unit 3: intermolecular forces

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40 Terms

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intermolecular forces

forces that act between molecules

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london dispersion forces/dispersion forces

temporary asymmetric distribution of electrons that cause short-lived dipoles in all atoms and molecules

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dipole-induced dipole interactions

a polar molecule induces a diple in a nearby nonpolar molecule

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dipole-dipole interactions

attraction between poles of two polar molecules

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hydrogen bonding

the interactions between a hydrogen covalently bonded to an N, O, or F molecule with another N, O, or F atom on another molecule

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states of matter

atoms and molecules with stronger intermolecular forces require more energy to pull apart

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vapor pressure

the pressure exerted by vapor at thermodynamic equilibrium with its liquid/solid phase in a closed system

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ionic solids

  • form a crystal/lattice structure and have high melting and boiling points

    • coulomb’s law applies → larger size of the atoms in the ions decreases lattice energy

      • lattice energy increases as ion charge increases and as the distance between atoms decreases (smaller atoms have higher lattice energy)

    • poor electrical conductors as a solid → but, good conductors when aqueous or molten since the ions can move freely

    • typically brittle and crack/shatter when enough pressure/stress is applied because the ions shift out of their lattice

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covalent network

  • each atom is connected to others with strong covalent bonds

    • carbon & silicon usually do this since they can form 4 bonds

    • high melting/boiling points and poor electrical conductivity (in all forms)

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metallic solids

  • form a crystal array of nuclei with core electrons while the valence electrons are delocalized and move throughout the solid

    • very good conductors

    • malleable, ductile; don’t crack/break because the metallic bond is nondirectional

      • the electrons aren’t affected much by force so they contribute to the malleable metallic properties

    • high melting/boiling points

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molecular solids

  • not held together by chemical bonds, but instead are held together by weak IMFs

    • low melting/boiling points, poor conductors

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solids

  • come in 2 structure types:

    • crystalline: highly ordered, repeating structure

    • amorphous: lacking a single repeating pattern

  • both types are hard and rigid

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ideal gas law

  • an equation used to approximate the macroscopic properties of gases

    • PV = nRT

      1. P = pressure (in atm/mmHg/torr, 1 atm = 760 mmHg = 760 torr)

      2. V = volume (usually liters)

      3. n = number of gas particles (moles)

      4. R = gas constant → MUST match pressure units

      5. T = temperature (in Kelvin → add 273 to Celsius units)

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total pressure

in a gas mixture, (P total) is equal to the sum of the partial pressures of each gas in the mixture

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partial pressure of a gas

the pressure exerted by one gas in a mixture

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kinetic molecular theory

the KMT for gases is a model that helps explain the macroscopic properties of gases

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ideal gas assumptions

  1. temperature is roughly equal to kinetic energy (K = 1/2mV^2)

  2. gas particles have no IMFs

  3. gas particles take up negligible volumes

  4. gas particles are in constant random motion and do not lose energy when they collide

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diffusion

the movement of gas particles from areas of high concentration to low concentration

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effusion

the movement of gas particles through a small hole/mean free path (only one particle can move through at a time)

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deviations from ideal behavior!

  1. intermolecular forces become significant, causing the gas particles to stick together, resulting in less-than-ideal pressures

    • extremely high pressures where gas particles are pressed close together

    • low temperatures or temperatures close to boiling point → cannot escape IMF pulls

    • gas particles with stronger IMFs deviate more often

  2. the volume of gas particles becomes significant at extremely tiny volume/pressure

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heterogeneous mixture

mixture of 2+ substances with an inconsistent composition throughout

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homogenous mixture

solution, a mixture of 2+ substances where the composition is consistent throughout

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molarity

number of moles of solute in 1 liter of solution

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chromatography

  • separates chemical species by taking advantage of IMF strength within and among the components of the solution

    • separates a mixture into component parts

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paper chromatography

  • the mixture sample is placed on a piece of filter paper, which is dipped into a liquid

    • solvent moves up the paper through capillary action

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mobile phase

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stationary phase

mixture sample

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retention (Rf) value

solute distance traveled Ă· solvent distance traveled (will be <1)

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thin layer chromatography

replace paper with special-coated, thin glass

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column chromatography

  • components travel down instead of up

    • fractions/elutions: collected molecules

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distillation

a laboratory technique that separates a mixture of 2+ liquids into their component parts by tracking advantage of differing boiling points

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distillate

collected liquid

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electromagnetic radiation

  • has properties of both waves and particles

    • travels at the speed of light

    • quantized energy, comes in photons

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microwave absorption

can change the rotational level of the molecule

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infrared wave absorption

can change the vibrational energy level of the molecule

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ultraviolet wave absorption

can increase the electron energy level/move electrons to an excited state

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photoelectric effect

the emission of electrons (photoelectrons) when electromagnetic radiation hits a material (usually solid elemental metal)

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E = hv

(energy = frequency x planck’s constant)

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c = λv

(speed of light constant = wavelength x frequency)

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spectrophotometer

used to measure how solute concentration in a solution affects the amount of light absorbed by a solution