1 / 39

Electron Configurations

Electron Configurations. Review of an Atom . This isn’t an accurate depiction. . Electron clouds are 3D, not flat Electrons are spread out as much as possible, not usually round, and are moving rapidly These things are hard to see in a still picture. Orbitals.

oded
Télécharger la présentation

Electron Configurations

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Electron Configurations

  2. Review of an Atom

  3. This isn’t an accurate depiction. • Electron clouds are 3D, not flat • Electrons are spread out as much as possible, not usually round, and are moving rapidly • These things are hard to see in a still picture

  4. Orbitals • Electrons spread out in orbitals • Orbitals have different SHAPES and ENERGY (distance from nucleus) • Quantum numbers describe orbitals • There are four quantum numbers

  5. Principal Quantum Number (n) • First of the four (n, #, #, #) • Describes the distance from the nucleus to the orbital (and therefore describes the ENERGY of the orbital) • Values: integers ≥ 1 • As the distance from the nucleus increases, n increases. • As the energy increases, n increases.

  6. Principal Quantum Number

  7. n relates to the Periodic Table! • Each period as a unique n value • Period 1: n=1 • Period 2: n=2 • Period 3: n=3 • ETC

  8. Lyman Series • The transition from n≥2 to n=1in a hydrogen atom • Result: ultraviolet emission lines of the hydrogen atom • Greater the difference in the principal quantum numbers, the higher the energy of the electromagnetic emission

  9. Lyman Series

  10. Balmer Series • The transition from n≥3 to n=2 in a hydrogen atom • Result: spectral line emissions of the hydrogen atom • As the n value increases, the wavelength emitted decreases (in nm)

  11. Balmer Series

  12. Paschen Series • The transition from n≥4 to n=3 in a hydrogen atom • Result: emission lines in the infrared band

  13. Paschen Series

  14. Angular Momentum (l) • Second of the four (n, l, #, #) • Shape of the sublevel • Range from 0 to n-1 (we will never deal with anything above l=3) • l=0 = s • l=1 = p • l=2 = d • l=3 = f

  15. s sublevel

  16. p sublevel

  17. d sublevel

  18. f orbitals

  19. Magnetic Number (ml) • Third of the four numbers (#, #, ml , #) • Denotes the orbital sublevel that is filled • s sublevel has ONE orbital (sphere has one orientation in space) • p sublevel has THREE orbitals (three orientations in space) • d sublevel has FIVE orbitals (five orientations in space) • f sublevel has SEVEN orbitals (seven orientations in space)

  20. Magnetic Number • s sublevel: one orbital • One orientation in space

  21. Magnetic Number • P sublevels: three orbitals • Three orientations in space

  22. Magnetic Number • d sublevels: five orbitals • Five orientations in space

  23. Magnetic Number • f sublevel: seven orbitals • Seven orientations in space

  24. Magnetic Number • Integers from -l to l • SO: • s: ml = 0 only since l= 0 • p: ml = -1,0,1 since l= 1 • d: ml = -2,-1,0,1,2 since l= 2 • f: ml = -3,-2,-1,0,1,2,3 since l= 3

  25. Spin (ms) • Fourth number (#, #, #, ms) • It is either -1/2 or ½ • Down or up

  26. What does all of this tell us? • There is a very specific order in which electrons fill orbitals. It is not random. There are some exceptions.

  27. Orbital Filling Order

  28. Three Important Principles • Aufbau (next) Principle • Pauli Exclusion Principle • Hund’s Rule

  29. Aufbau • Electrons fill the LOWEST energy sublevel before going to the next sublevel • 1s fills, then 2s fills, then 2p fills, then 3s fills, then 3p fills ….

  30. Pauli Exclusion Principle • Electrons pair according to OPPOSITE spins • ↑↓, not ↑↑ or ↓↓

  31. Hund’s Rule • Electrons spread out in equal energy sublevels before pairing electrons • (↑↑↑ and not ↑↓↑ _)

  32. Step by Step… • First level to fill is 1s level • Lowest energy sublevel • Holds two electrons • They are oppositely paired • A sublevel is represented by __ and holds 2 electrons

  33. Second sublevel is the 2s sublevel • It holds 2 electrons because of s • Electrons are oppositely paired

  34. So, we filled 1s, we filled 2s • Now comes 2p • Holds six electrons because p orbitals hold 6 electrons 1s22s22p6

  35. Finally.. • From 2p, 3s fills with 2 electrons • 3p fills with 6 electrons • 4s fills with 2 electrons • 3d fills with 10 electrons • 4p fills with 6 electrons • 5s fills with 2 electrons

  36. Example: Carbon • Neutral carbon: 6 electrons ↑↓↑↓↑↑ _ 1s 2s 2p • Six arrows for six electrons • 1s2 2s2 2p2

  37. Exceptions… • Some energy levels are SUPER close together • The levels are so close that electrons are able to move between these orbitals in order to minimize repulsion… • 4s and 3d orbitals are very close in energy • Exceptions exist for some period 4 d block elements • Cr is not 1s2 2s2 2p6 3s2 3p6 4s2 3d4 • Cr is 1s2 2s2 2p6 3s2 3p6 4s1 3d5 • It actually takes LESS energy to split the electrons between the 5 sublevels than it does to put them together in the 4s and 3d

More Related