1 / 52

Here’s what people said they learned.

Here’s what people said they learned. Ionic compounds: dating Molecules: married. LSU is the best school to go to EVER!. Water is a bent molecule, ain’t no HO. It’s not terrible to not use a calculator. Difference between molecular formula and empirical formula.

masato
Download Presentation

Here’s what people said they learned.

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. Here’s what people said they learned. Ionic compounds: dating Molecules: married LSU is the best school to go to EVER! Water is a bent molecule, ain’t no HO. It’s not terrible to not use a calculator. Difference between molecular formula and empirical formula. How to user periodic table better. I need to read those CEF guides! Welding is a physical transformation. (Mostly) The vertical columns on the periodic tables FEATURE elements with similar properties & behaviors. All is not lost!

  2. Here’s what people said they wanted to know better. Ionic compound formulas. How to get an A on the midterms. http://bezmuke.blogspot.com/2009/07/tigri-lei-gheparzi-leoparzi-pisici.html Problems on the quiz. Molecular formula vs. empirical formula. Balancing equations…where to begin. Calculator or no-calculator? I went no-calc and made a 65. I never made a 65 before. How to classify what is solid, liquid or gas? Why is H2O2 so much stronger as an oxidant than H2O? When will we start naming ions?

  3. Rarely, people forget to tear off their “action item for self study”; here is one such example.

  4. I want to revisit our energy relations W = DE = mad (energy due to acceleration) = mv2/2 (kinetic energy) E = W = mgh (potential energy against gravity) Q = m  C  DT And E = mc2 There are more! How about E = hn Does anyone recognize E= t  iV ?

  5. Where are we? • We have measured mass of proton: 1.66 x 10-24 g • We have measured mass of electron: 1836 times lighter than proton • We have measured charge of proton: +1.602 x 10-19 Coulombs • We have measured charge of electron: -1.602 x 10-19 Coulombs • We know protons are at the center of atom. • Neutrons were found—fixed the problem of “missing” atomic masses. • We expect neutrons to be at the center of atom, too (why?). • We imagine electrons are distributed around the atom somehow, • like satellites in orbit. • Because the electrons are so fast, we imagine them doing most of • work of chemistry: the currency of chemistry is electrons!

  6. I want to look at percents: here’s a CEF question. The nucleus contains approximately what percent of an atom’s mass ? •  10.02% • 60.49% • 80.50% • 99.97%  It’s going to depend on the atom, but ignore that and answer the question: ATQ.

  7. We are still in: 4 Read Chapters #4 later.

  8. Now we need to learn something about waves. Well, there are 2 kinds: Longitudinal (sound) Transverse (light)

  9. Let’s make some longitudinal waves with a speaker. High and low frequencies travel at the same speed (almost). This speed is called c = 1140 feet/second (in air). How long does it take sound to travel 1 mile? The sound gets louder and softer as we travel about the room.

  10. Drums & cymbals are the original woofers and tweeters.(Maybe boomers and clangers would be better). l l Low frequency = long l High frequency = short l http://www.replayphotos.com/lsuphotos/traditions-pictures/band_T_OBN__0001024.cfm

  11. Speed = frequency  wavelength c = nl “nu” “lambda” Let’s get those units!

  12. Pinpointing the electron positionsrequired 2 breakthroughs, one conjecture, and a lot of theoretical work. • The Einstein/Planck breakthrough (early 1900s). • Light can have wave AND particle properties! • The particles are called photons. • Each photon carries energy of: h = Planck’s constant c = speed of light = 3 x 108 m/s High energy = short wavelength = blue Low energy = long wavelength = red

  13. Graceful swans vs. hummingbirds

  14. This thing is called a Joule Hey, what what are the units of energy again? Energy is the capacity to do work. It has work units. Work is force times distance. Force is mass times acceleration. So…. E  W = f  d = m  a  d Units: kg  (m/s2)  m= kgm2/s2

  15. Joule, Calorie, Speed of light are all things worth remembering. 1 Joule = 1 ntm = kg m2/s2 4.184 Joule = 1 Calories = 0.001 Food Calories Planck’s constant: 6.63 x 10-34 Js c = 3  108 m/s (= 186,000 miles per second) How far IS 186,000 miles?

  16. Here’s a real-world sample problem. A device we use to measure the size and shape of molecules at CAMD (out on Jefferson Highway) produces 3 x 107 photons per second at l = 1.5 Ǻ (0.15 nm). What is this power output in Joules?

  17. Remember Emission Spectra—what was the point anyway?

  18. Bohr atom (the hypothesis): electrons have to stay on specific paths. Dotted orbit: the “ground” state of hydrogen. Solid orbit: one of the excited states of hydrogen in a discharge tube.

  19. When an electron in the excited state drops to lower state, light is emitted.

  20. When an electron comes out of a high orbit, into a lower one, light is given off. From the wavelength, l, you can calculate the difference in energies between the orbits. D E = hc /l We always deal with CHANGES in energy; absolute energy is a mystery. Needless to say, there are Bohr-ring videos! Energy transitions: http://www.youtube.com/watch?v=8TJ2GlWSPxI&feature=results_video&playnext=1&list=PLC1E620BA406E7A75 Bohr-Ring Children: http://www.youtube.com/watch?v=PLpZfJ4rGts Bohr-Ring Voice: http://www.youtube.com/watch?v=Ic8OnvRonb0

  21. What is this, physics? Where is the chemistry? View periodic tables!

  22. To explain* the periodic table, Bohr proposed that the number of electrons each orbit can support grows with the energy of that orbit, described by an “energy quantum number”, n : # of electrons = 2n2 n = 1, 2, 3…. 2n2 = 2, 8, 18… Energy and the number of electrons an orbit can hold both increase with n. *It can be argued that Bohr did not yet explain the table, but he figured out its “code”.

  23. Periodic Table in its Standard Form n=1 so 2n2 = 2  2 elements on top row n=2 so 2n2 = 8  8 elements on 2nd row n=3 so 2n2 = 18  ooops!

  24. Hey, it works….for small atoms.1st row of periodic table: 2 atoms2nd row: 8 atoms3rd row: ooops! That is a big “ooops” and, besides, Bohr was not able to explain WHY the electrons had to circle around on these discrete, quantized orbits.

  25. The periodic table we usually see cuts out Actinides and Lanthanides, “problem” elements with l=3 (f orbitals). This wide-screen version is better. http://www.sciencegeek.net/tables/LongTable2000.png

  26. The de Broglie Breakthrough (1924): Electrons are waves (and particles). Wave-particle duality l = h/mv   or... mvl= h m = mass v = velocity l (h = 6.63  10-34 Js)

  27. pronounced “lambda” pronounced “nu” Oh great….now even chemists, the masters of electrons, need to understand waves. Let’s do waves again. Oldest physics joke: what’s n?

  28. Waves diffract. They can “stand” if the dimension of their “container” is right.

  29. Wave addition is weird: out-of-phase waves cancel. + = Nothing

  30. In phase waves add. + = Bigger wave.

  31. Waves bounce (with inversion).

  32. What if there’s another wall located 4 wavelengths away?The waves “stand”. See later videos of standing waves. Now is a good time to Wiki.

  33. What if there’s another wall located 4.25 wavelengths away?

  34. It’s much better with video! String standing waves http://www.youtube.com/watch?v=-gr7KmTOrx0

  35. There is no net dissipation of energy in “standing waves”. Hmmm…..atoms don’t seem to need to have energy added, either, but where’s their wall? Do we need a wall for a standing wave? After crossing between the walls twice, the essential feature is that the wave has come back to where it once was.

  36. Bohr’s circular orbits turn out to be wrong, but we can at least see why orbits must be quantized: the waves would cancel themselves out unless the ends meet smoothly. This is called a “boundary condition”. Crest Trough Node Circumference = 2pli where i = 1, 2, 3

  37. There are no walls and no circular orbits in a real atom, but electrons are nevertheless “confined” in a zone, like sand on a vibrating plane: Click for standing waves without walls http://www.youtube.com/watch?v=GtiSCBXbHAg Note the complexity of the wave goes up with frequency…and one wave pattern gives way to another by a “jump”.

  38. When you work the math… • the actual position of electrons can't really be specified • best we can do is say where they PROBABLY are • they tend to locate in cloud-like zones (called orbitals, not orbits) • Orbital shape gets more complex with electron energy. • These shapes sort of "fall out of" the mathematics; • no human would have predicted them intuitively. • Additional quantum numbers • describe these shapes. Erwin Schrödinger

  39. n=1, l=0, m=0 n=2, l=1, m=0 n=3, l=2, m=0 n=2, l=0, m=0 n=3, l=1, m=0 n=4, l=3, m=1 s-type p-type d-type (top) f-type (bottom) Orbital shapes can be strange. Note the extra quantum numbers! http://www.albany.net/~cprimus/orb/

  40. Quantum Numbers are not that hard! • Our purpose: • Introduce the four quantum numbers • Explain how they relate to chemical periodicity • Explain how they relate to orbital shape & size • Give some more examples of physical periodicities • These are really the keys--keys as in open the door • to molecular understanding. • So pay attention!

  41. Four numbers describe more than 100 elements…that’s a beautiful simplification. This will help you understand angular momentum.

  42. But why do we have to learn Quantum Numbers? Isn’t that arcane? Because I had to learn Russian. And square dancing. And accounting. And Lissajous patterns. And tennis. http://www.youtube.com/watch?v=Ee_uujKuJMI It is easier to fit in when you know stuff. Try reading Zen & the Art of Motorcycle Maintenance! It’s about the quality of life, which definitely includes knowledge. Quantum makes it easier to understand later material. You will be buying quantum computers. Quantum Numbers are beautiful!

  43. A useless journey….but beautiful. Mt. Chapin Trail Rocky Mountain National Park August 2011

  44. The Energy quantum number determines how much diversity you can have. Energy-rich electrons can "buy" more “fancy” quantum states than energy-poor ones.

  45. n=1, l=0, m=0 n=2, l=1, m=0 n=3, l=2, m=0 n=2, l=0, m=0 n=3, l=1, m=0 n=4, l=3, m=1 s-type p-type d-type (top) f-type (bottom) Shapes of atomic orbitals have to do with orbital angular momentum: go back and watch gyroscope YouTube. http://www.albany.net/~cprimus/orb/

  46. Row 1 contains elements with only “low-energy” electrons. if n = 1, then you can have l = 0 only. Then you can only have ml = 0. ms can be +1/2 or - 1/2. Aha! There are only two elements, H and He, on the top line of the periodic table.

  47. Row 2: now some electrons (the ones that matter) have more energy. if n = 2, you can havel= 0 or 1 For l= 0, you can have ml= 0 only. ms can be +1/2 or - 1/2. Check out Li and Be For l = 1, you can have ml= 0 or +1 or -1 For each of these three ml values, you can have ms = +1/2 or - 1/2 for a total of SIX states Check out the six elements: B, C, N, O, F , Ne

  48. 1s 2s 2p 3s 3p 3d 4s 4p CrayolaPeriodicTable

  49. Electron configuration problems are easy! There are all kinds of mnemonic devices for this (see your textbook, CEF Study Guides, Virtual Book) but the easy solution is: Just follow the periodic table!   Example:  Calcium = 1s22s22p63s23p64s2

More Related