Temperature (Definition #1 – Macroscopic level Temperature (Definition #1 – Macroscopic level): a property that determines the direction of thermal.

Slides:



Advertisements
Similar presentations
Thermal Properties of Matter
Advertisements

The Kinetic Theory of Matter
Chapter 9- The States of Matter u Gases indefinite volume and shape, low density. u Liquids definite volume, indefinite shape, and high density. u Solids.
States of Matter Chapter 3.
Kinetic Theory and Exothermic/Endothermic Reactions.
The Newtonian World Thermal Physics.
PRESENTATION ON CHEMISTRY THREE STATES OF MATTER BY MRS. IRUM KHALID LECTURER DA SKBZ COLLEG E.
Topic 3.2 Thermal Properties of Matter
Matter. Review States of Matter Solid Liquid Gas Plasma.
Kinetic Molecular Theory. H-ch.13 CP-ch.10 & 12 u Gases indefinite volume and shape, low density. u Liquids definite volume, indefinite shape, and high.
Phases of Matter.
Phases of Matter.
States of Matter and Phase Changes. Kinetic Theory of Matter: Matter is made of particles that are in constant motion – Describes how close together the.
Topic 17: States of Matter Table of Contents Topic 17 Topic 17 Click box to view movie clip.
tivity/states_of_matter/
STATES OF MATTER Chemistry CP.
Chapter 13 States of Matter
 Matter takes up space and has mass  Matter is made of atoms, usually chemically bonded into molecules  Exists in different states.
Chapter 6.  Temperature ◦ Is something hot or cold? ◦ Relative measure.
Chem 1151: Ch. 6 States of Matter. Physical States of Matter Matter can exist as:  Solid  Liquid  Gas Temperature Dependent States
Science Proficiency Review
PHYSICAL BEHAVIOR OF MATTER
Thermal Physics Topic 3.2 Thermal Properties of Matter.
IB Physics Topic 3 – Introduction to Thermo physics Mr. Jean.
Thermal Physics Topic 3.2 Thermal Properties of Matter.
STATES OF MATTER CHAPTER 3. SOLIDS, LIQUIDS, AND GASES 3.1.
TrueFalseStatementTrueFalse Solids have a definite shape and volume, and their particles do not move Liquids have definite shape, not volume, and their.
Chapter 9- The States of Matter u Gases indefinite volume and shape, low density. u Liquids definite volume, indefinite shape, and high density. u Solids.
Ch. 11 States of matter. States of Matter Solid Definite volume Definite shape Liquid Definite volume Indefinite shape (conforms to container) Gas Indefinite.
Chapter 3 Solids, Liquids and Gases. Solids A solid has a definite shape and a definite volume. The particles in a solid are closely locked in position.
 Matter is anything that occupies space and has mass.  Matter is made up of tiny and discrete particles.  These particles are:  Atom.  Molecule.
States of Matter.
Chapter 3 – States of Matter
 Solid  Liquid  Gas  Plasma  Definite Shape and Volume  Particles are often arranged in repeating geometric patterns to form crystals  Some are.
Physical Behavior of Matter Phases of Matter 2 Forms of Energy Kinetic Energy Energy of motion Temperature is the measurement of the average K.E. Higher.
The kinetic theory is an explanation of how particles in matter behave. Kinetic Theory 16.1.
Kinetic molecular theory and liquids and solids
THE GAS LAWS. STATES OF MATTER  States of Matter  Solid state - particles(atoms, molecules, ions, etc) are rigidly stuck in place.  Particles vibrate,
Chapter #12 States of Matter Inter-particle Forces.
The 3 States of Matter. Kinetic Theory : Concepts for “States” of Matter All atoms and molecules are always in Motion Molecules in solids, liquids and.
States of Matter and Gases Unit 9. The States of Matter Solid: material has a definite shape and definite volume Solid: material has a definite shape.
 Solid  Liquid  Gas  Plasma  Solid  Liquid  Gas  Plasma.
States of Matter and Gases Unit 8. The States of Matter Solid: material has a definite shape and definite volume Solid: material has a definite shape.
 Solid  Liquid  Gas  Plasma  Solid  Liquid  Gas  Plasma.
List and define the three states of matter. S-94.
PHYSICS – Simple kinetic molecular model of matter (1)
Ideal Gas Laws. Pressure is defined as force per unit area  The fundamental (S.I.) unit for pressure is the Pascal (Pa), (1Pa = 1N/m 2 ).  Normal (or.
Thermal equilibrium Thermal equilibrium occurs when all parts of the system are at the same temperature. There is no exchange of thermal energy/please.
 Has fixed volume  Has fixed shape  Molecules are held in specific locations  by electrical forces  vibrate about equilibrium positions  Can be.
States of Matter u Matter exists in 4 states: SOLID, LIQUID, GAS, PLASMA Particles move more The state of the matter depends on its temperature.
Thermodynamics Phases (states) of Matter & Latent Heat States of Matter.
Thermal Physics Topic 10.1 Ideal Gases. Boyle’s Law w States that the pressure of a fixed mass of gas is inversely proportional to its volume at constant.
Chapter 10 The Kinetic Theory of Matter. Pre-Class Question Look at the two containers of liquid. Which container has the greater volume of liquid? Look.
3.2 Modeling a Gas. The Mole The mole is the amount of substance which contains the same number of elementary entities as there are in 12 grams of carbon-12.
Solids, Liquids, and Gases
Phases of Matter. Phases An element or a compound can exist in either a solid, liquid or gas These 3 types are called the phases of matter.
Kinetic Theory: all particles of matter are in constant motion. Particles of Matter: Smallest unit of pure substances, atoms or molecules.
Thermal properties You should be able to: -state the basic definitions of calorimetry, such as specific heat capacity and specific latent heats of fusion.
 R = atm L/mol K  Ideal gas equation predicts gas behavior 2.
DO NOW IN M.C. PACKET MATTER QUESTIONS AIM: REGENTS REVIEW TOPIC 4 – MATTER.
Thermal Properties of Matter
States of Matter What are the three main states of matter?
Reading Reference: Section 3.2: pages
Kinetic Molecular Theory
Chapter 13 States of Matter.
Liquids & Aqueous solutions
Thermal Properties of Matter
EDEXCEL Topic 14 PARTICLE MODEL
Kinetic Molecular Theory Video
Particle Theory of Matter
Presentation transcript:

Temperature (Definition #1 – Macroscopic level Temperature (Definition #1 – Macroscopic level): a property that determines the direction of thermal energy transfer between two objects ▪ gives indication of the degree of hotness or coldness of a body, measured by thermometer Thermal equilibrium Thermal equilibrium occurs when all parts of the system are at the same temperature. There is no thermal energy transfer. (This is how a thermometer works) Internal energy / Thermal energy Internal energy / Thermal energy is total potential energy and random kinetic energy of the molecules of a substance Potential energy Potential energy of the molecules arises from the intermolecular forces (bonds). Kinetic energy Kinetic energy of the molecules arises from random translational, vibrational and rotational motion. Heat Heat is the thermal energy transferred from one body or system of higher temperature to another of lower temperature.

Relative atomic mass Relative atomic mass is the mass of an atom in units of 1/12 of the mass of a carbon-12 atom. mole The mole is the amount of substance that contains the same number of atoms/molecules as kg of carbon-12. Molar Mass Molar Mass is the mass of one mole of a substance (kg/mol). 1 mole of a gas at STP occupies 22.4 l (dm 3 ) and contains 6.02 x molecules/mol. Atomic mass unit Atomic mass unit is the mass of 1/12 of the mass of a carbon-12 atom.

Thermal Capacity Thermal Capacity is the amount of thermal energy needed to raise the temperature of a substance/object by one degree Kelvin. Specific heat capacity Specific heat capacity is the amount of thermal energy required to raise the temperature of one kilogram of a substance by one Kelvin. The same amount of thermal energy is released when the temperature decreases by ΔT homogeneous substance: C = mc Amount of energy needed to raise temperature of an object by ∆T K is ∆Q = C∆T Amount of energy needed to raise temperature of 1 kg of a substance by ∆T K is ∆Q = cm∆T Thermal/heat capacity – object “specific” is ‘per kg’ of a substance

Latent heat Latent heat is the thermal energy that a substance/body absorbs or releases during a phase change at constant temperature. L = Q at const. temp. unit: J Specific latent heat Specific latent heat is the thermal energy required for a unit mass of a substance to undergo a phase change. If electrical energy is converted into increase of internal energy of the system, then: Q added = electrical energy = Pt = IVt = Q abosorbed P – power, I – current, V – voltage, t - time

4 Phases (States) of Matter solid, liquid, gas and plasma; ordinary matter – only three phases CharacteristicSolidLiquidGas Volume and shape definite volume and definite shape definite volume but its shape can change – it takes the shape of their containers. neither definite volume nor definite shape Compressibility Almost IncompressibleVery Slightly CompressibleHighly Compressible Bonds = intermolecular forces characterized by high density and the molecules are held in fixed position by strong bonds. Molecules vibrate around a mean (equilibrium) position. density is lower and molecules are further apart without fixed positions Molecules experience little resistance to motion and move freely about. There are still strong forces between the molecules but they are free to move around each other. the forces between molecules are very weak – molecules are essentially independent of one another but they do occasionally collide Comparative Density High Low Kinetic Energy Vibrational Vibrational, rotational, some translational Mostly translational, higher rotational and vibrational Potential Energy HighHigherHighest (ideal gas – zero) Mean molecular Separation r 0 ( size of the particle) > r r 0

Changes of State GASSOLIDLIQUIDFreezing/solidification vaporisation condensation Melting/fusion sublimation Thermal energy given out Thermal energy added Deposition/ Deposition/desublimation

melting While melting, vibrational kinetic energy increases and particles gain enough thermal energy to break from fixed positions. Potential energy of system increases. Melting point Melting point of a solid is the temperature at which it changes state from solid to liquid. Once at the melting point, any additional heat supplied does not increase the temperature. Instead is used to overcome the forces between the solid molecules increasing potential energy. ◌ At the melting point the solid and liquid phase exist in equilibrium. freezing While freezing, particles lose potential energy until thermal energy of the system is unable to support distance between particles and is overcome by the attraction force between them. Kinetic energy changes form from vibrational, rotational and part translational to merely vibrational. Potential energy decreases (It is negative!!! = attraction: intermolecular forces become stronger). boiling While boiling, substance gains enough potential energy to break free from inter-particle forces. Similar to evaporation, the only difference being that energy is supplied from external source so there is no decrease in temperature. condensing While condensing, the energy changes are opposite to that of boiling.

abrupt change The distinguishing characteristic of a phase transition is an abrupt change in one or more physical properties, in particular the heat capacity, and the strength of intermolecular forces. During a phase change, the thermal energy added or released is used to change (increase/decrease) the potential energy of the particles to either overcome or succumb to the inter-molecular force that pulls particles together. In the process, the average kinetic energy will not change, so temperature will not change.

Evaporation Evaporation is a change of phase from the liquid state to the gaseous state that occurs at a temperature below the boiling point. Evaporation causes cooling. A liquid at a particular temperature has a range of particle energies, so at any instant, a small fraction of the particles will have KE considerably greater than the average value. If these particles are near the surface of the liquid, they will have enough KE to overcome the attractive forces of the neighbouring particles and escape from the liquid as a gas. The escape of the higher-energy particles will lower the average kinetic energy and thus lower the temperature. rate of evaporation The rate of evaporation is the number of molecules escaping the liquid per second. Evaporation can be increased by increasing temperature/more particles have a higher KE Increasing surface area/more particles closer to the surface Increasing air flow above the surface (gives the particles somewhere to go to)/ decreasing the pressure of the air above liquid

Evaporation Evaporation – process whereby liquid turns to gas, as explained above - occurs at any temperature below the boiling temperature - occurs only at surface of liquid as molecules escape - causes cooling of liquid Boiling Boiling – process whereby liquid turns to gas when the vapor pressure of the liquid equals the atmospheric pressure of its surroundings - occurs at one fixed temperature, dependent on substance and pressure - occurs throughout liquid as bubbles form, rise to surface and are released temperature of substance remains constant throughout process Distinguish between evaporation and boiling.

Kinetic Model of an Ideal Gas Gas pressure is the force gas molecules exert due to their collisions (with a wall – imaginary or real), per unit area. Assumptions of the kinetic model of an ideal gas. PV = NkT P – pressure, V – volume, N – number of particles, k – Boltzmann constant, T - temperature Gases consist of tiny hard spheres/particles called atoms or molecules. The total number of molecules in any sample of a gas is extremely large. The molecules are in constant random motion. The range of the intermolecular forces is small compared to the average separation of the molecules The size of the particles is relatively small compared with the distance between them No forces act between particles except when they collide, and hence particles move in straight lines. Between collisions the molecules obey Newton’s Laws of motion. Collisions of short duration occur between molecules and the walls of the container and the collisions are perfectly elastic (no loss of kinetic energy).

Temperature is a measure of the average random kinetic energy of the molecules of an ideal gas. Macroscopic behavior of an ideal gas in terms of a molecular model. Increase in temperature is equivalent of an increase in average kinetic energy (greater average speed). This leads to more collisions and collisions with greater impulse. Thus resulting in higher pressure. Decrease in volume results in a smaller space for gas particles to move, and thus a greater frequency of collisions. This results in an increase in pressure. Also, depending on the speed at which the volume decreases, particles colliding with the moving container wall may bounce back at greater speeds. This would lead to an increase in average kinetic energy and thus an increase in temperature. An increase in volume would have an opposite effect.

Application of the "Kinetic Molecular Theory" to the Gas Laws Microscopic justification of the laws

Pressure Law (Gay-Lussac’s Law) Effect of a pressure increase at a constant volume Macroscopically: at constant volume the pressure of a gas is proportional to its temperature: PV = NkT → P = (const) T Microscopically: ∎ As T increases, KE of molecules increase ∎ That implies greater change in momentum when they hit the wall of the container ∎ Thus microscopic force from each molecule on the wall will be greater ∎ As the molecules are moving faster on average they will hit the wall more often ∎ The total force will increase, therefore the pressure will increase

The Charles’s law Effect of a volume increase at a constant pressure Macroscopically: at constant pressure, volume of a gas is proportional to its temperature: PV = NkT → V = (const) T Microscopically: ∎ An increase in temperature means an increase in the average kinetic energy of the gas molecules, thus an increase in speed ∎ There will be more collisions per unit time, furthermore, the momentum of each collision increases (molecules strike the wall harder) ∎ Therefore, there would be an increase in pressure ∎ If we allow the volume to change to maintain constant pressure, the volume will increase with increasing temperature

Boyle-Marriott’s Law Effect of a pressure decrease at a constant temperature Macroscopically: at constant temperature the pressure of a gas is inversely proportional to its volume: PV = NkT → P = (const)/V Microscopically: ∎ Constant T means that the average KE of the gas molecules remains constant ∎ This means that the average speed of the molecules, v, remains unchanged ∎ If the average speed remains unchanged, but the volume increases, this means that there will be fewer collisions with the container walls over a given time ∎ Therefore, the pressure will decrease