Kinematics on oblique axes

Similar documents
CHAPTER 3 : VECTORS. Definition 3.1 A vector is a quantity that has both magnitude and direction.

Physics 2A Chapter 3 - Motion in Two Dimensions Fall 2017

UNDERSTAND MOTION IN ONE AND TWO DIMENSIONS

different formulas, depending on whether or not the vector is in two dimensions or three dimensions.

6.1.1 Angle between Two Lines Intersection of Two lines Shortest Distance from a Point to a Line

VIII - Geometric Vectors

1. Linear Motion. Table of Contents. 1.1 Linear Motion: Velocity Time Graphs (Multi Stage) 1.2 Linear Motion: Velocity Time Graphs (Up and Down)

8.0 Definition and the concept of a vector:

Chapter 3 Motion in a Plane

Status: Unit 2, Chapter 3

Space Probe and Relative Motion of Orbiting Bodies

Unit 11: Vectors in the Plane

The Kinetic Theory of Gases

DO PHYSICS ONLINE. WEB activity: Use the web to find out more about: Aristotle, Copernicus, Kepler, Galileo and Newton.

Linear Momentum and Collisions Conservation of linear momentum

Physics 1: Mechanics

Chapter 11 Collision Theory

Chapter 7 Introduction to vectors

The number of marks is given in brackets [ ] at the end of each question or part question. The total number of marks for this paper is 72.

Physics Kinematics: Projectile Motion. Science and Mathematics Education Research Group

Motion in Two and Three Dimensions

Physics Department Tutorial: Motion in a Circle (solutions)

ONLINE: MATHEMATICS EXTENSION 2 Topic 6 MECHANICS 6.6 MOTION IN A CIRCLE

Would you risk your live driving drunk? Intro

VISUAL PHYSICS ONLINE RECTLINEAR MOTION: UNIFORM ACCELERATION

Section 6: PRISMATIC BEAMS. Beam Theory

Roberto s Notes on Linear Algebra Chapter 1: Geometric vectors Section 8. The dot product

Lesson 3: Free fall, Vectors, Motion in a plane (sections )

The Dot Product Pg. 377 # 6ace, 7bdf, 9, 11, 14 Pg. 385 # 2, 3, 4, 6bd, 7, 9b, 10, 14 Sept. 25

Vectors in R n. P. Danziger

(a)!! d = 17 m [W 63 S]!! d opposite. (b)!! d = 79 cm [E 56 N] = 79 cm [W 56 S] (c)!! d = 44 km [S 27 E] = 44 km [N 27 W] metres. 3.

Applications of Forces

Elastic collisions in two dimensions 5B

FOCUS ON CONCEPTS Section 7.1 The Impulse Momentum Theorem

9/29/2014. Chapter 3 Kinematics in Two Dimensions; Vectors. 3-1 Vectors and Scalars. Contents of Chapter Addition of Vectors Graphical Methods

Cases of integrability corresponding to the motion of a pendulum on the two-dimensional plane

Conservation of Momentum in Two Dimensions

2-9. The plate is subjected to the forces acting on members A and B as shown. If θ = 60 o, determine the magnitude of the resultant of these forces

A-level Mathematics. MM03 Mark scheme June Version 1.0: Final

Reversal in time order of interactive events: Collision of inclined rods

Scalar multiplication and algebraic direction of a vector

LECTURE 2: CROSS PRODUCTS, MULTILINEARITY, AND AREAS OF PARALLELOGRAMS

Relativistic Energy Derivation

sin! =! d y =! d T ! d y = 15 m = m = 8.6 m cos! =! d x ! d x ! d T 2 =! d x 2 +! d y =! d x 2 +! d y = 27.2 m = 30.0 m tan! =!

Motion in Two and Three Dimensions

General Lorentz Boost Transformations, Acting on Some Important Physical Quantities

Pearson Physics Level 20 Unit I Kinematics: Chapter 2 Solutions

Mathematics Trigonometry: Unit Circle

v v Downloaded 01/11/16 to Redistribution subject to SEG license or copyright; see Terms of Use at

A Geometric Review of Linear Algebra

θ Vman V ship α φ V β

Velocity, Acceleration and Equations of Motion in the Elliptical Coordinate System

Chapter 3 Kinematics in Two Dimensions; Vectors

Dynamics ( 동역학 ) Ch.2 Motion of Translating Bodies (2.1 & 2.2)

CJ57.P.003 REASONING AND SOLUTION According to the impulse-momentum theorem (see Equation 7.4), F t = mv

be ye transformed by the renewing of your mind Romans 12:2

Chapter 8 Vectors and Scalars

PHYS 100: Lecture 3. r r r VECTORS. RELATIVE MOTION in 2-D. uuur uur uur SG S W. B y j x x x C B. A y j. A x i. B x i. v W. v S.

Lecture 12! Center of mass! Uniform circular motion!

Displacement, Time, Velocity

4-vectors. Chapter Definition of 4-vectors

F = q v B. F = q E + q v B. = q v B F B. F = q vbsinφ. Right Hand Rule. Lorentz. The Magnetic Force. More on Magnetic Force DEMO: 6B-02.

Chapter 1. The Postulates of the Special Theory of Relativity

0 a 3 a 2 a 3 0 a 1 a 2 a 1 0

3301/1H. MATHEMATICS (SPECIFICATION A) 3301/1H Higher Tier Paper 1 Non-Calculator. General Certificate of Secondary Education November 2005

(a) Taking the derivative of the position vector with respect to time, we have, in SI units (m/s),

Quiz No. 1: Tuesday Jan. 31. Assignment No. 2, due Thursday Feb 2: Problems 8.4, 8.13, 3.10, 3.28 Conceptual questions: 8.1, 3.6, 3.12, 3.

Why does Saturn have many tiny rings?

Physics 111. Help sessions meet Sunday, 6:30-7:30 pm in CLIR Wednesday, 8-9 pm in NSC 098/099

Magnetic Fields Part 3: Electromagnetic Induction

( ) Momentum and impulse Mixed exercise 1. 1 a. Using conservation of momentum: ( )

Doppler shifts in astronomy

A Geometric Review of Linear Algebra

A vector in the plane is directed line segment. The directed line segment AB

A Derivation of Free-rotation in the Three-dimensional Space

Transmission lines using a distributed equivalent circuit

Lecture #8-6 Waves and Sound 1. Mechanical Waves We have already considered simple harmonic motion, which is an example of periodic motion in time.

27 ft 3 adequately describes the volume of a cube with side 3. ft F adequately describes the temperature of a person.

EINSTEIN S KINEMATICS COMPLETED

Residual migration in VTI media using anisotropy continuation

Kinematics - study of motion HIGHER PHYSICS 1A UNSW SESSION s o t See S&J , ,

a by a factor of = 294 requires 1/T, so to increase 1.4 h 294 = h

MOTION IN 2-DIMENSION (Projectile & Circular motion And Vectors)

The Dot Product

6.3 Vectors in a Plane

III. Relative Velocity

MCAT Physics - Problem Drill 06: Translational Motion

Recognise the Equation of a Circle. Solve Problems about Circles Centred at O. Co-Ordinate Geometry of the Circle - Outcomes

Elements of diffraction theory part II

Centripetal force. Objectives. Assessment. Assessment. Equations. Physics terms 5/13/14

Supplementary Information Microfluidic quadrupole and floating concentration gradient Mohammad A. Qasaimeh, Thomas Gervais, and David Juncker

Last Time: Start Rotational Motion (now thru mid Nov) Basics: Angular Speed, Angular Acceleration

Kinematics in Two Dimensions; Vectors

NUMERICAL SIMULATION OF HYDRODYNAMIC FIELD FROM PUMP-TURBINE RUNNER

Chapter 2: 1D Kinematics Tuesday January 13th

Lesson 2: Kinematics (Sections ) Chapter 2 Motion Along a Line

SPACE-TIME HOLOMORPHIC TIME-PERIODIC SOLUTIONS OF NAVIER-STOKES EQUATIONS. 1. Introduction We study Navier-Stokes equations in Lagrangean coordinates

jfpr% ekuo /kez iz.ksrk ln~xq# Jh j.knksm+nklth egkjkt

PY1008 / PY1009 Physics Rotational motion

(1) Recap of Differential Calculus and Integral Calculus (2) Preview of Calculus in three dimensional space (3) Tools for Calculus 3

Transcription:

Bolina 1 Kinematics on oblique axes arxi:physics/01111951 [physics.ed-ph] 27 No 2001 Oscar Bolina Departamento de Física-Matemática Uniersidade de São Paulo Caixa Postal 66318 São Paulo 05315-970 Brasil E-mail; bolina@if.usp.br Abstract We sole a difficult problem inoling elocity acceleration components along oblique axes, propose two problems of central force motion to be soled using oblique axes. Key Words: Oblique axes, plane motion. PACS numbers: -1.40.-d, 45.50.- j Copyright c 2001 by the author. Reproduction of this article in its entirety is permitted for non-commercial purposes.

Bolina 2 1 Introduction Any ector quantity can be resoled into components according to the parallelogram law, both by rectangular oblique resolution. In rectangular coordinates, one component is perpendicular to the other. In oblique coordinates, one component has a projection on the other. We hae to take this projection into account when finding elocity acceleration components along these axes. Because of this, problems inoling oblique axes are ery difficult. Howeer, once one realizes that a problem requires oblique axes, the solution is not in general that hard, although the deriation of the kinematics on oblique axes is somewhat disgusting. 2 The elocity components Consider the motion of a particle in a plane. Suppose that the geometry of the motion is such that the elocity of the particle is more coneniently referred to two oblique axes Oξ Oη which make angles respectiely with a fixed direction Ox in the plane, as shown in Fig. 1. Theses angles may ary arbitrarily with time as the particle moes. Suppose that at the time t the components of the elocity in the directions Oξ Oη are u, respectiely. The perpendicular projections of these components along Oξ Oη are, respectiely, u + cos( ) + u cos( ), (2.1) as shown in the figure for the projection on the Oξ axis only. At the time t + t the axes Oξ Oη take the positions ξ η, as shown in Fig. 2, with ξoξ = ηoη =. Let the components of the elocity along these axes at this time be u + u +. The perpendicular projections of these components along the axes Oξ Oη are, respectiely, (u + u) cos + ( + ) cos( + ) ( + ) cos + (u + u) cos( ). (2.2)

Bolina 3 Οη u Οξ cos ( ) O x Figure 1: Oblique coordinate system the components of the elocity along oblique axes. Each component has a projection on the other axis. By taking the difference between the projections (2.2) (2.1) of the elocities along the axes Oξ Oη at the corresponding times t + t t, diiding the result by t, letting t go to zero, we obtain the projections of the acceleration along those axes at the time t: u + cos( ) sin( ) (2.3) + u cos( ) + u sin( ), (2.4) where u is the limiting alue of u/ t, when t approaches zero. 3 The acceleration components Now let a ξ a η represent the components of the acceleration of the particle along Oξ Oη at the time t. The same relationship (2.1) for elocities hold for accelerations. Thus, the perpendicular projections of the components

Bolina 4 η Οη + + + u+ u u ξ Οξ Figure 2: The component of the elocity u + u along the new axis ξ is projected on the old axis Oξ. along the axes Oξ Oη are a ξ + a η cos( ) a η + a ξ cos( ). (3.5) On equating (2.2) (3.5) we obtain a ξ + a η cos( ) = u + cos( ) sin( ) a η + a ξ cos( ) = + u cos( ) + u sin( ), (3.6) from which we can sole for a ξ a η. The first two terms in equations (3.6) are the rates of change of the projections (2.1) along fixed axes. The last terms are the consequence of the motion of the axes themseles. (Reference [2] suggests an alternatie approach to obtaining these equations.)

Bolina 5 Οη line circle Οξ u point Figure 3: An example of a difficult problem whose solution depends on the kinematics of oblique axes. 4 A difficult problem As an illustration, consider the following mind boggling problem [3]: A circle, a straight line, a point lie in one plane, the position of the point is determined by the lengths τ of its tangent to the circle p of its perpendicular to the line. Proe that, if the elocity of the point in made up of components u, in the directions of these lengths, if their mutual inclination is θ, the component accelerations will be u u τ cosθ, u + τ. Solution. Take the axis Oξ to be the tangent to the circle, Oη to be the axis perpendicular to the line. Set θ = note that does not ary with time. It is then easy to check that equations (3.6), with due change in notation, reduce to the following set of equations a t + a p cosθ = u + cos θ

Bolina 6 line circle O R t τ Q P Figure 4: The geometry of the illustratie problem. The particle moes from the point O to the point P. Its position is determined by the tangent line to the circle also by a perpendicular to a gien line in the plane. The tangent lines at two different times meet at Q make an angle. a p + a t cosθ = + u cosθ + u sin θ. (4.7) If we sole (4.7) for a t a p we obtain a t = u cos θ sin θ u a p = + u sin θ. (4.8) To eliminate the ariable we need to consider the (messy) geometry of the problem. Let the two tangent lines to the circle, drawn from the two positions of the particle at O P, meet at a point Q, as shown in Fig. 4. Note that the lines OQ PQ form an angle with each other at Q. Next, draw from the point P a perpendicular to the gien line. Let this perpendicular meet the line OQ at a point R. The perpendicular PR makes an angle with OQ. For small t, P is near O, we hae, approximately, PQ = τ PR = t. The law

Bolina 7 of sines, applied to the triangle PQR, gies t = sin θ τ or sin θ =. (4.9) τ Substituting gien aboe in (4.8), we obtain the desired result. 4.1 Further examples The equations for elocity acceleration components on oblique axes can be used to proide solution to problems of motion in a central force field when these problems are phrased as follows. 1. A particle P moes in a plane in such a way that its elocity has two constant components u, with u parallel to a fixed direction in the plane while is normal to a straight line from the particle to a fixed point O in the plane. Show that the acceleration of the particle is directed along the line OP. (In fact, the particle moes in a ellipse of eccentricity u/, haing O as a focus.) 2. A boat crosses a rier with elocity of constant magnitude u always aimed toward a point S on the opposite shore directly across its starting position. The riers also runs with uniform elocity u. Compare this problem with the preceding one. (How far downstream from S does the boat reach the opposite shore?) Acknowlgement. I was supported by Fapesp under grant 01/08485-6. References [1] R.L. Halfman, Dynamics, Addison-Wesley, 1962, p.19 [2] A.S. Ramsey, Dynamics, Part II, Cambridge Uniersity Press, 1951. (Chapter 3, p.75, example 15.) [3] E.T. Whittaker, A Treatise on the Analytical Dynamics of Particles Rigid Bodies, Fourth Edition, Doer Publication, N.Y. 1944. (Chapter 1, p.24, problem 13.)