Unit 3: IMF, Gas Laws

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41 Terms

1
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Boyle’s Law

P1V1 = P2V2

2
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Charles’ Law

V1     V2

T1 = T2

  • pressure and moles are constant

3
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Gay-Lussac’s Law

P1      P2

T1  =  T2

  • volume and moles are constant

4
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Avogadro’s Law

V1    V2

n1 =  n2

  • pressure and temperature are constant

5
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Ideal Gas Law

PV = nRT

6
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Combined Gas Law

  • when number of moles of gas is constant

<ul><li><p>when number of moles of gas is constant</p></li></ul><p></p>
7
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Dalton’s Law of Partial Pressures

Ptotal = PA + PB + PC

8
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Open system

system that allows the open transfer of energy and matter/mass

9
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Closed system

system that allows the transfer of energy only

10
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Isolated system

system that does not allow the transfer of either energy or matter

11
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System

the volume that contains matter chemical and physical properties

12
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Intensive property

Amount independent; properties with values that do not add

  • EX: temperature and pressure

    • two water samples at 100 degree C do not total 200 when poured together

13
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Extensive property

Amount dependent; properties that do add together

  • EX: volume and moles

14
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State functions

depends only on how it ends (change of final - initial)

  • EX: temperature, volume, pressure, moles of gas, enthalpy, entropy, internal energy, Gibbs free energy

15
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Path function

function that keeps track of what is happening between the beginning and end

  • EX: heat, q, and work, w

16
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KMT assumptions

  1. gas particles have no volume

  2. gas particles undergo elastic collision (KE is conserved)

  3. gas particles have a KE that is proportional to temperature

  4. gas particles have a velocity that varies as the inverse square of the mass

17
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Which KMT assumptions are flawed?

  1. Gas particles DO have volume

  2. Gas particles can undergo collision that are inelastic (EX: water that sticks at room temp)

18
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At room temp, which of the naturally diatomic atoms is solid at room temp?

I2

19
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At room temp, which of the naturally diatomic atoms is liquid at room temp?

Br2

20
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Molecular Weight

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21
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Density (also include substitution into IGL)

p = m/v

<p>p = m/v</p>
22
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What is the volume of 1 mole of gas at STP?

22.4 L

23
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Consider the Maxwell-Boltzmann distribution of gases, if m stays constant, then as T increases…

V increases; KE increases

24
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Consider the Maxwell-Boltzmann distribution of gases, if T stays constant, then as m increases…

V decreases

25
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Graham’s Law of Diffusion/Effusion

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26
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What are the ideal conditions for an ideal gas?

Collisions are rare and elastic

27
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How can you manipulate each variable of IGL to make conditions of a gas more ideal?

  • P is low so don't collide

  • V is large so don't collide

  • n is small so don't collide

  • T is large so don't stick

28
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Consider the van der Waals correction factors, what does “a” correct?

“a” corrects for stickiness aka IMF

  • Large gases (molecular weight) and polar gases have large a, while small nonpolar gases have small a.

29
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Consider the van der Waals correction factors, what does “b” correct?

“b” corrects for size

  • Large molecules (molecular weight) have large b, small molecules have small b.

30
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Dispersion forces increase as

Molecular weight increases

31
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Dipole-dipole forces increase as

The change in electronegativity increases

32
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Hydrogen bonding increases as

the number of hydrogen bonds increase OR N-H < O-H

33
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Ionic IMF increases as 

Charge density increases (charge number and size)

34
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Define boiling point and relationship to IMF

Bulk phenomenon in which the atmospheric pressure equals the vapor pressure of the liquid, causing the liquid to become a vapor.

  • Direct to IMF.

35
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Define surface tension and relationship to IMF

Surface phenomenon in which an inward force reduces the surface area of liquid. This is why liquids like H2O bead up on windrows in the rain.

  • Direct to IMF.

36
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Define capillary action and relationship to IMF

Surface phenomenon in which the liquid climbs the walls of the container because of IMF.

  • Direct to IMF.

37
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Define viscosity and relationship to IMF

Tendency of a liquid to resist pouring because of IMF attraction to bulk solution.

  • Direct to IMF.

38
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Define Heat of Vaporization and relationship to IMF

The energy in IMF that must be overcome for a liquid on the surface to vaporize (become gas)

  • direct to IMF

39
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Define vapor pressure and relationship to IMF

Pressure of the vapor above the surface of a liquid

  • inverse to IMF

40
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Define evaporation rate and relationship to IMF

How quickly a liquid will vaporize from the surface of a liquid

  • inverse to IMF

41
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Order the h-bonds

NH3 < HF < H2O

  • NH3 - small EN even though it has 3 h bonds

  • HF - larger EN but only one h bond

  • H2O - sizeable EN and 2 h bonds