© 2010 Pearson Education, Inc. Conceptual Physics 11 th Edition Chapter 16: HEAT TRANSFER Conduction Convection Radiation Newton’s Law of Cooling Global.

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Presentation transcript:

© 2010 Pearson Education, Inc. Conceptual Physics 11 th Edition Chapter 16: HEAT TRANSFER Conduction Convection Radiation Newton’s Law of Cooling Global Warming and Greenhouse Effect

© 2010 Pearson Education, Inc. Heat Transfer Objects in thermal contact at different temperatures tend to reach a common temperature in three ways: [Image from Beodom.com Copyright Ecovolve S.A.S

© 2010 Pearson Education, Inc. Conduction Transfer of internal energy by electron and molecular collisions within a substance, especially a solid

© 2010 Pearson Education, Inc. Conduction Conductors Good conductors conduct heat quickly. –Substances with loosely held electrons transfer energy quickly to other electrons throughout the solid. Example: Silver, copper, and other solid metals [image of kettle downloqaded Feb from ]

© 2010 Pearson Education, Inc. Conduction Poor conductors are insulators. –molecules with tightly held electrons in a substance vibrate in place and transfer energy slowly—these are good insulators (and poor conductors). Examples: Glass, wool, wood, paper, cork, plastic foam, air [image downloaded Feb from ]

© 2010 Pearson Education, Inc. Insulation Doesn’t prevent the flow of internal energy Slows the rate at which internal energy flows Example: Rock wool or fiberglass between walls slows the transfer of internal energy from a warm house to a cool exterior in winter, and the reverse in summer. [image downloaded Feb from ]

© 2010 Pearson Education, Inc. Convection Transfer of heat involving only bulk motion of fluids Examples: Visible shimmer of air above a hot stove or above asphalt on a hot day Visible shimmers in water due to temperature difference

© 2010 Pearson Education, Inc. Convection Reason warm air rises Warm air expands, becomes less dense, and is buoyed upward. It rises until its density equals that of the surrounding air. Example: Smoke from a fire rises and blends with the surrounding cool air. [animation from ]

© 2010 Pearson Education, Inc. Winds Result of uneven heating of the air near the ground –Absorption of Sun’s energy occurs more readily on different parts of Earth’s surface. Sea breeze –The ground warms more than water in the daytime. –Warm air close to the ground rises and is replaced by cooler air from above the water. –At night the ground cools faster, and the cycle is reversed

© 2010 Pearson Education, Inc. Radiation Transfer of energy via electromagnetic waves such as light or infrared.

© 2010 Pearson Education, Inc. Radiation Transferred energy Exists as electromagnetic waves ranging from long (radio waves) to short wavelengths (X-rays) In visible region, ranges from long waves (red) to short waves (violet) [image from ]

© 2010 Pearson Education, Inc. Wavelength and Frequency

© 2010 Pearson Education, Inc. Radiation Every object above absolute zero radiates. From the Sun’s surface comes visible light, or solar radiation, which we can see. From the Earth’s surface comes terrestrial radiation in the form of infrared waves below our threshold of sight. [image downloaded Feb from ] Image in reflected, visible light Image in emitted, infrared radiation

© 2010 Pearson Education, Inc. Blackbody Radiation Frequency of radiation is proportional to the absolute temperature of the source ( ).

© 2010 Pearson Education, Inc. Radiation Range of temperatures of radiating objects Room-temperature emission is in the infrared. Temperature above 500  C, red light emitted, longest waves visible. About 600  C, yellow light emitted. At 1500  C, object emits white light (whole range of visible light).

© 2010 Pearson Education, Inc. Absorption and Emission Any material that absorbs more than it emits is a net absorber. Any material that emits more than it absorbs is a net emitter. Net absorption or emission is relative to temperature of surroundings. Good absorbers are good emitters Poor absorbers are poor emitters [image from ]

© 2010 Pearson Education, Inc. Reflection of radiant energy Any surface that reflects very little or no radiant energy looks dark Examples of dark objects: eye pupils, open ends of pipes in a stack, open doorways or windows of distant houses in the daytime Good reflectors are poor absorbers. Poor absorbers are poor emitters. A white container will radiate heat more slowly than a black container

© 2010 Pearson Education, Inc. Newton’s law of cooling: Rate of cooling ~  T Rate is proportional to the temperature difference,  T, between the object and its surroundings Also applies to rate of warming Examples: Warmer house leaks more internal energy to the outside than a house that is less warm. Frozen food will warm faster in a warm room than in a cold room. [ image downloaded Feb from ]

© 2010 Pearson Education, Inc. Greenhouse effect Named for a similar temperature-raising effect in florists’ greenhouses

© 2010 Pearson Education, Inc. Greenhouse Gases The Earth’s atmosphere contains mostly Nitrogen and Oxygen, both of which are transparent (non-absorbing) of both visible and infrared radiation Certain gases are transparent for visible radiation, but absorbing for infrared radiation These are called “greenhouse gases”: –Carbon Dioxide –Water vapour –Methane –Nitrous oxide [image from ]

© 2010 Pearson Education, Inc. Greenhouse Effect on Earth Energy absorbed as visible light from the Sun Part reradiated by Earth as longer-wavelength infrared radiation Terrestrial radiation absorbed by atmospheric greenhouse gases and re-emitted back to Earth. Equilibrium temperature determined by concentration of greenhouse gases in the atmosphere More greenhouse gases means higher temperature earth

© 2010 Pearson Education, Inc. To examine times before systematic direct measurements began in 1958, scientists rely on data from bubbles trapped in polar ice cores. For the past several thousand years, up until the last couple of centuries, average CO 2 concentration hovered in the 250 to 280 ppmv range.