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Lab 9 Atomic Structure  Emission Spectrum Electron Configuration
HISTORY OF THE ATOM 460 BC Democritus develops the idea of atoms he pounded up materials in his mortar and pestle until he...
Development of the  Model of an Atom <ul><li>400 BC </li></ul><ul><li>Democritus – Particle Model </li></ul><ul><ul><li>An...
HISTORY OF THE ATOM 1808 John Dalton suggested that all matter was made up of tiny spheres that were able to bounce around...
Dalton proposes  Atomic Theory in 1803 <ul><li>Based upon experimental evidence </li></ul><ul><li>All matter composed of a...
HISTORY OF THE ATOM 1898 Joseph John Thompson found that atoms could sometimes eject a far smaller negative particle which...
Thomson and the Discovery of Electrons
 
J. J. Thomson’s Experiment Devised an experiment to find the ratio of the cathode ray particle’s mass ( m e ) to the charg...
Thomson’s Plum Pudding Model <ul><li>Based upon the charge to mass ratio, the electron must be much smaller than the atom ...
HISTORY OF THE ATOM Thomson develops the idea that an atom was made up of electrons scattered unevenly within an elastic s...
Millikan’s Oil Drop Experiment Measuring the Charge on an electron
Unstable Atoms and Radioactivity <ul><li>Atoms are not indestructible </li></ul><ul><li>Atoms are composed of smaller part...
Radioactivity
Goldstein’s Discovery of Protons
Mass Spectrometer-  Determining the Percent Abundance of Different Isotopes of same element
Mass Spectrometer If a stream of positive ions having equal velocities is brought into a magnetic field, the lightest ions...
Mass Spectrometry EOS A record of the separation of ions is called a  mass spectrum
Isotopes of Neon <ul><li>Neon-20 </li></ul><ul><ul><li>10 protons </li></ul></ul><ul><ul><li>10 neutrons </li></ul></ul><u...
 
HISTORY OF THE ATOM 1910 Ernest Rutherford oversaw Geiger and Marsden carrying out his famous experiment.  They fired Heli...
Rutherford’s Gold Foil Experiment
Rutherford’s Gold Foil Experiment gold foil helium nuclei They found that while most of the helium nuclei passed through t...
Rutherford’s  Nuclear Model of the Atom <ul><li>Most the alpha particles (helium nuclei) pass through the gold foil </li><...
Visualizing the Pathway of Alpha Particles through a Gold Atom
ELECTROMAGNETIC RADIATION
Electromagnetic radiation.
Electromagnetic Radiation <ul><li>Most subatomic particles behave as PARTICLES and obey the physics of waves. </li></ul>
Electromagnetic Radiation
The Electromagnetic Spectrum
Wave Model of Light <ul><li>Wavelength   </li></ul><ul><ul><li>measured in meters (m) </li></ul></ul><ul><li>Frequency  ƒ...
Wavelength, Frequency and Energy <ul><li>Wavelength inversely related to frequency </li></ul><ul><ul><li>Increasing wavele...
Electromagnetic Radiation wavelength Visible light wavelength Ultaviolet radiation Amplitude Node
Electro magnetic   Spectrum In increasing energy, R O Y   G   B I V
 
Sunlight viewed through a spectroscope
Prisms and diffraction grating  bend light  <ul><li>Red light with longer wavelengths bend less </li></ul><ul><li>Violet l...
Photoelectric Effect
Photoelectric Effect <ul><li>Bright red light shined on the photocell has no effect- regardless of intensity or time </li>...
Explaining the Photoelectric Effect <ul><li>ONLY the photon or particle model can be used to explain these results </li></...
Light Spectrum Lab! Slit that allows light inside Line up the slit so that it is parallel with the spectrum tube (light bu...
The Emission Spectrum of Hydrogen-  Discrete Bands of Colored Light
Excited Gases  & Atomic Structure
Emission Spectra of Different Atoms: A Fingerprint to Identify
Rydberg and Balmer (1886) <ul><li>Independently develop mathematical equations that fit the data for hydrogen emission spe...
Rydberg Equation <ul><li>1/ λ   = R H   [1/n 1 2   -  1/n 2 2 ] </li></ul><ul><li>R H  = 1.09678 x 10 -2  nm -1 </li></ul>...
Bohr’s Model of the Atom (1910) <ul><li>Assumed electrons orbit the nucleus in circular orbits </li></ul><ul><li>Proposed ...
Bohr’s Model of the Atom (1910) <ul><li>When the atom absorbs energy </li></ul><ul><ul><li>Electron moves up to higher ene...
Bohr’s Calculations  of the Energy Δ E = -2.18 x 10 -18  J (1/n f 2  – 1/n i 2 ) n = the energy level Δ E = positive when ...
Niels Bohr (1885-1962) Δ E = -2.18 x 10 -18  J (1/n f 2  – 1/n i 2 ) Calculate the energy as an electron drops from level ...
ultraviolet infrared
Visualizing the Movement of the Electron
 
Line Spectra of Other Elements Oops.  Bohr’s equation does NOT predict these wavelengths.
 
Visualizing the “falling” e- Where does the electron have more potential energy?
Electron is a wave - De Broglie  <ul><li>De Broglie </li></ul><ul><ul><li>Since light is both particle and wave, perhaps s...
Quantum Mechanics <ul><li>Heisenberg </li></ul><ul><ul><li>Uncertainty principle </li></ul></ul><ul><ul><li>Given the wave...
E. Schrodinger 1887-1961 W. Heisenberg 1901-1976 Wave Functions:  Calculating the Probability of locating an electron in a...
The Wave Function and Orbitals
The region near the nucleus is separated from the outer region by a spherical  node  - a spherical shell in which the elec...
 
Quantum Numbers <ul><li>Values that emerge from the wave functions of Schrodinger </li></ul><ul><li>1 st  n = energy level...
Increasing Radius of s-orbital with higher values of n
s orbital p orbital d orbital
 
 
f Orbitals
 
 
 
The s-orbital Spherical shaped orbital ℓ  = 0 m ℓ  = 0 Only one s-orbital in any energy level
The p-orbital Double-lobe shaped orbital ℓ  = 1 mℓ = -1 or 0 or +1 Only three p-orbitals in any energy level- except for l...
Planes of zero probability
Model of d-orbital
Only electrons with opposite spins can be in the same orbital
Electron Configurations <ul><li>Show the electrons in orbitals </li></ul><ul><ul><ul><ul><li>Box used to represent orbital...
Use sum of first two quantum numbers to determine which orbital fills first
 
 
 
 
 
 
 
 
 
 
 
Nickel  Electron Configuration and quantum numbers 1s   2s  2p   3s  3p 1 0 0  ½  2 0 0 ½  2 1 -1 ½  2 1 0 ½  3 0 0 ½   3 ...
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Lab 8 atomic structure

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Transcript of "Lab 8 atomic structure"

  1. 1. Lab 9 Atomic Structure Emission Spectrum Electron Configuration
  2. 2. HISTORY OF THE ATOM 460 BC Democritus develops the idea of atoms he pounded up materials in his mortar and pestle until he had reduced them to smaller and smaller particles which he called ATOMS ( greek for indivisible )
  3. 3. Development of the Model of an Atom <ul><li>400 BC </li></ul><ul><li>Democritus – Particle Model </li></ul><ul><ul><li>Ancient Greek philosopher </li></ul></ul><ul><ul><li>Proposes that matter is composed of smallest particles called atoms </li></ul></ul><ul><ul><li>An idea with no evidence </li></ul></ul><ul><li>Aristotle – Continuous Model </li></ul><ul><ul><li>Alternative idea </li></ul></ul><ul><ul><li>Continuous model of matter- no smallest piece </li></ul></ul>
  4. 4. HISTORY OF THE ATOM 1808 John Dalton suggested that all matter was made up of tiny spheres that were able to bounce around with perfect elasticity and called them ATOMS
  5. 5. Dalton proposes Atomic Theory in 1803 <ul><li>Based upon experimental evidence </li></ul><ul><li>All matter composed of atoms </li></ul><ul><li>Atoms of same element have same mass and properties </li></ul><ul><li>Atoms are neither created nor destroyed, they are rather simply rearranged in chemical reactions </li></ul><ul><ul><li>Evidence – Lavoiser- Conservation of Mass </li></ul></ul><ul><li>Compounds are composed of elements in simple whole number ratios </li></ul><ul><ul><li>Evidence – Proust </li></ul></ul>
  6. 6. HISTORY OF THE ATOM 1898 Joseph John Thompson found that atoms could sometimes eject a far smaller negative particle which he called an ELECTRON
  7. 7. Thomson and the Discovery of Electrons
  8. 9. J. J. Thomson’s Experiment Devised an experiment to find the ratio of the cathode ray particle’s mass ( m e ) to the charge ( e ) m e / e = –5.686 x 10 –12 kg C –1
  9. 10. Thomson’s Plum Pudding Model <ul><li>Based upon the charge to mass ratio, the electron must be much smaller than the atom </li></ul><ul><li>Proposed negative electrons embedded in positive matrix of atom </li></ul>
  10. 11. HISTORY OF THE ATOM Thomson develops the idea that an atom was made up of electrons scattered unevenly within an elastic sphere surrounded by a soup of positive charge to balance the electron's charge 1904 PLUM PUDDING MODEL
  11. 12. Millikan’s Oil Drop Experiment Measuring the Charge on an electron
  12. 13. Unstable Atoms and Radioactivity <ul><li>Atoms are not indestructible </li></ul><ul><li>Atoms are composed of smaller particles </li></ul><ul><li>Alpha particles – positively charged </li></ul><ul><li>Beta particles – negatively charged </li></ul><ul><li>Gamma rays – no charge </li></ul>
  13. 14. Radioactivity
  14. 15. Goldstein’s Discovery of Protons
  15. 16. Mass Spectrometer- Determining the Percent Abundance of Different Isotopes of same element
  16. 17. Mass Spectrometer If a stream of positive ions having equal velocities is brought into a magnetic field, the lightest ions are deflected the most, making a tighter circle
  17. 18. Mass Spectrometry EOS A record of the separation of ions is called a mass spectrum
  18. 19. Isotopes of Neon <ul><li>Neon-20 </li></ul><ul><ul><li>10 protons </li></ul></ul><ul><ul><li>10 neutrons </li></ul></ul><ul><li>Neon-21 </li></ul><ul><ul><li>10 protons </li></ul></ul><ul><ul><li>11 neutrons </li></ul></ul><ul><li>Neon-22 </li></ul><ul><ul><li>10 protons </li></ul></ul><ul><ul><li>12 neutrons </li></ul></ul>
  19. 21. HISTORY OF THE ATOM 1910 Ernest Rutherford oversaw Geiger and Marsden carrying out his famous experiment. They fired Helium nuclei at a piece of gold foil which was only a few atoms thick. They found that although most of them passed through. About 1 in 10,000 hit
  20. 22. Rutherford’s Gold Foil Experiment
  21. 23. Rutherford’s Gold Foil Experiment gold foil helium nuclei They found that while most of the helium nuclei passed through the foil, a small number were deflected and, to their surprise, some helium nuclei bounced straight back.
  22. 24. Rutherford’s Nuclear Model of the Atom <ul><li>Most the alpha particles (helium nuclei) pass through the gold foil </li></ul><ul><ul><li>Atom mostly empty space </li></ul></ul><ul><ul><li>Alpha particles did not hit anything </li></ul></ul><ul><li>A very few deflected straight back </li></ul><ul><ul><li>Alpha particles deflected by a dense positive nucleus </li></ul></ul>
  23. 25. Visualizing the Pathway of Alpha Particles through a Gold Atom
  24. 26. ELECTROMAGNETIC RADIATION
  25. 27. Electromagnetic radiation.
  26. 28. Electromagnetic Radiation <ul><li>Most subatomic particles behave as PARTICLES and obey the physics of waves. </li></ul>
  27. 29. Electromagnetic Radiation
  28. 30. The Electromagnetic Spectrum
  29. 31. Wave Model of Light <ul><li>Wavelength  </li></ul><ul><ul><li>measured in meters (m) </li></ul></ul><ul><li>Frequency ƒ </li></ul><ul><ul><li>measured in waves per second (Hz) </li></ul></ul><ul><li>Energy E </li></ul><ul><ul><li>measured in Joules (J) </li></ul></ul>
  30. 32. Wavelength, Frequency and Energy <ul><li>Wavelength inversely related to frequency </li></ul><ul><ul><li>Increasing wavelength  decreasing frequency </li></ul></ul><ul><ul><li>Decreasing wavelength  increasing frequency </li></ul></ul><ul><ul><li>Wavelength x frequency = speed of light </li></ul></ul><ul><ul><li>c =  ƒ c = speed of light = 3.00 x 10 8 m/s </li></ul></ul><ul><li>Frequency directly related to energy </li></ul><ul><ul><li>Increasing frequency  increasing energy </li></ul></ul><ul><ul><li>Energy = Planck’s constant x frequency </li></ul></ul><ul><ul><li>E = h ƒ h = Planck’s constant = 6.63 x 10 -34 J/Hz </li></ul></ul>
  31. 33. Electromagnetic Radiation wavelength Visible light wavelength Ultaviolet radiation Amplitude Node
  32. 34. Electro magnetic Spectrum In increasing energy, R O Y G B I V
  33. 36. Sunlight viewed through a spectroscope
  34. 37. Prisms and diffraction grating bend light <ul><li>Red light with longer wavelengths bend less </li></ul><ul><li>Violet light with shorter wavelengths bend more </li></ul><ul><li>Separates white light into ROYGBIV </li></ul><ul><li>Red – Orange – Yellow – Green – Blue – Indigo – Violet </li></ul><ul><li>long waves short waves </li></ul><ul><li>low frequency high frequency </li></ul><ul><li>low energy high energy </li></ul>
  35. 38. Photoelectric Effect
  36. 39. Photoelectric Effect <ul><li>Bright red light shined on the photocell has no effect- regardless of intensity or time </li></ul><ul><li>Dim green light shined on the photocell causes electrons to be emitted and flow through the wire </li></ul><ul><li>Brighter green light emits more electrons per second- greater current </li></ul>
  37. 40. Explaining the Photoelectric Effect <ul><li>ONLY the photon or particle model can be used to explain these results </li></ul><ul><li>Energy is required to pull off negative electrons attracted to positive protons in nucleus- breaking attraction </li></ul><ul><li>Each red photon does not have enough energy to pull off an electron – regardless of how long the light is shined </li></ul><ul><li>Each green photon has more energy and can pull off the electron when the green photon collides </li></ul>
  38. 41. Light Spectrum Lab! Slit that allows light inside Line up the slit so that it is parallel with the spectrum tube (light bulb)
  39. 42. The Emission Spectrum of Hydrogen- Discrete Bands of Colored Light
  40. 43. Excited Gases & Atomic Structure
  41. 44. Emission Spectra of Different Atoms: A Fingerprint to Identify
  42. 45. Rydberg and Balmer (1886) <ul><li>Independently develop mathematical equations that fit the data for hydrogen emission spectrum </li></ul><ul><li>The electron had no yet been discovered </li></ul><ul><li>Neither had a model to explain the observed wavelengths </li></ul><ul><li>Just an equation that worked </li></ul>
  43. 46. Rydberg Equation <ul><li>1/ λ = R H [1/n 1 2 - 1/n 2 2 ] </li></ul><ul><li>R H = 1.09678 x 10 -2 nm -1 </li></ul><ul><li>Solve the equation for an electron moving from level 4 to 2. </li></ul>
  44. 47. Bohr’s Model of the Atom (1910) <ul><li>Assumed electrons orbit the nucleus in circular orbits </li></ul><ul><li>Proposed the energy of the orbit is proportional to the distance from the nucleus (increasing distance – increasing energy) </li></ul><ul><li>Assumed only certain allowable energies </li></ul><ul><li>Used angular momentum to calculate the allowable energy </li></ul>
  45. 48. Bohr’s Model of the Atom (1910) <ul><li>When the atom absorbs energy </li></ul><ul><ul><li>Electron moves up to higher energy with more potential energy farther away from nucleus </li></ul></ul><ul><ul><li>Unstable with higher PE </li></ul></ul><ul><li>Electron falls back down to lower levels </li></ul><ul><ul><li>Energy released </li></ul></ul><ul><ul><li>PE converted to KE as electron fall </li></ul></ul><ul><ul><li>The color of light observed reflects the energy released in the fall </li></ul></ul>
  46. 49. Bohr’s Calculations of the Energy Δ E = -2.18 x 10 -18 J (1/n f 2 – 1/n i 2 ) n = the energy level Δ E = positive when electron climbs up levels absorbing energy increasing PE Δ E = negative when e- falls down levels releasing energy decreasing PE
  47. 50. Niels Bohr (1885-1962) Δ E = -2.18 x 10 -18 J (1/n f 2 – 1/n i 2 ) Calculate the energy as an electron drops from level 6 down to level 2. Calculate the frequency and wavelength of this photon.
  48. 51. ultraviolet infrared
  49. 52. Visualizing the Movement of the Electron
  50. 54. Line Spectra of Other Elements Oops. Bohr’s equation does NOT predict these wavelengths.
  51. 56. Visualizing the “falling” e- Where does the electron have more potential energy?
  52. 57. Electron is a wave - De Broglie <ul><li>De Broglie </li></ul><ul><ul><li>Since light is both particle and wave, perhaps so is matter both particle and wave </li></ul></ul><ul><ul><li>Wavelength depends upon mass and velocity </li></ul></ul><ul><ul><li>Objects with large mass have </li></ul></ul><ul><ul><li>negligible, so small we can ignore </li></ul></ul><ul><ul><li>Electrons with very small mass have wave properties that cannot be ignored </li></ul></ul>λ = h/p
  53. 58. Quantum Mechanics <ul><li>Heisenberg </li></ul><ul><ul><li>Uncertainty principle </li></ul></ul><ul><ul><li>Given the wavelike nature of electron </li></ul></ul><ul><ul><li>Impossible to know both location and energy of electron </li></ul></ul><ul><ul><li>Can only calculate the probable location </li></ul></ul><ul><li>Schrodinger </li></ul><ul><ul><li>Used calculus to “locate” the electron within orbital </li></ul></ul><ul><ul><li>Orbitals – regions of space representing the most probable location of electron </li></ul></ul>
  54. 59. E. Schrodinger 1887-1961 W. Heisenberg 1901-1976 Wave Functions: Calculating the Probability of locating an electron in a region of space The Uncertainty Principle: Cannot both determine location and energy of electron
  55. 60. The Wave Function and Orbitals
  56. 61. The region near the nucleus is separated from the outer region by a spherical node - a spherical shell in which the electron probability is zero EOS
  57. 63. Quantum Numbers <ul><li>Values that emerge from the wave functions of Schrodinger </li></ul><ul><li>1 st n = energy level </li></ul><ul><li>2 nd ℓ = shape of orbital (s, p, d or f) </li></ul><ul><li>3 rd m ℓ = orientation (diff versions) </li></ul><ul><li>4 th m s = magnetic spin of electron </li></ul>
  58. 64. Increasing Radius of s-orbital with higher values of n
  59. 65. s orbital p orbital d orbital
  60. 68. f Orbitals
  61. 72. The s-orbital Spherical shaped orbital ℓ = 0 m ℓ = 0 Only one s-orbital in any energy level
  62. 73. The p-orbital Double-lobe shaped orbital ℓ = 1 mℓ = -1 or 0 or +1 Only three p-orbitals in any energy level- except for level one
  63. 74. Planes of zero probability
  64. 75. Model of d-orbital
  65. 76. Only electrons with opposite spins can be in the same orbital
  66. 77. Electron Configurations <ul><li>Show the electrons in orbitals </li></ul><ul><ul><ul><ul><li>Box used to represent orbital </li></ul></ul></ul></ul><ul><ul><ul><ul><li>Half arrow used to represent e- with opposite spins </li></ul></ul></ul></ul><ul><li>Electrons are placed in orbitals of lowest energy first </li></ul>
  67. 78. Use sum of first two quantum numbers to determine which orbital fills first
  68. 90. Nickel Electron Configuration and quantum numbers 1s 2s 2p 3s 3p 1 0 0 ½ 2 0 0 ½ 2 1 -1 ½ 2 1 0 ½ 3 0 0 ½ 3 1 0 ½ 2 1 0 ½ 3 1 -1 ½ 3 1 0 ½ 4s 3d 4 01 0 ½ 3 2 -2 ½ 3 2 -1 ½ 3 2 0 ½ 3 2 1 ½ 3 2 1 ½ 1 st # indicates energy level n = 1 1 st level n = 2 2 nd level 2 nd # type of orbital l = 0 is s-orbital l = 1 is p-orbital l = 2 is d-orbital
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