Episode 315: The inverse square law
|
|
- Candice Perry
- 5 years ago
- Views:
Transcription
1 Episode 315: The invese squae law This episode consides the ways in which the intensity o adiation deceases with distance om the souce. Summay Demonstation + discussion: adiation speading out, and an analogy. (0 minutes) Woked example: Thinking in popotions. (5 minutes) Student expeiment: Estimating the powe output o the Sun. (15 minutes) Student questions: Compaing lamps. (30 minutes) Demonstation + discussion: Radiation speading out and an analogy Set up thee simple demonstations: Bight lamp and phototansisto o othe light mete Micowave souce and detecto Gamma ay souce and Geige counte Show that the intensity o each type o adiation deceases with distance om the souce. (I students have aleady studied adioactivity, they may e awae o the invese squae law o gamma adiation.) Why does the intensity decease with distance? Ty to give two geneal easons. (Asoption and speading out.) Radiation speading out adially coves a igge and igge aea, popotional to, so its intensity deceases as 1/. It can help to think o a toast-utteing gun. The gun can utte a single slice o toast at a distance o 1 m. How can it utte ou slices simultaneously? (lace them in a aay at a distance o m.) How thick will the utte e? (1/4 o oiginal thickness.) Extend this to a 3 3 aay at 3 m, and so on. oint out that the intensity o adiation can e measued in watts pe squae mete (W m - ). Woked example: Thinking in popotions A coalt 60 souce gives a gamma dose ate o 160 μsv h -1 at 1.0 m away. At what distance will the dose ate e 40 μsv h -1? Answe: I the intensity has gone down y a acto o 4, the distance away must have douled to.0 m. O y k/d so I 1 /I d /d 1. 1
2 Student expeiment: Estimating the powe output o the Sun Students can make measuements to estimate the powe output o the Sun, making use o the invese squae law. Note that thee is a good oppotunity hee to discuss the validity o the answe otained. TA 315-1: Summe Sun ememeed Student questions: Compaing lamps Some calculations. TA 315-: Compaing intensities o lamps
3 TA 315-1: Summe Sun ememeed Measuing ightness, hoping to measue distance Compaing enegies incident on the ace allows an estimate o the distance o the Sun. You will need high-poweed lamp, pehaps 00 W (use a saety-patten atten lamp holde wied to plug diectly into a 13 A socket) ule patne Saety The second student is impotant, as one cheek will have to get quite close to the 00 W lamp. What to do Close you eyes, imagine lying on a each and ememe the summe Sun on you ace. How hot did it eel? Now ing you ace up close to a high-powe lamp take cae! A patne should watch you caeully, so that you do not touch the lamp. Aim to eel the same wamth that you ememe in the summe Sun. Recod the distance to the lamp and the powe o the lamp. ew cm 500 light seconds Sun 00 W powe? same osy glow same I lamp Sun ( lamp ) ( Sun ) 3
4 Can you use these data to suggest the powe output o the Sun? Rememe that the Sun is aout 500 light-seconds away. You have 1. Used the 1 / elationship to elate powe outputs. actical advice The incident powe pe squae mete is identical, and so application o the invese squae law will elate the powe outputs o the lamp and Sun to the distances o the two. A calculation can also show that the Sun's adiation at the Eath is o the ode 1 kw m. Saety The second student is impotant, as one cheek will have to get quite close to the 00 W lamp. Social and human context The powe output o the Sun might useully e compaed with the powe output o all human powe stations. Extenal eeence This activity is taken om Advancing hysics chapte 1, 50E 4
5 TA 315-: Compaing intensities o lamps Compaing ightness A low-powe lamp at close ange can oten appea as ight as a high-powe lamp much uthe away. Simila easoning is used to calculate the ightness o stas. Two ilament lamps Hee you compae two incandescent ilament lamps; one maked.5 V, 0.3 A and a second 100 W, 40 V. Assume that appoximately 0% o the powe dissipated y the lamps esults in visile photons eing emitted uniomly, and that oth ae eing un at nomal ightness. 1. Estimate the ightness o the 100 W lamp om 3 metes away, which is the luminous lux density in W m. Calculate how close you must e to the.5 V lamp to see it as eing the same lux density? Two loodlights This question is aout a 3 W icycle headlight and a 300 W exteio secuity loodlight. Both the loodlight and the headlight have appoximately the same shaped eam, a cone that coves appoximately 1 / 10 o a sphee. 3. Estimate the lux density o the icycle lamp om 0 metes away. 4. You pupil has a diamete o appoximately 0.01 m. How much light entes you eyeall pe second? 5. The loodlight looks just as ight as the icycle lamp. How a away is it? 5
6 actical advice All these questions involve use o the invese squae law, sameness o eam shape eing cucial in the questions aout the loodlights. Answes and woked solutions 1. 0 W as light, spead ove a sphee, o adius 3 m: 0 W 4 π 0 W 4 π 3 3 m 0.18 W m. owe as light.5 V x 0.3 A x W. This must spead ove a sphee, to give a lux density o 0.19 W m. 4π 4πI 4 π 0.18 W m 0.6 m W 3. 3 W as light, ocused onto 1 / 10 o sphee, o adius 0 m: 4 π 4 π 3 W ( 0 m) 6 mw m The pupil is catching light at 6 mw m : I A I π W m W. π The loodlight is 100 times moe poweul than a cycle light: m 6
7 π π I The loodlight is 10 times uthe away, 00 m. Extenal eeence This activity is taken om Advancing hysics chapte 1, 40S 7
Inverse Square Law and Polarization
Invese Squae Law and Polaization Objectives: To show that light intensity is invesely popotional to the squae of the distance fom a point light souce and to show that the intensity of the light tansmitted
More informationworking pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50
woking pages fo Paul Richads class notes; do not copy o ciculate without pemission fom PGR 2004/11/3 10:50 CHAPTER7 Solid angle, 3D integals, Gauss s Theoem, and a Delta Function We define the solid angle,
More informationF g. = G mm. m 1. = 7.0 kg m 2. = 5.5 kg r = 0.60 m G = N m 2 kg 2 = = N
Chapte answes Heinemann Physics 4e Section. Woked example: Ty youself.. GRAVITATIONAL ATTRACTION BETWEEN SMALL OBJECTS Two bowling balls ae sitting next to each othe on a shelf so that the centes of the
More informationBlack Body Radiation and Radiometric Parameters:
Black Body Radiation and Radiometic Paametes: All mateials absob and emit adiation to some extent. A blackbody is an idealization of how mateials emit and absob adiation. It can be used as a efeence fo
More informationGaia s Place in Space
Gaia s Place in Space The impotance of obital positions fo satellites Obits and Lagange Points Satellites can be launched into a numbe of diffeent obits depending on thei objectives and what they ae obseving.
More informationB. Spherical Wave Propagation
11/8/007 Spheical Wave Popagation notes 1/1 B. Spheical Wave Popagation Evey antenna launches a spheical wave, thus its powe density educes as a function of 1, whee is the distance fom the antenna. We
More information1) Emits radiation at the maximum intensity possible for every wavelength. 2) Completely absorbs all incident radiation (hence the term black ).
Radiation laws Blackbody adiation Planck s Law Any substance (solid, liquid o gas) emits adiation accoding to its absolute tempeatue, measued in units of Kelvin (K = o C + 73.5). The efficiency at which
More informationUniversal Gravitation
Chapte 1 Univesal Gavitation Pactice Poblem Solutions Student Textbook page 580 1. Conceptualize the Poblem - The law of univesal gavitation applies to this poblem. The gavitational foce, F g, between
More informationMASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 10 Solutions. r s
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Depatment Physics 8.033 Decembe 5, 003 Poblem Set 10 Solutions Poblem 1 M s y x test paticle The figue above depicts the geomety of the poblem. The position
More informationThe geometric construction of Ewald sphere and Bragg condition:
The geometic constuction of Ewald sphee and Bagg condition: The constuction of Ewald sphee must be done such that the Bagg condition is satisfied. This can be done as follows: i) Daw a wave vecto k in
More informationΔt The textbook chooses to say that the average velocity is
1-D Motion Basic I Definitions: One dimensional motion (staight line) is a special case of motion whee all but one vecto component is zeo We will aange ou coodinate axis so that the x-axis lies along the
More informationRelated Rates - the Basics
Related Rates - the Basics In this section we exploe the way we can use deivatives to find the velocity at which things ae changing ove time. Up to now we have been finding the deivative to compae the
More informationGravitation. AP/Honors Physics 1 Mr. Velazquez
Gavitation AP/Honos Physics 1 M. Velazquez Newton s Law of Gavitation Newton was the fist to make the connection between objects falling on Eath and the motion of the planets To illustate this connection
More informationMath 1525 Excel Lab 3 Exponential and Logarithmic Functions Spring, 2001
Math 1525 Excel Lab 3 Exponential and Logaithmic Functions 1 Math 1525 Excel Lab 3 Exponential and Logaithmic Functions Sping, 21 Goal: The goals of Lab 3 ae to illustate exponential, logaithmic, and logistic
More informationDEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS
DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS LSN 10-: MOTION IN A GRAVITATIONAL FIELD Questions Fom Reading Activity? Gavity Waves? Essential Idea: Simila appoaches can be taken in analyzing electical
More informationPhysics: Work & Energy Beyond Earth Guided Inquiry
Physics: Wok & Enegy Beyond Eath Guided Inquiy Elliptical Obits Keple s Fist Law states that all planets move in an elliptical path aound the Sun. This concept can be extended to celestial bodies beyond
More informationHW 7 Help. 60 s t. (4.0 rev/s)(1 min) 240 rev 1 min Solving for the distance traveled, we ll need to convert to radians:
HW 7 Help 30. ORGANIZE AND PLAN We ae given the angula velocity and the time, and we ae asked to ind the distance that is coveed. We can ist solve o the angula displacement using Equation 8.3: t. The distance
More informationChapter 3 Optical Systems with Annular Pupils
Chapte 3 Optical Systems with Annula Pupils 3 INTRODUCTION In this chapte, we discuss the imaging popeties of a system with an annula pupil in a manne simila to those fo a system with a cicula pupil The
More information7.2. Coulomb s Law. The Electric Force
Coulomb s aw Recall that chaged objects attact some objects and epel othes at a distance, without making any contact with those objects Electic foce,, o the foce acting between two chaged objects, is somewhat
More informationChapter 22: Electric Fields. 22-1: What is physics? General physics II (22102) Dr. Iyad SAADEDDIN. 22-2: The Electric Field (E)
Geneal physics II (10) D. Iyad D. Iyad Chapte : lectic Fields In this chapte we will cove The lectic Field lectic Field Lines -: The lectic Field () lectic field exists in a egion of space suounding a
More informationRevision Guide for Chapter 16
Revision Guide fo Chapte 16 Contents Revision Checklist Revision Notes lectic field... 5 Invese squae laws... 7 lectic potential... 9 lecton... 9 Foce on a moving chage... 10 Mass and enegy... 1 Relativistic
More informationBetween any two masses, there exists a mutual attractive force.
YEAR 12 PHYSICS: GRAVITATION PAST EXAM QUESTIONS Name: QUESTION 1 (1995 EXAM) (a) State Newton s Univesal Law of Gavitation in wods Between any two masses, thee exists a mutual attactive foce. This foce
More informationPhysics 122, Fall September 2012
Physics 1, Fall 1 7 Septembe 1 Today in Physics 1: getting V fom E When it s best to get V fom E, athe than vice vesa V within continuous chage distibutions Potential enegy of continuous chage distibutions
More informationr cos, and y r sin with the origin of coordinate system located at
Lectue 3-3 Kinematics of Rotation Duing ou peious lectues we hae consideed diffeent examples of motion in one and seeal dimensions. But in each case the moing object was consideed as a paticle-like object,
More informationPhysics 2B Chapter 22 Notes - Magnetic Field Spring 2018
Physics B Chapte Notes - Magnetic Field Sping 018 Magnetic Field fom a Long Staight Cuent-Caying Wie In Chapte 11 we looked at Isaac Newton s Law of Gavitation, which established that a gavitational field
More informationFlux. Area Vector. Flux of Electric Field. Gauss s Law
Gauss s Law Flux Flux in Physics is used to two distinct ways. The fist meaning is the ate of flow, such as the amount of wate flowing in a ive, i.e. volume pe unit aea pe unit time. O, fo light, it is
More informationLab #4: Newton s Second Law
Lab #4: Newton s Second Law Si Isaac Newton Reading Assignment: bon: Januay 4, 1643 Chapte 5 died: Mach 31, 1727 Chapte 9, Section 9-7 Intoduction: Potait of Isaac Newton by Si Godfey Knelle http://www.newton.cam.ac.uk/at/potait.html
More informationFlux Shape in Various Reactor Geometries in One Energy Group
Flux Shape in Vaious eacto Geometies in One Enegy Goup. ouben McMaste Univesity Couse EP 4D03/6D03 Nuclea eacto Analysis (eacto Physics) 015 Sept.-Dec. 015 Septembe 1 Contents We deive the 1-goup lux shape
More informationLecture 8 - Gauss s Law
Lectue 8 - Gauss s Law A Puzzle... Example Calculate the potential enegy, pe ion, fo an infinite 1D ionic cystal with sepaation a; that is, a ow of equally spaced chages of magnitude e and altenating sign.
More informationToday in Physics 122: getting V from E
Today in Physics 1: getting V fom E When it s best to get V fom E, athe than vice vesa V within continuous chage distibutions Potential enegy of continuous chage distibutions Capacitance Potential enegy
More informationPhysics 111. Ch 12: Gravity. Newton s Universal Gravity. R - hat. the equation. = Gm 1 m 2. F g 2 1. ˆr 2 1. Gravity G =
ics Announcements day, embe 9, 004 Ch 1: Gavity Univesal Law Potential Enegy Keple s Laws Ch 15: Fluids density hydostatic equilibium Pascal s Pinciple This week s lab will be anothe physics wokshop -
More informationTAMPINES JUNIOR COLLEGE 2009 JC1 H2 PHYSICS GRAVITATIONAL FIELD
TAMPINES JUNIOR COLLEGE 009 JC1 H PHYSICS GRAVITATIONAL FIELD OBJECTIVES Candidates should be able to: (a) show an undestanding of the concept of a gavitational field as an example of field of foce and
More informationChapter 13 Gravitation
Chapte 13 Gavitation In this chapte we will exploe the following topics: -Newton s law of gavitation, which descibes the attactive foce between two point masses and its application to extended objects
More informationNewton s Laws, Kepler s Laws, and Planetary Orbits
Newton s Laws, Keple s Laws, and Planetay Obits PROBLEM SET 4 DUE TUESDAY AT START OF LECTURE 28 Septembe 2017 ASTRONOMY 111 FALL 2017 1 Newton s & Keple s laws and planetay obits Unifom cicula motion
More informationMath Section 4.2 Radians, Arc Length, and Area of a Sector
Math 1330 - Section 4. Radians, Ac Length, and Aea of a Secto The wod tigonomety comes fom two Geek oots, tigonon, meaning having thee sides, and mete, meaning measue. We have aleady defined the six basic
More informationErrors in Nobel Prize for Physics (3) Conservation of Energy Leads to Probability Conservation of Parity, Momentum and so on
Eos in Nobel ize fo hysics (3) Conseation of Enegy Leads to obability Conseation of aity, Momentum and so on Fu Yuhua (CNOOC Reseach Institute, E-mail:fuyh945@sina.com) Abstact: One of the easons fo 957
More informationtransformation Earth V-curve (meridian) λ Conical projection. u,v curves on the datum surface projected as U,V curves on the projection surface
. CONICAL PROJECTIONS In elementay texts on map pojections, the pojection sufaces ae often descibed as developable sufaces, such as the cylinde (cylindical pojections) and the cone (conical pojections),
More informationPhysics 121 Hour Exam #5 Solution
Physics 2 Hou xam # Solution This exam consists of a five poblems on five pages. Point values ae given with each poblem. They add up to 99 points; you will get fee point to make a total of. In any given
More informationQualifying Examination Electricity and Magnetism Solutions January 12, 2006
1 Qualifying Examination Electicity and Magnetism Solutions Januay 12, 2006 PROBLEM EA. a. Fist, we conside a unit length of cylinde to find the elationship between the total chage pe unit length λ and
More informationENGI 4430 Non-Cartesian Coordinates Page xi Fy j Fzk from Cartesian coordinates z to another orthonormal coordinate system u, v, ˆ i ˆ ˆi
ENGI 44 Non-Catesian Coodinates Page 7-7. Conesions between Coodinate Systems In geneal, the conesion of a ecto F F xi Fy j Fzk fom Catesian coodinates x, y, z to anothe othonomal coodinate system u,,
More informationRays. CS348B Lecture 4 Pat Hanrahan, 2004
Page 1 Light Visible electomagnetic adiation Powe spectum 1 10 10 4 10 6 10 8 10 10 10 1 10 14 10 16 10 18 10 0 10 10 4 10 6 Powe Heat Radio Ulta- X-Rays Gamma Cosmic Infa- Red Violet Rays Rays 10 16 10
More informationPHYS 1444 Lecture #5
Shot eview Chapte 24 PHYS 1444 Lectue #5 Tuesday June 19, 212 D. Andew Bandt Capacitos and Capacitance 1 Coulom s Law The Fomula QQ Q Q F 1 2 1 2 Fomula 2 2 F k A vecto quantity. Newtons Diection of electic
More informationHomework 7 Solutions
Homewok 7 olutions Phys 4 Octobe 3, 208. Let s talk about a space monkey. As the space monkey is oiginally obiting in a cicula obit and is massive, its tajectoy satisfies m mon 2 G m mon + L 2 2m mon 2
More informationAnyone who can contemplate quantum mechanics without getting dizzy hasn t understood it. --Niels Bohr. Lecture 17, p 1
Anyone who can contemplate quantum mechanics without getting dizzy hasn t undestood it. --Niels Boh Lectue 17, p 1 Special (Optional) Lectue Quantum Infomation One of the most moden applications of QM
More informationAnswers to Coursebook questions Chapter 2.11
Answes to Couseook questions Chapte 11 1 he net foe on the satellite is F = G Mm and this plays the ole of the entipetal foe on the satellite, ie mv mv Equating the two gives π Fo iula motion we have that
More informationOSCILLATIONS AND GRAVITATION
1. SIMPLE HARMONIC MOTION Simple hamonic motion is any motion that is equivalent to a single component of unifom cicula motion. In this situation the velocity is always geatest in the middle of the motion,
More information( ) Make-up Tests. From Last Time. Electric Field Flux. o The Electric Field Flux through a bit of area is
Mon., 3/23 Wed., 3/25 Thus., 3/26 Fi., 3/27 Mon., 3/30 Tues., 3/31 21.4-6 Using Gauss s & nto to Ampee s 21.7-9 Maxwell s, Gauss s, and Ampee s Quiz Ch 21, Lab 9 Ampee s Law (wite up) 22.1-2,10 nto to
More informationElectric Forces: Coulomb s Law
Electic Foces: Coulomb s Law All the matte aound you contains chaged paticles, and it is the electic foces between these chaged paticles that detemine the stength of the mateials and the popeties of the
More informationDetermining solar characteristics using planetary data
Detemining sola chaacteistics using planetay data Intoduction The Sun is a G-type main sequence sta at the cente of the Sola System aound which the planets, including ou Eath, obit. In this investigation
More informationHomework # 3 Solution Key
PHYSICS 631: Geneal Relativity Homewok # 3 Solution Key 1. You e on you hono not to do this one by hand. I ealize you can use a compute o simply look it up. Please don t. In a flat space, the metic in
More informationHow Electric Currents Interact with Magnetic Fields
How Electic Cuents nteact with Magnetic Fields 1 Oested and Long Wies wote these notes to help ou with vaious diectional ules, and the equivalence between the magnetism of magnets and the magnets of electic
More informationPhysics 211: Newton s Second Law
Physics 211: Newton s Second Law Reading Assignment: Chapte 5, Sections 5-9 Chapte 6, Section 2-3 Si Isaac Newton Bon: Januay 4, 1643 Died: Mach 31, 1727 Intoduction: Kinematics is the study of how objects
More informationPhysics 312 Introduction to Astrophysics Lecture 7
Physics 312 Intoduction to Astophysics Lectue 7 James Buckley buckley@wuphys.wustl.edu Lectue 7 Eath/Moon System Tidal Foces Tides M= mass of moon o sun F 1 = GMm 2 F 2 = GMm ( + ) 2 Diffeence in gavitational
More informationSection 11. Timescales Radiation transport in stars
Section 11 Timescales 11.1 Radiation tanspot in stas Deep inside stas the adiation eld is vey close to black body. Fo a black-body distibution the photon numbe density at tempeatue T is given by n = 2
More informationPhys-272 Lecture 17. Motional Electromotive Force (emf) Induced Electric Fields Displacement Currents Maxwell s Equations
Phys-7 Lectue 17 Motional Electomotive Foce (emf) Induced Electic Fields Displacement Cuents Maxwell s Equations Fom Faaday's Law to Displacement Cuent AC geneato Magnetic Levitation Tain Review of Souces
More informationRadial Inflow Experiment:GFD III
Radial Inflow Expeiment:GFD III John Mashall Febuay 6, 003 Abstact We otate a cylinde about its vetical axis: the cylinde has a cicula dain hole in the cente of its bottom. Wate entes at a constant ate
More informationMathematisch-Naturwissenschaftliche Fakultät I Humboldt-Universität zu Berlin Institut für Physik Physikalisches Grundpraktikum.
Mathematisch-Natuwissenschaftliche Fakultät I Humboldt-Univesität zu Belin Institut fü Physik Physikalisches Gundpaktikum Vesuchspotokoll Polaisation duch Reflexion (O11) duchgefüht am 10.11.2009 mit Vesuchspatne
More informationPhysics 235 Chapter 5. Chapter 5 Gravitation
Chapte 5 Gavitation In this Chapte we will eview the popeties of the gavitational foce. The gavitational foce has been discussed in geat detail in you intoductoy physics couses, and we will pimaily focus
More informationAnnouncements. CS 188: Artificial Intelligence Fall Today. Uncertainty. Random Variables. Probabilities. Lecture 14: Probability 10/17/2006
C 188: Atificial Intelligence all 2006 Lectue 14: oaility 10/17/2006 Announcements Gades: Check midtem, p1.1, and p1.2 gades in glookup Let us know if thee ae polems, so we can calculate useful peliminay
More information! E da = 4πkQ enc, has E under the integral sign, so it is not ordinarily an
Physics 142 Electostatics 2 Page 1 Electostatics 2 Electicity is just oganized lightning. Geoge Calin A tick that sometimes woks: calculating E fom Gauss s law Gauss s law,! E da = 4πkQ enc, has E unde
More information2 x 8 2 x 2 SKILLS Determine whether the given value is a solution of the. equation. (a) x 2 (b) x 4. (a) x 2 (b) x 4 (a) x 4 (b) x 8
5 CHAPTER Fundamentals When solving equations that involve absolute values, we usually take cases. EXAMPLE An Absolute Value Equation Solve the equation 0 x 5 0 3. SOLUTION By the definition of absolute
More informationChap13. Universal Gravitation
Chap13. Uniesal Gaitation Leel : AP Physics Instucto : Kim 13.1 Newton s Law of Uniesal Gaitation - Fomula fo Newton s Law of Gaitation F g = G m 1m 2 2 F21 m1 F12 12 m2 - m 1, m 2 is the mass of the object,
More informationSection 8.2 Polar Coordinates
Section 8. Pola Coodinates 467 Section 8. Pola Coodinates The coodinate system we ae most familia with is called the Catesian coodinate system, a ectangula plane divided into fou quadants by the hoizontal
More informationII. Electric Field. II. Electric Field. A. Faraday Lines of Force. B. Electric Field. C. Gauss Law. 1. Sir Isaac Newton ( ) A.
II. Electic Field D. Bill Pezzaglia II. Electic Field. Faaday Lines of Foce B. Electic Field C. Gauss Law Updated 08Feb010. Lines of Foce 1) ction at a Distance ) Faaday s Lines of Foce ) Pinciple of Locality
More informationAuchmuty High School Mathematics Department Advanced Higher Notes Teacher Version
The Binomial Theoem Factoials Auchmuty High School Mathematics Depatment The calculations,, 6 etc. often appea in mathematics. They ae called factoials and have been given the notation n!. e.g. 6! 6!!!!!
More informationQuestion 1: The dipole
Septembe, 08 Conell Univesity, Depatment of Physics PHYS 337, Advance E&M, HW #, due: 9/5/08, :5 AM Question : The dipole Conside a system as discussed in class and shown in Fig.. in Heald & Maion.. Wite
More informationkg 2 ) 1.9!10 27 kg = Gm 1
Section 6.1: Newtonian Gavitation Tutoial 1 Pactice, page 93 1. Given: 1.0 10 0 kg; m 3.0 10 0 kg;. 10 9 N; G 6.67 10 11 N m /kg Requied: Analysis: G m ; G m G m Solution: G m N m 6.67!10 11 kg ) 1.0!100
More informationChapter Sixteen: Electric Charge and Electric Fields
Chapte Sixteen: Electic Chage and Electic Fields Key Tems Chage Conducto The fundamental electical popety to which the mutual attactions o epulsions between electons and potons ae attibuted. Any mateial
More information612 MHR Principles of Mathematics 9 Solutions. Optimizing Measurements. Chapter 9 Get Ready. Chapter 9 Get Ready Question 1 Page 476.
Chapte 9 Optimizing Measuements Chapte 9 Get Ready Chapte 9 Get Ready Question Page 476 a) P = w+ l = 0 + 0 = 0 + 40 = 60 A= lw = 0 0 = 00 The peimete is 60 cm, and the aea is 00 cm. b) P = w+ l = 5. 8
More informationFresnel Diffraction. monchromatic light source
Fesnel Diffaction Equipment Helium-Neon lase (632.8 nm) on 2 axis tanslation stage, Concave lens (focal length 3.80 cm) mounted on slide holde, iis mounted on slide holde, m optical bench, micoscope slide
More information1 Similarity Analysis
ME43A/538A/538B Axisymmetic Tubulent Jet 9 Novembe 28 Similaity Analysis. Intoduction Conside the sketch of an axisymmetic, tubulent jet in Figue. Assume that measuements of the downsteam aveage axial
More informationAstronomy 111, Fall October 2011
Astonomy 111, Fall 011 4 Octobe 011 Today in Astonomy 111: moe details on enegy tanspot and the tempeatues of the planets Moe about albedo and emissivity Moe about the tempeatue of sunlit, adiation-cooled
More information11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below.
Fall 2007 Qualifie Pat II 12 minute questions 11) A thin, unifom od of mass M is suppoted by two vetical stings, as shown below. Find the tension in the emaining sting immediately afte one of the stings
More informationThe Schwartzchild Geometry
UNIVERSITY OF ROCHESTER The Schwatzchild Geomety Byon Osteweil Decembe 21, 2018 1 INTRODUCTION In ou study of geneal elativity, we ae inteested in the geomety of cuved spacetime in cetain special cases
More informationUse Properties of Tangents
opeties of icles 1010.1 Use opeties of Tangents 10.2 Find c Measues 10.3 pply opeties of hods 10.4 Use Inscibed ngles and olygons 10.5 pply Othe ngle elationships in icles 10.6 Find egment Lengths in icles
More information1 Spherical multipole moments
Jackson notes 9 Spheical multipole moments Suppose we have a chage distibution ρ (x) wheeallofthechageiscontained within a spheical egion of adius R, as shown in the diagam. Then thee is no chage in the
More informationUniform Circular Motion
Unifom Cicula Motion Intoduction Ealie we defined acceleation as being the change in velocity with time: a = v t Until now we have only talked about changes in the magnitude of the acceleation: the speeding
More informationPhysics 411 Lecture 34. Sourced Radiation. Lecture 34. Physics 411 Classical Mechanics II
Physics 411 Lectue 34 Souced Radiation Lectue 34 Physics 411 Classical Mechanics II Novembe 21st, 2007 We ae eady to move on to the souce side of lineaized waves. The point of this whole section has been
More informationKinetic energy, work, and potential energy. Work, the transfer of energy: force acting through distance: or or
ENERGETICS So fa we have been studying electic foces and fields acting on chages. This is the dynamics of electicity. But now we will tun to the enegetics of electicity, gaining new insights and new methods
More informationPhys-272 Lecture 18. Mutual Inductance Self-Inductance R-L Circuits
Phys-7 ectue 8 Mutual nductance Self-nductance - Cicuits Mutual nductance f we have a constant cuent i in coil, a constant magnetic field is ceated and this poduces a constant magnetic flux in coil. Since
More informationOn the Sun s Electric-Field
On the Sun s Electic-Field D. E. Scott, Ph.D. (EE) Intoduction Most investigatos who ae sympathetic to the Electic Sun Model have come to agee that the Sun is a body that acts much like a esisto with a
More informationCHAPTER IV RADIATION BY SIMPLE ACOUSTIC SOURCE. or by vibratory forces acting directly on the fluid, or by the violent motion of the fluid itself.
CHAPTER IV RADIATION BY SIMPLE ACOUSTIC SOURCE 4.1 POINT SOURCE Sound waves ae geneated by the vibation of any solid body in contact with the fluid medium o by vibatoy foces acting diectly on the fluid,
More informationGravitation on the PC
Pupose: To undestand obital mechanics and the Law of Univesal Gavitation. Equipment: Inteactive Physics Pencil, Pape, Calculato Theoy: It was Galileo, back in the seventeenth centuy, who finally discedited
More informationTailoring Materials and Radiation to Explore Cloaking Phenomena
Tailoing Mateials and Radiation to Exploe Cloaking Phenomena Jonathan Samoajski Septembe 22, 2009 1 Intoduction Radiation-matte inteaction is vey impotant in enegy eseach, especially in the aeas of fusion
More informationContact impedance of grounded and capacitive electrodes
Abstact Contact impedance of gounded and capacitive electodes Andeas Hödt Institut fü Geophysik und extateestische Physik, TU Baunschweig The contact impedance of electodes detemines how much cuent can
More informationPhysics 2A Chapter 10 - Moment of Inertia Fall 2018
Physics Chapte 0 - oment of netia Fall 08 The moment of inetia of a otating object is a measue of its otational inetia in the same way that the mass of an object is a measue of its inetia fo linea motion.
More informationGeneral Railgun Function
Geneal ailgun Function An electomagnetic ail gun uses a lage Loentz foce to fie a pojectile. The classic configuation uses two conducting ails with amatue that fits between and closes the cicuit between
More informationAppendix B The Relativistic Transformation of Forces
Appendix B The Relativistic Tansfomation of oces B. The ou-foce We intoduced the idea of foces in Chapte 3 whee we saw that the change in the fou-momentum pe unit time is given by the expession d d w x
More informationCircular Orbits. and g =
using analyse planetay and satellite motion modelled as unifom cicula motion in a univesal gavitation field, a = v = 4π and g = T GM1 GM and F = 1M SATELLITES IN OBIT A satellite is any object that is
More informationPhysics 231 Lecture 21
Physics 3 Lectue Main points o today s lectue: Angula momentum: L Newton s law o univesal gavitation: GMm F PE GMm Keple s laws and the elation between the obital peiod and obital adius. T π GM 4 3 Rolling
More informationPhys 222 Sp 2009 Exam 1, Wed 18 Feb, 8-9:30pm Closed Book, Calculators allowed Each question is worth one point, answer all questions
Phys Sp 9 Exam, Wed 8 Feb, 8-9:3pm Closed Book, Calculatos allowed Each question is woth one point, answe all questions Fill in you Last Name, Middle initial, Fist Name You ID is the middle 9 digits on
More informationPotential Energy and Conservation of Energy
Potential Enegy and Consevation of Enegy Consevative Foces Definition: Consevative Foce If the wok done by a foce in moving an object fom an initial point to a final point is independent of the path (A
More informationCS 188: Artificial Intelligence Fall Announcements
C 188: Atificial Intelligence Fall 2006 Lectue 14: oaility 10/17/2006 Dan Klein UC Bekeley Announcements Gades: Check midtem, p1.1, and p1.2 gades in glookup Let us know if thee ae polems, so we can calculate
More informationWelcome to Physics 272
Welcome to Physics 7 Bob Mose mose@phys.hawaii.edu http://www.phys.hawaii.edu/~mose/physics7.html To do: Sign into Masteing Physics phys-7 webpage Registe i-clickes (you i-clicke ID to you name on class-list)
More informationKinematics in 2-D (II)
Kinematics in 2-D (II) Unifom cicula motion Tangential and adial components of Relative velocity and acceleation a Seway and Jewett 4.4 to 4.6 Pactice Poblems: Chapte 4, Objective Questions 5, 11 Chapte
More informationPhysics 161: Black Holes: Lecture 5: 22 Jan 2013
Physics 161: Black Holes: Lectue 5: 22 Jan 2013 Pofesso: Kim Giest 5 Equivalence Pinciple, Gavitational Redshift and Geodesics of the Schwazschild Metic 5.1 Gavitational Redshift fom the Schwazschild metic
More informationCh 13 Universal Gravitation
Ch 13 Univesal Gavitation Ch 13 Univesal Gavitation Why do celestial objects move the way they do? Keple (1561-1630) Tycho Bahe s assistant, analyzed celestial motion mathematically Galileo (1564-1642)
More informationPHY2061 Enriched Physics 2 Lecture Notes. Gauss Law
PHY61 Eniched Physics Lectue Notes Law Disclaime: These lectue notes ae not meant to eplace the couse textbook. The content may be incomplete. ome topics may be unclea. These notes ae only meant to be
More informationExtra notes for circular motion: Circular motion : v keeps changing, maybe both speed and
Exta notes fo cicula motion: Cicula motion : v keeps changing, maybe both speed and diection ae changing. At least v diection is changing. Hence a 0. Acceleation NEEDED to stay on cicula obit: a cp v /,
More informationPhysics 521. Math Review SCIENTIFIC NOTATION SIGNIFICANT FIGURES. Rules for Significant Figures
Physics 51 Math Review SCIENIFIC NOAION Scientific Notation is based on exponential notation (whee decimal places ae expessed as a powe of 10). he numeical pat of the measuement is expessed as a numbe
More information