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In analytical mechanics, **generalized coordinates** are a set of parameters used to represent the state of a system in a configuration space. These parameters must uniquely define the configuration of the system relative to a reference state.^{[1]} The **generalized velocities** are the time derivatives of the generalized coordinates of the system. The adjective "generalized" distinguishes these parameters from the traditional use of the term "coordinate" to refer to Cartesian coordinates.

An example of a generalized coordinate would be to describe the position of a pendulum using the angle of the pendulum relative to vertical, rather than by the x and y position of the pendulum.

Although there may be many possible choices for generalized coordinates for a physical system, they are generally selected to simplify calculations, such as the solution of the equations of motion for the system. If the coordinates are independent of one another, the number of independent generalized coordinates is defined by the number of degrees of freedom of the system.^{[2]}^{[3]}

Generalized coordinates are paired with generalized momenta to provide canonical coordinates on phase space.

Generalized coordinates are usually selected to provide the minimum number of independent coordinates that define the configuration of a system, which simplifies the formulation of Lagrange's equations of motion. However, it can also occur that a useful set of generalized coordinates may be *dependent*, which means that they are related by one or more constraint equations.

For a system of N particles in 3D real coordinate space, the position vector of each particle can be written as a 3-tuple in Cartesian coordinates:

Any of the position vectors can be denoted **r**_{k} where *k* = 1, 2, …, *N* labels the particles. A *holonomic constraint* is a *constraint equation* of the form for particle k^{[4]}^{[a]}

which connects all the 3 spatial coordinates of that particle together, so they are not independent. The constraint may change with time, so time t will appear explicitly in the constraint equations. At any instant of time, any one coordinate will be determined from the other coordinates, e.g. if x_{k} and z_{k} are given, then so is y_{k}. One constraint equation counts as *one* constraint. If there are C constraints, each has an equation, so there will be C constraint equations. There is not necessarily one constraint equation for each particle, and if there are no constraints on the system then there are no constraint equations.

So far, the configuration of the system is defined by 3*N* quantities, but C coordinates can be eliminated, one coordinate from each constraint equation. The number of independent coordinates is *n* = 3*N* − *C*. (In D dimensions, the original configuration would need ND coordinates, and the reduction by constraints means *n* = *ND* − *C*). It is ideal to use the minimum number of coordinates needed to define the configuration of the entire system, while taking advantage of the constraints on the system. These quantities are known as **generalized coordinates** in this context, denoted *q _{j}*(

which is a point in the *configuration space* of the system. They are all independent of one other, and each is a function of time. Geometrically they can be lengths along straight lines, or arc lengths along curves, or angles; not necessarily Cartesian coordinates or other standard orthogonal coordinates. There is one for each degree of freedom, so the number of generalized coordinates equals the number of degrees of freedom, n. A degree of freedom corresponds to one quantity that changes the configuration of the system, for example the angle of a pendulum, or the arc length traversed by a bead along a wire.

If it is possible to find from the constraints as many independent variables as there are degrees of freedom, these can be used as generalized coordinates.^{[5]} The position vector **r**_{k} of particle k is a function of all the n generalized coordinates (and, through them, of time),^{[6]}^{[7]}^{[8]}^{[5]}^{[nb 1]}

and the generalized coordinates can be thought of as parameters associated with the constraint.

The corresponding time derivatives of **q** are the generalized velocities,

(each dot over a quantity indicates one time derivative). The velocity vector **v**_{k} is the total derivative of **r**_{k} with respect to time

and so generally depends on the generalized velocities and coordinates. Since we are free to specify the initial values of the generalized coordinates and velocities separately, the generalized coordinates q_{j} and velocities *dq _{j}*/

A mechanical system can involve constraints on both the generalized coordinates and their derivatives. Constraints of this type are known as non-holonomic. First-order non-holonomic constraints have the form

An example of such a constraint is a rolling wheel or knife-edge that constrains the direction of the velocity vector. Non-holonomic constraints can also involve next-order derivatives such as generalized accelerations.

The total kinetic energy of the system is the energy of the system's motion, defined as^{[9]}

in which · is the dot product. The kinetic energy is a function only of the velocities **v**_{k}, not the coordinates **r**_{k} themselves. By contrast an important observation is^{[10]}

which illustrates the kinetic energy is in general a function of the generalized velocities, coordinates, and time if the constraints also vary with time, so *T* = *T*(**q**, *d***q**/*dt*, *t*).

In the case the constraints on the particles are time-independent, then all partial derivatives with respect to time are zero, and the kinetic energy is a homogeneous function of degree 2 in the generalized velocities.

Still for the time-independent case, this expression is equivalent to taking the line element squared of the trajectory for particle k,

and dividing by the square differential in time, *dt*^{2}, to obtain the velocity squared of particle k. Thus for time-independent constraints it is sufficient to know the line element to quickly obtain the kinetic energy of particles and hence the Lagrangian.^{[11]}

It is instructive to see the various cases of polar coordinates in 2D and 3D, owing to their frequent appearance. In 2D polar coordinates (*r*, *θ*),

in 3D cylindrical coordinates (*r*, *θ*, *z*),

in 3D spherical coordinates (*r*, *θ*, *φ*),

The *generalized momentum* "canonically conjugate to" the coordinate q_{i} is defined by

If the Lagrangian L does *not* depend on some coordinate q_{i}, then it follows from the Euler–Lagrange equations that the corresponding generalized momentum will be a conserved quantity, because the time derivative is zero implying the momentum is a constant of the motion;

For a bead sliding on a frictionless wire subject only to gravity in 2d space, the constraint on the bead can be stated in the form *f* (**r**) = 0, where the position of the bead can be written **r** = (*x*(*s*), *y*(*s*)), in which s is a parameter, the arc length s along the curve from some point on the wire. This is a suitable choice of generalized coordinate for the system. Only *one* coordinate is needed instead of two, because the position of the bead can be parameterized by one number, s, and the constraint equation connects the two coordinates x and y; either one is determined from the other. The constraint force is the reaction force the wire exerts on the bead to keep it on the wire, and the non-constraint applied force is gravity acting on the bead.

Suppose the wire changes its shape with time, by flexing. Then the constraint equation and position of the particle are respectively

which now both depend on time t due to the changing coordinates as the wire changes its shape. Notice time appears implicitly via the coordinates *and* explicitly in the constraint equations.

The relationship between the use of generalized coordinates and Cartesian coordinates to characterize the movement of a mechanical system can be illustrated by considering the constrained dynamics of a simple pendulum.^{[12]}^{[13]}

A simple pendulum consists of a mass M hanging from a pivot point so that it is constrained to move on a circle of radius L. The position of the mass is defined by the coordinate vector **r** = (*x*, *y*) measured in the plane of the circle such that y is in the vertical direction. The coordinates x and y are related by the equation of the circle

that constrains the movement of M. This equation also provides a constraint on the velocity components,

Now introduce the parameter θ, that defines the angular position of M from the vertical direction. It can be used to define the coordinates x and y, such that

The use of θ to define the configuration of this system avoids the constraint provided by the equation of the circle.

Notice that the force of gravity acting on the mass m is formulated in the usual Cartesian coordinates,

where g is the acceleration due to gravity.

The virtual work of gravity on the mass m as it follows the trajectory **r** is given by

The variation δ**r** can be computed in terms of the coordinates x and y, or in terms of the parameter θ,

Thus, the virtual work is given by

Notice that the coefficient of δ*y* is the y-component of the applied force. In the same way, the coefficient of δ*θ* is known as the generalized force along generalized coordinate θ, given by

To complete the analysis consider the kinetic energy T of the mass, using the velocity,

so,

D'Alembert's form of the principle of virtual work for the pendulum in terms of the coordinates x and y are given by,

This yields the three equations

in the three unknowns, x, y and λ.

Using the parameter θ, those equations take the form

which becomes,

or

This formulation yields one equation because there is a single parameter and no constraint equation.

This shows that the parameter θ is a generalized coordinate that can be used in the same way as the Cartesian coordinates x and y to analyze the pendulum.

The benefits of generalized coordinates become apparent with the analysis of a double pendulum.
For the two masses *m _{i}* (

and

The formulation of Lagrange's equations for this system yields six equations in the four Cartesian coordinates *x _{i}*,

Now introduce the generalized coordinates *θ _{i}* (

The force of gravity acting on the masses is given by,

where g is the acceleration due to gravity. Therefore, the virtual work of gravity on the two masses as they follow the trajectories **r**_{i} (*i* = 1, 2) is given by

The variations δ**r**_{i} (*i* = 1, 2) can be computed to be

Thus, the virtual work is given by

and the generalized forces are

Compute the kinetic energy of this system to be

Euler–Lagrange equation yield two equations in the unknown generalized coordinates *θ _{i}* (

and

The use of the generalized coordinates *θ _{i}* (

For a 3D example, a spherical pendulum with constant length l free to swing in any angular direction subject to gravity, the constraint on the pendulum bob can be stated in the form

where the position of the pendulum bob can be written

in which (*θ*, *φ*) are the spherical polar angles because the bob moves in the surface of a sphere. The position **r** is measured along the suspension point to the bob, here treated as a point particle. A logical choice of generalized coordinates to describe the motion are the angles (*θ*, *φ*). Only two coordinates are needed instead of three, because the position of the bob can be parameterized by two numbers, and the constraint equation connects the three coordinates (*x*, *y*, *z*) so any one of them is determined from the other two.

The *principle of virtual work* states that if a system is in static equilibrium, the virtual work of the applied forces is zero for all virtual movements of the system from this state, that is, δ*W* = 0 for any variation δ**r**.^{[15]} When formulated in terms of generalized coordinates, this is equivalent to the requirement that the generalized forces for any virtual displacement are zero, that is *F*_{i} = 0.

Let the forces on the system be **F**_{j} (*j* = 1, 2, …, *m*) be applied to points with Cartesian coordinates **r**_{j} (*j* = 1, 2, …, *m*), then the virtual work generated by a virtual displacement from the equilibrium position is given by

where δ**r**_{j} (*j* = 1, 2, …, *m*) denote the virtual displacements of each point in the body.

Now assume that each δ**r**_{j} depends on the generalized coordinates *q _{i}* (

and

The n terms

are the generalized forces acting on the system. Kane^{[16]} shows that these generalized forces can also be formulated in terms of the ratio of time derivatives,

where **v**_{j} is the velocity of the point of application of the force **F**_{j}.

In order for the virtual work to be zero for an arbitrary virtual displacement, each of the generalized forces must be zero, that is

Wikiquote has quotations related to **Generalized coordinates**.

**^**Some authors e.g. Hand & Finch take the form of the position vector for particle k, as shown here, as the condition for the constraint on that particle to be holonomic.

**^**Some authors set the constraint equations to a constant for convenience with some constraint equations (e.g. pendulums), others set it to zero. It makes no difference because the constant can be subtracted to give zero on one side of the equation. Also, in Lagrange's equations of the first kind, only the derivatives are needed.

**^**Ginsberg 2008, p. 397, §7.2.1 Selection of generalized coordinates**^**Farid M. L. Amirouche (2006). "§2.4: Generalized coordinates".*Fundamentals of multibody dynamics: theory and applications*. Springer. p. 46. ISBN 0-8176-4236-6.**^**Florian Scheck (2010). "§5.1 Manifolds of generalized coordinates".*Mechanics: From Newton's Laws to Deterministic Chaos*(5th ed.). Springer. p. 286. ISBN 978-3-642-05369-6.**^**Goldstein, Poole & Safko 2002, p. 12- ^
^{a}^{b}Kibble & Berkshire 2004, p. 232 **^**Torby 1984, p. 260**^**Goldstein, Poole & Safko 2002, p. 13**^**Hand & Finch 1998, p. 15**^**Torby 1984, p. 269**^**Goldstein, Poole & Safko 2002, p. 25**^**Landau & Lifshitz 1976, p. 8**^**Greenwood, Donald T. (1987).*Principles of Dynamics*(2nd ed.). Prentice Hall. ISBN 0-13-709981-9.**^**Richard Fitzpatrick, Newtonian Dynamics.**^**Eric W. Weisstein, Double Pendulum, scienceworld.wolfram.com. 2007**^**Torby 1984**^**T. R. Kane and D. A. Levinson, Dynamics: theory and applications, McGraw-Hill, New York, 1985

- Ginsberg, Jerry H. (2008).
*Engineering dynamics*(3rd ed.). Cambridge UK: Cambridge University Press. ISBN 978-0-521-88303-0. - Goldstein, Herbert; Poole, Charles; Safko, John (2002).
*Classical Mechanics*(3rd ed.). San Francisco, CA: Addison Wesley. ISBN 0-201-65702-3. - Hand, Louis N.; Finch, Janet D. (1998).
*Analytical mechanics*. Cambridge: Cambridge University Press. ISBN 978-0521575720. - Kibble, T.W.B; Berkshire, F.H. (2004).
*Classical Mechanics*(5th ed.). River Edge NJ: Imperial College Press. ISBN 1860944248. - Landau, L. D.; Lifshitz, E.M. (1976).
*Mechanics*(Third ed.). Oxford. ISBN 978-0750628969.`{{cite book}}`

: CS1 maint: location missing publisher (link) - Torby, Bruce (1984). "Energy Methods".
*Advanced Dynamics for Engineers*. HRW Series in Mechanical Engineering. United States of America: CBS College Publishing. ISBN 0-03-063366-4.