Circular Motion Gravitation Labs

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New York University *

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MISC

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Physics

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Jan 9, 2024

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AP Physics B Course Outline % on Dates Unit Exam Title Possible Labs Math and Data Collection Review 8/19-8/23 -Round Things -Determining G using a spring scale Newtonian Mechanics Kinematics (1D/2D) 15 8/26-9/13 Kinematics LTF #1 Constant Velocity LTF #2 Acceleration on a Ramp LTF #3 Not-So Free Fall LTF #4 Freefalling Washers LTF #5 Vector Scavenger Hunt LTF #6 Map of Texas LTF #7 Projectile Motion LTF #8 Dart Gun -Force Tables Newton’s Laws 17 9/16-10/8 Newton’s Laws LTF #9 Newton's 2" Law LTF #10 Atwood Machine LTF #11 Coefficient of Friction Work, Power, and Energy 10/9-10/18 Work, Power, and Energy LTF #15 Running the Stairs LTF #18 Roller Coaster Momentum 10/21-10/31 Momentum LTF #13 Crumple Zone LTF #14 Conservation of Momentum Particles/linear momentum Circular Motion/Gravitation 14 11/7-11/22 Circular Motion/Gravitation Circular motion/rotation LTF #12 Centripetal Force -Kepler's Laws Virtual Lab Oscillation/gravitation LTF #21 Waves in a Spring LTF #16 The Pendulum Swings LTF #17 Simple Harmonic Motion Wave Motion and Sound 2/26-3/7 Wave motion and sound Fluid mechanics and thermal 15 Thermodynamics and Fluids 13 11/25-12/13 Thermodynamics & Fluids Fluid mechanics -Buoyancy lab -Pressure-depth lab Temperature &heat -Calorimetry lab Kinetic theory/thermo Electricity and magnetism 25
Centripetal Force Exploring Uniform Circular Motion An object that moves in a circle at constant speed, v, is said to experience uniform circular motion (UCM). The magnitude of the velocity remains constant, but the direction of the velocity is continuously changing, as shown in Figure 1. Figure ] Notice that the velocity vectors are not pointing in the same direction. The velocity vector is always tangent to the circular path. This is why, should the string break, the object flies off in a straight line. Figure 2 An object revolving in a circle is continuously accelerating, even when the speed remains constant. The acceleration vector is always pointing toward the center of the circular path and it is always perpendicular to the velocity vector, as shown in Figure 2. Centripetal (center-seeking) acceleration, a., is defined as: Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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If we measure the period, 7, the time needed for the object to make a complete revolution, we can calculate the speed of the object in UCM. During this time, it travels a distance equal to the circumference of the circle, 277, where r is the radius of the circular path. The object’s speed, then, is represented by v = % According to Newton’s second law (XF = ma), an object that is accelerating must have a net force acting upon it and we call this force centripetal force. This force is acting in the same direction as the acceleration which is toward the center of the circle (Figure 3). Figure 3 The equation for centripetal force can be expressed as 271\ [vz} T an’y F=ma=ma,=m|— |=m|——|=m r Centripetal force is the net force which points toward the center of the circle, and, as examples, can take the form of a gravitational force, frictional force, or tension in a string. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www./tftraining.org.
PURPOSE In this activity you will verify the relationship between centripetal force, mass, and ve1001ty in an object in uniform circular motion. You will be using the assumption that the centripetal force generated by the whirling stopper balances the force of weight for the hanging mass. MATERIALS Each lab group will need the followmg calculator, TI® graphing Centripetal Force Apparatus, set meter stick stopwatch washers or hanging weight set SAFETY ALERT 1. Goggles must be worn at all times. 2. Make sure you have enough room to swing your stopper without hitting other students. 3. Check to see that your cord is not frayed before beginning your experiment. PROCEDURE 1. Put your goggles on and leave them on for the entire laboratory period. 2. One partner should construct your apparatus as pictured in Figure 4 below. Rubber stopper T Glass tube wrapped with tape Figure 4 Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
10. a. Mass the rubber stopper and record its mass in kilograms in Data Table 1 on your student answer page. Attach one end of the cord securely to the rubber stopper. b. Pass the other end of the cord through the glass or plastic tube. ¢. Bend a large paperclip into a hook and attach it to the free end of the cord. This hook needs to support several large washers. . The other partner should use a balance to mass your group’s washers + hook. Keep adding washers until the mass exceeds 100 grams. Record the mass of your stack of washers and hook in kilograms in Data Table 1 on your student answer page. Load the stack of washers onto the hook. If the stack is too large to hang securely from the hook, you can secure the stack together with a piece of string and hang the string from the hook. If you choose this method, re-weigh your hook as well as the stack of washers with the string attached. Adjust the cord so that there is about 0.75 m of cord between the top of the tube and the stopper. The partner that is going to operate the apparatus should support the stack of washers in one hand and hold the tube with the other. Begin whirling the stopper by moving the tube in a circular motion. Slowly release the stack of washers and adjust the speed of the stopper so that the stack of washers remains relatively stationary, meaning the stack is no longer climbing or falling. Important: Keep the stopper whirling in an elevated, horizontal circle as pictured in Figure 4. The tube should be held high enough in the air so that the spinning stopper does not threaten any part of the spinner’s head. Make several trial runs to master the technique. Be mindful of your space so that you do not accidentally hit any other students with your spinning stopper. When you have learned how to keep the velocity of the stopper and the position of the washers relatively constant, have your partner measure the time it takes for 20 revolutions by counting down the revolutions “5,4,3,2,1, go! 1,2,3, .... Record this time in Data Table 1 on your student answer page. The partner with the apparatus should stop the whirling stopper by placing his or her finger at the fop of the tube so as to capture the length of the radius of your circle. Use caution when performing this task so as not to be hit by the stopper. Once the stopper comes to rest, keep your finger in place so that the length of the cord will not change. Measure the radius, r, from the center of the tube to the center of the stopper. Use the appropriate number of significant digits and record the value in Data Table 1 on your student answer page. Repeat the procedure for two additional trials keeping the same stopper and the same stack of washers, but varying the radius. Keep the radius between 0.50 m and 0.90 m. Record all data to the appropriate number of significant digits in your data table. Copyright © 2012 Laying the Foundation®, Inc., Dalfas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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11. Repeat the procedure for three additional trials keeping the same radius [you may need to mark your cord at the point where it exits the tube so you can have a visual cue that your radius is consistent] but varying the'size of your stopper. Record all data to the appropriate number of significant digits in your data table. 12. Repeat the procedure for a final three trials keeping the same radius and same stopper, but varying the mass of your washer stack. Record all data to the appropriate number of significant digits in your data table. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
Centripetal Force Exploring Uniform Circular Motion DATA AND OBSERVATIONS IS o T e e | AR P DDatanlableil B ST A S T T T | e Trial Mass of Mass of stopper Total Time Radius Washers (kg) (ke) (s) (m) Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
ANALYSIS 1. Calculate the force of weight, Fiy, of the hanging mass and enter it in Table 2 as centripetal force, F.. F, =mg=F, and g=9.8fl2 s 2. Calculate the period of revolution by dividing the total time by the number of revolutions and enter it in Table 2. time(s) - 20 revolutions 3. Calculate the circumference of revolution from the radius and enter it inTable 2. circumference = zd = 27zr 4. Use the circumference and period to find the velocity and enter it in Table 2. circumference V = - T 11010 (PR OF.N D @) B) B7.§ 4 (O AN Trial Centripetal Force, F Period, T Circumference Velocity N) (s) (m) (m/s) 1 2 3 4 5 6 7 8 9 Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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CONCLUSION QUESTIONS 1. Survey the data in Table 2. What is the relationship between the velocity of a whirling object and the centripetal force that is exerted on it? What is the relationship between the radius of revolution and the velocity of an object in uniform circular motion? What is the relationship between the mass and velocity of an object in uniform circular motion? Step one of the analysis section assumes that 'y = F, by using the assumption that the centripetal force supplied by the weight of the washers causes the whirling stopper to move in a curved path. What additional assumption is made regarding the value for the centripetal acceleration? A student neglects to reweigh the stack of washers after tying them together before performing one of the trials. How will this error affect the reported centripetal force? State clearly whether the centripetal force increases, decreases, or remains the same and mathematically justify your answer. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
6. A 13.0-g rubber stopper is attached to a 0.93-m string. The stopper is swung in a horizontal circle, making one revolution in 1.18s. Calculate the centripetal force exerted by the string on the stopper. 7. A coin is placed on a vinyl stereo record making 33' revolutions per minute. a. In what direction is the acceleration of the coin? b. Calculate the magnitude of the acceleration when the coin is placed 10.0 cm from the center of the record. 8. A carnival ride has a 2.0 m radius and rotates once each 0.90 s. a. Calculate the speed of a rider at this radius. b. Calculate the centripetal acceleration of the rider. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itftraining.org.
9. As you whirled the mass in a circular path, you did your best to keep it swinging in a horizontal circle. Is it possible to keep the mass whirling in a perfectly horizontal circle (parallel to the floor)? Explain your answer and draw and label the forces acting on the mass from a side view using the diagram below. i B 10. A student tries to swing a stopper of mass 40 grams in a horizontal circle, but finds that the stopper “droops” down a little due to the gravitational force acting on the stopper, as shown in the figure below. The string has a length L = 0.50 m, and is swung so that it remains an angle of 8 = 60° from the vertical. Sy O el e i e a. On the diagram above, draw and label all of the forces acting on the stopper as it travels around the circle. (Remember: centripetal force is not an “extra” force that acts on the mass, but is the sum of the forces which point toward the center of the horizontal circle.) b. Can we say that the tension in the string is the centripetal force? Explain your answer. c. Show the horizontal and vertical components of the tension force on the diagram above. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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d. Determine the vertical component 7}, of the tension in the string. e. Determine the horizontal component 7 of the tension in the string. f. Determine the tangential speed v necessary to keep the mass revolving in this circle. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
Physics SITF LAYING THE FOUNDATION Building Academic Excellence The Pendulum Swings Happiness Is A Straight Line In this activity, you will determine the relationship between the period 7 of a pendulum and its mass m, amplitude 4, and length L. Your teacher will instruct you on how to construct your pendulum. You will make and record measurements throughout this activity, and you will create your own graphs to display your data. Purpose You will investigate the relationship between the mass, amplitude, and length of a pendulum and its period. From the data collected, you will also apply your graphing skills either manually or by using computer graphing software to generate graphs and find relationships. You will also linearize your data if necessary. Materials Each lab group will need the following: meter stick string protractor, with hole tape, masking scissors 3 washers, 2 in. stopwatch Copyright © 2012 Laying the Foundation®, inc., Dallas, Texas. All rights reserved. Visit us online gt www.ltftraining.org. 1
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Student Activity The Pendulum Swings Procedure 1. Listen carefully to your teacher’s instructions. You will be asked to describe your actual procedure in your laboratory report. 2. Organize your data according to the three data tables following, and use a computer graphing program or graph paper to graph the period versus each of the variables tested (mass, amplitude, and length). For this activity, keep the period on the y-axis for each graph. | 0.40 10 1 0.60 10 1 0.80 10 1 1.00 10 1 1.20 10 Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itftraining.org. 2
Student Activity The Pendulum Swings Lab Report Include the following sections when writing your lab report: I. Title II. Purpose III. Apparatus (labeled sketch) IV. Procedure V. Data VI. Analysis VII. Conclusion (include the answers to the Conclusion Questions here) Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 3
Student Activity The Pendulum Swings Conclusion Questions 1. What are the variables in this experiment? 2. What data should be recorded for your pendulum? 3. What steps did you take to maximize accuracy and precision, and minimize your systemic error while collecting your data? 4. What effect does varying the mass of the pendulum have on its period? Justify your answer. 5. What effect does varying the amplitude of the swing of the pendulum have on its period? Justify your answer. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itftraining.org. 4
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Student Activity - The Pendulum Swings Conclusion Questions (continued) 6. What effect does varying the length of the pendulum have on its period? Justify your answer. 7. According to your data relating the period of the pendulum to its length, would it be accurate to say that the period of a pendulum is directly proportional to its length, inversely proportional to its length, directly proportional to the square of the length, or directly proportional to the square root of the length? Explain your answer. 8. Add another column to your data table for length variations and square the period. Graph the period squared versus the length. Write an equation that relates the period to the length, and include the value of the slope. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 5
Student Activity The Pendulum Swings Conclusion Questions (continued) 9. You will be given a period and asked to calculate and construct a pendulum of the appropriate length using the equation you derived. Your teacher will time your pendulum and its period. Use the space provided to calculate the length of your pendulum and to compute your percent error. 10. Use the slope of your straight line and rearrange the equation for a simple pendulum, T=27r\/Z g to determine a value for the acceleration due to gravity, g. Find the percent error between your value for g and the accepted value of 9.81 m/s?. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 6
Simple Harmonic Motion Investigating a Mass Oscillating on a Spring A spring that is hanging vertically from a support with no mass at the end of the spring has a length L (called its rest length). When a mass is added to the spring, its length increases by x. The equilibrium position of the mass is now a distance L + x from the spring’s support. The spring exerts a restoring force, ' = -kx, where x is the distance the spring is displaced from equilibrium and k is the force constant of the spring (also called the spring constant). The negative sign indicates that the force exerted by the spring on the mass is directed opposite to the direction of the displacement of the mass. The restoring force causes the mass to oscillate up and down, and is always directed toward the equilibrium position. The period of oscillation depends on the mass and the spring constant. PURPOSE In this lab you will determine the spring constant for a spring, predict the period of oscillation for several different masses using the measured spring constant, and find their relative error. A graph of position vs. time and velocity vs. time for a mass in simple harmonic motion will be constructed and analyzed for the energy aspects of the motion. MATERIALS Each lab group will need the following: calculator, TI® graphing clamp, pendulum computer electronic file LabQuest® meter stick ring stand sensor, motion detector spring weights, hanging sets Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itffraining.org.
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PROCEDURE PART I: FINDING THE SPRING CONSTANT & 1. Attach a clamp to a ring stand so that your spring will hang over the edge of the table. I 1~ Z v Figure 1 2. Hang a mass hanger on the spring so that it will slightly stretch your spring and hang at rest. With your meter stick, measure the distance from the bottom of the hanger to the floor where the motion detector will eventually be positioned. Make all successive measurements from this same position, which will serve as the equilibrium position. This will be considered your unstretched length. 3. Measure the amount of stretch for 5 different masses added to the spring. The amount of stretch is the difference between the unstretched length and the stretched length. Record your measurements in Data Table 1 on your student answer page. PART II: ADDITIONAL METHOD FOR FINDING THE SPRING CONSTANT K 1. Attach a motion detector to your computer and start the appropriate software. 2. Place the motion detector on the floor directly beneath the spring. Make sure that the mass does not come closer than the measurement limit for your motion detector, usually 15 cm for Vernier motion detectors or PASCO Motion Detector II’s. When Logger Pro is opened, if it does not automatically identify your motion detector, then drag the motion detector icon to Digital Channel 1. A graph of position vs. time and a second graph of velocity vs. time should open. "W I~ Figure 2 Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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3. Using each of the 5 masses from Part I, set the mass into smooth oscillations, with amplitudes of about 10 cm (depending on the original length of your spring). Start the motion detector data collection. Gather data for about 3 seconds or until you have more than 10 complete oscillations with each of the 5 masses. 4. Using the analysis tool on Logger Pro or your software, find the time for ten complete oscillations of your spring. Record this, as well as the mass on the spring, in Table 2 on your student answer page. PART III: ENERGY IN SIMPLE HARMONIC MOTION 1. With the motion detector placed on the floor as in Part II, zero the motion detector when the mass is motionless. To zero the motion detector, click on the LabPro icon on the tool bar. Double click on the motion sensor icon, and then select “zero”. This is your equilibrium position. This will have to be repeated with each mass. 2. Set the mass into smooth oscillations with amplitude of about 10 cm (depending on the original length of your spring). Collect data for about three seconds. 3. Using the analysis tool, determine both the position and velocity for the mass at its maximum amplitude and for the next position of zero amplitude. Record these values in Table 3 on your student answer page. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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Simple Harmonic Motion Investigating a Mass Oscillating on a Spring DATA AND OBSERVATIONS PART I: DETERMINING THE SPRING CONSTANT k Data Table 1 Run # | Mass on Spring | Force [Position 1 with only| Position 2 with Amount of (kg) N) hanger added mass stretch (m) (m) (m) 1 2 3 4 5 Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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ANALYSIS PART I: DETERMINING THE SPRING CONSTANT K 1. On the mass below, draw and label the forces acting on the mass when it is hanging at rest on the end of the spring. I 2. Using either graph paper or graphing software, construct a graph of Force (N) vs. Amount of Stretch (m). Find the slope of this graph. a. What are the units for the slope? b. The equation relating the magnitude of the force and the stretch is F = kx . How does this equation relate to the slope of your graph? Force vs Stretch - Linear Fit For: Data Set:Force y= mx+b /fl m(Slope): 2.85 Nim 1.0 b(Y-Intercept): 0.117 N / Correlation:0.999 [l (O] S p i <4 o [F 0.5 /@/ 1 1 I I T L) T I | L) L) T 1 0.10 0.20 0.30 Stretch ¢ (m) (0.247568, 0.662008) Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itftraining.org.
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Data Set Streteh (%) Force (m) | 1 0.04400 0.29500 | & PEIEen 0.11500 0.44100 3 0.18500 0.63700 AN 0.25900 0.89300 5 0.32500 1,03000 . 4 || PART IlI: ADDITIONAL METHOD FOR FINDING THE SPRING CONSTANT K 1. The period of oscillation for your mass spring system can be calculated using the following equation. Rearrange this equation to solve for the spring constant k, and show your work below. For each of your five Runs, calculate a value for the spring constant and then find the average of these values. Place your calculations in Table 2. T=27r\/E k Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. Al rights reserved. Visit us online at www.ltftraining.org.
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i 1) [ Mass on Spring Time for 10 Measured Period | Calculated value for Run # (kg) oscillations (s) k (s) (N/m) 1 2 3 4 5 Avg. n/a n/a n/a 2. Compare the average value for & that you calculated in Part II to the value you found for & in Part I. Find a relative error for the two values. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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PART III: ENERGY IN SIMPLE HARMONIC MOTION 1. For this oscillating system, the energy of the system should remain constant for short periods of time involving one or two oscillations. Over time friction will convert some of the energy to heat, but for a single oscillation, the elastic potential energy Us of the system at maximum amplitude should be relatively close to the kinetic energy KE when the system returns to the equilibrium position. Calculate these values and compare them by finding a relative error. U, = L T2 1 KE =—mv 2 : , KE| Relative Error = x100 Table 3 Mass on | Amplitude Velocity at Calculated [Calculated] Relative Run # Spring | of stretch [equilibrium position EPE KE Error (kg) (m) (m/s) Q) @ (“e) | |WIN|— 2. The errors in this part of the lab may be relatively large. Write a statement analyzing the errors in this lab and suggest ways that the errors might be reduced. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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CONCLUSION QUESTIONS 1. A person who weighs 670 N steps onto a spring scale in the bathroom, and the spring compresses by 0.79 cm. (a) What is the spring constant? Be sure to specify your units. (b) What is the weight of another person who compresses the spring by 0.34 cm? 2. What is the shape of the plot of data for the oscillating spring-mass system on your graph? Describe the shape physically. 3. In terms of the changes in force, displacement, acceleration, and energy, describe one full oscillation of a mass on a spring. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org.
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4. When a 2.8-kg object is suspended from a spring, the length increases by 0.018 m. If the frequency of vibration is f= 3.0 Hz, how much mass is attached to this spring? 5. What is the maximum speed of the mass in question 4? Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltffraining.org.
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Physics SITF LAYING THE FOUNDATION Building Academic Excellence Waves in a Spring Observing the Characteristics of Waves Purpose In this activity, you will observe and investigate important wave properties. What you observe about waves in a spring can be applied to other types of waves including sound waves, water waves, and light waves. Materials Each lab group will need the following: meter stick spring (slinky) stopwatch spring, 6 ft (snakey) SAFETY ALERT! » Coiled springs are social creatures. Avoid releasing either end of the stretched spring. The untangling process can be quite difficult. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 1
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Student Activity Waves in a Spring Procedure Answer the questions as you perform this activity. You and your lab partner should hold opposite ends of a spring and stretch it out on the floor to an appropriate length. Experiment to determine the best stretch distance for your spring but be careful not to exceed the elastic limit of the material. Data and Observations Longitudinal and Transverse Waves 1. Pinch a clump of coils together with your free hand and release the clump of coils. Do not let go of the end of the spring. Observe the pulse that travels back and forth through the spring. Why is it called a longitudinal pulse? Sketch the wave pulse in the space provided. 2. Give one end of the spring a few vigorous sideways (fransverse) shakes. How is this wave different from the longitudinal wave? Sketch the wave pulse in the space provided. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 2
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Student Activity Waves in a Spring Data and Observations (continued) 3. The stretched spring is the medium through which the pulse travels. Send a short transverse pulse down the spring. Observe the shape of the pulse as it moves along the spring. a. How does the shape change? Can you suggest a reason for this change? b. Upon what does the initial amplitude of the pulse depend? c. Does the speed of the pulse appear to change with its shape? d. Generate single pulses of various (small, medium, and large) amplitudes. Does the pulse speed appear to depend on the size of the pulse? e. What could you do to produce wave pulses that travel faster in the spring? Can this be done by shaking the spring more vigorously? How about shaking the spring faster? Copyright © 2012 Laying the Foundation®, inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 3
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Data and Observations (continued) Student Activity Waves in a Spring 4. Measure the length of a stretched spring (do not change this length) and the travel time of a pulse generated at one end. Use a stopwatch to time how long a wave takes to travel up and down the spring. Calculate the speed of the traveling wave pulse for pulse sizes that are small, medium, and large. Record your results in Table 1. Is the speed of the wave pulse affected by the amplitude of the pulse? Use your data and d = vt to answer this question. Transverse Small Transverse Medium Transverse Large Longitudinal -- 5. Change the length of your stretched spring and determine the pulse speed as you did previously. Record your results in Table 2. Examine three different lengths for the stretched spring. Is the speed of the wave pulse affected by the length of the stretched spring (the tension)? Under different tensions, does the stretched spring represent the same or different media? Table 2. Spring Length Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 4
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Student Activity Waves in a Spring Data and Observations (continued) Interference 6. Have your lab partner generate a wave pulse toward you on the same side of the spring that you send a pulse toward your partner. This interaction between the two wave pulses is called interference. a. Describe the interference of the two wave pulses. How does the pulse amplitude during interference compare with the individual amplitudes before and after this interaction? b. Repeat the experiment but with the two pulses traveling on opposite sides of the spring. Compare the interference with that of the previous interaction. When the two pulses meet, does the displacement of the spring at that instant get larger or smaller? c. Did the two pulses pass through each other or bounce off each other? If you are not sure, have your partner send a transverse wave pulse down the spring at the same time you send a longitudinal wave pulse. What can you say about the interaction of these two wave pulses? Do the wave pulses bounce off each other or do they pass through each other? d. What conclusions can you draw about the displacement of the medium at a point where two pulses interfere? (This is called the principle of superposition.) Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itftraining.org. 5
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Student Activity Waves in a Spring Data and Observations (continued) Reflection 7. With the far end of the spring held firmly in place by your lab partner (the “fixed end”), send a single pulse down one side of the spring. Observe the reflected pulse. a. Compare the amplitude of this pulse with that of the transmitted pulse just before reflection. What is the orientation of the reflected pulse relative to the transmitted pulse? b. Attach a light string about 2 m long to the far end of the spring, and maintain the tension on the spring by holding the end of this string. This is called a free-end termination for the spring. Send a pulse down one side of the spring as before and observe the pulse reflected from the “free” end. Compare the reflected pulse from the “free” end of the spring with the reflected pulse from the fixed end. Periodic and Standing Waves 8. By moving your hand steadily back and forth, you can produce a series of pulses called a periodic wave. The distance between any two adjacent crests or troughs on a periodic wave is called the wavelength. The rate at which you move your hand back and forth determines the frequency. Generate a periodic wave and take a “snapshot” of the wave. Sketch the picture on the axes provided in Figure 1. On your diagram, show the amplitude of the periodic wave. Sketch one wavelength and, using the total distance of the wave, determine the value for this wavelength. How does the wavelength depend on the frequency? distance displacement o Figure 1. Periodic wave Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltffraining.org. 6
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Student Activity Waves in a Spring Data and Observations (continued) 9. Have your partner generate a continuous periodic wave while you try and match it. You have produced a standing wave. While your partner holds the end of the spring steady, you will form transverse standing waves having first one, two, three, and then four loops. Find the frequency needed to produce each standing wave pattern. The frequency is the number of times your hand moves through a complete cycle (back and forth) every second. It will be easier to find the frequency if you time 10 cycles of your hand. After you find the frequency, you will be able to find the speed of the waves just created using v = f4. Table 3. Standing Waves 2 A=L 3 A=%x%xL 4 A=Y xL Record your results in Table 3, where L is the distance between both lab partners holding either end of the spring. a. What are the loops called? b. What are the places called where the spring does not appear to move? c. What is the general relationship between the number of loops and the frequency of the wave? Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 7
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Student Activity Waves in a Spring Analysis 1. How does the product of frequency and wavelength (fA) for the various standing wave patterns compare with one another? 2. How do these values compare with the speeds of the pulses calculated for the transverse wave? 3. How are the speed, frequency, and wavelength of a transverse wave related to one another? 4. Consider the power (number of joules of work per second) you are expending as you sweep your hand back and forth to create transverse standing waves. Does the power you expend to create waves depend on the frequency of the waves? 5. Does the power required depend on the amplitude of the wave? Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.itftraining.org. 8
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Student Activity Waves in a Spring Conclusion Questions 1. Suppose a flute player and a tuba player start playing at the same time, each from equally far away. Which instrument will you hear first? Why? 2. Which travels faster: red light or blue light? Blue light has a greater frequency. 3. For the waves shown in Figure 2, sketch the sum of the two waves. a ? d e b | I 0 c -1 -2 = = 4 3 2 1 0 -1 -2 Figure 2. Sum of two waves Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 9
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Student Activity Waves in a Spring Conclusion Questions (continued) 4. What happens to the displacement when two waves meet in phase (crest on crest)? 5. What happens to the displacement when two waves meet out of phase (crest on trough)? 6. What happens to the pulses after they pass through each other? 7. Explain how the reflection of a wave from a rigid barrier (a fixed end) and a less rigid barrier (a free end) affect the wave’s phase. 8. What happens to the speed, wavelength, and frequency of a wave when it reaches the boundary between two media? Copyright © 2012 Laying the Foundation®, inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 10
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Student Activity Waves in a Spring Conclusion Questions (continued) 9. A string is attached to a vibrating machine that has a frequency of 120 Hz, as shown in Figure 3. The other end of the string is passed over a pulley of negligible mass and friction, and is attached to a weight hanger that holds a mass m = 0.5 kg. Figure 3. Vibrating machine with standing wave a. Determine the tension in the string. b. The speed of the wave in the string is related to the tension by the equation where F_ is the tension in the string and 4 is the linear density of the string. If the linear density of this string is 0.05 kg/m, determine the speed of the wave in the string. c. Determine the wavelength of the wave in the string. d. Determine the length of the string from the point of attachment on the vibrating machine to the pulley. e. Would you need to increase or decrease the mass on the hanger to produce fewer loops? Explain. Copyright © 2012 Laying the Foundation®, Inc., Dallas, Texas. All rights reserved. Visit us online at www.ltftraining.org. 11
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Explor#learning ................................................................................................................ Student Exploration: Orbital Motion Kepler’s Laws Vocabulary: astronomical unit, eccentricity, ellipse, force, gravity, Kepler's first law, Kepler's second law, Kepler's third law, orbit, orbital radius, period, vector, velocity Prior Knowledge Questions (Do these BEFORE using the Gizmo.) 1. The orbit of Halley’s Comet, shown at right, has an oval shape. In which part of its orbit do you think Halley’s Comet travels fastest? Slowest? Mark these points on the diagram at right. 2. How might a collision between Neptune and Halley’s Comet affect Neptune’s orbit? Gizmo Warm-up The path of each planet around the Sun is determined by two factors: its current velogity (speed and direction) and the force of gravity on the planet. You can manipulate both of these factors as you investigate planetary orbits in the Orbital Motion Kepler's Laws Gizmo™. On the CONTROLS pane of the Gizmo, turn on Show trails and check that Show vectors is on. Click Play (). 1. What is the shape of the planet’s orbit? 2. Watch the orbit over time. Does the orbit ever change, or is it stable? 3. Click Reset ((©)). Drag the tip of the purple arrow to shorten it and reduce the planet’s initial velocity. Click Play. How does this affect the shape of the orbit?
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Activity A: Shape of orbits Get the Gizmo ready: ¢ Click Reset. e Turn on Show grid. 7~ -1T123 Introduction: The velocity of a planet is represented by an arrow called a vector. The vector is described by two components: the i component represents east-west speed and the j component represents north-south speed. The unit of speed is kilometers per second (km/s). Question: How do we describe the shape of an orbit? 1. Sketch: The distance unit used her is the astronomical unit (AU), equal to the average Earth-Sun distance. Place the planet on the i axis at r = -3.00i AU. Move the velocity vector so that v = -8.0j km/s (|v| = 8.00 km/s). The resulting vectors should look like the vectors in the image at right. (Vectors do not have to be exact.) Click Play, and then click Pause ((CD) after one revolution. Sketch the resulting orbit on the grid. [ N w &~ o arta,=by+ b i = el LelbA-5C W 2. Identify: The shape of the orbit is an ellipse, a type of flattened circle. An ellipse has a center (C) and two points called foci (F1 and F,). If you picked any point on the ellipse, the sum of the distances to the foci is constant. For example, in the ellipse at right: Turn on Show foci and center. The center is represented by a red dot, and the foci are shown by two blue dots. What do you notice about the position of the Sun? 3. Experiment: Try several other combinations of initial position and velocity. A. What do you notice about the orbits? B. What do you notice about the position of the Sun? You have just demonstrated Keplér’s first1aw, one of three laws discovered by the German astronomer Johannes Kepler (1571-1630). Kepler's first law states that planets travel around the Sun in elliptical orbits with the Sun at one focus of the ellipse. (Activity A continued on next page) Wizmos
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Activity A (continued from previous page) 4. Observe: Use the Gizmo to create an orbit that is nearly circular. Then create an orbit that is flattened. Observe the foci in each ellipse. A. What do you notice about the spacing of the foci when the ellipse is very round? B. What do you notice about the spacing of the foci when the ellipse is very flat? 5. Calculate: The eccentricity of an ellipse is a number that describes the flatness of the ellipse. Eccentricity is equal to the distance between foci divided by the total width of the ellipse. There are no units for eccentricity. Click Reset. Move the planet to r = —5.00i AU (does not have to be exact) and drag the velocity vector to set the velocity close to —8.0j km/s. Click Play, and then click Pause after one full revolution. A. What is the distance between the foci? B. What is the approximate width of the ellipse? C. What is the eccentricity of the ellipse? D. Click Reset, and change the initial velocity to —4.0j km/s. Click Play. What is the eccentricity of this ellipse? Distance between foci: Width: Eccentricity: 6. Draw conclusions: Think about the eccentricity and shape of each ellipse. A. What is the relationship between the eccentricity of an ellipse and its shape? B. What is the eccentricity of a circle? Explain. C. What is the eccentricity of a completely flat ellipse? Explain. The eccentricity of Earth’s orbit is 0.17. What can you infer about the shape of Earth’s orbit? @}izmos
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Activity B: Get the Gizmo ready: \"[ o Velocity and area P ClcREse Tl 2__, 3 y e Turn off Show foci and center. Introduction: After establishing that planetary orbits were ellipses, Kepler next looked at the speed of a planet as it traveled around the Sun. Question: How does the velocity of a planet vary as it travels in its orbit? 1. Observe: Place the planet at —5.00i AU and set the velocity to -4.0j km/s (does not have to be exact). Turn off Show vectors. Click Play. Observe the speed of the planet. A. At what point does the planet move fastest? B. At what point does it move slowest? 2. Observe: Click Reset, and turn on Show vectors. Look at the green vector that represents the force of gravity pulling on the planet. Click Play. A. In which direction does the green vector always point? B. In which part of the orbit does the gravity vector point in almost the same direction as the velocity vector? C. In which part of the orbit does the gravity vector point in the opposite direction as the velocity vector? 3. Explain: Based on your observations of the gravity vector, why does the planet accelerate as it approaches the Sun and slow down as it moves away from the Sun? 4. Measure: Click Reset. Imagine a line connecting the planet to the Sun. As the planet moves around the Sun, the line will sweep out an area. Click Play, and then click Sweep area. Record the area below, and then press Sweep area four more times to complete the table. Trial 1 2 3 4 5 Area (km?) (Activity B continued on next page)
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Activity B (continued from previous page) 5. Analyze: What pattern do you notice? 6. Test: Try the same experiment with several different orbits and different numbers of days to sweep an area. Does the same rule hold true for each orhit? Kepler’s second law states that a planet accelerates as it approaches the Sun and decelerates as it moves farther from the Sun. As it orbits, the planet sweeps out equal areas in equal times. 7. Think and discuss: Why do you think the area swept out by a planet in a given period of time remains constant, even as the planet speeds up and slows down? (Hint: Think of each area swept out as a triangle. The height of the triangle is the distance between the planet and the Sun, while the base of the triangle is equal to the distance the planet travels in the given time period.)
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Get the Gizmo ready: & AEHvIy GE e Click Reset. A Radius and period e Set the Sun mass to medium, close to the mass sl e of our Sun, e e Introduction: Kepler's last law relates the period (T) of a planet, or the time it takes to complete an orbit, to the planet’s orbital radius (a), or average distance from the Sun. Question: How does the period of a planet relate to its average distance from the Sun? 1. Predict: How do you expect the period of a planet to change as its average distance from the Sun increases? 2. Measure: Place the planet at -4.00i AU and set the velocity to -15.00j km/s (does not have to be exact). Click Play, and then click Pause when the planet completes one orbit. A. B. What is the approximate period of the planet in days? Select the TABLE tab and click Record data. What is the actual period (T) of the planet in Earth days and years? days years What is the orbital radius (a) of the planet? Click Reset. Place the planet at -2.00i AU and set the velocity to -20.0j km/s. Click Play and Record data. \What is the period now? days years What is the new orbital radius? How does the distance between the planet and the Sun affect its period? 3. Gather data: Experiment with the Gizmo to create a series of larger and larger orbits. Record each orbit’s radius (a) and period (7). Leave the last two columns blank for now. Orbit a (AU) T (years) 1 alhlwWw|IN (Activity C continued on next page) &}izmos
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Activity C (continued from previous page) 4. Analyze: How does the period change as the orbital radius increases? 5. Interpret: Select the GRAPH tab, and check that the graph of T vs. a is selected. Use the zoom controls to adjust the graph so you can see all your data and it fills the graph. A. What does the graph indicate? B. Does the graph of T vs. a form a straight line? 6. Investigate: Choose other options in the dropdown menus until you find a graph that makes a perfectly straight line. (If you cannot see your data, click the [@ controls to zoom out.) Which relationship makes a straight line? When you have achieved a straight line, take a snapshot of the graph and paste it into a blank document you will turn in with this worksheet. 7. Calculate: On the table on the previous page, label the third column “a® and the fourth column “T2” Use a calculator to cube each value of a and square each value of T. What do you notice? Kepler’s third law states that the cube of a planet’s orbital radius is proportional to the square of a planet’s period: a’ = kT2 for some constant k. If the radius is measured in astronomical units, the period is measured in Earth years, and the mass of the star is equal to the mass of our Sun, the value of k is equal to 1 AU%/y?. 8. Challenge: The orbital radii of the planets are given in the table below. Calculate the period of each planet (in Earth years), and then check your values with your teacher. Planet a (AU) T (years) Planet a (AU) T (years) Mercury 0.39 Jupiter 5.20 Venus 0.72 Saturn 9.54 Earth 1.00 Uranus 19.18 Mars 1.52 Neptune 30.06 %}izmos
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Explorslearning ............................................................................................................... Teacher Guide: Orbital Motion Kepler’s Laws fifé? Learning Objectives Students will ... e Observe that planetary orbits are stable (assuming zero friction). ¢ Understand that planets travel in elliptical orbits with the Sun at one focus. o Calculate the eccentricity of an ellipse. e Explain why planets accelerate as they approach the Sun and decelerate as they move away from the Sun. ¢ Discover that planets sweep out equal areas in equal times. e Show that the square of a planet’s period is proportional to the cube of its orbital radius. @‘) Vocabulary astronomical unit, eccentricity, ellipse, force, gravity, Kepler’s first law, Kepler's second law, Kepler's third law, orbit, orbital radius, period, vector, velocity fii% Lesson Overview Several decades after Nicholas Copernicus revived the heliocentric (Sun-centered) model of the solar system, Johannes Kepler sought to determine the mathematical laws that govern planetary motion. His painstaking work resulted in the discovery of three fundamental laws of planetary motion. The Orbital Motion Kepler's Laws Gizmo™ allows students to model planetary orbits and discover Kepler's laws for themselves. A planet orbits a star. The Student Exploration sheet contains three activities: e Activity A Students observe that planets orbit in ellipses with the Sun at one focus. e Activity B —- Students discover that planets sweep out equal areas in equal times. e Activity C Students find the relationship between a planet’s orbital radius and period. Suggested Lesson Sequence o o 1. Pre-Gizmo activity: Solar System Explorer (€& 45 60 minutes) Use the Solar System Explorer Gizmo to introduce students to the geometry of planetary orbits. While doing the Student Exploration sheet for this Gizmo, students will see that planetary orbits are nearly, but not exactly, circular. After doing the Solar System Explorer Gizmo, have your students practice drawing ellipses and calculating their eccentricity. This activity is described in the Solar System Explorer Teacher Guide. In addition, you may wish to discuss the historical background to Kepler’s laws of planetary motion. (See the Scientific Background for details.) Explain the influence of Nicholas Copernicus, Tycho Brahe, and others on Kepler's work. wizmos
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2. Prior to using the Gizmo (68 10 15 minutes) Before students are at the computers, pass out the Student Exploration sheets and ask students to complete the Prior Knowledge Questions. Discuss student answers as a class, but do not provide correct answers at this point. Afterwards, if possible, use a projector to introduce the Gizmo and demonstrate its basic operations. Demonstrate how to take a screenshot and paste the image into a blank document. 3. Gizmo activities (€& 15 20 minutes per activity) Assign students to computers. Students can work individually or in small groups. Ask students to work through the activities in the Student Exploration using the Gizmo. Alternatively, you can use a projector and do the Exploration as a teacher-led activity. 4. Discussion questions (&8 15 30 minutes) As students are working or just after they are done, discuss the following questions: ¢ What would happen if a planet were hit by a large object that slowed it down? Would it have a different orbit or would it spiral into the Sun? [As long as the planet didn’t directly hit the Sun, it would go into a different stable orbit.] e What would happen to an orbit of a planet if it were traveling through a medium that caused the planet to gradually slow down? [The planet would spiral into the Sun. This doesn’t happen in our solar system because there is no friction in empty space.] ¢ In which direction does the gravity vector always point? e Try to create a series of orbits that are nearly circular. How does the speed of the planet relate to its distance from the Sun? Why is this true? [The closer the planet is to the Sun, the faster it must go to maintain a nearly circular orbit.] e How does the mass of the Sun affect the speed of a planet in orbit? ¢ If the Sun mass and Planet mass are set to medium, can you create an orbit that has an orbital radius closeto 1 AU? What is the period of this orbit? [This orbit is similar to Earth’s orbit and has a period close to 1 Earth year.] e As a planet orbits the Sun, does the Sun move? [To investigate this question, have students set the Sun mass to small, the Planet mass to large, and click Play. Students can then zoom in on the Sun as much as possible to see its motion, which is an ellipse that has the same shape as the planet’s orbit.] 5. Follow-up activity: Swinging milk carton (82 10 20 minutes) Planets orbit stars because of the force of gravity acting on the planet. At the same time, the planet exerts an equal force on the star. To model these forces, tie a rope securely around the handle of a 1-gallon milk carton. Choose an outdoor location with plenty of open space. Students can take turns whirling the heavy container around their bodies. Students will feel the strong pull of the milk carton on their arms. They will also discover that as the speed of the milk carton increases, the force required to hold on to the carton increases as well. Experiment with different lengths of rope and compare the speed of the orbiting milk carton with different orbital radii. Point out that once the carton is orbiting, the orbit can be maintained with only an inward pull, just as gravity pulls the planet toward the Sun. @;izmos
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Scientific Background Johannes Kepler (1571-1630) was a transitional figure in the development of modern astronomy. On one hand, Kepler was a theologian and astrologer whose motivation for studying the stars was to illuminate God’s plan for the universe. But Kepler was also a pioneer of using mathematics to analyze and find patterns in quantitative data. Although Kepler’'s laws were a key step in the development of modern science, he never abandoned his mystical idea that the spacing of planetary orbits was determined by the nesting of geometric solids, illustrated at right. Kepler's big break came in 1600, when he was invited to work for the Danish astronomer Tycho Brahe. Kepler spent years analyzing Tycho’s data to determine the exact shape of the orbit of Mars. After unsuccessfully applying a variety of geometric shapes to the orbit, Kepler eventually discovered that an elliptical model with the Sun at one focus matched observations perfectly. Subsequent analysis confirmed that all planetary orbits are elliptical. This is Kepler’s first law. While analyzing the orbit of Mars, Kepler observed that planets travel faster when closer to the Sun and more slowly when farther from the Sun. Kepler then discovered a remarkable relationship: A line joining a planet to the Sun sweeps out equal areas in equal times. In the diagram at left, both pink wedges were swept out in the same time period and are equal in area. This is Kepler's second law. Kepler's third law was discovered later, in 1619. Throughout his life, Kepler was obsessed by the “harmonies” that ruled the universe. Kepler was convinced that there was a harmonious relationship between the period of a planet (T) and its average orbital radius (a). After much trial and error, Kepler discovered that the square of the period is proportional to the cube of the radius. If the period is measured in Earth years and the orbital radius is measured in astronomical units (AU), the two values are nearly equal: 72 = a°. Although Kepler did not understand the causes of planetary motions, his work inspired Isaac Newton. Newton’s Philosophiae Naturalis Principia Mathematica, published in 1687, demonstrated that all of Kepler's laws arise from the law of universal gravitation. Selected Web Resources Planetary motion: http://farside.ph.utexas.edu/teaching/336k/Newton/node45.html Drawing ellipses activity: http://www.sciencebyjones.com/ellipse lab.htm Kepler's laws: http://csep10.phys.utk.edu/astr161/lect/history/kepler.html, http://www.physicsclassroom.com/class/circles/u6l4a.cfm, http://www.mathacademy.com/pr/prime/articles/kepler/index.asp Kepler biography: http://www-groups.dcs.st-and.ac.uk/~history/Biographies/Kepler.html Related Gizmos: Solar System Explorer. http://www.explorelearning.com/gizmo/id?441 Solar System: http://www.explorelearning.com/gizmo/id?636 Gravity Pitch: http://www.explorelearning.com/gizmo/id?648 Gravitational Force: http://www.explorelearning.com/gizmo/id?411 %}izmos
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