Phys 201A. Homework 5 Solutions

Size: px
Start display at page:

Download "Phys 201A. Homework 5 Solutions"

Transcription

1 Phys 201A Homewok 5 Solutions 3. In each of the thee cases, you can find the changes in the velocity vectos by adding the second vecto to the additive invese of the fist and dawing the esultant, and by adding the thid vecto to the additive invese of the second and dawing the esultant. (a) 5 since minus is the same as plus which equals (b) Hee, finding the diffeence gives us a change in diection of the velocity vecto that points to the ight, which is choice 1. (c) In this case, the change in diection of the velocity vecto is staight downwad choice The point P is displaced vetically by 2R, whee R is the adius of the wheel. It is displaced hoizontally by half the cicumfeence of the wheel, o R. Since R = m, the hoizontal component of the displacement is m and the vetical component of the displacement is m. If the x axis is hoizontal and the y axis is vetical, the vecto displacement is = ((1.414 m) ˆ i + (0.900 m) ˆ j ). (b) The displacement has a magnitude of = ( πr) 2 + ( 2R) 2 = R π = 1.68 m and (b) an angle of tan 1 2R πr = tan 1 2 π = 32.5

2 above the floo. In physics thee ae no exact measuements, yet that angle computation seemed to yield something exact. Howeve, thee has to be some uncetainty in the obsevation that the wheel olled half of a evolution, which intoduces some indefiniteness in ou esult. 13. The diagam shows the displacement vectos fo the two segments of he walk, labeled A and B, and the total ( final ) displacement vecto, labeled Δ. We take east to be the +x diection and noth to be the +y diection. We obseve that the angle between A and the x axis is 60. Thus, the components of A ae A x = (250 m)(cos 60 ) = 125 m and A y = (250 m)(sin 30 ) = m. The components of B ae B x = 175 m and B y = 0 m. The components of the total displacement ae Δx = A x + B x = 125 m m = 300 m and Δy = A y + B y = m + 0 m = m. (a) The magnitude of the esultant displacement is Δ =Δ = Δx 2 +Δy 2 = (300 m) 2 + (216.5 m) 2 = 370 m. (b) The angle the esultant displacement makes with the +x axis is Δy tan 1 Δx = tan m 300 m = 36.

3 (c) The total distance walked is d = 250 m m = 425 m. (d) The total distance walked, d, is geate than the magnitude of the esultant displacement, Δ. The diagam shows why: A and B ae not collinea. 34. (a) The x-component of a is 3.00 m. (b) The y-component of a is 0 m. (c) The x-component of b is ( 4.00 m)cos 30 = 3.46 m. (d) The y-component of b is ( 4.00 m)sin30 = 2.00 m. (e) The x-component of c is ( 10.0 m )cos120 = 5.00 m. (f) The y-component of c is ( 10.0 m)sin120 = 8.66 m. (g) and (h) Since a has no y-component, q times the y-component of b must equal the y- component of c so q(2.00 m) = 8.66 m and q = Also, p times the x-component of a plus q times the x-component of b must equal the x- component of c. pa x + qb x = c x p(3.00 m) (3.46 m) = 5.00 m p = 6.66 m 3. We adopt the positive diection choices used in the textbook so that equations such as those in Table 5-1 ae diectly applicable. The initial velocity is hoizontal so that v 1 y = 0 m / s and v 1 x = v 1 = 161 km h. Conveting to SI units, this is v 1 x = 44.7 m/s.

4 (a) With the oigin at the initial point (whee the ball leaves the pitche s hand), the y-coodinate of the ball is given by y = 1 2 g( Δt) 2, and the x-coodinate is given by x = v 1 x Δt. Fom the latte equation, we have a simple popotionality between hoizontal distance and time, which means the time to tavel half the total distance is half the total time. Specifically, if x = (18.3 m)/2, then t = (9.15 m)/(44.7 m/s)= s. (b) And the time to tavel the next 9.15 m must also be s. It can be useful to wite the hoizontal equation as Δx = v 1 x Δt in ode that this esult can be seen moe clealy. (c) Fom y = 1 2 g( Δt) 2, we see that the y-coodinate of the ball is 1 2 ( 9.8 m / s 2 )( s) 2 = m at the moment the ball is halfway to the batte. (d) The ball s y-coodinate when it eaches the batte is 1 2 ( 9.8 m / s 2 )( s) 2 = m, which, when subtacted fom the pevious esult, implies it has fallen anothe m. Since the value of y is not simply popotional to t, we do not expect equal time-intevals to coespond to equal height-changes; in a physical sense, this is due to the fact that the initial y-velocity fo the fist half of the motion is not the same as the initial y-velocity fo the second half of the motion. 11. Taking the y axis to be upwad and placing the oigin at the fiing point, the y-coodinate is given by y = v 1 Δt sin θ g( Δt) 2 and the y-component of the velocity is given by v 2 y = v 1 sin 1 gt. The maximum height occus when v 2 y = 0. Thus, t = (v 1 /g) sin 1 and v 1g y max = v 1 sinθ 1 sinθ g(v 1 sinθ 1 ) 2 g = (v 1sinθ 1 ) 2 2 2g. 21. We adopt the positive diection choices used in the textbook so that equations such as those in Table 5-1 ae diectly applicable. The coodinate oigin is at gound level diectly below the elease point. We wite 1 = 37 fo the angle measued fom +x, since the angle given in the poblem is measued fom the y diection. We note that the initial speed of the pojectile is the plane s speed at the moment of elease. (a) We use Eq. 5-7 to find v 1.

5 y 2 y 1 = (v 1 sinθ 1 ) Δt 1 2 g( Δt) 2 0 m 730 m = v 1 sin( 37 )(5.00 s) 1 2 (9.8 m / s 2 )(5.00 s) 2 which yields v 1 = 202 m/s. (b) The hoizontal distance taveled using Eq. 5-5 is x = v 1 cos 1 t = (202 m/s)cos( 37.0 )(5.00 s) = 806 m. (c) The x-component (hoizontal) of the velocity (just befoe impact) is v x = v 1 cos 1 = (202 m/s) cos( 37.0 ) = 161 m/s. (d) The y-component (vetical) of the velocity (just befoe impact) is v 2 y = v 1 sin 1 gt = (202 m/s) sin ( 37 ) (9.80 m/s 2 )(5.00 s) = 171 m/s. 23. We adopt the positive diection choices used in the textbook so that equations such as those in Table 5-1 ae diectly applicable. The coodinate oigin is at gound level diectly below impact point between bat and ball. (a) We want to know how high the ball is fom the gound when it is at x = 97.5 m, which equies knowing the initial velocity. Using the given maximum ange infomation and Eq. 5-5, we solve fo t and then substitute that expession into Eq. 5-7 to solve fo v 1 : Δx = v 1 cos θ 1 Δt Δt = Δx = 107 m v 1 cos θ 1 v 1 cos 45.

6 Δy = v 1 sinθ 1 Δt 1 2 gδt 2 Δx 0 m = v 1 sinθ 1 1 Δx 2 g v 1 cos θ 1 v 1 cosθ 1 sinθ 1 Δx ( Δx) 2 = cos θ 1 2 g 1 v 1 = () v 2 1 cos θ 1 ( ) 2 gδx 2sinθ 1 cos θ 1 = 2 ( 9.8 m / s 2 )107 m 2 sin 45 o ( ) ( )( cos 45 o ) = 32.4 m / s. Then, Eq. 5-5 with the actual distance to the fence tells us when it is above the fence: Δt = Δx = 97.5 m = 4.26 s. v 1 cos θ 1 ( 32.4 m / s)cos 45 At this moment, the ball is at a height (above the gound) of y 2 = y 1 + ( v 1 sinθ 1 )Δt 1 g( Δt 2 )2 = 1.22 m + ( 32.4 m / s) ( sin 45 )4.26 ( s) m / s 2 ( )( 4.26 s) 2 = 9.88 m which implies it does indeed clea the 7.32 m high fence. (b) At t = 4.26 s, the cente of the ball is 9.88 m 7.32 m = 2.56 m above the fence. 32. The (x,y) coodinates of the points ae A = (15 m, 15 m), B = (30 m, 45 m), C = (20 m, 15 m), and D = (45 m, 45 m). The espective times ae t A = 0 s, t B = 300 s, t C = 600 s, and t D = 900 s. Aveage velocity is defined by Eq Each displacement Δ is undestood to oiginate at point A. The magnitudes of the thee displacements ae ( 15 m) 2 + ( 30 m) 2 = 34 m, 5 m, and ( 30 m) 2 + ( 60 m) 2 = 67 m. (a) The aveage velocity having the least magnitude is fo the displacement going fom A to C. v = ( 5 m) /( 600 s) = m / s at 0 (measued ccw fom the +x axis).

7 (b) The aveage velocity having the geatest magnitude fo the displacement going fom A to B: v = ( 15 m) 2 + ( 30 m) s = 0.11 m / s at θ = tan 1 30 m 15 m = 297 (ccw fom +x) o 63 (which is equivalent to measuing 63 clockwise fom the +x axis). 43. Since the x and y components of the acceleation ae constants, then we can use Table 2-1 fo the motion along both axes. This can be handled individually (fo x and y) o togethe with the unit-vecto notation (fo ). (a) Since 1 = 0 m, the position vecto of the paticle is (adapting Eq. 2-17) = v 1 Δt a ( Δt) 2 = [( 8.0 m / s)ˆ j ]Δt + 1 2[ ( 4.0 m / s 2 )ˆ i + ( 2.0 m / s2)ˆ j ]Δt ( ) 2 = [( 2.0 m / s 2 )( Δt) 2 ]ˆ i + {[ ( 8.0 m / s )Δt ]+ [( 1.0 m / s 2 ) ( Δt ) 2 ]}ˆ j. Theefoe, we find when x = 29 m, by solving ( 2.0 m / s 2 )( Δt) 2 = 29 m, which leads to t = 3.8 s. The y-coodinate at that time is y = (8.0 m/s)(3.8 s) + (1.0 m/s 2 )(3.8 s) 2 = 45 m. (b) Adapting Eq. 2-11, the velocity of the paticle is given by v 2 = v 1 + a Δt. Thus, at t = 3.8 s, the velocity is v = [ ( 8.0 m/s )ˆ j ]+ [( 4.0 m / s 2 )ˆ i + ( 2.0 m / s2)ˆ j ]3.8 ( s) = ( 15.2 m / s)ˆ i + ( 15.6 m / s)ˆ j which has a magnitude (speed) of

8 v = v = v x2 + v y2 = ( 15.2 m / s) 2 + ( 15.6 m / s) 2 = 22 m / s. 49. We apply Eq to solve fo speed v and Eq to find the magnitude of the acceleation a. (a) Since the adius of Eath is m, the adius of the satellite obit is m m = m. Theefoe, the speed of the satellite is ( ) ( ) = m/s. v = 2π T = 2π m ( 98.0 min)60 s / min (b) The magnitude of the acceleation is ( ) 2 a = v2 = m/s m = 8.00 m/ s We wite ou magnitude-angle esults in the fom ( R,θ). All angles ae measued counteclockwise fom +x, but we will occasionally efe to angles which ae measued counteclockwise fom the vetical line between the cicle-cente and the coodinate oigin and the line dawn fom the cicle-cente to the paticle location (see in the figue). We note that the speed of the paticle is v = 2/T whee = 3.00 m and the peiod T = 20.0 s so v = m/s. The paticle is moving counteclockwise in Fig (a) At t = 5.00 s, the paticle has taveled a faction of t T = 5.00 s 20.0 s ev = 1 4 ev

9 aound the cicle (stating at the oigin). Thus, elative to the cicle-cente, the paticle is at φ = 1 4 (360 ) = 90 measued fom vetical (as explained above). Refeing to Fig. 5-39, we see that this position (which is the 3 o clock position on the cicle) coesponds to x = 3.00 m and y = 3.00 m elative to the coodinate oigin. In ou magnitude-angle notation, this is expessed as ( 4.24 m, 45 ). Although this position is easy to analyze without esoting to tigonometic elations, it is useful (fo the computations below) to note that these values of x and y elative to coodinate oigin can be gotten fom the angle fom the elations x = sin and y = cos. Of couse, = x 2 + y 2 and comes fom choosing the appopiate possibility fom tan 1 (y/x) (o by using paticula functions of vecto-capable calculatos). (b) At t = 7.50 s, the paticle has taveled a faction of ( 7.50 s) /20.0 ( s)= 3/8 of a evolution aound the cicle (stating at the oigin). Relative to the cicle-cente, the paticle is theefoe at = 3/8 (360 ) = 135 measued fom vetical in the manne discussed above. Refeing to Fig. 5-39, we compute that this position coesponds to x = (3.00 m)(sin 135 ) = 2.12 m and y = 3.00 m (3.00 m)(cos 135 ) = 5.12 m elative to the coodinate oigin. In ou magnitude-angle notation, this is expessed as (R, ) = (5.54 m, 67.5 ). (c) At t = 10.0 s, the paticle has taveled a faction of (10.0 s)/(20.0 s) = 1/2 of a evolution aound the cicle. Relative to the cicle-cente, the paticle is at = 180 measued fom vetical (see explanation, above). Refeing to Fig. 5-39, we see that this position coesponds to x = 0 m and y = 6.00 m elative to the coodinate oigin. In ou magnitude-angle notation, this is expessed as ( R, θ)= ( 6.00 m, 90.0 ). (d) We subtact the position vecto in pat (a) fom the position vecto in pat (c): ( 6.00 m, 90.0 ) ( 4.24 m, 45 )= 4.24 m, 135 using vecto-capable calculatos). If we wish instead to use unit-vecto notation, we wite ( ) using magnitude-angle notation (convenient when Δ = (0 m 3.00 m) ˆ i + (6.00 m 3.00 m) ˆ j = ( 3.00 m) ˆ i + ( 3.00 m) ˆ j

10 which leads to Δ = 4.24 m and = 135. (e) Fom Eq. 5-22, we have v = Δ Δt whee Δt = 5.00 s which poduces ( m / s) ˆ i + ( m / s) ˆ j in unit-vecto notation o (0.849 m, 135 ) in magnitude-angle notation. (f) The speed has aleady been noted (v = m/s), but its diection is best seen by efeing again to Fig The velocity vecto is tangent to the cicle at its 3 o clock position (see pat (a)), which means v is vetical. Thus, ou esult is ( m / s, 90 ). (g) Again, the speed has been noted above (v = m/s), but its diection is best seen by efeing to Fig The velocity vecto is tangent to the cicle at its 12 o clock position (see pat (c)), which means v is hoizontal. Thus, ou esult is ( m, 180 ). (h) The acceleation has magnitude v 2 / = m/s 2, and at this instant (see pat (a)) it is hoizontal (towads the cente of the cicle). Thus, ou esult is m / s 2, 180 ( ). (i) Again, the acceleation has a magnitude v 2 / = m/s 2, but at this instant (see pat (c)) it is vetical (towads the cente of the cicle). Thus, ou esult is m / s 2, 270 ( ). 57. To calculate the centipetal acceleation of the stone, we need to know its speed duing its cicula motion (this is also its initial speed when it flies off). We use the kinematic equations of pojectile motion fom Table 5-1 to find that speed. Taking the +y diection to be upwad and placing the oigin at the point whee the stone leaves its cicula obit, then the coodinates of the stone duing its motion as a pojectile ae given by x = v 1 x Δt and y = 1 2 a y Δt 2 = 1 2 gδt 2 (since

11 v 1 y = 0 m / s ). It hits the gound at x = 10 m and y = 2.0 m. Fomally solving the second equation fo the time, we obtain Δt = 2y / g, which we substitute into the fist equation to find the x- component of it: v 1 x = x g 2y = 10 m ( ) 9.8 m / s 2 2( 2.0 m) Theefoe, the magnitude of the centipetal acceleation is = 15.7 m / s. a = v2 ( 15.7 m/ s) 2 = 1.5 m = 160 m/ s 2.

Motion in Two Dimensions

Motion in Two Dimensions SOLUTIONS TO PROBLEMS Motion in Two Dimensions Section 3.1 The Position, Velocity, and Acceleation Vectos P3.1 x( m) 0!3 000!1 70!4 70 m y( m)!3 600 0 1 70! 330 m (a) Net displacement x + y 4.87 km at

More information

Physics 11 Chapter 3: Vectors and Motion in Two Dimensions. Problem Solving

Physics 11 Chapter 3: Vectors and Motion in Two Dimensions. Problem Solving Physics 11 Chapte 3: Vectos and Motion in Two Dimensions The only thing in life that is achieved without effot is failue. Souce unknown "We ae what we epeatedly do. Excellence, theefoe, is not an act,

More information

4. Two and Three Dimensional Motion

4. Two and Three Dimensional Motion 4. Two and Thee Dimensional Motion 1 Descibe motion using position, displacement, elocity, and acceleation ectos Position ecto: ecto fom oigin to location of the object. = x i ˆ + y ˆ j + z k ˆ Displacement:

More information

INTRODUCTION. 2. Vectors in Physics 1

INTRODUCTION. 2. Vectors in Physics 1 INTRODUCTION Vectos ae used in physics to extend the study of motion fom one dimension to two dimensions Vectos ae indispensable when a physical quantity has a diection associated with it As an example,

More information

Physics 4A Chapter 8: Dynamics II Motion in a Plane

Physics 4A Chapter 8: Dynamics II Motion in a Plane Physics 4A Chapte 8: Dynamics II Motion in a Plane Conceptual Questions and Example Poblems fom Chapte 8 Conceptual Question 8.5 The figue below shows two balls of equal mass moving in vetical cicles.

More information

Describing Circular motion

Describing Circular motion Unifom Cicula Motion Descibing Cicula motion In ode to undestand cicula motion, we fist need to discuss how to subtact vectos. The easiest way to explain subtacting vectos is to descibe it as adding a

More information

PHYS Summer Professor Caillault Homework Solutions

PHYS Summer Professor Caillault Homework Solutions PHYS 1111 - Summe 2007 - Pofesso Caillault Homewok Solutions Chapte 3 13. Pictue the Poblem: The whale dives along a staight line tilted 20.0 below hoizontal fo 150 m as shown in the figue. Stategy: Resolve

More information

Rotational Motion. Lecture 6. Chapter 4. Physics I. Course website:

Rotational Motion. Lecture 6. Chapter 4. Physics I. Course website: Lectue 6 Chapte 4 Physics I Rotational Motion Couse website: http://faculty.uml.edu/andiy_danylov/teaching/physicsi Today we ae going to discuss: Chapte 4: Unifom Cicula Motion: Section 4.4 Nonunifom Cicula

More information

6.4 Period and Frequency for Uniform Circular Motion

6.4 Period and Frequency for Uniform Circular Motion 6.4 Peiod and Fequency fo Unifom Cicula Motion If the object is constained to move in a cicle and the total tangential foce acting on the total object is zeo, F θ = 0, then (Newton s Second Law), the tangential

More information

Physics 111 Lecture 5 (Walker: 3.3-6) Vectors & Vector Math Motion Vectors Sept. 11, 2009

Physics 111 Lecture 5 (Walker: 3.3-6) Vectors & Vector Math Motion Vectors Sept. 11, 2009 Physics 111 Lectue 5 (Walke: 3.3-6) Vectos & Vecto Math Motion Vectos Sept. 11, 2009 Quiz Monday - Chap. 2 1 Resolving a vecto into x-component & y- component: Pola Coodinates Catesian Coodinates x y =

More information

Chapter 8. Accelerated Circular Motion

Chapter 8. Accelerated Circular Motion Chapte 8 Acceleated Cicula Motion 8.1 Rotational Motion and Angula Displacement A new unit, adians, is eally useful fo angles. Radian measue θ(adians) = s = θ s (ac length) (adius) (s in same units as

More information

3.2 Centripetal Acceleration

3.2 Centripetal Acceleration unifom cicula motion the motion of an object with onstant speed along a cicula path of constant adius 3.2 Centipetal Acceleation The hamme thow is a tack-and-field event in which an athlete thows a hamme

More information

Circular Motion. Mr. Velazquez AP/Honors Physics

Circular Motion. Mr. Velazquez AP/Honors Physics Cicula Motion M. Velazquez AP/Honos Physics Objects in Cicula Motion Accoding to Newton s Laws, if no foce acts on an object, it will move with constant speed in a constant diection. Theefoe, if an object

More information

Kinematics in 2-D (II)

Kinematics 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 information

Ch04: Motion in two and three dimensions (2D and 3D)

Ch04: Motion in two and three dimensions (2D and 3D) Ch4: Motion in two and thee dimensions (D and 3D) Displacement, elocity and acceleation ectos Pojectile motion Cicula motion Relatie motion 4.: Position and displacement Position of an object in D o 3D

More information

r cos, and y r sin with the origin of coordinate system located at

r 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 information

Physics 107 TUTORIAL ASSIGNMENT #8

Physics 107 TUTORIAL ASSIGNMENT #8 Physics 07 TUTORIAL ASSIGNMENT #8 Cutnell & Johnson, 7 th edition Chapte 8: Poblems 5,, 3, 39, 76 Chapte 9: Poblems 9, 0, 4, 5, 6 Chapte 8 5 Inteactive Solution 8.5 povides a model fo solving this type

More information

Physics 111 Lecture 5 Circular Motion

Physics 111 Lecture 5 Circular Motion Physics 111 Lectue 5 Cicula Motion D. Ali ÖVGÜN EMU Physics Depatment www.aovgun.com Multiple Objects q A block of mass m1 on a ough, hoizontal suface is connected to a ball of mass m by a lightweight

More information

PHYS Summer Professor Caillault Homework Solutions

PHYS Summer Professor Caillault Homework Solutions PHYS 1111 - Summe 007 - Pofesso Caillault Homewok Solutions Chapte 4 3. Pictue the Poblem: The ca moves up the 5.5 incline with constant acceleation, changing both its hoizontal and vetical displacement

More information

PHYS Summer Professor Caillault Homework Solutions. Chapter 9

PHYS Summer Professor Caillault Homework Solutions. Chapter 9 PHYS - Summe 007 - Pofesso Caillault Homewok Solutions Chapte 9 3. Pictue the Poblem The owne walks slowly towad the notheast while the cat uns eastwad and the dog uns nothwad. Stategy Sum the momenta

More information

OSCILLATIONS AND GRAVITATION

OSCILLATIONS 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

Physics 2001 Problem Set 5 Solutions

Physics 2001 Problem Set 5 Solutions Physics 2001 Poblem Set 5 Solutions Jeff Kissel Octobe 16, 2006 1. A puck attached to a sting undegoes cicula motion on an ai table. If the sting beaks at the point indicated in the figue, which path (A,

More information

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j.

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j. 7. We denote the two foces F A + F B = ma,sof B = ma F A. (a) In unit vecto notation F A = ( 20.0 N)ˆ i and Theefoe, Phys 201A Homewok 6 Solutions F A and F B. Accoding to Newton s second law, a = [ (

More information

Physics 201 Homework 4

Physics 201 Homework 4 Physics 201 Homewok 4 Jan 30, 2013 1. Thee is a cleve kitchen gadget fo dying lettuce leaves afte you wash them. 19 m/s 2 It consists of a cylindical containe mounted so that it can be otated about its

More information

Graphs of Sine and Cosine Functions

Graphs of Sine and Cosine Functions Gaphs of Sine and Cosine Functions In pevious sections, we defined the tigonometic o cicula functions in tems of the movement of a point aound the cicumfeence of a unit cicle, o the angle fomed by the

More information

DYNAMICS OF UNIFORM CIRCULAR MOTION

DYNAMICS OF UNIFORM CIRCULAR MOTION Chapte 5 Dynamics of Unifom Cicula Motion Chapte 5 DYNAMICS OF UNIFOM CICULA MOTION PEVIEW An object which is moing in a cicula path with a constant speed is said to be in unifom cicula motion. Fo an object

More information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 10 Solutions. r s

MASSACHUSETTS 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 information

Chapter. s r. check whether your calculator is in all other parts of the body. When a rigid body rotates through a given angle, all

Chapter. s r. check whether your calculator is in all other parts of the body. When a rigid body rotates through a given angle, all conveted to adians. Also, be sue to vanced to a new position (Fig. 7.2b). In this inteval, the line OP has moved check whethe you calculato is in all othe pats of the body. When a igid body otates though

More information

ω = θ θ o = θ θ = s r v = rω

ω = θ θ o = θ θ = s r v = rω Unifom Cicula Motion Unifom cicula motion is the motion of an object taveling at a constant(unifom) speed in a cicula path. Fist we must define the angula displacement and angula velocity The angula displacement

More information

Lab #9: The Kinematics & Dynamics of. Circular Motion & Rotational Motion

Lab #9: The Kinematics & Dynamics of. Circular Motion & Rotational Motion Reading Assignment: Lab #9: The Kinematics & Dynamics of Cicula Motion & Rotational Motion Chapte 6 Section 4 Chapte 11 Section 1 though Section 5 Intoduction: When discussing motion, it is impotant to

More information

Sections and Chapter 10

Sections and Chapter 10 Cicula and Rotational Motion Sections 5.-5.5 and Chapte 10 Basic Definitions Unifom Cicula Motion Unifom cicula motion efes to the motion of a paticle in a cicula path at constant speed. The instantaneous

More information

Between any two masses, there exists a mutual attractive force.

Between 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 information

PS113 Chapter 5 Dynamics of Uniform Circular Motion

PS113 Chapter 5 Dynamics of Uniform Circular Motion PS113 Chapte 5 Dynamics of Unifom Cicula Motion 1 Unifom cicula motion Unifom cicula motion is the motion of an object taveling at a constant (unifom) speed on a cicula path. The peiod T is the time equied

More information

Chapter 7-8 Rotational Motion

Chapter 7-8 Rotational Motion Chapte 7-8 Rotational Motion What is a Rigid Body? Rotational Kinematics Angula Velocity ω and Acceleation α Unifom Rotational Motion: Kinematics Unifom Cicula Motion: Kinematics and Dynamics The Toque,

More information

Centripetal Force. Lecture 11. Chapter 8. Course website:

Centripetal Force. Lecture 11. Chapter 8. Course website: Lectue 11 Chapte 8 Centipetal Foce Couse website: http://faculty.uml.edu/andiy_danylov/teaching/physicsi PHYS.1410 Lectue 11 Danylov Depatment of Physics and Applied Physics Today we ae going to discuss:

More information

Easy. P4.2 Since the car is moving with constant speed and in a straight line, the. resultant force on it must be regardless of whether it is moving

Easy. P4.2 Since the car is moving with constant speed and in a straight line, the. resultant force on it must be regardless of whether it is moving Chapte 4 Homewok Solutions Easy P4. Since the ca is moving with constant speed and in a staight line, the zeo esultant foce on it must be egadless of whethe it is moving (a) towad the ight o the left.

More information

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session.

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session. - 5 - TEST 1R This is the epeat vesion of TEST 1, which was held duing Session. This epeat test should be attempted by those students who missed Test 1, o who wish to impove thei mak in Test 1. IF YOU

More information

Physics 181. Assignment 4

Physics 181. Assignment 4 Physics 181 Assignment 4 Solutions 1. A sphee has within it a gavitational field given by g = g, whee g is constant and is the position vecto of the field point elative to the cente of the sphee. This

More information

Vectors and 2D Motion. Vectors and Scalars

Vectors and 2D Motion. Vectors and Scalars Vectos and 2D Motion Vectos and Scalas Vecto aithmetic Vecto desciption of 2D motion Pojectile Motion Relative Motion -- Refeence Fames Vectos and Scalas Scala quantities: equie magnitude & unit fo complete

More information

Physics 2B Chapter 22 Notes - Magnetic Field Spring 2018

Physics 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 information

AP * PHYSICS B. Circular Motion, Gravity, & Orbits. Teacher Packet

AP * PHYSICS B. Circular Motion, Gravity, & Orbits. Teacher Packet AP * PHYSICS B Cicula Motion, Gavity, & Obits Teache Packet AP* is a tademak of the College Entance Examination Boad. The College Entance Examination Boad was not involved in the poduction of this mateial.

More information

The Laws of Motion ( ) N SOLUTIONS TO PROBLEMS ! F = ( 6.00) 2 + ( 15.0) 2 N = 16.2 N. Section 4.4. Newton s Second Law The Particle Under a Net Force

The Laws of Motion ( ) N SOLUTIONS TO PROBLEMS ! F = ( 6.00) 2 + ( 15.0) 2 N = 16.2 N. Section 4.4. Newton s Second Law The Particle Under a Net Force SOLUTIONS TO PROBLEMS The Laws of Motion Section 4.3 Mass P4. Since the ca is moving with constant speed and in a staight line, the esultant foce on it must be zeo egadless of whethe it is moving (a) towad

More information

Physics Fall Mechanics, Thermodynamics, Waves, Fluids. Lecture 6: motion in two and three dimensions III. Slide 6-1

Physics Fall Mechanics, Thermodynamics, Waves, Fluids. Lecture 6: motion in two and three dimensions III. Slide 6-1 Physics 1501 Fall 2008 Mechanics, Themodynamics, Waves, Fluids Lectue 6: motion in two and thee dimensions III Slide 6-1 Recap: elative motion An object moves with velocity v elative to one fame of efeence.

More information

Δt The textbook chooses to say that the average velocity is

Δt 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 information

Section 8.2 Polar Coordinates

Section 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 information

Relative motion (Translating axes)

Relative motion (Translating axes) Relative motion (Tanslating axes) Paticle to be studied This topic Moving obseve (Refeence) Fome study Obseve (no motion) bsolute motion Relative motion If motion of the efeence is known, absolute motion

More information

Trigonometric Functions of Any Angle 9.3 (, 3. Essential Question How can you use the unit circle to define the trigonometric functions of any angle?

Trigonometric Functions of Any Angle 9.3 (, 3. Essential Question How can you use the unit circle to define the trigonometric functions of any angle? 9. Tigonometic Functions of An Angle Essential Question How can ou use the unit cicle to define the tigonometic functions of an angle? Let be an angle in standad position with, ) a point on the teminal

More information

Centripetal Force OBJECTIVE INTRODUCTION APPARATUS THEORY

Centripetal Force OBJECTIVE INTRODUCTION APPARATUS THEORY Centipetal Foce OBJECTIVE To veify that a mass moving in cicula motion expeiences a foce diected towad the cente of its cicula path. To detemine how the mass, velocity, and adius affect a paticle's centipetal

More information

Introduction and Vectors

Introduction and Vectors SOLUTIONS TO PROBLEMS Intoduction and Vectos Section 1.1 Standads of Length, Mass, and Time *P1.4 Fo eithe sphee the volume is V = 4! and the mass is m =!V =! 4. We divide this equation fo the lage sphee

More information

rt () is constant. We know how to find the length of the radius vector by r( t) r( t) r( t)

rt () is constant. We know how to find the length of the radius vector by r( t) r( t) r( t) Cicula Motion Fom ancient times cicula tajectoies hae occupied a special place in ou model of the Uniese. Although these obits hae been eplaced by the moe geneal elliptical geomety, cicula motion is still

More information

PHYS Summer Professor Caillault Homework Solutions. Chapter 5

PHYS Summer Professor Caillault Homework Solutions. Chapter 5 PHYS 1111 - Summe 2007 - Pofesso Caillault Homewok Solutions Chapte 5 7. Pictue the Poblem: The ball is acceleated hoizontally fom est to 98 mi/h ove a distance of 1.7 m. Stategy: Use equation 2-12 to

More information

c) (6) Assuming the tires do not skid, what coefficient of static friction between tires and pavement is needed?

c) (6) Assuming the tires do not skid, what coefficient of static friction between tires and pavement is needed? Geneal Physics I Exam 2 - Chs. 4,5,6 - Foces, Cicula Motion, Enegy Oct. 10, 2012 Name Rec. Inst. Rec. Time Fo full cedit, make you wok clea to the gade. Show fomulas used, essential steps, and esults with

More information

Physics 101 Lecture 6 Circular Motion

Physics 101 Lecture 6 Circular Motion Physics 101 Lectue 6 Cicula Motion Assist. Pof. D. Ali ÖVGÜN EMU Physics Depatment www.aovgun.com Equilibium, Example 1 q What is the smallest value of the foce F such that the.0-kg block will not slide

More information

21 MAGNETIC FORCES AND MAGNETIC FIELDS

21 MAGNETIC FORCES AND MAGNETIC FIELDS CHAPTER 1 MAGNETIC ORCES AND MAGNETIC IELDS ANSWERS TO OCUS ON CONCEPTS QUESTIONS 1. (d) Right-Hand Rule No. 1 gives the diection of the magnetic foce as x fo both dawings A and. In dawing C, the velocity

More information

Physics C Rotational Motion Name: ANSWER KEY_ AP Review Packet

Physics C Rotational Motion Name: ANSWER KEY_ AP Review Packet Linea and angula analogs Linea Rotation x position x displacement v velocity a T tangential acceleation Vectos in otational motion Use the ight hand ule to detemine diection of the vecto! Don t foget centipetal

More information

Rotational Motion. Every quantity that we have studied with translational motion has a rotational counterpart

Rotational Motion. Every quantity that we have studied with translational motion has a rotational counterpart Rotational Motion & Angula Momentum Rotational Motion Evey quantity that we have studied with tanslational motion has a otational countepat TRANSLATIONAL ROTATIONAL Displacement x Angula Position Velocity

More information

Physics 11 Chapter 4: Forces and Newton s Laws of Motion. Problem Solving

Physics 11 Chapter 4: Forces and Newton s Laws of Motion. Problem Solving Physics 11 Chapte 4: Foces and Newton s Laws of Motion Thee is nothing eithe good o bad, but thinking makes it so. William Shakespeae It s not what happens to you that detemines how fa you will go in life;

More information

PDF Created with deskpdf PDF Writer - Trial ::

PDF Created with deskpdf PDF Writer - Trial :: A APPENDIX D TRIGONOMETRY Licensed to: jsamuels@bmcc.cun.edu PDF Ceated with deskpdf PDF Wite - Tial :: http://www.docudesk.com D T i g o n o m e t FIGURE a A n g l e s Angles can be measued in degees

More information

CIRCULAR MOTION. Particle moving in an arbitrary path. Particle moving in straight line

CIRCULAR MOTION. Particle moving in an arbitrary path. Particle moving in straight line 1 CIRCULAR MOTION 1. ANGULAR DISPLACEMENT Intoduction: Angle subtended by position vecto of a paticle moving along any abitay path w..t. some fixed point is called angula displacement. (a) Paticle moving

More information

Ch 13 Universal Gravitation

Ch 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 information

PROJECTILE MOTION. At any given point in the motion, the velocity vector is always a tangent to the path.

PROJECTILE MOTION. At any given point in the motion, the velocity vector is always a tangent to the path. PROJECTILE MOTION A pojectile is any object that has been thown though the ai. A foce must necessaily set the object in motion initially but, while it is moing though the ai, no foce othe than gaity acts

More information

e.g: If A = i 2 j + k then find A. A = Ax 2 + Ay 2 + Az 2 = ( 2) = 6

e.g: If A = i 2 j + k then find A. A = Ax 2 + Ay 2 + Az 2 = ( 2) = 6 MOTION IN A PLANE 1. Scala Quantities Physical quantities that have only magnitude and no diection ae called scala quantities o scalas. e.g. Mass, time, speed etc. 2. Vecto Quantities Physical quantities

More information

Circular motion. Objectives. Physics terms. Assessment. Equations 5/22/14. Describe the accelerated motion of objects moving in circles.

Circular motion. Objectives. Physics terms. Assessment. Equations 5/22/14. Describe the accelerated motion of objects moving in circles. Cicula motion Objectives Descibe the acceleated motion of objects moving in cicles. Use equations to analyze the acceleated motion of objects moving in cicles.. Descibe in you own wods what this equation

More information

MAGNETIC FIELD INTRODUCTION

MAGNETIC FIELD INTRODUCTION MAGNETIC FIELD INTRODUCTION It was found when a magnet suspended fom its cente, it tends to line itself up in a noth-south diection (the compass needle). The noth end is called the Noth Pole (N-pole),

More information

7.2. Coulomb s Law. The Electric Force

7.2. 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 information

to point uphill and to be equal to its maximum value, in which case f s, max = μsfn

to point uphill and to be equal to its maximum value, in which case f s, max = μsfn Chapte 6 16. (a) In this situation, we take f s to point uphill and to be equal to its maximum value, in which case f s, max = μsf applies, whee μ s = 0.5. pplying ewton s second law to the block of mass

More information

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE.

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE. Unit 6 actice Test 1. Which one of the following gaphs best epesents the aiation of the kinetic enegy, KE, and of the gaitational potential enegy, GE, of an obiting satellite with its distance fom the

More information

Uniform Circular Motion

Uniform Circular Motion Unifom Cicula Motion constant speed Pick a point in the objects motion... What diection is the velocity? HINT Think about what diection the object would tavel if the sting wee cut Unifom Cicula Motion

More information

Chap 5. Circular Motion: Gravitation

Chap 5. Circular Motion: Gravitation Chap 5. Cicula Motion: Gavitation Sec. 5.1 - Unifom Cicula Motion A body moves in unifom cicula motion, if the magnitude of the velocity vecto is constant and the diection changes at evey point and is

More information

Translation and Rotation Kinematics

Translation and Rotation Kinematics Tanslation and Rotation Kinematics Oveview: Rotation and Tanslation of Rigid Body Thown Rigid Rod Tanslational Motion: the gavitational extenal foce acts on cente-of-mass F ext = dp sy s dt dv total cm

More information

Circular Motion. x-y coordinate systems. Other coordinates... PHY circular-motion - J. Hedberg

Circular Motion. x-y coordinate systems. Other coordinates... PHY circular-motion - J. Hedberg Cicula Motion PHY 207 - cicula-motion - J. Hedbeg - 2017 x-y coodinate systems Fo many situations, an x-y coodinate system is a geat idea. Hee is a map on Manhattan. The steets ae laid out in a ectangula

More information

Trigonometry Standard Position and Radians

Trigonometry Standard Position and Radians MHF 4UI Unit 6 Day 1 Tigonomety Standad Position and Radians A. Standad Position of an Angle teminal am initial am Angle is in standad position when the initial am is the positive x-axis and the vetex

More information

Circular Orbits. and g =

Circular 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 information

Magnetic Field. Conference 6. Physics 102 General Physics II

Magnetic Field. Conference 6. Physics 102 General Physics II Physics 102 Confeence 6 Magnetic Field Confeence 6 Physics 102 Geneal Physics II Monday, Mach 3d, 2014 6.1 Quiz Poblem 6.1 Think about the magnetic field associated with an infinite, cuent caying wie.

More information

1121 T Question 1

1121 T Question 1 1121 T1 2008 Question 1 ( aks) You ae cycling, on a long staight path, at a constant speed of 6.0.s 1. Anothe cyclist passes you, tavelling on the sae path in the sae diection as you, at a constant speed

More information

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE.

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE. Unit 6 actice Test 1. Which one of the following gaphs best epesents the aiation of the kinetic enegy, KE, and of the gaitational potential enegy, GE, of an obiting satellite with its distance fom the

More information

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1

AST 121S: The origin and evolution of the Universe. Introduction to Mathematical Handout 1 Please ead this fist... AST S: The oigin and evolution of the Univese Intoduction to Mathematical Handout This is an unusually long hand-out and one which uses in places mathematics that you may not be

More information

Motion in a Plane Uniform Circular Motion

Motion in a Plane Uniform Circular Motion Lectue 11 Chapte 8 Physics I Motion in a Plane Unifom Cicula Motion Couse website: http://faculty.uml.edu/andiy_danylo/teaching/physicsi PHYS.1410 Lectue 11 Danylo Depatment of Physics and Applied Physics

More information

CHAPTER 5: Circular Motion; Gravitation

CHAPTER 5: Circular Motion; Gravitation CHAPER 5: Cicula Motion; Gavitation Solution Guide to WebAssign Pobles 5.1 [1] (a) Find the centipetal acceleation fo Eq. 5-1.. a R v ( 1.5 s) 1.10 1.4 s (b) he net hoizontal foce is causing the centipetal

More information

Determining solar characteristics using planetary data

Determining 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 information

Introduction to Mechanics Centripetal Force

Introduction to Mechanics Centripetal Force Intoduction to Mechanics Centipetal Foce Lana heidan De Anza College Ma 9, 2016 Last time intoduced unifom cicula motion centipetal foce Oveview using the idea of centipetal foce Detemine (a) the astonaut

More information

Uniform Circular Motion

Uniform 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 information

Motion along curved path *

Motion along curved path * OpenStax-CNX module: m14091 1 Motion along cuved path * Sunil Kuma Singh This wok is poduced by OpenStax-CNX and licensed unde the Ceative Commons Attibution License 2.0 We all expeience motion along a

More information

= 4 3 π( m) 3 (5480 kg m 3 ) = kg.

= 4 3 π( m) 3 (5480 kg m 3 ) = kg. CHAPTER 11 THE GRAVITATIONAL FIELD Newton s Law of Gavitation m 1 m A foce of attaction occus between two masses given by Newton s Law of Gavitation Inetial mass and gavitational mass Gavitational potential

More information

Multiple choice questions [100 points] As shown in the figure, a mass M is hanging by three massless strings from the ceiling of a room.

Multiple choice questions [100 points] As shown in the figure, a mass M is hanging by three massless strings from the ceiling of a room. Multiple choice questions [00 points] Answe all of the following questions. Read each question caefully. Fill the coect ule on you scanton sheet. Each coect answe is woth 4 points. Each question has exactly

More information

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion AH Mechanics Checklist (Unit ) AH Mechanics Checklist (Unit ) Cicula Motion No. kill Done 1 Know that cicula motion efes to motion in a cicle of constant adius Know that cicula motion is conveniently descibed

More information

Physics 2A Chapter 10 - Moment of Inertia Fall 2018

Physics 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 information

Homework 7 Solutions

Homework 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 information

Revision Guide for Chapter 11

Revision Guide for Chapter 11 Revision Guide fo Chapte 11 Contents Revision Checklist Revision Notes Momentum... 4 Newton's laws of motion... 4 Wok... 5 Gavitational field... 5 Potential enegy... 7 Kinetic enegy... 8 Pojectile... 9

More information

b) (5) What average force magnitude was applied by the students working together?

b) (5) What average force magnitude was applied by the students working together? Geneal Physics I Exam 3 - Chs. 7,8,9 - Momentum, Rotation, Equilibium Nov. 3, 2010 Name Rec. Inst. Rec. Time Fo full cedit, make you wok clea to the gade. Show fomulas used, essential steps, and esults

More information

Physics 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 =

Physics 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 information

Chapter 5 Force and Motion

Chapter 5 Force and Motion Chapte 5 Foce and Motion In chaptes 2 and 4 we have studied kinematics i.e. descibed the motion of objects using paametes such as the position vecto, velocity and acceleation without any insights as to

More information

b) (5) What is the magnitude of the force on the 6.0-kg block due to the contact with the 12.0-kg block?

b) (5) What is the magnitude of the force on the 6.0-kg block due to the contact with the 12.0-kg block? Geneal Physics I Exam 2 - Chs. 4,5,6 - Foces, Cicula Motion, Enegy Oct. 13, 2010 Name Rec. Inst. Rec. Time Fo full cedit, make you wok clea to the gade. Show fomulas used, essential steps, and esults with

More information

Chapters 5-8. Dynamics: Applying Newton s Laws

Chapters 5-8. Dynamics: Applying Newton s Laws Chaptes 5-8 Dynamics: Applying Newton s Laws Systems of Inteacting Objects The Fee Body Diagam Technique Examples: Masses Inteacting ia Nomal Foces Masses Inteacting ia Tensions in Ropes. Ideal Pulleys

More information

MODULE 5 ADVANCED MECHANICS GRAVITATIONAL FIELD: MOTION OF PLANETS AND SATELLITES VISUAL PHYSICS ONLINE

MODULE 5 ADVANCED MECHANICS GRAVITATIONAL FIELD: MOTION OF PLANETS AND SATELLITES VISUAL PHYSICS ONLINE VISUAL PHYSICS ONLIN MODUL 5 ADVANCD MCHANICS GRAVITATIONAL FILD: MOTION OF PLANTS AND SATLLITS SATLLITS: Obital motion of object of mass m about a massive object of mass M (m

More information

Chapter 5. Uniform Circular Motion. a c =v 2 /r

Chapter 5. Uniform Circular Motion. a c =v 2 /r Chapte 5 Unifom Cicula Motion a c =v 2 / Unifom cicula motion: Motion in a cicula path with constant speed s v 1) Speed and peiod Peiod, T: time fo one evolution Speed is elated to peiod: Path fo one evolution:

More information

Lecture 1a: Satellite Orbits

Lecture 1a: Satellite Orbits Lectue 1a: Satellite Obits Outline 1. Newton s Laws of Motion 2. Newton s Law of Univesal Gavitation 3. Calculating satellite obital paametes (assuming cicula motion) Scala & Vectos Scala: a physical quantity

More information

16.1 Permanent magnets

16.1 Permanent magnets Unit 16 Magnetism 161 Pemanent magnets 16 The magnetic foce on moving chage 163 The motion of chaged paticles in a magnetic field 164 The magnetic foce exeted on a cuent-caying wie 165 Cuent loops and

More information

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once.

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once. Honos Physics Fall, 2016 Cicula Motion & Toque Test Review Name: M. Leonad Instuctions: Complete the following woksheet. SHOW ALL OF YOUR WORK ON A SEPARATE SHEET OF PAPER. 1. Detemine whethe each statement

More information

Radian and Degree Measure

Radian and Degree Measure CHAT Pe-Calculus Radian and Degee Measue *Tigonomety comes fom the Geek wod meaning measuement of tiangles. It pimaily dealt with angles and tiangles as it petained to navigation, astonomy, and suveying.

More information