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Atomic Theory & Periodicity
Chapters 6 & 7
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Light How does an incandescent light bulb work?
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Light Electricity is turned on Metal filament heats up
Hot metal gives off light Blackbody Radiation
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Blackbody radiation
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Blackbody Radiation Max Planck proposed that the energy of light given off could only be emitted in little bundles, called quanta Bundles of light were multiples of a smaller unit E=hπ h = x 10-34Js Planckβs Constant
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Photoelectric Effect Light shining on a photo-sensitive metal plate will emit electrons.
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Photoelectric Effect Frequency must be above a minimum (threshold) frequency Brighter light (higher intensity) produces more electrons, but with the same energy Light with higher frequency will emit electrons with higher energy
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Photoelectric Effect
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Photoelectric Effect βπ= πΎπΈ πππ₯ + π
Einstein expanded on Planckβs work to explain photoelectric effect Nobel Prize in 1921 Energy of Photon = Energy of ejected electron + work needed to eject electron (work function, Ξ¦) βπ= πΎπΈ πππ₯ + π
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Atomic Model Review Daltonβs Hard Sphere Model Plum Pudding Model
Atom is indivisible, indestructible sphere Plum Pudding Model Uniform positive sphere with negative electrons embedded within Rutherford Model Atom is mostly empty space, dense positive nucleus, electrons randomly outside nucleus
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Bohr Model Rutherford Model could not explain chemical properties
Niels Bohr proposed electrons in energy levels Valence electrons Electrons can move between energy levels by gaining or losing energy
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Electron Transitions When electrons gain energy they move to higher energy levels When electrons drop to lower energy levels they release energy as light Energy is related to the distance between energy levels
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π=ππ πΈ=βπ= βπ π Light Waves review Wave Equation Energy Equation
Color is based on frequency, π π=ππ πΈ=βπ= βπ π
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Electromagnetic Spectrum
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Energy Practice Calculate the energy of a photon of yellow light that has a wavelength of 589 nm. Calculate the energy of a mole of photons of yellow light with a wavelength of 589 nm. πΈ=βπ= βπ π = (6.626 π₯ 10 β34 )(2.998 π₯ ) 589 π₯ 10 β9 πΈ=3.37 π₯ 10 β19 π½ πΈ=(3.37 π₯ 10 β19 )(6.022 π₯ ) πΈ=2.03 π₯ π½/πππ
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Quantum Mechanics Physics of the small New in the early 20th century
High level math Thought experiments Led to many advances in technology
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SchrΓΆdingerβs Cat Thought Experiment
Cat, vial of poison, Geiger counter with radioactive sample in a sealed box. Canβt know if cat is alive or dead without interrupting the experiment (opening the box) The cat is considered BOTH alive and dead
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Heisenberg Uncertainty
Limit to what we can know The more precisely the momentum of a particle is known the less precisely the position can be known βπ₯βπβ₯ β 2
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SchrΓΆdinger Wave Equation
Differential equation for wave functions of particles πβ πΏ πΏπ‘ Ξ¨ π,π‘ =[ β β 2 2π π» 2 +π(π,π‘)]Ξ¨(π,π‘)
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Wave Equation Solutions
Solving the wave equation for an electron provides wave functions that include quantum numbers that describes where there is a high probability of finding an electron
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Principle Quantum Number
Denotes the principle energy level n Integers equal to or larger than 1 n = 1, 2, 3, β¦
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Angular Quantum Number
Denotes the sublevel within an energy level β (lower case cursive L) Integers ranging from 0 to nβ1 0 = s, 1 = p, 2 = d, 3 = f, 4 = g,β¦.
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Magnetic Quantum Number
Denotes the orbitals in each sublevel mβ Integers ranging from ββ to +β β = 0, mβ = 0 (1 s orbital) β = 1, mβ = β1, 0, +1 (3 p orbitals) β = 2, mβ = β2, β1, 0, +1, +2 (5 d orbitals)
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Spin Quantum Number Describes the magnetic property of the electron, βspinβ ms Β½ or βΒ½
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Pauli Exclusion Principle
2 electrons in an atom canβt have the same set of quantum numbers Each orbital can hold up to 2 electrons Must be different βspinβ
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Ξ¨2 Probability density and radial distribution function
Describes the shape of an orbital
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Orbitals
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Orbitals
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Orbitals
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Electron Configurations
Describes the number of electrons in an atom and their location 1s2 Number of electrons in sublevel Energy level Sublevel
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Aufbau Principle Electrons will fill the lowest available orbitals
Na (Regents) 1s22s22p63s1 (AP)
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Electron Config Examples
Be 1s22s2 C 1s22s22p2 F 1s22s22p5 S 1s22s22p63s23p4
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Electron Configurations
Sublevels overlap each other More overlap the farther away from the nucleus K 1s22s22p63s23p64s1 4s sublevel is lower in energy than the 3d sublevel
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Electron Orbital Configuration
Sublevel order 1s 2s 2p 3s 3p 3d 4s 4p 4d 4f 5s 5p 5d 5f 5g 6s 6p 6d 6f 6g 6h 7s 7p 7d 7f 7g 7h 7i
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Condensed Electron Configβs
Sr 1s22s22p63s23p63d104s24p65s2 Use noble gas for inner electrons Sr [Kr]5s2
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Orbital Diagram Visual representation Electrons as arrows H He
Lines or boxes Electrons as arrows Different βspinβ, different arrow direction H He 1s 1s
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Orbital Diagram 1s 2s Li Be B 1s 2s 1s 2s 2p
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Hundβs Rule Lowest energy is achieved when the number of electrons with the same spin is maximized C N 1s 2s 2p 1s 2s 2p
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Electron Config Anomalies
Because of how close in energy some sublevels are, some transition metals have partially filled ns sublevels with partially filled (n-1)d sublevels Sometimes ns = 0 Have to be determined experimentally
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Electron Config Anomalies
Cr [Ar]4s23d4 [Ar]4s13d5 Cu [Ar]4s23d9 [Ar]4s13d10
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Magnetism Paramagnetism Diamagnetism
Weak attraction to magnetic field due to unpaired electrons Diamagnetism Weak repulsion to magnetic field due to paired electrons
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Photoelectron Spectroscopy
Experimental method used to determine the electronic structure of an atom Photoemission Spectroscopy PES Based on the Photoelectric Effect specifically the Work Function
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Photoelectric Effect (Review)
Light shining on a photo-sensitive metal plate will emit electrons. Energy of Photon = Energy of ejected electron + work needed to eject electron (work function, Ξ¦) βπ= πΎπΈ πππ₯ + π
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Photoelectron Spectroscopy
Graph shows relative number of electrons and amount of energy required to remove them. Binding energy Often energy scale on x axis is reversed Zero to the right end Not always, have to pay attention!
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Photoelectron Spectroscopy
Inner most electrons Outer most electrons
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Periodic Table Developed by Mendeleev in 1869
Initially arranged by atomic mass Certain elements rearranged by chemical properties Predicted missing elements with very accurate prediction of missing elementβs properties
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Periodic Table Henry Moseley determined atomic numbers using X-ray Spectroscopy Proved Mendeleevβs Periodic Table correct Died in WWI at age of 27 Most likely would have won 1916 Nobel Prize Not awarded to anyone in 1916
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Periodic Table
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Periodicity (Regents Review)
Atomic Radius β Size of an atom Ionic Radius β Size of an ion Ionization Energy β energy required to remove outermost electron Electronegativity β ability to attract electrons while in a compound
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Periodicity (Regents Review)
Atomic Radius Decreases left to right Increases top to bottom Ionic Radius
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Periodicity (Regents Review)
Ionization Energy Increases left to right Decreases top to bottom Electronegativity
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Periodicity (Regents Review)
Metallic Character Decreases left to right Increases top to bottom
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Periodicity (Regents Review)
Valence Electrons Electrons in outermost occupied energy level Elements in same group have similar physical and chemical properties because they have the same number of valence electrons
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Coulombβs Law Electrons in an atom are attracted to the protons in the nucleus Electrons are also repelled by other electrons in the atom Attraction of outer electrons to nuclear protons is diminished by inner electrons βShieldingβ
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Effective Nuclear Charge, Zeff
Actual attractive force felt by electrons Zeff = Z β S Z = nuclear charge S = shielding constant Approx = # of core electrons
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Atomic Radius 2 types of measurements
van der Waals radius = non-bonding Covalent radius = bonding radius
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Atomic Radius Atomic Radius decreases across a period
Additional electrons are in the same energy level Effective nuclear charge is increasing
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Atomic Radius Atomic Radius increases down a group
Additional electrons are in next higher energy level Effective nuclear charge doesnβt change (much)
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Atomic Radius
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Ionic Radius Metals tend to lose electrons when they form ions
Valence electrons are lost The βnewβ valence electrons experience a larger effective nuclear charge, making them even smaller Less repulsion between electrons Na 1s22s22p63s1 Na+ 1s22s22p6
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Ionic Radius Nonmetals tend to gain electrons when they form ions
More valence electrons are added The βnewβ valence electrons experience a smaller effective nuclear charge, making them larger More repulsion between electrons F 1s22s22p5 F- 1s22s22p6
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Ionic Radius For cations, ionic radius decreases across a period
For anions, ionic radius decreases across a period Additional electrons are in the same energy level Effective nuclear charge is increasing
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Ionic Radius Ionic radius increases down a group
Additional electrons are in next higher energy level Effective nuclear charge doesnβt change (much)
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Ionic Radius
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Isoelectronic Series Ions have the same number of electrons
Ionic radius decreases with an increasing nuclear charge
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Ionization Energy Energy required to remove electron
Each successive electron requires more energy to remove 1st < 2nd < 3rd < 4thβ¦.. After valence electrons, there is a large increase in energy to remove
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Ionization Energy
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Ionization Energy Ionization energy increases across a period
Effective nuclear charge is increasing Atomic radius is decreasing Ionization energy decreases down group Valence electron is farther from nucleus Atomic radius increases
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Ionization Energy
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Ionization Energy Anomalies
Transition from group 2 to group 13 Electron is removed from a farther out sublevel, p-sublevel instead of s-sublevel Transition from group 15 to group 16 Electron being removed from group 16 is from a paired orbital, resulting in a half-filled sublevel Repulsion due to pairing helps too
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Electronegativity Electronegativity increases across a period
Effective nuclear charge is increasing Atomic radius is decreasing Electronegativity decreases down group Atomic radius is increasing
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