe Aufbau principle –electron will fill lower energy orbitals first. Energy of electrons: –low energy s < p < d < f high energy –low energy nearer < farther high energy –low energy level 1 < level 7 high energy Total energy of an electron: –Product of energy of its shell and the energy of its orbital. –Guess: Which is lower in energy, an electron found in 3d or one found in 4s? s  low energy d  high energy close  low energy far  high energy Total energy = Shell x orbital shape The 4s electrons are lower in energy!

18. Back ©Bires, 2002 Slide 18 Bires, 2009 Writing Electron Configurations Orbital filling diagram –Shows how electrons fill into levels and orbitals  Don’t Copy this

19. Back ©Bires, 2002 Slide 19 Bires, 2009 Building the Orbital Filling Diagram Begin by listing the shells 1, 2, 3, 4, 5, 6, 7 vertically. These are your “s” orbitals. Next, add another column of number, beginning with 2. These are your “p” orbitals. Do the same for “d” and “f” orbitals, beginning with “3” for the “d” orbitals and “4” for the “f” orbitals. Next, add your orbital letters. Finally, draw diagonal lines as shown. 1 2 3 6 5 4 7 2 3 6 5 4 7 3 6 5 4 7 6 5 4 7s s s s s s s p p p p p p d d d d d f f f f spdf

20. Back ©Bires, 2002 Slide 20 Bires, 2009 Electron Configurations of Some Atoms Consider Fluorine, with 9 electrons What about Copper, with 29 electrons? Notice the position of the last electron… Both used

21. Back ©Bires, 2002 Slide 21 Bires, 2009 Noble Gas Shorthand Notice the configurations of the noble gases: We can shorten the electron configuration of larger elements with NGS. Consider Mg: We can substitute Neon’s e - config, and write Mg: Similarly, Titanium’s (Ti) e - config: Can be shortened to:

22. Back ©Bires, 2002 Slide 22 Bires, 2009 Ion e - configurations Ions (elements with more/less electrons) also have electron configurations. Consider Sulfur (S): What if sulfur gained two electrons? Consider Calcium (Ca): What if calcium lost two electrons?

23. Back ©Bires, 2002 Slide 23 Bires, 2009 Octets! Octets: –Atoms with filled s and p orbitals in the same, highest level. –Have noble gas-like configurations –Have special stability Both atoms and ions can have complete octets.

24. Back ©Bires, 2002 Slide 24 Bires, 2009 Question: –Why do the atomic radii (size) of atoms decrease as electrons and protons are added to the atom, as you move from left to right across a period? electrostatic attraction –attraction between the electrons (-) in the shells and the protons(+) in the nucleus – pulls the electrons in This is what we call a periodic trend End of chapter 4

25. Back ©Bires, 2002 Slide 25 Bires, 2009 CCSD Syllabus Objectives 5.4: Quantum Model of the Atom 5.6: Electron Configurations