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Lecture 5 Heat Transfer –Conduction –Convection –Radiation Phase Changes.

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Presentation on theme: "Lecture 5 Heat Transfer –Conduction –Convection –Radiation Phase Changes."— Presentation transcript:

1 Lecture 5 Heat Transfer –Conduction –Convection –Radiation Phase Changes

2 Heat Transfer The 3 mechanisms of heat transfer:

3 Conduction Conduction: transfer of heat resulting from collisions between particles. –Heat travels between two points at different temperatures. Metals = good conductors of heat. –Electrons in metals are highly mobile and transfer energy quickly.

4 Conduction Insulators: poor conductors of heat (glass, wood, air, plastic foam, wool). Hot coals are a poor conductor of heat.

5 Conduction Insulators do not prevent heat flow, they only decrease rate of flow. –Electrons are not mobile – energy transfer very gradual. –Air spaces in many insulators – air is a poor conductor. –Example: snow is a good insulator because of air- spaces.

6 Convection Convection: transfer of heat by the motion of fluid as it rises and sinks. Occurs only in fluids (liquids and gases).

7 Radiant Energy Radiant Energy: a form of energy that does not require a medium (matter) to travel through. Electromagnetic Waves: a wide spectrum of radiant energy which includes visible light. –Travels through a vacuum at 300,000 km/s (186,000 miles/s).

8 Radiant Energy Dark materials are good absorbers of radiant energy.

9 Terms to be familiar with: Thermal Energy: energy matter has due to the vibration of atoms and molecules. –Sum of the kinetic energies of all particles in a sample. Temperature: quantity that indicates how warm or cold an object is relative to some standard. –Related to average kinetic energy per particle.

10 A simulation of the motions of helium gas atoms – slowed down two trillion times from room temperature.

11 Thermal Energy Heat: the thermal energy transferred from one thing to another due to temperature difference. Second Law of Thermodynamics: heat never spontaneously flows from a cold substance to a hot substance. –Energy has a tendency to become more dispersed – greater entropy or disorder.

12 Temperature Celsius Scale – most common temperature scale used worldwide. 0°C – melting/freezing point of water. 100°C – boiling point of water.

13 Absolute Zero: lower limit of temperature at which molecules have lost all kinetic energy = - 273°C The volume of a gas changes by 1/273 of its volume at 0°C with each 1°C change in temperature.

14 Temperature Kelvin Temperature Scale: –Absolute Zero = 0 K K = °C + 273 0°C = 273 K 100°C = 373 K - 273°C = 0 K

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16 Particle collisions within CERN’s Large Hadron Collider have resulted in temperatures exceeding 5 Trillion K.

17 Thermal Energy Thermal Expansion: as temperature increases, molecules move more rapidly and farther apart. –Most materials expand when heated and contract when cooled.

18 Expansion joints in a bridge allow for the structure to expand and contract without buckling.

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21 Different substances expand at different rates.

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23 Three Phases of Water at Earth’s Surface Liquid Solid (Ice) Gas (Vapor) Energy is captured or released upon change from one phase to another

24 Molecular Structure of Ice

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26 Liquid Water H 2 O (l) Water

27 Gas (Steam) H 2 O (g) Steam

28 Water Vapor (Steam) Condenses into liquid droplets

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30 Energy and Change of Phase Ice Ice + Water Water Water + Vapor Vapor Heat of Vaporization Heat of Fusion

31 Energy and Phase Changes Only one or the other can occur - not both at the same time: –Change in temperature –Change in phase


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