Rigid-Body Dynamics with Friction and Impact∗
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Rotational Motion (The Dynamics of a Rigid Body)
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Robert Katz Publications Research Papers in Physics and Astronomy 1-1958 Physics, Chapter 11: Rotational Motion (The Dynamics of a Rigid Body) Henry Semat City College of New York Robert Katz University of Nebraska-Lincoln, [email protected] Follow this and additional works at: https://digitalcommons.unl.edu/physicskatz Part of the Physics Commons Semat, Henry and Katz, Robert, "Physics, Chapter 11: Rotational Motion (The Dynamics of a Rigid Body)" (1958). Robert Katz Publications. 141. https://digitalcommons.unl.edu/physicskatz/141 This Article is brought to you for free and open access by the Research Papers in Physics and Astronomy at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Robert Katz Publications by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. 11 Rotational Motion (The Dynamics of a Rigid Body) 11-1 Motion about a Fixed Axis The motion of the flywheel of an engine and of a pulley on its axle are examples of an important type of motion of a rigid body, that of the motion of rotation about a fixed axis. Consider the motion of a uniform disk rotat ing about a fixed axis passing through its center of gravity C perpendicular to the face of the disk, as shown in Figure 11-1. The motion of this disk may be de scribed in terms of the motions of each of its individual particles, but a better way to describe the motion is in terms of the angle through which the disk rotates. -
Chapter 3 Dynamics of Rigid Body Systems
Rigid Body Dynamics Algorithms Roy Featherstone Rigid Body Dynamics Algorithms Roy Featherstone The Austrailian National University Canberra, ACT Austrailia Library of Congress Control Number: 2007936980 ISBN 978-0-387-74314-1 ISBN 978-1-4899-7560-7 (eBook) Printed on acid-free paper. @ 2008 Springer Science+Business Media, LLC All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. 9 8 7 6 5 4 3 2 1 springer.com Preface The purpose of this book is to present a substantial collection of the most efficient algorithms for calculating rigid-body dynamics, and to explain them in enough detail that the reader can understand how they work, and how to adapt them (or create new algorithms) to suit the reader’s needs. The collection includes the following well-known algorithms: the recursive Newton-Euler algo- rithm, the composite-rigid-body algorithm and the articulated-body algorithm. It also includes algorithms for kinematic loops and floating bases. -
Dynamics of Multibody Systems in Research and Education
Editorial Dynamics of Multibody Systems in Research and Education prof. Ing. Štefan Segľa, CSc. Technical University of Košice, Faculty of Mechanical Engineering, Department of Applied Mechanics and Mechanical Engineering Štefan Segľa, prof., Ing., CSc., (born in 1954) is a professor at the Technical University of Košice, Faculty of Mechanical Engineering, Institute of Design and Process Engineering. He graduated from the Faculty of Mechanical Engineering, Czech Technical University in Prague in 1978. His research areas are kinematic and dynamic analysis and optimization of mechanical and mechatronical systems. He is an author of three monographs, twelve textbooks and more than one hundred scientific publications in journals and conference proceedings in Slovakia and abroad. Forteen papers are registered in Web of Science and SCOPUS. He is a member of IFToMM (International Federation for the Promotion of Mechanism and Machine Science), its Permanent Commission for the Standardization of Terminology and Multibody Dynamics, a vice-chairman of the Slovak National Committee of IFToMM, a member of the Czech Society of Mechanics, Slovak Society of Mechanics and Central European Association for Computational Mechanics. Many common mechanisms and machines such as vehicle and aircraft subsystems, robotic systems, biomechanical and mechatronic systems consist of rigid and deformable bodies that undergo large rigid body motion. The bodies are interconnected with kinematical constraints and coupling elements. The dynamics of these large-scale and nonlinear systems under dynamic loading in most cases can only be solved with methods of computational mechanics. For these systems the concept of the multibody dynamics can be successfuly utilized. Their mechanical models should be as complex as necessary but also as simple as possible. -
Lie Group Formulation of Articulated Rigid Body Dynamics
Lie Group Formulation of Articulated Rigid Body Dynamics Junggon Kim 12/10/2012, Ver 2.01 Abstract It has been usual in most old-style text books for dynamics to treat the formulas describing linear(or translational) and angular(or rotational) motion of a rigid body separately. For example, the famous Newton's 2nd law, f = ma, for the translational motion of a rigid body has its partner, so-called the Euler's equation which describes the rotational motion of the body. Separating translation and rotation, however, causes a huge complexity in deriving the equations of motion of articulated rigid body systems such as robots. In Section1, an elegant single equation of motion of a rigid body moving in 3D space is derived using a Lie group formulation. In Section2, the recursive Newton-Euler algorithm (inverse dynamics), Articulated-Body algorithm (forward dynamics) and a generalized recursive algorithm (hybrid dynamics) for open chains or tree-structured articulated body systems are rewritten with the geometric formulation for rigid body. In Section3, dynamics of constrained systems such as a closed loop mechanism will be described. Finally, in Section4, analytic derivatives of the dynamics algorithms, which would be useful for optimization and sensitivity analysis, are presented.1 1 Dynamics of a Rigid Body This section describes the equations of motion of a single rigid body in a geometric manner. 1.1 Rigid Body Motion To describe the motion of a rigid body, we need to represent both the position and orien- tation of the body. Let fBg be a coordinate frame attached to the rigid body and fAg be an arbitrary coordinate frame, and all coordinate frames will be right-handed Cartesian from now on. -
Rigid Body Dynamics 2
Rigid Body Dynamics 2 CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2017 Cross Product & Hat Operator Derivative of a Rotating Vector Let’s say that vector r is rotating around the origin, maintaining a fixed distance At any instant, it has an angular velocity of ω ω dr r ω r dt ω r Product Rule The product rule of differential calculus can be extended to vector and matrix products as well da b da db b a dt dt dt dab da db b a dt dt dt dA B dA dB B A dt dt dt Rigid Bodies We treat a rigid body as a system of particles, where the distance between any two particles is fixed We will assume that internal forces are generated to hold the relative positions fixed. These internal forces are all balanced out with Newton’s third law, so that they all cancel out and have no effect on the total momentum or angular momentum The rigid body can actually have an infinite number of particles, spread out over a finite volume Instead of mass being concentrated at discrete points, we will consider the density as being variable over the volume Rigid Body Mass With a system of particles, we defined the total mass as: n m m i i1 For a rigid body, we will define it as the integral of the density ρ over some volumetric domain Ω m d Angular Momentum The linear momentum of a particle is 퐩 = 푚퐯 We define the moment of momentum (or angular momentum) of a particle at some offset r as the vector 퐋 = 퐫 × 퐩 Like linear momentum, angular momentum is conserved in a mechanical system If the particle is constrained only -
Modeling of Flexible Multibody Systems Excited by Moving Loads with Application to a Robotic Portal System
CORE Metadata, citation and similar papers at core.ac.uk Provided by Institute of Transport Research:Publications The 2nd Joint International Conference on Multibody System Dynamics May 29–June 1, 2012, Stuttgart, Germany Modeling of Flexible Multibody Systems Excited by Moving Loads with Application to a Robotic Portal System Stefan Hartweg and Andreas Heckmann Department of System Dynamics and Control Robotics and Mechatronics Center (RMC) German Aerospace Center (DLR) Muenchner Strasse 20, D-82234 Wessling, Germany [Stefan.Hartweg, Andreas.Heckmann]@DLR.de ABSTRACT In this paper, an approach to solve mechanical problems with moving loads and flexible bodies is presented. Therefore, the multi-disciplinary modeling language Modelica together with the DLR FlexibleBodies Li- brary is utilized. Rather than solving the equations of motion analytically, this approach solves them numer- ically. While large overall motions of the flexible parts are described using the Floating Frame of Reference (FFR) method, the deformation is represented by appropriate shape functions. It is shown how a subsystem with masses and spring-damper elements can be connected to the flexible body and how the occurring forces of this moving load affect it. The equations of motion are derived in a general way, yielding a formulation compatible to e. g. a finite element models which are reduced to global shape functions. The usage of this formulation is shown for the simulation of a robotic portal system. 1 INTRODUCTION A variety of structures in the field of engineering is subject to moving loads. These loads can result from external forces, masses or whole subsystems moving with constant or varying velocity along the structure. -
Rigid Body Dynamics II
An Introduction to Physically Based Modeling: Rigid Body Simulation IIÐNonpenetration Constraints David Baraff Robotics Institute Carnegie Mellon University Please note: This document is 1997 by David Baraff. This chapter may be freely duplicated and distributed so long as no consideration is received in return, and this copyright notice remains intact. Part II. Nonpenetration Constraints 6 Problems of Nonpenetration Constraints Now that we know how to write and implement the equations of motion for a rigid body, let's consider the problem of preventing bodies from inter-penetrating as they move about an environment. For simplicity, suppose we simulate dropping a point mass (i.e. a single particle) onto a ®xed ¯oor. There are several issues involved here. Because we are dealing with rigid bodies, that are totally non-¯exible, we don't want to allow any inter-penetration at all when the particle strikes the ¯oor. (If we considered our ¯oor to be ¯exible, we might allow the particle to inter-penetrate some small distance, and view that as the ¯oor actually deforming near where the particle impacted. But we don't consider the ¯oor to be ¯exible, so we don't want any inter-penetration at all.) This means that at the instant that the particle actually comes into contact with the ¯oor, what we would like is to abruptly change the velocity of the particle. This is quite different from the approach taken for ¯exible bodies. For a ¯exible body, say a rubber ball, we might consider the collision as occurring gradually. That is, over some fairly small, but non-zero span of time, a force would act between the ball and the ¯oor and change the ball's velocity. -
Newton Euler Equations of Motion Examples
Newton Euler Equations Of Motion Examples Alto and onymous Antonino often interloping some obligations excursively or outstrikes sunward. Pasteboard and Sarmatia Kincaid never flits his redwood! Potatory and larboard Leighton never roller-skating otherwhile when Trip notarizes his counterproofs. Velocity thus resulting in the tumbling motion of rigid bodies. Equations of motion Euler-Lagrange Newton-Euler Equations of motion. Motion of examples of experiments that a random walker uses cookies. Forces by each other two examples of example are second kind, we will refer to specify any parameter in. 213 Translational and Rotational Equations of Motion. Robotics Lecture Dynamics. Independence from a thorough description and angular velocity as expected or tofollowa userdefined behaviour does it only be loaded geometry in an appropriate cuts in. An interface to derive a particular instance: divide and author provides a positive moment is to express to output side can be run at all previous step. The analysis of rotational motions which make necessary to decide whether rotations are. For xddot and whatnot in which a very much easier in which together or arena where to use them in two backwards operation complies with respect to rotations. Which influence of examples are true, is due to independent coordinates. On sameor adjacent joints at each moment equation is also be more specific white ellipses represent rotations are unconditionally stable, for motion break down direction. Unit quaternions or Euler parameters are known to be well suited for the. The angular momentum and time and runnable python code. The example will be run physics examples are models can be symbolic generator runs faster rotation kinetic energy. -
Rotation: Moment of Inertia and Torque
Rotation: Moment of Inertia and Torque Every time we push a door open or tighten a bolt using a wrench, we apply a force that results in a rotational motion about a fixed axis. Through experience we learn that where the force is applied and how the force is applied is just as important as how much force is applied when we want to make something rotate. This tutorial discusses the dynamics of an object rotating about a fixed axis and introduces the concepts of torque and moment of inertia. These concepts allows us to get a better understanding of why pushing a door towards its hinges is not very a very effective way to make it open, why using a longer wrench makes it easier to loosen a tight bolt, etc. This module begins by looking at the kinetic energy of rotation and by defining a quantity known as the moment of inertia which is the rotational analog of mass. Then it proceeds to discuss the quantity called torque which is the rotational analog of force and is the physical quantity that is required to changed an object's state of rotational motion. Moment of Inertia Kinetic Energy of Rotation Consider a rigid object rotating about a fixed axis at a certain angular velocity. Since every particle in the object is moving, every particle has kinetic energy. To find the total kinetic energy related to the rotation of the body, the sum of the kinetic energy of every particle due to the rotational motion is taken. The total kinetic energy can be expressed as .. -
Leonhard Euler - Wikipedia, the Free Encyclopedia Page 1 of 14
Leonhard Euler - Wikipedia, the free encyclopedia Page 1 of 14 Leonhard Euler From Wikipedia, the free encyclopedia Leonhard Euler ( German pronunciation: [l]; English Leonhard Euler approximation, "Oiler" [1] 15 April 1707 – 18 September 1783) was a pioneering Swiss mathematician and physicist. He made important discoveries in fields as diverse as infinitesimal calculus and graph theory. He also introduced much of the modern mathematical terminology and notation, particularly for mathematical analysis, such as the notion of a mathematical function.[2] He is also renowned for his work in mechanics, fluid dynamics, optics, and astronomy. Euler spent most of his adult life in St. Petersburg, Russia, and in Berlin, Prussia. He is considered to be the preeminent mathematician of the 18th century, and one of the greatest of all time. He is also one of the most prolific mathematicians ever; his collected works fill 60–80 quarto volumes. [3] A statement attributed to Pierre-Simon Laplace expresses Euler's influence on mathematics: "Read Euler, read Euler, he is our teacher in all things," which has also been translated as "Read Portrait by Emanuel Handmann 1756(?) Euler, read Euler, he is the master of us all." [4] Born 15 April 1707 Euler was featured on the sixth series of the Swiss 10- Basel, Switzerland franc banknote and on numerous Swiss, German, and Died Russian postage stamps. The asteroid 2002 Euler was 18 September 1783 (aged 76) named in his honor. He is also commemorated by the [OS: 7 September 1783] Lutheran Church on their Calendar of Saints on 24 St. Petersburg, Russia May – he was a devout Christian (and believer in Residence Prussia, Russia biblical inerrancy) who wrote apologetics and argued Switzerland [5] forcefully against the prominent atheists of his time. -
Lecture L27 - 3D Rigid Body Dynamics: Kinetic Energy; Instability; Equations of Motion
J. Peraire, S. Widnall 16.07 Dynamics Fall 2008 Version 2.0 Lecture L27 - 3D Rigid Body Dynamics: Kinetic Energy; Instability; Equations of Motion 3D Rigid Body Dynamics In Lecture 25 and 26, we laid the foundation for our study of the three-dimensional dynamics of rigid bodies by: 1.) developing the framework for the description of changes in angular velocity due to a general motion of a three-dimensional rotating body; and 2.) developing the framework for the effects of the distribution of mass of a three-dimensional rotating body on its motion, defining the principal axes of a body, the inertia tensor, and how to change from one reference coordinate system to another. We now undertake the description of angular momentum, moments and motion of a general three-dimensional rotating body. We approach this very difficult general problem from two points of view. The first is to prescribe the motion in term of given rotations about fixed axes and solve for the force system required to sustain this motion. The second is to study the ”free” motions of a body in a simple force field such as gravitational force acting through the center of mass or ”free” motion such as occurs in a ”zero-g” environment. The typical problems in this second category involve gyroscopes and spinning tops. The second set of problems is by far the more difficult. Before we begin this general approach, we examine a case where kinetic energy can give us considerable insight into the behavior of a rotating body. This example has considerable practical importance and its neglect has been the cause of several system failures. -
Lecture Notes for PHY 405 Classical Mechanics
Lecture Notes for PHY 405 Classical Mechanics From Thorton & Marion's Classical Mechanics Prepared by Dr. Joseph M. Hahn Saint Mary's University Department of Astronomy & Physics November 21, 2004 Problem Set #6 due Thursday December 1 at the start of class late homework will not be accepted text problems 10{8, 10{18, 11{2, 11{7, 11-13, 11{20, 11{31 Final Exam Tuesday December 6 10am-1pm in MM310 (note the room change!) Chapter 11: Dynamics of Rigid Bodies rigid body = a collection of particles whose relative positions are fixed. We will ignore the microscopic thermal vibrations occurring among a `rigid' body's atoms. 1 The inertia tensor Consider a rigid body that is composed of N particles. Give each particle an index α = 1 : : : N. The total mass is M = α mα. This body can be translating as well as rotating. P Place your moving/rotating origin on the body's CoM: Fig. 10-1. 1 the CoM is at R = m r0 M α α α 0 X where r α = R + rα = α's position wrt' fixed origin note that this implies mαrα = 0 α X 0 Particle α has velocity vf,α = dr α=dt relative to the fixed origin, and velocity vr,α = drα=dt in the reference frame that rotates about axis !~ . Then according to Eq. 10.17 (or page 6 of Chap. 10 notes): vf,α = V + vr,α + !~ × rα = α's velocity measured wrt' fixed origin and V = dR=dt = velocity of the moving origin relative to the fixed origin.