THE ROCKET EXPERIMENT 1. «Homogenous» gravitational field

Size: px
Start display at page:

Download "THE ROCKET EXPERIMENT 1. «Homogenous» gravitational field"

Transcription

1 THE OCKET EXPEIENT. «Hoogenous» gravitational field Let s assue, fig., that we have a body of ass Μ and radius. fig. As it is known, the gravitational field of ass Μ (both in ters of geoetry and dynaics) can never be hoogenous, fig.. In certain cases, however, the gravitational field of ass Μ, ay be considered «locally» very nearly hoogenous. Thus, e.g. at a distance h near the surface of ass Μ, to which the following relation applies: h 0 () The gravitational field of ass Μ ay be considered «locally» hoogenous in the sense that, its dynaic lines are parallel and its intensity g is constant fro the surface of ass Μ, to height h. Thus, in a celestial body of ass Μ and radius = 6000 k the gravitational field at a height h = 00 fro its surface, ay be considered very nearly hoogenous, because based on relation () we have:

2 h 0 = =,6 0 5 h i.e., 0 A NOTABLE OBSEVATION As observed, the hoogenous field of a body of ass Μ and radius, only relates to the radius and never the ass Μ of this body.. Free fall of a body in a hoogenous gravitational field Let s assue, fig. that we have a body of ass Μ and radius. fig. At a height h, we place a point ass. We now allow asses and Μ to ove freely under the influence of the force of universal attraction. In this case, ass will fall freely towards ass Μ and ass Μ will fall freely towards ass. Let s say that, at the oent of collision of the two asses and Μ, is the velocity of ass and V is the velocity of ass Μ, relative to an inertial observer O.

3 Thus, in the syste of the two bodies, by applying the principle of conservation of energy and the principle of conservation of oentu, we have: G + h = + V = V G () Where G is the constant of universal attraction and the nubers h,,,v are positive. Solving the equation syste (), relative to and V, we have: = V= h G (+ h) + h G (+ h) + (.) elations (.) are of great iportance, in ters of physics, as they express the free fall of ass in the non-hoogenous gravitational field of ass Μ. We now place ass at a height h, to which the following relation applies: h 0 (.) in this case, the gravitational field of ass Μ fro its surface and up to height h, can be considered very nearly hoogenous, with constant intensity g, as entioned above. Thus, fro relation (.), we have: h 0 h h + h (.3) Based on relation (.3), relations (.), yield (approxiately):

4 = G V= h + G h + (.4) Because, however, the intensity g of the hoogenous gravitational field of ass, fro its surface to height h, is considered constant, we have: g= G (.5) Thus, based on relation (.5), relations (.4), yield (approxiately): = gh + (.6) V= gh + As observed in relations (.6) velocity is a factor of ass and velocity V is a factor of ass Μ, obviously taking sizes g and h as constant. elations (.6) are of great iportant, in ters of physics, as they express the free fall of ass in the non-hoogenous gravitational field of ass Μ. In relations (.6), if we agree that ass is uch saller than ass Μ, i.e.: 0 the relations (.6) yield: = gh V = 0 (.7) elations (.7), are the well-known relations of Eleental echanics.

5 As observed, relations (.7) are independent of the ass of the body, which falls freely in the gravitational field of ass Μ. Obviously, relations (.7) expresses Galileo s well-know, erroneous law on the free fall of bodies. As observed, the conclusion of relations (.) and (.6) is in total contrast with Galileo s law on the free fall of bodies, which clais that: The velocity of bodies falling freely in the gravitational field of a ass Μ is independent fro the ass of the falling body. In other words, all bodies fall with the sae velocity in the gravitational field of a ass Μ, regardless of how large or sall their ass ay be. Obviously, what Galileo (and Einstein) clais is a big istake, because: LAW: The velocity of bodies falling freely in the gravitational field of a ass Μ, is always a function of their ass, whether the gravitational field of ass Μ is non-hoogenous, relations (.), or it is considered hoogenous (at a sall distance h near the surface of ass Μ, relations (.6)). Only equal asses fall with the sae velocity through the above gravitational fields (non-hoogenous or hoogenous), and never, under any circustances, unequal asses. In other words, therefore, believing that, «all bodies (regardless of their ass), fall with the sae velocity» in a hoogenous gravitational field is a grave istake. NOTE: elations (.6) also result fro relations: g ( + h) = V = + V + g (.8) by applying the principle of conservation of energy and the principle of conservation of oentu to the syste of the two bodies Μ of fig.. Solving the equation syste (.8) relative to and V, yields relations (.6). At this point, we need to stress thatin a syste of two bodies, fig. relations (.8) are only valid when: h i.e. when ass is in the hoogenous field of ass Μ) and obviously relations (.8) are never valid for just any h. That is a very «sensitive issue», which we ust bear in ind when referring to relations (.8). 0 ECAPITULATION Following what we looked at above, in a syste of two bodies and taking e.g. ass, as a point ass, fig., we have:. elations (.), apply to any asses and Μ and to any h.. elations (.6) are only valid when: h 0

6 i.e., when ass is within the hoogenous field of ass Μ. 3. elations (.7) are only valid when: h 0 and 0 i.e., when ass is within the hoogenous field of ass Μ and only when ass is uch saller that ass Μ, as, e.g. is the case in Galileo s experient (the leaning tower of Pisa). 3. The Proble Let s assue that we have a rocket S, within which there is an astronaut Ο. Thus, we tell astronaut Ο: Your rocket S will ove in one of the following phases, i.e.: PHASE Ι: Your rocket S will perfor unifor accelerated otion with constant acceleration γ, relative to an inertial observer O, fig. 3(a), or PHASE ΙΙ: Your rocker S will be placed otionless on the surface of a celestial body of ass Μ and radius. In this case, you will consider the gravitational field within your chaber as hoogenous and of constant intensity g, fig. 3 (b). fig.3 Next, we assign the astronaut Ο with the following proble: Can you, fro within your chaber, and by conducting various echanics experients, prove in which of the above two phases (Phase I or Phase II) your rocket is?

7 That is the proble assigned to astronaut Ο. 4. The astronaut s experients Astronaut Ο, in order o prove which of the two phases (Phase I or Phase II) his rocket is in, acts as follows: a. The device for easuring velocity To begin with, astronaut Ο places near the floor CD of his chaber, a device Ε that radiates e.g. two parallel laser beas L and L. Those parallel laser beas are at a sall distance d fro one another, and are parallel to the floor CD of the chaber. Beas L and L are connected to e.g. an oscilloscope, which acts as a chronoeter. Also, beas L and L are interrupted during the fall e.g. of a ass, and the oscilloscope (chronoeter) records the tie taken by ass to cross the distance d the two parallel beas L and L. In this way, astronaut Ο easures the velocity with which a ass, which was released fro the top AB of his chaber, falls onto the floor CD. Velocity is calculated using relation: d = (a) t where t is the tie recorded by the oscilloscope (chronoeter), when ass crossed the known distance d between the two parallel Laser beas L and L. b. Perforing the experients Astronaut Ο, after installing the device Ε for easuring velocity, as described above, now perfors the following experients: To begin with, he releases, fro the top AB of his chaber, a ass, which falls freely to the floor CD of his chaber and, using device E (in accordance with relation (a)), easures the velocity of the fall of ass. He then repeats the sae experient with a different ass, ( < ) and easures, once again using device E, the velocity with which ass falls on the floor CD of his chaber. In other words, astronaut Ο allows asses and to fall separately (first ass and the repeats the process with ass ) and does not allow asses and to fall siultaneously fro the top of his chaber. Now astronaut Ο copares the velocities and of asses and and concludes that: Α. If velocities and are equal, then his rocket S is in Phase Ι. Astronaut Ο bases this conclusion on the fundaental property of accelerating reference systes to give all bodies (regardless of their ass) the sae acceleration and, subsequently, velocity. Β. Conversely, if velocities and are unequal, and if, specifically >, the rocket S is in Phase II. Astronaut Ο bases this concussion on the first of relations (.6). Subsequently, conclusions Α and Β, as detailed above, are astronaut O s answer to the proble we set hi. Obviously, this answer provided by astronaut Ο is correct and in accordance with reality, regarding the Phase (Phase Ι or Phase II) in which rocket S actually is. NOTE:

8 Ι. The body of ass Μ and radius entioned above, ay be, for exaple:. A balloon full of air, of a radius e.g. =6000 k.. A sphere, ade of cork or iron, of a radius e.g. =000 k. 3. A sall asteroid, the oon, the Earth, a planet, etc, etc. II. The asses and used by astronaut Ο in the experients he conducts within his chaber ay be, for exaple:. A sall sphere ade of cork, of diaeter e.g. D= c.. An iron sphere, of diaeter e.g. D=50 c. 3. A sphere, consisting of the aterial of a neutron star (the density of which is known to be d= 0 5 kg/c 3 ), of diaeter e.g. D=0 c, etc, etc. III. The height h of the astronaut s chaber is sall, easuring a few etres, e.g. h = 0 (saller or larger) so that the gravitational field of ass Μ within the astronaut s chaber can be considered very nearly hoogenous (for the above nuerical exaple Ι), in accordance with the «notable observation» entioned at the beginning of this project. 5. Various other conclusions drawn by the astronaut Astronaut O, following the above correct answer he gave to the proble we set hi, now proceeds to other conclusions regarding the Phase (Phase I or Phase II) his rocket S is in. Astronaut Ο follows the thought process below: Astronaut Ο says: a. In accordance with the above, if I reach conclusion (b.a) then, by placing a dynaoeter D at the top of y chaber, I can calculate the acceleration γ with which y rocket oves, relative to the inertial observer O, i.e.: F γ= (3) where F is the reading of dynaoeter D and is a known ass attached to the end of the dynaoeter s spring. Since the inertial force field within the chaber is hoogenous, with constant intensity g (g =γ). b. If, however (says astronaut Ο) I reach conclusion (b.b), and because the gravitational field within y chaber is hoogenous, with constant intensity g, then I will act as follows: As, with the help of device Ε, I have found out the velocities and of asses and, that fall towards the floor CD of y chaber, I will obviously also know their ratio k, i.e.: = k (4) Thus, fro the first of relations (.6) the velocity of ass, is:

9 gh = (5) + and the velocity of ass, is: gh = (6) + Fro relations (5) and (6), because <, it follows that >. Dividing now by eber relations (5) and (6), we have: + = (7) + And based on relation (4), relation (7) yields: k = (8) k In relation (8), because,, k are known, astronaut Ο also knows the ass Μ of the celestial body, where his rocket S is docked. Also, fro the first of relations (.6), we have = gh + or gh = (9) + Now, by replacing the Μ in relation (9) with that of relation (8), we have: ( k ) = + h k g (0) In relation (0) factors, h,, k are known.

10 Subsequently, fro relation (0), astronaut Ο also knows the intensity g of the hoogenous gravitational field of ass Μ, where his rocket is S is docked. Finally, fro the relation: g= G () We have: G = () g Where G is the constant of universal attraction. Substituting, now, in relation () the Μ and g provided by relations (8) and (0) results in: ( k ) ( )( k ) h = G (3) In relation (3) factors G, h,,,, k are known. Subsequently, on the basis of relation (3), astronaut Ο also knows the radius of ass Μ, where his rocket S is docked. Following what we discussed above, regarding the rocket experient, we are led to this basic conclusion: CONCLUSION Ι Under no circustances can a hoogenous gravitational field, with intensity g, be equivalent to a hoogenous inertial force field, with acceleration γ, (γ= g). In other words: An observer Ο, who is within chaber S (and by conducting various echanics experients), can easily ascertain: whether his chaber is perforing unifor accelerated otion with constant acceleration γ, relative to an inertial observer O or whether his chaber is otionless in a hoogenous gravitational field with constant intensity g, of a ass Μ, which is outside his chaber. Thus, according to the above conclusion, the «equivalence principle» of the General Theory of elativity is copletely erroneous. ANOTHE ISTAKE BY EINSTEIN... As is well known, in the «equivalence principle» (weak equivalence principle), Einstein clais that: «A reference syste S (e.g. an elevator), falling freely in the gravitational field of a ass Μ, is locally equivalent to an inertial reference syste». Einstein s clai, however, is wrong, because: Let s assue, fig. 4, that we have a spherical shell (e.g. a spherical elevator), of ass and radius, falling freely fro

11 a height h, in the gravitational field of a ass Μ. An observer Ο, who is within the elevator, places a ass, ( < ) at he centre Κ of the spherical elevator chaber. fig. 4 Now, if what Einstein clais above, fig. 4, on the «equivalence principle» were correct, then, during the elevator s free fall in the gravitational field of ass Μ, ass would reain at the centre Κ of the elevator chaber (as would be the case if the elevator were an inertial reference syste S, away fro gravitational fields). As we have proven in a previous chapter of our project, however (See, link: «Galileo and Einstein are wrong») the ass of the spherical elevator falls at a greater velocity than the velocity of ass, relative to an inertial observer O. Subsequently, observer Ο, ο who is within the elevator, will observe ass oving fro the centre Κ towards the «ceiling» of the chaber during the elevator s free fall in the gravitational field of ass Μ. After exaining the above, we are led to the following basic conclusion:

12 CONCLUSION II A reference syste S, falling freely in the non-hoogenous or hoogenous gravitational field of a ass Μ can never be locally equivalent to an inertial reference syste. In other words: An observer Ο, who is within a reference syste S, which is falling freely in the gravitational field of a ass, by conducting various echanics experients (such as, e.g. the ass placed at the centre K of the spherical elevator, as described above) can easily ascertain whether his reference syste is falling freely in the gravitational field of a ass, or whether his reference syste S is an inertial reference syste, away fro gravitational fields. Specifically, in ters of our experient above:. If ass reains at the centre Κ of the spherical elevator chaber, the observer Ο, who is within the elevator, will know that his chaber is an inertial reference syste, away fro gravitational fields.. If ass oves fro the centre Κ of the spherical elevator chaber, the observer Ο, who is within the elevator, will know that his chaber is a reference syste S, falling freely in the gravitational field of a ass Μ, which is outside his chaber. Thus, in accordance wit the above, the «equivalence principle» of the General Theory of elativity ust be rejected as copletely erroneous. A QUESTION ON THE «EQUIVALENCE PINCIPLE»... It is well known that, in the «strong equivalence principle», Einstein accepts that: «All bodies (regardless of their ass) fall with the sae velocity in the gravitational field of a ass», (See book:clifford. Will, Was Einstein right?. QUESTION: Can «Einstein» (the relativists) show us the atheatical relation that the above conclusion is based on? Which is that atheatical relation? Let «Einstein» (the relativists) present us with this atheatical relation, so that we can see and judge it or ourselves. ECAPITULATION Following all that we exained in our project, and on the basis on Conclusion I and Conclusion II, it is clearly and undoubtedly proven that the «equivalence principle» (weak and strong equivalence principle) is a copletely erroneous theory of Physics. Subsequently, the General Theory of elativity (which, as we know, is based on the «equivalence principle») ust also be considered as a copletely erroneous theory of Physics. Christos A. Tsolkas tsolkas@otenet.gr

Physics 140 D100 Midterm Exam 2 Solutions 2017 Nov 10

Physics 140 D100 Midterm Exam 2 Solutions 2017 Nov 10 There are 10 ultiple choice questions. Select the correct answer for each one and ark it on the bubble for on the cover sheet. Each question has only one correct answer. (2 arks each) 1. An inertial reference

More information

Rationality Problems of the Principles of Equivalence and General Relativity

Rationality Problems of the Principles of Equivalence and General Relativity Rationality Probles of the Principles of Equivalence and General Relativity Mei Xiaochun (Departent of Physics, Fuzhou University, E-ail: xc1@163.co Tel:86-591-8761414) (N.7-B, South Building, Zhongfu

More information

NB1140: Physics 1A - Classical mechanics and Thermodynamics Problem set 2 - Forces and energy Week 2: November 2016

NB1140: Physics 1A - Classical mechanics and Thermodynamics Problem set 2 - Forces and energy Week 2: November 2016 NB1140: Physics 1A - Classical echanics and Therodynaics Proble set 2 - Forces and energy Week 2: 21-25 Noveber 2016 Proble 1. Why force is transitted uniforly through a assless string, a assless spring,

More information

m A 1 m mgd k m v ( C) AP Physics Multiple Choice Practice Oscillations

m A 1 m mgd k m v ( C) AP Physics Multiple Choice Practice Oscillations P Physics Multiple Choice Practice Oscillations. ass, attached to a horizontal assless spring with spring constant, is set into siple haronic otion. Its axiu displaceent fro its equilibriu position is.

More information

Work, Energy and Momentum

Work, Energy and Momentum Work, Energy and Moentu Work: When a body oves a distance d along straight line, while acted on by a constant force of agnitude F in the sae direction as the otion, the work done by the force is tered

More information

8.1 Force Laws Hooke s Law

8.1 Force Laws Hooke s Law 8.1 Force Laws There are forces that don't change appreciably fro one instant to another, which we refer to as constant in tie, and forces that don't change appreciably fro one point to another, which

More information

BALLISTIC PENDULUM. EXPERIMENT: Measuring the Projectile Speed Consider a steel ball of mass

BALLISTIC PENDULUM. EXPERIMENT: Measuring the Projectile Speed Consider a steel ball of mass BALLISTIC PENDULUM INTRODUCTION: In this experient you will use the principles of conservation of oentu and energy to deterine the speed of a horizontally projected ball and use this speed to predict the

More information

Department of Physics Preliminary Exam January 3 6, 2006

Department of Physics Preliminary Exam January 3 6, 2006 Departent of Physics Preliinary Exa January 3 6, 2006 Day 1: Classical Mechanics Tuesday, January 3, 2006 9:00 a.. 12:00 p.. Instructions: 1. Write the answer to each question on a separate sheet of paper.

More information

Lecture #8-3 Oscillations, Simple Harmonic Motion

Lecture #8-3 Oscillations, Simple Harmonic Motion Lecture #8-3 Oscillations Siple Haronic Motion So far we have considered two basic types of otion: translation and rotation. But these are not the only two types of otion we can observe in every day life.

More information

Reading from Young & Freedman: For this topic, read the introduction to chapter 25 and sections 25.1 to 25.3 & 25.6.

Reading from Young & Freedman: For this topic, read the introduction to chapter 25 and sections 25.1 to 25.3 & 25.6. PHY10 Electricity Topic 6 (Lectures 9 & 10) Electric Current and Resistance n this topic, we will cover: 1) Current in a conductor ) Resistivity 3) Resistance 4) Oh s Law 5) The Drude Model of conduction

More information

Potential Energy 4/7/11. Lecture 22: Chapter 11 Gravity Lecture 2. Gravitational potential energy. Total energy. Apollo 14, at lift-off

Potential Energy 4/7/11. Lecture 22: Chapter 11 Gravity Lecture 2. Gravitational potential energy. Total energy. Apollo 14, at lift-off Lecture 22: Chapter 11 Gravity Lecture 2 2 Potential Energy r Gravitational potential energy Escape velocity of a point ass for ass distributions Discrete Rod Spherical shell Sphere Gravitational potential

More information

Newton's Laws. Lecture 2 Key Concepts. Newtonian mechanics and relation to Kepler's laws The Virial Theorem Tidal forces Collision physics

Newton's Laws. Lecture 2 Key Concepts. Newtonian mechanics and relation to Kepler's laws The Virial Theorem Tidal forces Collision physics Lecture 2 Key Concepts Newtonian echanics and relation to Kepler's laws The Virial Theore Tidal forces Collision physics Newton's Laws 1) An object at rest will reain at rest and an object in otion will

More information

P (t) = P (t = 0) + F t Conclusion: If we wait long enough, the velocity of an electron will diverge, which is obviously impossible and wrong.

P (t) = P (t = 0) + F t Conclusion: If we wait long enough, the velocity of an electron will diverge, which is obviously impossible and wrong. 4 Phys520.nb 2 Drude theory ~ Chapter in textbook 2.. The relaxation tie approxiation Here we treat electrons as a free ideal gas (classical) 2... Totally ignore interactions/scatterings Under a static

More information

Physics 120 Final Examination

Physics 120 Final Examination Physics 120 Final Exaination 12 August, 1998 Nae Tie: 3 hours Signature Calculator and one forula sheet allowed Student nuber Show coplete solutions to questions 3 to 8. This exaination has 8 questions.

More information

Dimensions and Units

Dimensions and Units Civil Engineering Hydraulics Mechanics of Fluids and Modeling Diensions and Units You already know how iportant using the correct diensions can be in the analysis of a proble in fluid echanics If you don

More information

In the session you will be divided into groups and perform four separate experiments:

In the session you will be divided into groups and perform four separate experiments: Mechanics Lab (Civil Engineers) Nae (please print): Tutor (please print): Lab group: Date of lab: Experients In the session you will be divided into groups and perfor four separate experients: (1) air-track

More information

ma x = -bv x + F rod.

ma x = -bv x + F rod. Notes on Dynaical Systes Dynaics is the study of change. The priary ingredients of a dynaical syste are its state and its rule of change (also soeties called the dynaic). Dynaical systes can be continuous

More information

U V. r In Uniform Field the Potential Difference is V Ed

U V. r In Uniform Field the Potential Difference is V Ed SPHI/W nit 7.8 Electric Potential Page of 5 Notes Physics Tool box Electric Potential Energy the electric potential energy stored in a syste k of two charges and is E r k Coulobs Constant is N C 9 9. E

More information

8.012 Physics I: Classical Mechanics Fall 2008

8.012 Physics I: Classical Mechanics Fall 2008 MIT OpenCourseWare http://ocw.it.edu 8.012 Physics I: Classical Mechanics Fall 2008 For inforation about citing these aterials or our Ters of Use, isit: http://ocw.it.edu/ters. MASSACHUSETTS INSTITUTE

More information

Note-A-Rific: Mechanical

Note-A-Rific: Mechanical Note-A-Rific: Mechanical Kinetic You ve probably heard of inetic energy in previous courses using the following definition and forula Any object that is oving has inetic energy. E ½ v 2 E inetic energy

More information

Particle dynamics Physics 1A, UNSW

Particle dynamics Physics 1A, UNSW 1 Particle dynaics Physics 1A, UNSW Newton's laws: S & J: Ch 5.1 5.9, 6.1 force, ass, acceleration also weight Physclips Chapter 5 Friction - coefficients of friction Physclips Chapter 6 Hooke's Law Dynaics

More information

EN40: Dynamics and Vibrations. Midterm Examination Tuesday March

EN40: Dynamics and Vibrations. Midterm Examination Tuesday March EN4: Dynaics and Vibrations Midter Exaination Tuesday March 8 16 School of Engineering Brown University NAME: General Instructions No collaboration of any kind is peritted on this exaination. You ay bring

More information

The accelerated expansion of the universe is explained by quantum field theory.

The accelerated expansion of the universe is explained by quantum field theory. The accelerated expansion of the universe is explained by quantu field theory. Abstract. Forulas describing interactions, in fact, use the liiting speed of inforation transfer, and not the speed of light.

More information

PART 4. Theoretical Competition

PART 4. Theoretical Competition PART 4 Theoretical Copetition Exa coission page 98 Probles in English page 99 Solutions in English page 106 Probles in three other languages and back-translations of these page 117 Exaples of student papers

More information

PY241 Solutions Set 9 (Dated: November 7, 2002)

PY241 Solutions Set 9 (Dated: November 7, 2002) PY241 Solutions Set 9 (Dated: Noveber 7, 2002) 9-9 At what displaceent of an object undergoing siple haronic otion is the agnitude greatest for the... (a) velocity? The velocity is greatest at x = 0, the

More information

PY /005 Practice Test 1, 2004 Feb. 10

PY /005 Practice Test 1, 2004 Feb. 10 PY 205-004/005 Practice Test 1, 2004 Feb. 10 Print nae Lab section I have neither given nor received unauthorized aid on this test. Sign ature: When you turn in the test (including forula page) you ust

More information

Physics 218 Exam 3 Fall 2010, Sections

Physics 218 Exam 3 Fall 2010, Sections Physics 28 Exa 3 Fall 200, Sections 52-524 Do not fill out the inforation below until instructed to do so! Nae Signature Student ID E-ail Section # : SOUTIONS ules of the exa:. You have the full class

More information

ROTATIONAL MOTION FROM TRANSLATIONAL MOTION

ROTATIONAL MOTION FROM TRANSLATIONAL MOTION ROTATIONAL MOTION FROM TRANSLATIONAL MOTION Velocity Acceleration 1-D otion 3-D otion Linear oentu TO We have shown that, the translational otion of a acroscopic object is equivalent to the translational

More information

9. h = R. 10. h = 3 R

9. h = R. 10. h = 3 R Version PREVIEW Torque Chap. 8 sizeore (13756) 1 This print-out should have 3 questions. ultiple-choice questions ay continue on the next colun or page find all choices before answering. Note in the dropped

More information

Question 1. [14 Marks]

Question 1. [14 Marks] 6 Question 1. [14 Marks] R r T! A string is attached to the dru (radius r) of a spool (radius R) as shown in side and end views here. (A spool is device for storing string, thread etc.) A tension T is

More information

Name: Partner(s): Date: Angular Momentum

Name: Partner(s): Date: Angular Momentum Nae: Partner(s): Date: Angular Moentu 1. Purpose: In this lab, you will use the principle of conservation of angular oentu to easure the oent of inertia of various objects. Additionally, you develop a

More information

Lecture 8.2 Fluids For a long time now we have been talking about classical mechanics, part of physics which studies macroscopic motion of

Lecture 8.2 Fluids For a long time now we have been talking about classical mechanics, part of physics which studies macroscopic motion of Lecture 8 luids or a long tie now we have een talking aout classical echanics part of physics which studies acroscopic otion of particle-like ojects or rigid odies Using different ethods we have considered

More information

m A 9. The length of a simple pendulum with a period on Earth of one second is most nearly (A) 0.12 m (B) 0.25 m (C) 0.50 m (D) 1.0 m (E) 10.

m A 9. The length of a simple pendulum with a period on Earth of one second is most nearly (A) 0.12 m (B) 0.25 m (C) 0.50 m (D) 1.0 m (E) 10. P Physics Multiple Choice Practice Oscillations. ass, attache to a horizontal assless spring with spring constant, is set into siple haronic otion. Its axiu isplaceent fro its equilibriu position is. What

More information

CHAPTER 15: Vibratory Motion

CHAPTER 15: Vibratory Motion CHAPTER 15: Vibratory Motion courtesy of Richard White courtesy of Richard White 2.) 1.) Two glaring observations can be ade fro the graphic on the previous slide: 1.) The PROJECTION of a point on a circle

More information

Chapter 11: Vibration Isolation of the Source [Part I]

Chapter 11: Vibration Isolation of the Source [Part I] Chapter : Vibration Isolation of the Source [Part I] Eaple 3.4 Consider the achine arrangeent illustrated in figure 3.. An electric otor is elastically ounted, by way of identical isolators, to a - thick

More information

USEFUL HINTS FOR SOLVING PHYSICS OLYMPIAD PROBLEMS. By: Ian Blokland, Augustana Campus, University of Alberta

USEFUL HINTS FOR SOLVING PHYSICS OLYMPIAD PROBLEMS. By: Ian Blokland, Augustana Campus, University of Alberta 1 USEFUL HINTS FOR SOLVING PHYSICS OLYMPIAD PROBLEMS By: Ian Bloland, Augustana Capus, University of Alberta For: Physics Olypiad Weeend, April 6, 008, UofA Introduction: Physicists often attept to solve

More information

Ocean 420 Physical Processes in the Ocean Project 1: Hydrostatic Balance, Advection and Diffusion Answers

Ocean 420 Physical Processes in the Ocean Project 1: Hydrostatic Balance, Advection and Diffusion Answers Ocean 40 Physical Processes in the Ocean Project 1: Hydrostatic Balance, Advection and Diffusion Answers 1. Hydrostatic Balance a) Set all of the levels on one of the coluns to the lowest possible density.

More information

PH 221-1D Spring Oscillations. Lectures Chapter 15 (Halliday/Resnick/Walker, Fundamentals of Physics 9 th edition)

PH 221-1D Spring Oscillations. Lectures Chapter 15 (Halliday/Resnick/Walker, Fundamentals of Physics 9 th edition) PH 1-1D Spring 013 Oscillations Lectures 35-37 Chapter 15 (Halliday/Resnick/Walker, Fundaentals of Physics 9 th edition) 1 Chapter 15 Oscillations In this chapter we will cover the following topics: Displaceent,

More information

Angular Momentum. chapter

Angular Momentum. chapter chapter 11 Angular Moentu 11.1 The Vector Product and Torque 11.2 Analysis Model: Nonisolated yste (Angular Moentu) 11.3 Angular Moentu of a Rotating Rigid Object 11.4 Analysis Model: Isolated yste (Angular

More information

2 Q 10. Likewise, in case of multiple particles, the corresponding density in 2 must be averaged over all

2 Q 10. Likewise, in case of multiple particles, the corresponding density in 2 must be averaged over all Lecture 6 Introduction to kinetic theory of plasa waves Introduction to kinetic theory So far we have been odeling plasa dynaics using fluid equations. The assuption has been that the pressure can be either

More information

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics UNIVERSITY OF SASKATCHEWAN Departent of Physics and Engineering Physics 017 Saskatchewan High School Physics Scholarship Copetition Wednesday May 10, 017 Tie allowed: 90 inutes This copetition is based

More information

For a situation involving gravity near earth s surface, a = g = jg. Show. that for that case v 2 = v 0 2 g(y y 0 ).

For a situation involving gravity near earth s surface, a = g = jg. Show. that for that case v 2 = v 0 2 g(y y 0 ). Reading: Energy 1, 2. Key concepts: Scalar products, work, kinetic energy, work-energy theore; potential energy, total energy, conservation of echanical energy, equilibriu and turning points. 1.! In 1-D

More information

2009 Academic Challenge

2009 Academic Challenge 009 Acadeic Challenge PHYSICS TEST - REGIONAL This Test Consists of 5 Questions Physics Test Production Tea Len Stor, Eastern Illinois University Author/Tea Leader Doug Brandt, Eastern Illinois University

More information

SRI LANKAN PHYSICS OLYMPIAD MULTIPLE CHOICE TEST 30 QUESTIONS ONE HOUR AND 15 MINUTES

SRI LANKAN PHYSICS OLYMPIAD MULTIPLE CHOICE TEST 30 QUESTIONS ONE HOUR AND 15 MINUTES SRI LANKAN PHYSICS OLYMPIAD - 5 MULTIPLE CHOICE TEST QUESTIONS ONE HOUR AND 5 MINUTES INSTRUCTIONS This test contains ultiple choice questions. Your answer to each question ust be arked on the answer sheet

More information

Chapter 4 FORCES AND NEWTON S LAWS OF MOTION PREVIEW QUICK REFERENCE. Important Terms

Chapter 4 FORCES AND NEWTON S LAWS OF MOTION PREVIEW QUICK REFERENCE. Important Terms Chapter 4 FORCES AND NEWTON S LAWS OF MOTION PREVIEW Dynaics is the study o the causes o otion, in particular, orces. A orce is a push or a pull. We arrange our knowledge o orces into three laws orulated

More information

,... m n. , m 2. , m 3. 2, r. is called the moment of mass of the particle w.r.t O. and m 2

,... m n. , m 2. , m 3. 2, r. is called the moment of mass of the particle w.r.t O. and m 2 CENTRE OF MASS CENTRE OF MASS Every physical syste has associated with it a certain point whose otion characterises the otion of the whole syste. When the syste oves under soe external forces, then this

More information

Physics 139B Solutions to Homework Set 3 Fall 2009

Physics 139B Solutions to Homework Set 3 Fall 2009 Physics 139B Solutions to Hoework Set 3 Fall 009 1. Consider a particle of ass attached to a rigid assless rod of fixed length R whose other end is fixed at the origin. The rod is free to rotate about

More information

Energy and Momentum: The Ballistic Pendulum

Energy and Momentum: The Ballistic Pendulum Physics Departent Handout -10 Energy and Moentu: The Ballistic Pendulu The ballistic pendulu, first described in the id-eighteenth century, applies principles of echanics to the proble of easuring the

More information

Chapter 11 Simple Harmonic Motion

Chapter 11 Simple Harmonic Motion Chapter 11 Siple Haronic Motion "We are to adit no ore causes of natural things than such as are both true and sufficient to explain their appearances." Isaac Newton 11.1 Introduction to Periodic Motion

More information

Problem T1. Main sequence stars (11 points)

Problem T1. Main sequence stars (11 points) Proble T1. Main sequence stars 11 points Part. Lifetie of Sun points i..7 pts Since the Sun behaves as a perfectly black body it s total radiation power can be expressed fro the Stefan- Boltzann law as

More information

Stern-Gerlach Experiment

Stern-Gerlach Experiment Stern-Gerlach Experient HOE: The Physics of Bruce Harvey This is the experient that is said to prove that the electron has an intrinsic agnetic oent. Hydrogen like atos are projected in a bea through a

More information

Lecture 6. Announcements. Conservation Laws: The Most Powerful Laws of Physics. Conservation Laws Why they are so powerful

Lecture 6. Announcements. Conservation Laws: The Most Powerful Laws of Physics. Conservation Laws Why they are so powerful Conseration Laws: The Most Powerful Laws of Physics Potential Energy gh Moentu p = + +. Energy E = PE + KE +. Kinetic Energy / Announceents Mon., Sept. : Second Law of Therodynaics Gie out Hoework 4 Wed.,

More information

Tutorial Exercises: Incorporating constraints

Tutorial Exercises: Incorporating constraints Tutorial Exercises: Incorporating constraints 1. A siple pendulu of length l ass is suspended fro a pivot of ass M that is free to slide on a frictionless wire frae in the shape of a parabola y = ax. The

More information

Problem Set 14: Oscillations AP Physics C Supplementary Problems

Problem Set 14: Oscillations AP Physics C Supplementary Problems Proble Set 14: Oscillations AP Physics C Suppleentary Probles 1 An oscillator consists of a bloc of ass 050 g connected to a spring When set into oscillation with aplitude 35 c, it is observed to repeat

More information

Physics 201, Lecture 15

Physics 201, Lecture 15 Physics 0, Lecture 5 Today s Topics q More on Linear Moentu And Collisions Elastic and Perfect Inelastic Collision (D) Two Diensional Elastic Collisions Exercise: Billiards Board Explosion q Multi-Particle

More information

The Lagrangian Method vs. other methods (COMPARATIVE EXAMPLE)

The Lagrangian Method vs. other methods (COMPARATIVE EXAMPLE) The Lagrangian ethod vs. other ethods () This aterial written by Jozef HANC, jozef.hanc@tuke.sk Technical University, Kosice, Slovakia For Edwin Taylor s website http://www.eftaylor.co/ 6 January 003 The

More information

Ph 20.3 Numerical Solution of Ordinary Differential Equations

Ph 20.3 Numerical Solution of Ordinary Differential Equations Ph 20.3 Nuerical Solution of Ordinary Differential Equations Due: Week 5 -v20170314- This Assignent So far, your assignents have tried to failiarize you with the hardware and software in the Physics Coputing

More information

P235 Midterm Examination Prof. Cline

P235 Midterm Examination Prof. Cline P235 Mier Exaination Prof. Cline THIS IS A CLOSED BOOK EXAMINATION. Do all parts of all four questions. Show all steps to get full credit. 7:00-10.00p, 30 October 2009 1:(20pts) Consider a rocket fired

More information

Physics 204A FINAL EXAM Chapters 1-14 Spring 2006

Physics 204A FINAL EXAM Chapters 1-14 Spring 2006 Nae: Solve the following probles in the space provided Use the back of the page if needed Each proble is worth 0 points You ust show your work in a logical fashion starting with the correctly applied physical

More information

Physics 221B: Solution to HW # 6. 1) Born-Oppenheimer for Coupled Harmonic Oscillators

Physics 221B: Solution to HW # 6. 1) Born-Oppenheimer for Coupled Harmonic Oscillators Physics B: Solution to HW # 6 ) Born-Oppenheier for Coupled Haronic Oscillators This proble is eant to convince you of the validity of the Born-Oppenheier BO) Approxiation through a toy odel of coupled

More information

Practice Final Exam PY 205 Monday 2004 May 3

Practice Final Exam PY 205 Monday 2004 May 3 Practice Final Exa PY 05 Monday 004 May 3 Nae There are THREE forula pages. Read all probles carefully before attepting to solve the. Your work ust be legible, and the organization ust be clear. Correct

More information

15 Newton s Laws #2: Kinds of Forces, Creating Free Body Diagrams

15 Newton s Laws #2: Kinds of Forces, Creating Free Body Diagrams Chapter 15 ewton s Laws #2: inds of s, Creating ree Body Diagras 15 ewton s Laws #2: inds of s, Creating ree Body Diagras re is no force of otion acting on an object. Once you have the force or forces

More information

Some Perspective. Forces and Newton s Laws

Some Perspective. Forces and Newton s Laws Soe Perspective The language of Kineatics provides us with an efficient ethod for describing the otion of aterial objects, and we ll continue to ake refineents to it as we introduce additional types of

More information

Motion Analysis of Euler s Disk

Motion Analysis of Euler s Disk Motion Analysis of Euler s Disk Katsuhiko Yaada Osaka University) Euler s Disk is a nae of a scientific toy and its otion is the sae as a spinning coin. In this study, a siple atheatical odel is proposed

More information

Kinematics and dynamics, a computational approach

Kinematics and dynamics, a computational approach Kineatics and dynaics, a coputational approach We begin the discussion of nuerical approaches to echanics with the definition for the velocity r r ( t t) r ( t) v( t) li li or r( t t) r( t) v( t) t for

More information

Chapter 2: Introduction to Damping in Free and Forced Vibrations

Chapter 2: Introduction to Damping in Free and Forced Vibrations Chapter 2: Introduction to Daping in Free and Forced Vibrations This chapter ainly deals with the effect of daping in two conditions like free and forced excitation of echanical systes. Daping plays an

More information

m potential kinetic forms of energy.

m potential kinetic forms of energy. Spring, Chapter : A. near the surface of the earth. The forces of gravity and an ideal spring are conservative forces. With only the forces of an ideal spring and gravity acting on a ass, energy F F will

More information

Kinetic Theory of Gases. Chapter 33 1/6/2017. Kinetic Theory of Gases

Kinetic Theory of Gases. Chapter 33 1/6/2017. Kinetic Theory of Gases 1/6/017 Kinetic Theory of Gases Kinetic Theory of Gases Chapter 33 Kinetic theory of gases envisions gases as a collection of atos or olecules in otion. Atos or olecules are considered as particles. This

More information

NUMERICAL MODELLING OF THE TYRE/ROAD CONTACT

NUMERICAL MODELLING OF THE TYRE/ROAD CONTACT NUMERICAL MODELLING OF THE TYRE/ROAD CONTACT PACS REFERENCE: 43.5.LJ Krister Larsson Departent of Applied Acoustics Chalers University of Technology SE-412 96 Sweden Tel: +46 ()31 772 22 Fax: +46 ()31

More information

Field Mass Generation and Control. Chapter 6. The famous two slit experiment proved that a particle can exist as a wave and yet

Field Mass Generation and Control. Chapter 6. The famous two slit experiment proved that a particle can exist as a wave and yet 111 Field Mass Generation and Control Chapter 6 The faous two slit experient proved that a particle can exist as a wave and yet still exhibit particle characteristics when the wavefunction is altered by

More information

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics UNIVERSITY OF SASKATCHEWAN Departent of Physics and Engineering Physics 05 Saskatchewan High School Physics Scholarship Copetition May, 05 Tie allowed: 90 inutes This copetition is based on the Saskatchewan

More information

The Characteristic Planet

The Characteristic Planet The Characteristic Planet Brano Zivla, bzivla@gail.co Abstract: I have calculated a relation significant for planets fro a logical starting point that a whole and its parts are ianently depandant on each

More information

1 Statistics of volumes, swept by spheroidal particles, in a turbulent flow.

1 Statistics of volumes, swept by spheroidal particles, in a turbulent flow. 1 Statistics of volues, swept by spheroidal particles, in a turbulent flow. B. Grits*, M. Pinsky, and A. Khain Institute of Earth Science, The Hebrew University of Jerusale 1. INTRODUCTION Collisions between

More information

National 5 Summary Notes

National 5 Summary Notes North Berwick High School Departent of Physics National 5 Suary Notes Unit 3 Energy National 5 Physics: Electricity and Energy 1 Throughout the Course, appropriate attention should be given to units, prefixes

More information

EN40: Dynamics and Vibrations. Final Examination Tuesday May 15, 2011

EN40: Dynamics and Vibrations. Final Examination Tuesday May 15, 2011 EN40: ynaics and Vibrations Final Exaination Tuesday May 15, 011 School of Engineering rown University NME: General Instructions No collaboration of any ind is peritted on this exaination. You ay use double

More information

Analysis of Impulsive Natural Phenomena through Finite Difference Methods A MATLAB Computational Project-Based Learning

Analysis of Impulsive Natural Phenomena through Finite Difference Methods A MATLAB Computational Project-Based Learning Analysis of Ipulsive Natural Phenoena through Finite Difference Methods A MATLAB Coputational Project-Based Learning Nicholas Kuia, Christopher Chariah, Mechatronics Engineering, Vaughn College of Aeronautics

More information

XI PHYSICS M. AFFAN KHAN LECTURER PHYSICS, AKHSS, K. https://promotephysics.wordpress.com

XI PHYSICS M. AFFAN KHAN LECTURER PHYSICS, AKHSS, K. https://promotephysics.wordpress.com XI PHYSICS M. AFFAN KHAN LECTURER PHYSICS, AKHSS, K affan_414@live.co https://prootephysics.wordpress.co [MOTION] CHAPTER NO. 3 In this chapter we are going to discuss otion in one diension in which we

More information

Chapter GRAVITATION. Activity Gravitation. Let us try to understand the motion of the moon by recalling activity 8.11.

Chapter GRAVITATION. Activity Gravitation. Let us try to understand the motion of the moon by recalling activity 8.11. Chapter 10 GRAVITATION In Chapters 8 and 9, we have learnt about the otion of objects and force as the cause of otion. We have learnt that a force is needed to change the speed or the direction of otion

More information

Final Exam, vers Physics Fall, 2012

Final Exam, vers Physics Fall, 2012 1 Final Exa, - Physics 1110 - Fall, 01 NAME Signature Student ID # TA s Nae(Circle one): Clarissa Briner, Effie Fine, Mathis Habich, Ada Keith, Willia Lewis, John Papaioannou, WeisenShen, JiayiXie, Jian

More information

Year 12 Physics Holiday Work

Year 12 Physics Holiday Work Year 1 Physics Holiday Work 1. Coplete questions 1-8 in the Fields assessent booklet and questions 1-3 In the Further Mechanics assessent booklet (repeated below in case you have lost the booklet).. Revise

More information

Massachusetts Institute of Technology Quantum Mechanics I (8.04) Spring 2005 Solutions to Problem Set 4

Massachusetts Institute of Technology Quantum Mechanics I (8.04) Spring 2005 Solutions to Problem Set 4 Massachusetts Institute of Technology Quantu Mechanics I (8.04) Spring 2005 Solutions to Proble Set 4 By Kit Matan 1. X-ray production. (5 points) Calculate the short-wavelength liit for X-rays produced

More information

Intelligent Systems: Reasoning and Recognition. Perceptrons and Support Vector Machines

Intelligent Systems: Reasoning and Recognition. Perceptrons and Support Vector Machines Intelligent Systes: Reasoning and Recognition Jaes L. Crowley osig 1 Winter Seester 2018 Lesson 6 27 February 2018 Outline Perceptrons and Support Vector achines Notation...2 Linear odels...3 Lines, Planes

More information

Molecular interactions in beams

Molecular interactions in beams Molecular interactions in beas notable advanceent in the experiental study of interolecular forces has coe fro the developent of olecular beas, which consist of a narrow bea of particles, all having the

More information

KINETIC THEORY. Contents

KINETIC THEORY. Contents KINETIC THEORY This brief paper on inetic theory deals with three topics: the hypotheses on which the theory is founded, the calculation of pressure and absolute teperature of an ideal gas and the principal

More information

EN40: Dynamics and Vibrations. Midterm Examination Tuesday March

EN40: Dynamics and Vibrations. Midterm Examination Tuesday March EN4: Dynaics and ibrations Midter Exaination Tuesday Marc 4 14 Scool of Engineering Brown University NAME: General Instructions No collaboration of any kind is peritted on tis exaination. You ay bring

More information

Take-Home Midterm Exam #2, Part A

Take-Home Midterm Exam #2, Part A Physics 151 Due: Friday, March 20, 2009 Take-Hoe Midter Exa #2, Part A Roster No.: Score: NO exa tie liit. Calculator required. All books and notes are allowed, and you ay obtain help fro others. Coplete

More information

Instruction Sheet Martin Henschke, Ballistic Pendulum art. no.:

Instruction Sheet Martin Henschke, Ballistic Pendulum art. no.: Physics Educational Tools Dr. Martin Henschke Gerätebau Dieselstr. 8, 5374 Erftstadt, Gerany www.henschke-geraetebau.de/english/ Instruction Sheet Martin Henschke, 4-6-1 Ballistic Pendulu art. no.: 6573

More information

2.003 Engineering Dynamics Problem Set 2 Solutions

2.003 Engineering Dynamics Problem Set 2 Solutions .003 Engineering Dynaics Proble Set Solutions This proble set is priarily eant to give the student practice in describing otion. This is the subject of kineatics. It is strongly recoended that you study

More information

increases. In part (b) the impulse and initial momentum are in opposite directions and the velocity decreases.

increases. In part (b) the impulse and initial momentum are in opposite directions and the velocity decreases. 8IDENTIFY and SET U: p = K = EXECUTE: (a) 5 p = (, kg)( /s) = kg /s 5 p kg /s (b) (i) = = = 6 /s (ii) kg =, so T T SUV SUV, kg ( /s) 68 /s T SUV = T = = SUV kg EVALUATE:The SUV ust hae less speed to hae

More information

.c, C CD. m s. C.c DISCLAIMER

.c, C CD. m s. C.c DISCLAIMER cu Q).c, G r e. 8 C. CD S s : v. C.c DSCLAMER This report was prepared as an account of work sponsored by an agency of the United States Governent. Neither the United States Governent nor any agency thereof,

More information

Welcome to Vibrationdata

Welcome to Vibrationdata Welcoe to Vibrationdata Acoustics Shock Vibration Signal Processing July 006 Newsletter Pax Vobiscu Feature Articles Given the absence of a third choice, the Universe is either filled with soe hypothetical

More information

I. Understand get a conceptual grasp of the problem

I. Understand get a conceptual grasp of the problem MASSACHUSETTS INSTITUTE OF TECHNOLOGY Departent o Physics Physics 81T Fall Ter 4 Class Proble 1: Solution Proble 1 A car is driving at a constant but unknown velocity,, on a straightaway A otorcycle is

More information

9 HOOKE S LAW AND SIMPLE HARMONIC MOTION

9 HOOKE S LAW AND SIMPLE HARMONIC MOTION Experient 9 HOOKE S LAW AND SIMPLE HARMONIC MOTION Objectives 1. Verify Hoo s law,. Measure the force constant of a spring, and 3. Measure the period of oscillation of a spring-ass syste and copare it

More information

Physics Circular Motion: Energy and Momentum Conservation. Science and Mathematics Education Research Group

Physics Circular Motion: Energy and Momentum Conservation. Science and Mathematics Education Research Group F FA ACULTY C U L T Y OF O F EDUCATION E D U C A T I O N Departent of Curriculu and Pedagogy Physics Circular Motion: Energy and Moentu Conservation Science and Matheatics Education Research Group Supported

More information

ME Machine Design I. FINAL EXAM. OPEN BOOK AND CLOSED NOTES. Friday, May 8th, 2009

ME Machine Design I. FINAL EXAM. OPEN BOOK AND CLOSED NOTES. Friday, May 8th, 2009 ME 5 - Machine Design I Spring Seester 009 Nae Lab. Div. FINAL EXAM. OPEN BOOK AND LOSED NOTES. Friday, May 8th, 009 Please use the blank paper for your solutions. Write on one side of the paper only.

More information

Q5 We know that a mass at the end of a spring when displaced will perform simple m harmonic oscillations with a period given by T = 2!

Q5 We know that a mass at the end of a spring when displaced will perform simple m harmonic oscillations with a period given by T = 2! Chapter 4.1 Q1 n oscillation is any otion in which the displaceent of a particle fro a fixed point keeps changing direction and there is a periodicity in the otion i.e. the otion repeats in soe way. In

More information

CHAPTER 7 TEST REVIEW -- MARKSCHEME

CHAPTER 7 TEST REVIEW -- MARKSCHEME AP PHYSICS Nae: Period: Date: Points: 53 Score: IB Curve: DEVIL PHYSICS BADDEST CLASS ON CAMPUS 50 Multiple Choice 45 Single Response 5 Multi-Response Free Response 3 Short Free Response 2 Long Free Response

More information

Today s s topics are: Collisions and Momentum Conservation. Momentum Conservation

Today s s topics are: Collisions and Momentum Conservation. Momentum Conservation Today s s topics are: Collisions and P (&E) Conservation Ipulsive Force Energy Conservation How can we treat such an ipulsive force? Energy Conservation Ipulsive Force and Ipulse [Exaple] an ipulsive force

More information

Periodic Motion is everywhere

Periodic Motion is everywhere Lecture 19 Goals: Chapter 14 Interrelate the physics and atheatics of oscillations. Draw and interpret oscillatory graphs. Learn the concepts of phase and phase constant. Understand and use energy conservation

More information

26 Impulse and Momentum

26 Impulse and Momentum 6 Ipulse and Moentu First, a Few More Words on Work and Energy, for Coparison Purposes Iagine a gigantic air hockey table with a whole bunch of pucks of various asses, none of which experiences any friction

More information