Kinematics

From Wikipedia, the free encyclopedia

Kinematics (Greek κινειν,kinein, to move) is a branch of dynamics which describes the motion of objects without consideration of the circumstances leading to the motion. In contrast, kinetics is concerned with the forces and interactions that produce or affect the motion.^[1]^[2]^[3]^[4]

It is natural to begin this discussion by considering the various possible types of motion in themselves, leaving out of account for a time the causes to which the initiation of motion may be ascribed; this preliminary enquiry constitutes the science of Kinematics.

– Whittaker, E. T. (1988). A treatise on the analytical dynamics of particles and rigid bodies: with an introduction to the problem of three bodies. Chapter 1, p. 1.

The simplest application of kinematics is to point particle motion (translational kinematics or linear kinematics). The description of rotation (rotational kinematics or angular kinematics) is more complicated. The state of a generic rigid body may be described by combining both translational and rotational kinematics (rigid-body kinematics). A more complicated case is the kinematics of a system of rigid bodies, possibly linked together by mechanical joints. The kinematic description of fluid flow is even more complicated, and not generally thought of in the context of kinematics.

[edit] Translational motion

Translational or curvilinear kinematics^[5]^[6] is the description of the motion in space of a point along a trajectory. This path can be linear, or curved as seen with projectile motion. There are three basic concepts that are required for understanding translational motion:

Displacement (denoted by r below )is the shortest distance between two points: the origin and the displaced point. The origin is (0,0) on a coordinate system that is defined by the observer. Because displacement has both magnitude (length) and direction, it is a vector whose initial point is the origin and terminal point is the displaced point.

Velocity (denoted by υ below) is the rate of change in displacement with respect to time; that is the displacement of a point changes with time. Velocity is also a vector. For a constant velocity, every unit of time adds the length of the velocity vector (in the same direction) to the displacement of the moving point. Instantaneous velocity (the velocity at an instant of time) is defined as

$\boldsymbol v = \frac {d \boldsymbol r}{d t} \ ,$

where dr is an infinitesimally small displacement and dt is an infinitesimally small length of time. Because dr is necessarily the distance between two infinitesimally spaced points along the trajectory of the point, it is the same as an increment in arc length along the path of the point, customarily denoted ds. Average velocity (velocity over a length of time) is defined as $\boldsymbol v = \frac {\Delta \boldsymbol s}{\Delta t}$ , where Δs is the change in displacement and Δt is the interval of time over which displacement changes.

Acceleration (denoted by a below) is the rate of change in velocity with respect to time. Acceleration is also a vector. As with velocity if acceleration is constant, for every unit of time the length of the acceleration vector (in the same direction) is added to the velocity. If the change in velocity (a vector) is known, the acceleration is parallel to it. Instantaneous acceleration (the acceleration at an instant of time) is defined as:

$\boldsymbol a = \frac {d \boldsymbol v}{d t} \ ,$

where d υ is an infinitesimally small change in velocity and dt is an infinitesimally small length of time. Average acceleration (acceleration over a length of time) is defined as:

$\boldsymbol a = \frac {\Delta \boldsymbol v}{\Delta t} \ ,$

where Δ υ is the change in velocity and Δt is the interval of time over which velocity changes.

[edit] Integral relations

The above definitions can be inverted by integration to find:

$\boldsymbol{v}(t) =\boldsymbol{v}_0+\ \int_0^t \ dt' \ \boldsymbol{a} (t')$

$\boldsymbol{r}(t) =\boldsymbol{r}_0+\ \int_0^t \ dt' \ \boldsymbol{v} (t')$

$=\boldsymbol{r}_0+\boldsymbol{v}_0\ t +\ \int_0^t \ dt' \int_0^{t'} \ dt'' \ \boldsymbol{a} (t'')$

$=\boldsymbol{r}_0+\boldsymbol{v}_0\ t +\ \int_0^t \ dt' \left(t-t'\right) \ \boldsymbol{a} (t') \ ,$

where the double integration is reduced to one integration by interchanging the order of integration, and subscript 0 signifies evaluation at t = 0 (initial values).

[edit] Constant acceleration

When acceleration is constant both in direction and in magnitude, the point is said to be undergoing uniformly accelerated motion. In this case, the above equations can be simplified:

Eq. (1): $\boldsymbol v = \int_0^{t} \boldsymbol a dt = \boldsymbol{ v}_0 + \boldsymbol a t$

Those who are familiar with calculus may recognize this as an initial value problem. Because acceleration ( a ) is a constant, integrating it with respect to time (t) gives a change in velocity. Adding this to the initial velocity ( υ₀) gives the final velocity ( υ ).

Eq. (2): $\boldsymbol r = \int_0^t \boldsymbol v dt = \int_0^t \left( \boldsymbol v_0 + \boldsymbol a t \right) dt = \boldsymbol v_0 t + \frac{1}{2} \boldsymbol a t^2$

Using the above formula, we can substitute for υ to arrive at this equation, where r is displacement.

Eq. (3): $\boldsymbol r = \frac{\boldsymbol v+ \boldsymbol v_0}{2} t$

By using the definition of an average, this equation states that average velocity times time equals displacement. Using Eq. (1) to find υ−υ₀ and multiplying by Eq. (3) we find a connection between the final velocity at time t and the displacement at that time:

$\boldsymbol {r \cdot a} t = \left( \boldsymbol v - \boldsymbol {v}_0 \right)\boldsymbol{ \cdot} \frac{\boldsymbol v + \boldsymbol {v}_0}{2} t \ ,$

where the "•" denotes a vector dot product. Dividing the t on both sides and carrying out the dot-products:

Eq. (4): $2 \boldsymbol{r \cdot a} = v^2 - v_0^2 \ .$

For the case where r is parallel to a resulting in a straight-line motion, the vector r has magnitude equal to the path length s at time t, and this equation becomes:

$v^2= v_0^2 + 2 a s\ ,$

which can be a useful result when time is not known explicitly.

[edit] Relative velocity

Main article: Relative velocity

To describe the motion of object A with respect to object B, when we know how each is moving with respect to a reference object O, we can use vector algebra. Choose an origin for reference, and let the positions of objects A, B, and O be denoted by r_A, r_B, and r_O. Then the position of A relative to the reference object O is

$\boldsymbol{r}_{A/O} = \boldsymbol{r}_{B} - \boldsymbol{r}_{O} \,\!$

Consequently, the position of A relative to B is

$\boldsymbol{r}_{A/B} = \boldsymbol{r}_A - \boldsymbol{r}_B = \boldsymbol{r}_A - \boldsymbol{r}_O - \left(\boldsymbol{r}_B-\boldsymbol{r}_O\right) = \boldsymbol{r}_{A/O}-\boldsymbol{r}_{B/O} \ .$

The above relative equation states that the motion of A relative to B is equal to the motion of A relative to O minus the motion of B relative to O. It may be easier to visualize this result if the terms are re-arranged:

$\boldsymbol{r}_{A/O} = \boldsymbol{r}_{A/B} + \boldsymbol{r}_{B/O} \ ,$

or, in words, the motion of A relative to the reference is that of B plus the relative motion of A with respect to B. These relation between displacements become relations between velocities by simple time-differentiation, and a second differentiation makes them apply to accelerations.

For example, let Ann move with velocity $\boldsymbol{V}_{A}$ relative to the reference (we drop the O subscript for convenience) and let Bob move with velocity $\boldsymbol{V}_{B}$ , each velocity given with respect to the ground (point O). To find how fast Ann is moving relative to Bob (we call this velocity $\boldsymbol{V}_{A/B}$ ), the equation above gives:

$\boldsymbol{V}_{A} = \boldsymbol{V}_{B} + \boldsymbol{V}_{A/B} \,\! .$

To find $\boldsymbol{V}_{A/B}$ we simply rearrange this equation to obtain:

$\boldsymbol{V}_{A/B} = \boldsymbol{V}_{A} -\boldsymbol{V}_{B} \,\! .$

At velocities comparable to the speed of light, these equations are not valid. They are replaced by equations derived from Einstein's theory of special relativity.

Example: Rectilinear (1D) motion

Figure A: An object is fired upwards, reaches its apex, and then begins its descent under a constant acceleration.

Consider an object that is fired directly upwards and falls back to the ground so that its trajectory is contained in a straight line. If we adopt the convention that the upward direction is the positive direction, the object experiences a constant acceleration of approximately -9.81 m/s². Therefore, its motion can be modeled with the equations governing uniformly accelerated motion.

For the sake of example, assume the object has an initial velocity of +50 m/s. There are several interesting kinematic questions we can ask about the particle's motion:

[edit] How long will it be airborne?

To answer this question, we apply the formula

$x_f - x_i = v_i t + \frac{1}{2} at^2.$

Since the question asks for the length of time between the object leaving the ground and hitting the ground on its fall, the displacement is zero.

$0 = v_i t + \frac{1}{2} at^2 = t(v_i + \frac{1}{2} at)$

We find two solutions for it. The trivial solution says the time is zero; this is actually also true, it is the first moment the displacement is zero: just when it starts motion. However, the solution of interest is

$t = -\frac{2v_i}{a} = -\frac{2*50}{-9.81} = 10.2 \ s$

[edit] What altitude will it reach before it begins to fall?

In this case, we use the fact that the object has a velocity of zero at the apex of its trajectory. Therefore, the applicable equation is:

$v_f^2 = v_i^2 + 2 a (x_f - x_i)$

If the origin of our coordinate system is at the ground, then $x i$ is zero. Then we solve for $x f$ and substitute known values:

$x_f = \frac{v_f^2 - v_i^2}{2 a} + x_i = \frac{0-50^2}{2*-9.81}+0 = 127.55 \ m$

[edit] What will its final velocity be when it reaches the ground?

To answer this question, we use the fact that the object has an initial velocity of zero at the apex before it begins its descent. We can use the same equation we used for the last question, using the value of 127.55 m for $x i$ .

$v_f = \sqrt{v_i^2 + 2 a (x_f - x_i)} = \sqrt{0^2 + 2 (-9.81) (0 - 127.55)} = 50\ m/s$

Assuming this experiment were performed in a vacuum (negating drag effects), we find that the final and initial speeds are equal, a result which agrees with conservation of energy.

Example: Projectile (2D) motion

Figure B: An object fired at an angle

θ

from the ground follows a parabolic trajectory.

Suppose that an object is not fired vertically but is fired at an angle $θ$ from the ground. The object will then follow a parabolic trajectory, and its horizontal motion can be modeled independently of its vertical motion. Assume that the object is fired at an initial velocity of 50 m/s and 30 degrees from the horizontal.

[edit] How far will it travel before hitting the ground?

The object experiences an acceleration of -9.81 ms^-2 in the vertical direction and no acceleration in the horizontal direction. Therefore, the horizontal displacement is

$\Delta x = x_f - x_i = v_i \cos \theta \ t + \frac{1}{2} at^2 = v_i \cos \theta \ t$

In order to solve this equation, we must find t. This can be done by analyzing the motion in the vertical direction. If we impose that the vertical displacement is zero, we can use the same procedure we did for rectilinear motion to find t.

$0 = v_i \sin \theta \ t + \frac{1}{2} at^2 = t(v_i \sin \theta + \frac{1}{2} at)$

We now solve for t and substitute this expression into the original expression for horizontal displacement. (Note the use of the trigonometric identity $2sinθcosθ = sin2θ$ )

$\Delta x = v_i \cos \theta \left(\frac{-2 v_i \sin \theta}{a}\right) = -\frac{v_i^2 \sin 2\theta}{a} = 220.93 \ m$

[edit] Rotational motion

Main article: Circular motion

Figure 1: The angular velocity vector Ω points up for counterclockwise rotation and down for clockwise rotation, as specified by the right-hand rule. Angular position θ(t) changes with time at a rate ω(t) = dθ / dt.

Rotational kinematics is the description of the rotation of an object.^[7] The description of rotation requires some method for describing orientation, for example, the Euler angles. In what follows attention is restricted to simple rotation about an axis of fixed orientation for convenience chosen as the z-axis..

Description of rotation then involves these three quantities:

Angular position: The oriented distance from a selected origin on the rotational axis to a point of an object is a vector r ( t ) locating the point. The vector r ( t ) has some projection (or, equivalently, some component) r ( t ) on a plane perpendicular to the axis of rotation. Then the angular position of that point is the angle θ from a reference axis (typically the positive x-axis) to the vector r ( t ) in a known rotation sense (typically given by the right-hand rule).

Angular velocity: The angular velocity ω is the rate at which the angular position θ changes with respect to time t:

$\mathbf{\omega} = \frac {\mathrm{d}\theta}{\mathrm{d}t}$

The angular velocity is represented in Figure 1 by a vector Ω pointing along the axis of rotation with magnitude ω and sense determined by the direction of rotation as given by the right-hand rule.

Angular acceleration: The magnitude of the angular acceleration $α$ is the rate at which the angular velocity $ω$ changes with respect to time t:

$\mathbf{\alpha} = \frac {\mathrm{d}\mathbf{\omega}}{\mathrm{d}t}$

The equations of translational kinematics can easily be extended to planar rotational kinematics with simple variable exchanges:

$\,\!\theta_f - \theta_i = \omega_i t + \frac{1}{2} \alpha t^2 \qquad \theta_f - \theta_i = \frac{1}{2} (\omega_f + \omega_i)t$

$\,\!\omega_f = \omega_i + \alpha t \qquad \alpha = \frac{\omega_f - \omega_i}{t} \qquad \omega_f^2 = \omega_i^2 + 2 \alpha (\theta_f - \theta_i)\ .$

Here $\,\!\theta_i$ and $\,\!\theta_f$ are, respectively, the initial and final angular positions, $\,\!\omega_i$ and $\,\!\omega_f$ are, respectively, the initial and final angular velocities, and $\,\!\alpha$ is the constant angular acceleration. Although position in space and velocity in space are both true vectors (in terms of their properties under rotation), as is angular velocity, angle itself is not a true vector.

[edit] Point object in circular motion

See also: Rigid body and Orientation

Figure 2: Velocity and acceleration for nonuniform circular motion: the velocity vector is tangential to the orbit, but the acceleration vector is not radially inward because of its tangential component a_θ that increases the rate of rotation: dω / dt = | a_θ | / R.

This example deals with a "point" object, by which is meant that complications due to rotation of the body itself about its own center of mass are ignored.

Displacement. An object in circular motion is located at a position r ( t ) given by:

$\boldsymbol{r} (t) = R \mathbf{u}_R (t) \ ,$

where u_R is a unit vector pointing outward from the axis of rotation toward the periphery of the circle of motion, located at a radius R from the axis.

Linear velocity. The velocity of the object is then

$\boldsymbol{v} (t) =\frac{d}{dt} \boldsymbol{r} (t) = R \frac{d}{dt}\mathbf{u}_R (t) \ .$

The magnitude of the unit vector u_R (by definition) is fixed, so its time dependence is entirely due to its rotation with the radius to the object, that is,

$\frac{d}{dt}\mathbf{u}_R (t) = \boldsymbol{\Omega} \mathbf{\times u}_R = \omega (t) \mathbf{ u}_{\theta} \ ,$

where u_θ is a unit vector perpendicular to u_R pointing in the direction of rotation, ω ( t ) is the (possibly time varying) angular rate of rotation, and the symbol × denotes the vector cross product. The velocity is then:

$\boldsymbol{v} (t) = R\omega (t) \mathbf{ u}_{\theta} \ .$

The velocity therefore is tangential to the circular orbit of the object, pointing in the direction of rotation, and increasing in time if ω increases in time.

Linear acceleration. In the same manner, the acceleration of the object is defined as:

$\boldsymbol{a} (t) = \frac{d}{dt} \boldsymbol{v} (t) = R\frac{d}{dt}\omega\mathbf{ u}_{\theta} \$

$=\mathbf{ u}_{\theta} R\frac{d}{dt}\omega + R\omega\frac{d}{dt}\mathbf{ u}_{\theta}$

$=\mathbf{ u}_{\theta} R\frac{d}{dt}\omega + R\omega \boldsymbol{\Omega}\mathbf{ \times u}_{\theta}$

$=\mathbf{ u}_{\theta} R\frac{d}{dt}\omega - \mathbf{ u}_{R}\omega^2R\$

$=\mathbf{a}_{\theta} + \mathbf{a}_R \ ,$

which shows a leading term a_θ in the acceleration tangential to the orbit related to the angular acceleration of the object (supposing ω to vary in time) and a second term a_R directed inward from the object toward the center of rotation, called the centripetal acceleration.

[edit] Coordinate systems

See also: Generalized coordinates, Curvilinear coordinates, Orthogonal coordinates, and Frenet-Serret formulas

In any given situation, the most useful coordinates may be determined by constraints on the motion, or by the geometrical nature of the force causing or affecting the motion. Thus, to describe the motion of a bead constrained to move along a circular hoop, the most useful coordinate may be its angle on the hoop. Similarly, to describe the motion of a particle acted upon by a central force, the most useful coordinates may be polar coordinates.

[edit] Fixed rectangular coordinates

In this coordinate system, vectors are expressed as an addition of vectors in the x, y, and z direction from a non-rotating origin. Usually i, j, k are unit vectors in the x-, y-, and z-directions.

The position vector, r (or s), the velocity vector, v, and the acceleration vector, a are expressed using rectangular coordinates in the following way:

$\boldsymbol{ r} = x\ \hat {\mathbf{ i}} + y \ \hat {\mathbf{ j}} + z \ \hat {\mathbf{ k}} \, \!$

$\boldsymbol{ v} = \dot {\boldsymbol{ r}} = \dot {x} \ \hat {\mathbf{ i}} + \dot {y} \ \hat {\mathbf{ j}} + \dot {z} \ \hat {\mathbf{ k}} \, \!$

$\boldsymbol{ a} = \ddot {\boldsymbol{ r}} = \ddot {x} \ \hat {\mathbf{ i}} + \ddot {y} \ \hat {\mathbf{ j}} + \ddot {z} \ \hat {\mathbf{ k}} \, \!$

Note: $\dot {x} = \frac{\mathrm{d}x}{\mathrm{d}t}$ , $\ddot {x} = \frac{\mathrm{d}^2x}{\mathrm{d}t^2}$

[edit] Two dimensional rotating reference frame

See also: Centripetal force

This coordinate system expresses only planar motion. It is based on three orthogonal unit vectors: the vector i, and the vector j which form a basis for the plane in which the objects we are considering reside, and k about which rotation occurs. Unlike rectangular coordinates, which are measured relative to an origin that is fixed and non-rotating, the origin of these coordinates can rotate and translate - often following a particle on a body that is being studied.

[edit] Derivatives of unit vectors

The position, velocity, and acceleration vectors of a given point can be expressed using these coordinate systems, but we have to be a bit more careful than we do with fixed frames of reference. Since the frame of reference is rotating, the unit vectors also rotate, and this rotation must be taken into account when taking the derivative of any of these vectors. If the coordinate frame is rotating at angular rate ω in the counterclockwise direction (that is, Ω = ω k using the right hand rule) then the derivatives of the unit vectors are as follows:

$\dot{\hat {\mathbf{ i}}} = \omega \hat {\mathbf{ k}} \times \hat {\mathbf{ i}} = \omega\hat {\mathbf{ j}}$

$\dot{\hat {\mathbf{ j}}} = \omega \hat {\mathbf{ k}}\times \hat {\mathbf{ j}} = - \omega \hat {\mathbf{ i}}$

[edit] Position, velocity, and acceleration

Given these identities, we can now figure out how to represent the position, velocity, and acceleration vectors of a particle using this reference frame.

[edit] Position

Position is straightforward:

$\boldsymbol{ r} = x \ \hat {\mathbf{ i}} + y \ \hat {\mathbf{ j}}$

It is just the distance from the origin in the direction of each of the unit vectors.

[edit] Velocity

Velocity is the time derivative of position:

$\boldsymbol{ v} = \frac{\mathrm{d}\boldsymbol{ v}}{\mathrm{d}t} = \frac{\mathrm{d} (x \ \hat {\mathbf{ i}})}{\mathrm{d}t} + \frac{\mathrm{d} (y \ \hat {\mathbf{ j}})}{\mathrm{d}t}$

By the product rule, this is:

$\boldsymbol{ v} = \dot x \ \hat {\mathbf{ i}} + x \dot{\ \hat {\mathbf{ i}}} + \dot y \ \hat {\mathbf{ j}} + y \dot{ \ \hat {\mathbf{ j}}}$

Which from the identities above we know to be:

$\boldsymbol{ v} = \dot x \ \hat {\mathbf{ i}} + x \omega \ \hat {\mathbf{ j}} + \dot y \ \hat {\mathbf{ j}} - y \omega \ \hat {\mathbf{ i}} = (\dot x - y \omega) \ \hat {\mathbf{ i}} + (\dot y + x \omega) \ \hat {\mathbf{ j}}$

or equivalently

$\boldsymbol{ v}= (\dot x \ \hat {\mathbf{ i}} + \dot y \ \hat {\mathbf{ j}}) + (y \dot{ \hat {\mathbf{ j}}} + x \dot{\hat {\mathbf{ i}}}) = \boldsymbol{ v}_{rel} + \boldsymbol{\Omega} \times \boldsymbol{r}$

where v_rel is the velocity of the particle relative to the rotating coordinate system.

[edit] Acceleration

Acceleration is the time derivative of velocity.

We know that:

$\boldsymbol{ a} = \frac{\mathrm{d}}{\mathrm{d}t} \boldsymbol{ v} = \frac{\mathrm{d} \boldsymbol{ v}_{rel}}{\mathrm{d}t} + \frac{\mathrm{d}}{\mathrm{d}t} \boldsymbol{\Omega} \times \boldsymbol{r}$

Consider the $\stackrel{\frac{ \mathrm{d} } { \mathrm{d} t }}{}$ $\boldsymbol{ v}_{rel}$ part. $\boldsymbol{ v}_{rel}$ has two parts we want to find the derivative of: the relative change in velocity ( $\boldsymbol{ a}_{rel}$ ), and the change in the coordinate frame ( $\boldsymbol{\Omega} \times \boldsymbol{ v}_{rel}$ ).

$\frac{\mathrm{d} \boldsymbol{ v}_{rel}}{\mathrm{d}t} = \boldsymbol{ a}_{rel} + \boldsymbol{\Omega} \times \boldsymbol{ v}_{rel}$

Next, consider $\stackrel{\frac{\mathrm{d}}{\mathrm{d}t}}{}$ $(\boldsymbol{\Omega} \times\boldsymbol{ r})$ . Using the chain rule:

$\frac{\mathrm{d} (\boldsymbol{\Omega} \times \boldsymbol{ r})}{\mathrm{d}t} = \dot{\boldsymbol{\Omega}} \times \boldsymbol{ r} + \boldsymbol{\Omega} \times \dot{\boldsymbol{ r}}$

$\dot{\boldsymbol{ r}}=\boldsymbol{ v}=\boldsymbol{ v}_{rel} + \boldsymbol{\Omega} \times \boldsymbol{ r}$ from above:

$\frac{\mathrm{d} (\boldsymbol{\Omega} \times \boldsymbol{ r})}{\mathrm{d}t} = \dot{\boldsymbol{\Omega}} \times \boldsymbol{ r} + \boldsymbol{\Omega} \times (\boldsymbol{\Omega} \times\boldsymbol{ r}) + \boldsymbol{\Omega} \times \boldsymbol{ v}_{rel}$

So all together:

$\boldsymbol{ a} = \boldsymbol{ a}_{rel} + \boldsymbol{\Omega} \times \boldsymbol{ v}_{rel} + \dot{\boldsymbol{\Omega}} \times \boldsymbol{ r} + \boldsymbol{\Omega} \times (\boldsymbol{\Omega} \times \boldsymbol{ r}) + \boldsymbol{\Omega} \times \boldsymbol{ v}_{rel}$

And collecting terms:^[8]

$\boldsymbol{ a} = \boldsymbol{ a}_{rel} + 2(\boldsymbol{\Omega} \times \boldsymbol{ v}_{rel}) + \dot{\boldsymbol{\Omega}} \times \boldsymbol{ r} + \boldsymbol{\Omega} \times (\boldsymbol{\Omega} \times \boldsymbol{ r})\ .$

[edit] Three dimensional rotating coordinate frame

(to be written)

[edit] Kinematic constraints

Please help improve this section by expanding it.
Further information might be found on the talk page or at requests for expansion.

A kinematic constraint is any condition relating properties of a dynamic system that must hold true at all times. Below are some common examples:

[edit] Rolling without slipping

An object that rolls against a surface without slipping obeys the condition that the velocity of its center of mass is equal to the cross product of its angular velocity with a vector from the point of contact to the center of mass,

$\boldsymbol{ v}_G(t) = \boldsymbol{\Omega} \times \boldsymbol{ r}_{G/O}$ .

For the case of an object that does not tip or turn, this reduces to v = R ω.

[edit] Inextensible cord

This is the case where bodies are connected by some cord that remains in tension and cannot change length. The constraint is that the sum of all components of the cord, however they are defined, is the total length, and the time derivative of this sum is zero.

[edit] References and notes

^ Joseph Stiles Beggs (1983). Kinematics. Taylor & Francis, p. 1. ISBN 0891163557.
^ O. Bottema & B. Roth (1990). Theoretical Kinematics. Dover Publications. ISBN 0486663469.
^ Thomas Wallace Wright (1896). Elements of Mechanics Including Kinematics, Kinetics and Statics. E and FN Spon, Chapter 1.
^ Edmund Taylor Whittaker & William McCrea (1988). A Treatise on the Analytical Dynamics of Particles and Rigid Bodies. Cambridge University Press, Chapter 1. ISBN 0521358833.
^ James R. Ogden & Max Fogiel (1980). The Mechanics Problem Solver. Research and Education Association, p. 184. ISBN 0878915192.
^ R. Douglas Gregory (2006). Classical Mechanics: An Undergraduate Text. Cambridge UK: Cambridge University Press, Chapter 2. ISBN 0521826780.
^ R. Douglas Gregory (2006). Chapter 16. ISBN 0521826780.
^ R. Douglas Gregory (2006). pp. 475-476. ISBN 0521826780.

[edit] See also

Look up kinematics in
Wiktionary, the free dictionary.

[edit] External links

Java applet of 1D kinematics
Flash animated tutorial for 1D kinematics
Physclips: Mechanics with animations and video clips from the University of New South Wales
KINEMATICS FOR HIGH SCHOOL AND IIT JEE LEVEL
KMODDL: Kinematic Models for Design Digital Library, Cornell University Library

Kinematics
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Categories: Classical mechanics | Kinematics