Answers to test yourself questions

Similar documents
Chapter 7.1. Q4 (a) In 1 s the energy is 500 MJ or (i) 5.0! 10 J, (ii) 5.0! 10 kw! hr " 140 kwh or (iii) MWh. (b) In one year the energy is

1. What is the phenomenon that best explains why greenhouse gases absorb infrared radiation? D. Diffraction (Total 1 mark)

Introducing nuclear fission The Fizzics Organization

m, kg, s, ampere, mole, K

MNFFY 221/SIF 4082 Energy and Environmental Physics. 2002

Energy, Temperature, & Heat. Energy, Temperature, & Heat. Temperature Scales 1/17/11

10/31/2017. Calculating the temperature of earth (The greenhouse effect) IR radiation. The electromagnetic spectrum

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group

M10/4/PHYSI/SPM/ENG/TZ1/XX+ Physics Standard level Paper 1. Monday 10 May 2010 (afternoon) 45 minutes INSTRUCTIONS TO CANDIDATES

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Nuclear Physics 2. D. atomic energy levels. (1) D. scattered back along the original direction. (1)

COURSE CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION

Course Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2. Changing climate. 3. Future climate change

u d Fig. 6.1 (i) Identify the anti-proton from the table of particles shown in Fig [1]

Physics Standard level Paper 1

8.5 GREENHOUSE EFFECT 8.6 GLOBAL WARMING HW/Study Packet

molar mass = 0.239kg (1) mass needed = = kg (1) [7]

[2] State in what form the energy is released in such a reaction.... [1]

Most of the energy from the light sources was transferred to the sand by the process of A) conduction B) convection C) radiation D) transpiration

Composition, Structure and Energy. ATS 351 Lecture 2 September 14, 2009

(b) total power required = ( =)360kW; 1

(a) (i) State the proton number and the nucleon number of X.

Course Outline. About Me. Today s Outline CLIMATE SCIENCE A SHORT COURSE AT THE ROYAL INSTITUTION. 1. Current climate. 2.

turbine (a) (i) Which part of the power station provides thermal (heat) energy from a chain reaction?

Energy and Radiation. GEOG/ENST 2331 Lecture 3 Ahrens: Chapter 2

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection.

Chapter 10. Answers to examination-style questions. Answers Marks Examiner s tips. 1 (a) (i) 238. (ii) β particle(s) 1 Electron antineutrinos 1

The Atmosphere is the layer of air surrounding the Earth

( 1 d 2 ) (Inverse Square law);

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface.

Glaciology HEAT BUDGET AND RADIATION

Investigating Planets Name: Block: E1:R6

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

Surface Processes and the Hydrosphere Unit Heating the Earth s Atmosphere Chapter 11 (pg )

Episode 528: Controlling fission

Lithosphere: (Rocky Sphere) Solid, rocky, outer layer of the Earth. Includes the crust and part of the upper mantle. Lithosphere

Write down the nuclear equation that represents the decay of neptunium 239 into plutonium 239.

ATS150 Global Climate Change Spring 2019 Candidate Questions for Exam #1

The greenhouse effect

Section 2: The Atmosphere

When a body is accelerating, the resultant force acting on it is equal to its

2. What are the four most common gasses in the atmosphere and their percentages?

Physics 3204 UNIT 3 Test Matter Energy Interface

,Solar Energy, Greenhouse effect, Convection.notebook October 31, 2016

Very Dynamic! Energy in the Earth s Atmosphere. How Does it Get Here? All Objects Radiate Energy!

Term 3 Week 2 Nuclear Fusion & Nuclear Fission

Nuclear Energy Learning Outcomes

Nuclear Energy Learning Outcomes. Nuclear Fission. Chain Reaction

Kinds of Energy. Defining Energy is Hard! EXPLAIN: 1. Energy and Radiation. Conservation of Energy. Sco; Denning CSU ESMEI ATS 1

Slide 1 / 57. Nuclear Physics & Nuclear Reactions Practice Problems

FOLLOW THE ENERGY! EARTH S DYNAMIC CLIMATE SYSTEM

TRANSMISSION OF HEAT

Theoretical Task 3 (T-3) : Solutions 1 of 9

Radiative Balance and the Faint Young Sun Paradox

Quiz, Physics & Chemistry

Lecture 4: Global Energy Balance

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model.

Learning goals. Good absorbers are good emitters Albedo, and energy absorbed, changes equilibrium temperature

Physics 111. Lecture 36 (Walker: ) Heat Capacity & Specific Heat Heat Transfer. May 1, Quiz (Chaps. 14 & 16) on Wed.

Earth: the Goldilocks Planet

N09/4/PHYSI/SPM/ENG/TZ0/XX+ Physics Standard level Paper 1. Monday 16 November 2009 (afternoon) 45 minutes INSTRUCTIONS TO CANDIDATES

Multiple Choice Questions

ATM 10. Severe and Unusual Weather. Prof. Richard Grotjahn.

Greenhouse Effect. Julia Porter, Celia Hallan, Andrew Vrabel Miles, Gary DeFrance, and Amber Rose

Physical and mathematical models of the greenhouse effect

IB Physics Lesson Year Two: Standards from IB Subject Guide beginning 2016

The Atmosphere - Chapter Characteristics of the Atmosphere

Central Coast Climate Science Education Dr. Ray Weymann

Hand in Question sheets with answer booklets Calculators allowed Mobile telephones or other devices not allowed

Absorptivity, Reflectivity, and Transmissivity

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

Lecture Presentation. Chapter 6. Thermochemistry. Sherril Soman Grand Valley State University Pearson Education, Inc.

Lecture 3: Global Energy Cycle

Lecture # 04 January 27, 2010, Wednesday Energy & Radiation

WEATHER. Review Note Cards

The Greenhouse Effect. Lan Ma

Chapter 2. Heating Earth's Surface & Atmosphere

Unpressurized steam reactor. Controlled Fission Reactors. The Moderator. Global energy production 2000

The Atmosphere. Composition of the Atmosphere. Section 2

Energy Changes in Chemical and Nuclear Reactions

GCSE 0247/02 SCIENCE HIGHER TIER PHYSICS 3

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

Chapter 12: Nuclear Reaction

Energy, Work, and Simple Machines

11/18/2010. Only part of the spectrum we can see. A rainbow of colors, each corresponding to a different wavelength.

The Structure and Motion of the Atmosphere OCEA 101

Ocean s Influence on Weather and Climate

What Is Air Temperature?

Lecture 6. Solar vs. terrestrial radiation and the bare rock climate model.

1. Weather and climate.

3.1and 3.2 Thermal. Rise in temperature in deg C Final temperature in C A B C D

Atmosphere - Part 2. High and Low Pressure Systems

THE EXOSPHERIC HEAT BUDGET

Astronomy 104: Second Exam

Climate Change and Biomes

Trial Examination VCE Physics Unit 1. Written Examination. Suggested Solutions

Chapter 2: The global ledger of radiation and heat

Data and formulas at the end. Exam would be Weds. May 8, 2008

Transcription:

Answers to test yourself questions Topic 8 8. Energy sources a pecific energy is the energy that can be extracted from a unit mass of a fuel while energy density is the energy that can be extracted from a unit volume of fuel. b The available energy is mgh. The energy density is the energy per unit volume that can be obtained and mgh so E mgh D gh V m 3 5 3 ρ 0. 8 75 7. 0 J m ρ a n s the energy is 500 MJ. b n one year the energy is 5.0 0 8 35 0 0. 0 J. 3 a The overall efficiency is 0.80 0.0 0. 0.5 0.05. b.5 3 00.5 80 0 8 8 a The energy produced by burning the fuel is 0 7 30 0 3.0 0 J. Of this 70% is converted to useful 0. 30 3. 0 0 energy and so the power output is P. 0 0 W. 0 0 0. 70 3. 0 0 b The rate at which energy is discarded is P discard. 3 0 W. 0 0 c Use m c θ P to get m Pdiscard. 3 0 5 discard t c. 0 kg s. θ 00 5 5 n time t the energy used by the engine is 0 0 3 t. The energy available is 0.0 3 0 J and so 0 0 3 t 0.0 3 0 t 80 s. The distance travelled is then x vt.0 80. km. The useful energy produced each day is E Pt.0 0 0 0 8. 0 3 J. The energy produced 3 8. 0 by burning the coal is therefore 0. 0 Ec. 0 J. o the mass of coal to be burned is Ec. 0 m 7. 0 kg per day. 30 0 physics for the B Diploma Cambridge University Press 05 ANWER TO TET YOURELF QUETON 8

7 a The fissionable isotope of uranium is U 35. This is found in very small concentrations in uranium ore which is mostly U 38. Enrichment means increasing the concentration of U 35 in a sample of uranium. b The moderator is the part of the nuclear reactor where neutrons released from the fission reactions slow down as a result of collisions with the atoms of the moderator. The temperature of the moderator can be kept constant with a cooling system that removes the excess thermal energy generated in the moderator. c Critical mass refers to the least mass of uranium that must be present for nuclear fission reactions to be sustained. f the mass of uranium is too small (i.e. below the critical mass) the neutrons may escape without causing fission reactions. 35 0 8 a The reaction is U+ 0n 5Xe + 38r + 0n. The mass difference is δ ( 35. 03 0. 0005) +. 008 5 ( ( 3. 3 5 0. 0005) + ( 3. 5 30 38 0. 0005) +. 0085) ) 0. 8 33 u And so the energy released is E 0.833 3.5c MeVc - 85 MeV. b With N reactions per second the power output is N 85 MeVs -. n other words, N 85 0. 0-00 0 N.8 0 8 s -. a One kilogram of uranium corresponds to 000. moles and so..0 0 3.57 0 35 nuclei. Each nucleus produces 00 MeV and so the energy produced by kg (the energy density) is.57 0 00 0. 0-8 0 3 J kg -. 3 8 0 b. 7 0 kg 30 0 500 0 0 a The energy that must be produced in s is E. 5 0 J. Hence the number of fission 0. 0. 5 0 reactions per second is 3. 0. 00 0. 0 b The number of nuclei required to fission per second is 3. 0 which corresponds to 3. 0 5. 5 0 mol, i.e. a mass of.5 0-5 35 0-3.5 0-5 kg s -. 3. 0 0 control rods (can be raised or lowered) generator fuel rod control rods (can be raised or lowered) fuel rod coolant (pressurised water) pump pressurised water reactor (PWR) water water generator gas-cooled reactor pump coolant (carbon dioxide gas) solid moderator (graphite) a i fuel rods are pipes in which the fuel (i.e. uranium 35) is kept. ii control rods are rods that can absorb neutrons. These are lowered in or raised out of the moderator so that the rate of reactions is controlled. The rods are lowered in if the rate is too high the rods absorb neutrons so that these neutrons do not cause additional reactions. They raised out if the rate is too small leaving the neutrons to cause further reactions. iii The moderator is the part of the nuclear reactor where neutrons released from the fission reactions slow down as a result of collisions with the atoms of the moderator. The temperature of the moderator can be kept constant with a cooling system that removes the excess thermal energy generated in the moderator. ANWER TO TET YOURELF QUETON 8 physics for the B Diploma Cambridge University Press 05

b t is kinetic energy of the neutrons produced which is converted into thermal energy in the moderator as the neutrons collide with the moderator atoms. A solar panel receives solar radiation incident on it and uses it to heat up water, i.e. it converts solar energy into thermal energy. The photovoltaic cell converts the solar incident on it to electrical energy. 3 a The power that must be supplied is 3.0 kw and this equals 700 A 0.70 0.50. Hence 700 A 0.70 0.50 3.0 0 3 A m. b 85 kw 5 kw 30 kw 30 kw The power that is provided is 0.5 0 A and this must equal mc θ 300 00 35 0 0. 300 00 35 Hence 0. 5 700 A A. 5 m. 0 0 5 The power incident on the panel is 00.0 0.0 0W. The energy needed to warm the water is 7 mc θ 50 00 30.8 0 7 7. 8 0 J and so 0 t. 8 0 t. 3 0 s 3. hr. 0 a From the graph this is about T 338 K b P A 00 800W c The useful power is the 30 W that is extracted. The efficiency is thus 30 0. 0. 800 7 The power supplied at the given speed is (reading from the graph) 00 kw. Hence the energy supplied in 00 hrs is 00 0 3 000 0 0 3. 0 J. 8 We look at the power formula for windmills, P 3 ρ Av to deduce: a i the area will increase by a factor of if the length is doubled and so the power goes up by a factor of, ii the power will increase by a factor of 3 8 iii the combined effect is 8 3 b Not all the kinetic energy of the wind can be extracted because not all the wind is stopped by the windmill (as the formula has assumed). n addition, there will be frictional losses as the turbines turn as well as losses due to turbulence. Assumptions include: i no losses of energy due to frictional forces as the turbines turn ii no turbulence in the air iii that all the air stops at the turbines so that the speed of the air behind the turbines is zero (which is impossible). physics for the B Diploma Cambridge University Press 05 ANWER TO TET YOURELF QUETON 8 3

0 The power in the wind before hitting the turbine is 3 ρ Av and right after passing through the turbine is 3 ρ Av so the extracted power is 3 3 3 ρ 5 8 0 8 3 Av ρ Av π. (....0 3 ). 0 kw. From P 3 3 3 ρ Av we get 5 0. A. 0 A 57. m and so πr 57. R. 3 m. The assumptions made are the usual ones (see question ) i no losses of energy due to frictional forces as the turbines turn ii no turbulence in the air, and iii that all the air stops at the turbines so that the speed of the air behind the turbines is zero (which is impossible). The potential energy of a mass m of water is mgh and so the power developed is the rate of change of this energy i.e. m 5 5 gh 500. 8 0. 0. 0 0 W. 3 The potential energy of a mass m of water is mgh and so the power developed is the rate of change of this energy i.e. m V gh ρ gh ρ Qgh. The amount of electrical energy generated will always be less than the energy required to raise the water back to its original height. This is because the electrical energy generated is less than what theoretically could be provided by the water (because of various losses). o this claim cannot be correct. 5 a Coal power plant: chemical energy of coal thermal energy kinetic energy of kinetic energy of turbine electrical energy. b hydroelectric power plant: potential energy of water kinetic energy of water kinetic energy of turbine electrical energy. c wind turbine: kinetic energy of wind kinetic energy of turbine electrical energy. d nuclear power plant: nuclear energy of fuel kinetic energy of neutrons thermal energy in moderator kinetic energy of kinetic energy of turbine electrical energy. Chapter 8. Thermal energy transfer a Energy has to be conserved so whatever energy enters the junction has to leave the junction and so the rates of energy transfer are the same. b The temperature differences are not the same because X and Y have different thermal conductivity. 7 There is; in order to send the warm air that collects higher up in the room downwards. 8 Power is proportional to T 00 and so the ratio is 3 8 300 a A black body is any body at absolute temperature T whose radiated power per unit area is given by σt. A black body appears black when its temperature is very low. t absorbs all the radiation incident on it and reflects none. b A piece of charcoal is a good approximation to a black body as is the opening of a soft drink can. c t increases by 73 + 00 8 73 + 50. 30 a The wavelength at the peak of the graph is determined by temperature and since the wavelength is the same so is the temperature. b The ratio of the intensities at the peak is about. 0... P 3 We have that eσ AT P T i.e. T eσ A. 35 0 0. 800 5. 7 0 5. 00 0 8 78 K. ANWER TO TET YOURELF QUETON 8 physics for the B Diploma Cambridge University Press 05

3 a We must have that σ AT T. d d b Using our knowledge of propagation of uncertainties, we deduce that T d and so T d T T. 0% 0. 005. Hence, T 0.005T 0.005 88. K. 33 a ntensity is the power received per unit area from a source of radiation. b P e σ AT. P 0.0 5.7 0-8.0 (73 + 37) 75 W. Assuming uniform radiation in all directions, the P intensity is then d 75. W m. π π( 5. 0) 3 a magine a sphere centered at the source of radius d. The power P radiated by the source is distributed over the P P surface area A of this imaginary sphere. The power per unit area i.e. the intensity is thus A π d. b We have assumed that the radiation is uniform in all directions. 35 a The peak wavelength is approximately λ 0 0.5 0-5 m and so from Wien s law: λ 0 T. 0-3 Km we find 3. 0 T 50 K. 5 0. 5 0 b The curve would be similar in shape but taller and the peak would be shifted to the left. 3 a Albedo is the ratio of the reflected intensity to the incident intensity on a surface. b The albedo of a planet depends on factors such as cloud cover in the atmosphere, amount of ice on the surface, amount of water on the surface and color and nature of the soil. 37 a The earth receives radiant energy from the sun and in turn radiates itself. The radiated energy is in the infrared region of the electromagnetic spectrum. Gases in the atmosphere absorb part of this radiated energy and reradiate it in all directions. ome of this radiation returns to the earth surface warming it further. b The main greenhouse gases are water vapour, carbon dioxide and methane. ee page 33 for sources. 38 a The energy flow diagram is similar to that in Fig. 8.0 on page 33. b The reflected intensity is 350-50 00 Wm - and so the albedo is 00 0.. 350 c t has to be equal to that absorbed i.e. 50 Wm -. 50 d Use eσt T i.e. (assuming a black body) T 58 K. You must be careful with 8 eσ A 5. 7 0 these calculations in the exam. You must be sure as to whether the question wants you to assume a black body or not. trictly speaking, in a model without an atmosphere the earth surface cannot be taken to be a black body if it were no radiation would be reflected! 3 a The intensity radiated by the surface is and a fraction t of this escapes so we know that 3 t. The intensity of radiation entering the surface is ( α) + α +. This must equal the intensity of radiation leaving the surface which is : ( α) + α +. The intensity of radiation entering the atmosphere is (- α ) and that leaving it is + 3. Hence + 3 (- α ). o we have to solve the equations (we used 3 t ) ( α) + α + + t ( α) These simplify to ( α) + ( α) ( α ) ( α t) t physics for the B Diploma Cambridge University Press 05 ANWER TO TET YOURELF QUETON 8 5

Hence ( α t) ( α) + ( α) ( α t) ( α) ( α) ( α + t) ( α) ( α) α + t Therefore, t α + t ( α) α and 3 t ( α) α + t as required. b The intensity entering is. The intensity leaving is α + 3 +. The intensity leaving simplifies to t ( α) α t α α + + α α + t α + t ( ) t + ( ) ( ) + + α t α α + α t α t α + t α + ( α) α + t ( α + ( α) ) c The intensity radiated by the surface is temperature. Hence ( α) and must equal σ T, where T is the surface α + t ( α) σt α + t ( α) t + α σt ( 0. 30) 350 t + 0. 30 8 5. 7 0 88 t 0. 55 d i Let an intensity be incident on the atmosphere of emissivity e. An amount e will be absorbed and reradiated, an amount α will be reflected and an amount t will be transmitted. By energy conservation we have that e + α + t from which e - α - t as required. t ii We equate α + t ( α) to e σ T where T is the atmosphere temperature to get α (recall that e - α - t) α t α eσt α + t ( ) ( α) σt α + t ( 0. 30) 350 T 8 0. 30 + 0. 55 5. 7 0 T K ANWER TO TET YOURELF QUETON 8 physics for the B Diploma Cambridge University Press 05

0 Radiation is a main mechanism to both the atmosphere and to space. n addition there is conduction to the atmosphere, as well as convection. a Dry sub tropical land has a high albedo, around 0. whereas a warm ocean has an albedo of less than 0.. b Radiation and convection currents are the main mechanisms. c Replacing dry land by water reduces the albedo of the region. Reducing the albedo means that less radiation is reflected and more is absorbed and so an increase in temperature might be expected. The increase in temperature might involve additional evaporation and so more rain. The rate of evaporation from water depends on the temperature of the water and the temperature of the surrounding air. These are both higher in the case of the tropical ocean water and evaporation will be more significant in that case. 3 There is more evaporation in region b implying that it is both warmer and wet. The fact that region b is warmer is further supported by the somewhat greater conduction which would be expected if the difference in temperature between the atmosphere and the land were larger. We have that the original average albedo of the area was 0. 0.0 + 0. 0.3 0.8 and the new one is 0.7 0.0 + 0.3 0.3 0. for a reduction in albedo of 0.0. Hence the expected temperature change is estimated to be C. physics for the B Diploma Cambridge University Press 05 ANWER TO TET YOURELF QUETON 8 7