Liquids, Solids, Thermodynamics, and Phase Transitions

0.0(0)
studied byStudied by 0 people
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
Card Sorting

1/59

flashcard set

Earn XP

Description and Tags

Comprehensive flashcards covering key concepts from a Chemistry lecture on liquids, solids, thermodynamics, and phase transitions. These cards are designed to help students review and prepare for exams.

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

60 Terms

1
New cards

Solid

Definite shape and volume, fixed position, vibrate due to energy, closely packed.

2
New cards

Liquid

Definite volume, variable shape, short-ranged ordering, ability to move around, packed together.

3
New cards

Gas

Variable shape and volume, random ordering, complete freedom of motion, large amounts of space, can expand/contract.

4
New cards

Volume

Amount of 3D space occupied.

5
New cards

Temperature

Measure of possessed kinetic (thermal) energy.

6
New cards

Kinetic Molecular Theory (KMT)

State of matter depends on the amount of kinetic energy and the strength of attractions between particles.

7
New cards

More Kinetic Energy (KE)

More motion of particles and more freedom possible.

8
New cards

More motion

Higher temperature

9
New cards

Ideal Gas

Particles have complete freedom of motion.

10
New cards

Liquids (KMT)

Limited translational freedom; some particles have enough KE for rotational/vibrational freedom, some do not.

11
New cards

Solids (KMT)

No translational or rotational freedom, only vibrational.

12
New cards

Intermolecular Forces (IMFs)

Attractive forces between opposite charges (Formal/Informal).

13
New cards

Ion-Ion

Cation (+) and anion (-).

14
New cards

Dipole-Dipole

Polar molecules with partial charges (δ+ and δ-).

15
New cards

London Dispersion Forces

Temporary dipole of a nonpolar molecule due to fluctuations in electron distribution.

16
New cards

Hydrogen Bonding

Special type of dipole-dipole interaction involving hydrogen bonded to a very electronegative atom (O, N, F).

17
New cards

Phase Changes (Increasing Energy)

Melting/Fusion (s -> l), Sublimation (s -> g), Boiling/Vaporization/Evaporation (l -> g).

18
New cards

Phase Changes (Decreasing Energy)

Solidification/Freezing (l -> s), Condensation (g -> l), Deposition (g -> s).

19
New cards

Vaporization

Occurs at the surface of a liquid; molecules with enough KE overcome IMFs.

20
New cards

Vapor Pressure

Amount of molecules in gas phase above its liquid, dependent on molecule and temperature.

21
New cards

Condensation

Some gas molecules lose energy due to collisions and are recaptured by the liquid.

22
New cards

Open Container (Vaporization/Condensation)

Vapor escapes and spreads out, rate of vaporization > rate of condensation; net loss of liquid.

23
New cards

Closed Container (Vaporization/Condensation)

Vapor cannot spread out; at equilibrium, rate of vaporization = rate of condensation.

24
New cards

Volatile Liquids

Liquids that evaporate easily.

25
New cards

Nonvolatile Liquids

Hard to evaporate.

26
New cards

Boiling Point

The temperature at which a liquid's vapor pressure equals the external pressure.

27
New cards

Enthalpy

Thermal energy; enthalpy of vaporization.

28
New cards

Sublimation

Solid to gas; no liquid stage.

29
New cards

Deposition

Gas to solid.

30
New cards

Specific Heat

Related to heat; resistance to change in temperature; molecular and phase-specific.

31
New cards

Phase Diagram

Plot of pressure vs. temperature; experimentally determined.

32
New cards

Triple Point

Pressure and temperature where all 3 states are in equilibrium.

33
New cards

Critical Point

Pressure and temperature above which a substance exists as a 'Supercritical Fluid'.

34
New cards

Thermodynamics

Study of energy and its relationship to heat and work.

35
New cards

Zeroth Law of Thermodynamics

If system A is in equilibrium with system B, and system B is in equilibrium with system C, then A is also in equilibrium with C.

36
New cards

First Law of Thermodynamics

Energy cannot be created nor destroyed, only changed from one form to another.

37
New cards

Calorimetry

Experimental application of 1st law.

38
New cards

Bomb Calorimetry

Holds volume constant; ΔV = 0; ΔU = q = mcΔT.

39
New cards

Enthalpy

H = U + PV; enthalpy = heat at constant pressure; ΔH = q.

40
New cards

Standard State

State of a material at a defined set of conditions (pure gas/solid/liquid at 1 atm, specified temperature, most stable form).

41
New cards

Standard Enthalpy of Change

Enthalpy change when all reactants and products are in standard states.

42
New cards

Standard Enthalpy of Formation

Enthalpy change for a reaction forming 1 mol of a pure compound from its constituent elements in their standard states.

43
New cards

Hess' Law

Any reaction can be written as the sum of formation reactions or their reverses; ΔHrxn = ΣnΔHf(products) - ΣnΔHf(reactants).

44
New cards

Reversible Process

A process that stays in equilibrium the entire time.

45
New cards

Irreversible Process

A process that occurs because of some change (immediate, sudden, etc.).

46
New cards

Spontaneity

Whether a process will occur naturally under a given set of conditions.

47
New cards

Spontaneous Process

Occurs without input of energy.

48
New cards

Nonspontaneous Process

Requires input of energy/change in conditions.

49
New cards

Clausing

Discovered amount of 'reversible heat' (qrev) was related to Temperature (T) and some other quantity, Entropy (S).

50
New cards

Boltzmann

Statistical model of Entropy (probability).

51
New cards

Microstates

Specific configurations of all possible locations and/or energies of atoms/molecules in a system.

52
New cards

Entropy

Disorder, Chaos.

53
New cards

Second Law of Thermodynamics

Entropy of an isolated system must always increase; any isolated system evolves towards equilibrium where entropy is maximized.

54
New cards

Third Law of Thermodynamics

Entropy of a system approaches a constant value as Temperature approaches absolute zero (0 Kelvins).

55
New cards

State Functions

Only final and initial states are considered.

56
New cards

Dissolution

Energy dispersion; less contained particles, more (w, Г).

57
New cards

Gibb's Free Energy

Difficult to determine spontaneity because highly temperature/condition dependent; requires entropy of system and surroundings.

58
New cards

Gibb's Free Energy equation

G = H - TS; energy available for process to occur.

59
New cards

Equilibrium (AG = 0)

Point where a process goes from non-spontaneous to spontaneous.

60
New cards

Calculating Standard Free Energy

Use ΔH° and ΔS° (and T) to find ΔG°.