Chem 11 Unit 8: Atomic theory (2-1)

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Properties of Metals (5)

  • Solid at room temp (Except Hg)

  • Shiny/lustrous when freshly cut/polished

  • Good conductors of heat + energy

  • Generally malleable & ductile

  • Forms cations

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Properties of Metalloids (5)

  • When temp increases

    • Metal → conductivity decreases

    • Metalloids → conductivity increases

  • B, Si, Ge, As, Sb, + Te = confirmed metalloids

  • Po + As = debateable

    • Po = metal OR metalloid

    • As = Non-metal OR metalloid

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Properties of Non-metals (4)

  • Usually gases/brittle solids at room temp (except liquid bromine)

  • Bad conductors of heat and energy

  • Solids are dull to lustrous in appearance and opaque to translucent

  • Forms anions

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Periodic table trend principles (3)

  1. e- in large orbits = farther from the nucleus, less attraction to p+ bc more shielding

  2. More p+ = more attraction for e- from nucleus→ effective nuclear charge (Zₑff)

  3. e- in the same subshell repel each other

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Atomic Radius (3)

Measure of the radius from the nucleus to the Ve- in an atom

  • Down group → AR increases: More shells (higher n value) + shielding

  • Across period → AR decreases: Zeff & Protons increases (Added e- joins same orbital)

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Ionic Radius (4)

AR of an ion

  • Cations = smaller than neutral

    • Loses electrons so AR decreases

  • Anions = larger than neutral

    • Gains elections so AR increases

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Ionization Energy (IE) (6)

Amount of energy needed to remove an e-

  • First ionization energy (IE₁): the energy required to remove the first e-

  • Trend = opposite to AR, small AR → high IE

    • Elements on left need to get rid of e- to become stable

    • Elements on right need to gain e- to become stable

  • Exceptions: O = lower IE₁ than N bc O wants to lose 1e- to become half filled

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Electronegativity (EN) (5)

The ability to attract e-

  • Measurement of an atom’s Zeff on OTHER atoms

  • Atoms w/ high EN pull bonded e- closer to their nuclei

  • Noble gasses have no EN value (shells stable)

  • EN has the same trend as IE

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Metallic Character (2)

  • Down group = more metallic

  • Across period = less metallic

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Intramolecular interactions (2)

  • Occur WITHIN molecules/compounds/crystals

  • Includes: ionic, covalent, metallic bonds

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Ionic Bonds (5)

  • Forms when large difference between EN and IE of both atoms (EN >1.8)

  • Metal w/ low IE/EN transfers Ve- → Non-metal w/ high IE/EN

  • Electrostatic attraction-both atoms become ions after transfer

  • Sometimes forms into a crystal lattice (Ex. NaCl)

    • Makes compound have a high melting point (Caused by a vast number of attractive forces in structure)

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Covalent bonds (gen) (3)

  • Non-metal and non-metal

  • Share valence electrons

  • Tend to have lower MP than ionic compounds

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Polar Covalent Bonds (3)

  • Forms when EN = 0.5-1.8

    • When e- are pulled more towards one atom bc of higher EN, one side of the moc becomes more negative than the other side (unequal sharing of e-)

      • Causes dipole (One side more negative)

<ul><li><p>Forms when EN = 0.5-1.8</p><ul><li><p>When e- are pulled more towards one atom bc of higher EN, one side of the moc becomes more negative than the other side (unequal sharing of e-)</p><ul><li><p>Causes dipole (One side more negative)</p></li></ul></li></ul></li></ul><p></p>
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Non-polar Covalent Bonds (7)

  • Forms when EN < 0.4

    • Between identical/same charged non-metals

      • EN value = same; ΔEN = 0

    • Collision of atoms = electron clouds overlap

      • Attractive forces (nucleus) may begint o overlap repulsive forces (e-)

        • Pair of Ve- shared between both

        • The electrons will not be more attracted to one nuclei over the other (equidistant)

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Metallic Bonds (3)

  • Protons swarmed by electrons

    • “sea” of electrons makes metal malleable + conductive

    • Forms metallic crystals

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Early Atomic Theory Timeline (6 ppl)

Democritus (he was right all along)

  • First coherent atomic theory

    • Matter is made of tiny indivisible particles called atoms

Aristotle (More influential)

  • Everything is made up of 4 elements: Fire, air, earth, water

  • Criticized Democritus because it didn’t explain properties of matter or chemical reactions

John Dalton

  • First “modern” atomic theory (Revived Democritus’ theory through experiments)

    • Atoms = solid spheres (different types of spheres make up different elements)

  • Proposed Billiard Ball Model

    • Spheres arranged in a triangle

J.J. Thomson

  • Discovered electron (Atoms are not the smallest particles of matter - there are more inside)

    • Aluminum Plates in a Cathode Ray Tube

  • Proposed Plum Pudding Model

    • Positive sphere w/ negative charged particles

Ernest Rutherford

  • Discovered nucleus (proton confirmed + neutron proposed)

    • Gold Foil Experiment: A lot of α particles went through, some rebounded. Like a net.

  • Proposed Planetary/nuclear Model

    • Positive charge in center/nucleus w/ electron surrounding it

    • Flaw: What is stopping the e- from meeting the p+? Atoms would just collapse.

Niels Bohr

  • Positive nucleus w/ electrons orbiting in shells of different energy levels (higher shell = higher energy)

    • Chadwick proposed neutrons

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Periodic Table history (4 ppl - not important?)

William Odling:

  • Proposed elements could be divided into 13 groups based on chemical & physical properties

John Newlands:

  • Assigned H a mass of 1

  • Law of Octaves: Every 8th element shares similar properties (only up to Ca)

    • Did not allow for prediction of new elements. Table had to be rearranged each time a new element was discovered.

Dimitri Mendeleev:

  • Organized elements by atomic mass and properties.

    Recognized periodic recurrence of properties, leaving gaps for undiscovered elements.

  • His (first widely recognized) table helped chemists organize data and predict new properties.

  • Periodic Law: Elements ordered by increasing atomic mass (later revised to atomic number) exhibit similar recurring properties.

Henry Moseley:

  • Proposed atomic number - revised periodic law slightly

  • Elements still grouped by properties, similar properties in the same column

  • Added a column of elements Mendeleev didn’t know about

Modern table:

  • Strutt & Dorn added noble gases in 1894

  • Lanthanides & Actinides added mid 1900’s

  • Continuously changing, currently at 118 elements

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Energy Levels & Orbitals (4)

  • Energy difference betw 2 levels is called the QUANTUM energy

  • Electrons occupy regions of space called orbitals in a particular energy level (THEY DON’T ORBIT)

  • SHELL: The set of orbitals having the same n value

    • Ex. 3rd shell = 3s, 3p, 3d

  • SUBSHELL: A set of orbitals of the same type

    • There’s a set of five 3d orbitals in the 3rd subshell

<ul><li><p>Energy difference betw 2 levels is called the QUANTUM energy</p></li><li><p>Electrons occupy regions of space called orbitals in a particular energy level (THEY DON’T ORBIT)</p></li><li><p>SHELL: The set of orbitals having the same n value</p><ul><li><p>Ex. 3rd shell = 3s, 3p, 3d</p></li></ul></li><li><p>SUBSHELL: A set of orbitals of the same type</p><ul><li><p>There’s a set of five 3d orbitals in the 3rd subshell</p></li></ul></li></ul><p></p>
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Core Notation/Exceptions (4)

  • Anions: Add an electron to the last unfilled subshell

  • Cations: Remove an electron from the highest energy subshell

    • Ex. 4s before 3d

    • Ex. np e- before ns e- before nd e-

  • Exceptions: Cr & Cu - d subshell wants to be half or fully filled (most subshells do, but esp d)

  • Valence: all e- except core e- and filled d or f subshells. Noble gases and isoelectronic atoms/ions have 0 valence.

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Orbital rules (3)

  • Aufbau Principle: Electrons fill the LOWEST energy orbitals first.

  • Pauli Exclusion Principle: Max of 2 electrons per orbital

  • Hund’s Rule: Each orbital must have a single electron before doubling up with an e- of opposite spin

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Isotopes & Percent abundance (3)

  • Isotopes: Different form of same element - Same # protons, diff # neutrons

    • Mass # is always WHOLE (Proton + Neutron)

  • Atomic mass = weighted avg of all existing isotopes

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Emission Spectra (7)

  • When light hits electrons, they jump up a shell

    • If it isn’t the right coloured light, it won’t move

    • Ex. e- that needs red light won’t move if it’s hit with a yellow light

  • When they drop down a shell they release specifically coloured light

  • Proves the existence of e- shells

    • Solid lines of colour are observed

    • If there was no shells, it’d be a blur of colour

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Families / Groups (10)

G1: Alkali Metals

  • Very reactive

  • Reactivity decreases down group

  • Forms 1+ ions

G2: Alkali Earth Metals

  • Reactive but not as much as Alkali Metals

  • Reactivity decreases down group

  • Forms 2+ ions

G3-12: Transition Metals

  • D-orbitals filled last (except Cr, Cu, + Au)

  • Forms many ions (multivalent)

G13: Boron Group

  • Forms 3+ ions

G14: Carbon Group

  • Forms 4+ ions (C can form 4- ions)

G15: Nitrogen Group

  • Forms 3- ions

G16: Oxygen Groups

  • Forms 2- ions

G17: Halogens

  • Very reactive

  • Reactivity increases up group

G18: Noble Gases

  • Very low reactivity, very stable, full Ve- shell

Hydrogen

  • Shares properties w/ many families

<p>G1: Alkali Metals</p><ul><li><p>Very reactive</p></li><li><p>Reactivity decreases down group</p></li><li><p>Forms 1+ ions</p></li></ul><p></p><p>G2: Alkali Earth Metals</p><ul><li><p>Reactive but not as much as Alkali Metals</p></li><li><p>Reactivity decreases down group</p></li><li><p>Forms 2+ ions</p></li></ul><p></p><p>G3-12: Transition Metals</p><ul><li><p>D-orbitals filled last (except Cr, Cu, + Au)</p></li><li><p>Forms many ions (multivalent)</p></li></ul><p></p><p>G13: Boron Group</p><ul><li><p>Forms 3+ ions</p></li></ul><p></p><p>G14: Carbon Group</p><ul><li><p>Forms 4+ ions (C can form 4- ions)</p></li></ul><p></p><p>G15: Nitrogen Group</p><ul><li><p>Forms 3- ions</p></li></ul><p></p><p>G16: Oxygen Groups</p><ul><li><p>Forms 2- ions</p></li></ul><p></p><p>G17: Halogens</p><ul><li><p>Very reactive</p></li><li><p>Reactivity increases up group</p></li></ul><p></p><p>G18: Noble Gases</p><ul><li><p>Very low reactivity, very stable, full Ve- shell</p></li></ul><p></p><p>Hydrogen</p><ul><li><p>Shares properties w/ many families</p></li></ul><p></p>
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Octet Rule (5)

  • All atoms form stable octet when bonding

    • Stable + low-energy config.

  • EXCEPTIONS (sometimes):

    • H makes 1 bond

    • B takes less

    • S and P take more

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Intermolecular Forces (4)

  • Occurs BETWEEN covalent molecules

  • Strength/weakness affects state of matter + chemical properties

    • Strong IMF = High BP (solid/liquid)

    • Weak IMF = Low BP (liquid/gas)

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London Dispersion Forces (11)

  • Weakest force

  • Between 2 non-polar molecules

  • Always present

  • Creates temporary dipole

    • E- from molec1 → nucleus of molec2

      • Molec2 e- repulsed by molec1 e-

  • Attraction increases w/ atomic number

    • Dipole increases when more e- is added

  • Attraction increases w/ larger molecules

    • More spaces to attract

  • If only LDF present → low BP + MP

<ul><li><p>Weakest force</p></li><li><p>Between 2 <strong>non-polar</strong> molecules</p></li><li><p><strong>Always present</strong></p></li><li><p>Creates temporary dipole</p><ul><li><p>E- from molec1 → nucleus of molec2</p><ul><li><p>Molec2 e- repulsed by molec1 e-</p></li></ul></li></ul></li><li><p>Attraction increases w/ atomic number</p><ul><li><p>Dipole increases when more e- is added</p></li></ul></li><li><p>Attraction increases w/ larger molecules</p><ul><li><p>More spaces to attract</p></li></ul></li><li><p>If only LDF present → low BP + MP</p></li></ul><p></p>
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Dipole-dipole (4)

  • 2nd strongest force

  • Between 2 polar molecules

  • δ+ from molec1 attracted to δ- from molec2

  • Stronger bonding = Higher BP + MP

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Hydrogen Bonding (5)

  • Strongest force

  • Type of dipole-dipole (only for H)

  • H bonded with atoms with high EN

    • Ex. N, O, F

  • Molecules share a H