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Physics · Ch 6 — System of Particles and Rotational Motion

Angular Velocity and its Relation with Linear Velocity

6.6

Angular Velocity and its Relation with Linear Velocity

Opening the Idea: What is Angular Velocity?

When a rigid body rotates about a fixed axis, different points on the body move with different linear speeds. A point farther from the axis covers a larger circumference in the same time, so its linear speed is greater. Yet, every point on the body sweeps out the same angle in the same time. This common rate of angular displacement is the angular velocity of the body.

Angular velocity is a vector quantity. Its magnitude, denoted by ω\omega (omega), is the rate of change of angular displacement θ\theta:

ω=dθdt\omega = \frac{d\theta}{dt}

The direction of the angular velocity vector is along the axis of rotation, given by the right-hand rule: if you curl the fingers of your right hand in the direction of rotation, your thumb points along the axis in the direction of ω⃗\vec{\omega}.

Important

For a rigid body rotating about a fixed axis, every particle of the body has the same angular velocity ω⃗\vec{\omega}. This is what makes angular velocity a property of the body as a whole, not of individual particles.


Relating Linear Velocity to Angular Velocity

Consider a rigid body rotating about a fixed axis with angular velocity ω⃗\vec{\omega}. Take any particle of the body located at a perpendicular distance rr from the axis. Let its position vector with respect to a point on the axis be r⃗\vec{r}.

As the body rotates, this particle moves in a circle of radius rr (the perpendicular distance from the axis). Its linear velocity v⃗\vec{v} is always tangential to this circle.

The fundamental relation is:

v⃗=ω⃗×r⃗\vec{v} = \vec{\omega} \times \vec{r}

This vector cross product gives both the magnitude and direction of the linear velocity.

Magnitude:

∣v⃗∣=∣ω⃗∣ ∣r⃗∣sin⁡ϕ|\vec{v}| = |\vec{\omega}| \, |\vec{r}| \sin\phi, where ϕ\phi is the angle between ω⃗\vec{\omega} and r⃗\vec{r}. Since ω⃗\vec{\omega} is along the axis and r⃗\vec{r} is perpendicular to the axis (for the component that matters), ϕ=90∘\phi = 90^\circ and sin⁡90∘=1\sin 90^\circ = 1. Therefore:

v=ω rv = \omega \, r

Here rr is the perpendicular distance of the particle from the axis of rotation.

Direction:

The cross product ω⃗×r⃗\vec{\omega} \times \vec{r} gives a vector perpendicular to both ω⃗\vec{\omega} and r⃗\vec{r}. This direction is exactly the tangent to the circular path of the particle, consistent with the right-hand rule.

Watch out

A common mistake is to use the full position vector from an arbitrary origin. The rr in v=ωrv = \omega r is always the perpendicular distance from the axis of rotation, not the distance from some arbitrary point.


Properties of the Relation v⃗=ω⃗×r⃗\vec{v} = \vec{\omega} \times \vec{r}

The textbook lists three important properties that follow from this vector relation. Each is derived below.

›Proof

Property (I): For a particle on the axis of rotation, v=0v = 0.

If a particle lies exactly on the axis of rotation, its perpendicular distance from the axis is r=0r = 0. Substituting into v=ωrv = \omega r gives v=0v = 0. Physically, points on the axis do not move — they are stationary as the body rotates around them. This is why we speak of a "fixed axis."

›Proof

Property (II): For a given ω\omega, vv is proportional to rr. …

Figure 6.16Rotation about a fixed axis. A particle P moves in a circle with centre C on the axis.
Fig. 6.16 — Rotation about a fixed axis. A particle P moves in a circle with centre C on the axis.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your textbook's own diagram.

The figure shows a rigid body rotating about a fixed vertical axis — the zz-axis. The origin OO is placed somewhere on that axis. The yy-axis points to the right, and the xx-axis points down and to the left (a standard right-handed coordinate system). A dashed horizontal circle is drawn with its centre CC on the zz-axis; this circle lies in a plane perpendicular to the axis of rotation.

A particle PP of the rigid body is shown on that circle. The radius of the circle — the perpendicular distance from PP to the axis — is labelled rr. A nearby position P′P' is also marked, separated from PP by a small angular displacement Δθ\Delta \theta. The velocity vector v\mathbf{v} of the particle is drawn tangent to the circle at PP, perpendicular to the radius CPCP.

The physical idea is straightforward: when a rigid body rotates about a fixed axis, every particle moves in a circle whose centre lies on the axis. The particle's linear velocity is not the same for all particles — it depends on how far the particle is from the axis. But every particle shares the same angular velocity ω\boldsymbol{\omega}, which points along the axis of rotation (upward for counterclockwise rotation, by the right-hand rule).

The key relation the textbook develops from this figure is the connection between angular velocity and linear velocity:

v=ω×r\mathbf{v} = \boldsymbol{\omega} \times \mathbf{r}

Here r\mathbf{r} is the position vector of the particle taken from any point on the axis (often from CC or from OO). The magnitude of this cross product gives v=ωrsin⁡ϕv = \omega r \sin\phi, where ϕ\phi is the angle between ω\boldsymbol{\omega} and r\mathbf{r}. Since ω\boldsymbol{\omega} is along the axis and r\mathbf{r} is perpendicular to the axis for a particle on the circle, ϕ=90∘\phi = 90^\circ and sin⁡ϕ=1\sin\phi = 1, so:

v=ωrv = \omega r

The direction of v\mathbf{v} is given by the right-hand rule: curl the fingers of your right hand in the direction of rotation; your thumb points along ω\boldsymbol{\omega}. For a particle, v\mathbf{v} is tangent to the circle, perpendicular to both ω\boldsymbol{\omega} and r\mathbf{r}.

Watch out

A common mistake is to think that r\mathbf{r} in v=ω×r\mathbf{v} = \boldsymbol{\omega} \times \mathbf{r} is the distance from the axis. It is not — it is the full position vector from a point on the axis to the particle. The perpendicular distance r⊥=rsin⁡ϕr_\perp = r\sin\phi is what actually appears in the magnitude formula v=ωr⊥v = \omega r_\perp. For the particle PP in the figure, r⊥=rr_\perp = r because the particle lies in a plane perpendicular to the axis. …

Figure 6.17(a) Right-handed screw rule for ω. (b) The angular velocity ω along the axis; v = ω × r is perpendicular to both, tangent to the circle.
Fig. 6.17 — (a) Right-handed screw rule for ω. (b) The angular velocity ω along the axis; v = ω × r is perpendicular to both, tangent to the circle.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your textbook's own diagram.

The figure has two panels, (a) and (b), and they serve two different but connected purposes.

Panel (a) establishes the direction of angular velocity ω\boldsymbol{\omega}. It shows two shaded disks, each rotating in opposite senses. For each disk, the vector ω\boldsymbol{\omega} is drawn along the axis of rotation. The key idea is the right-handed screw rule: if you curl the fingers of your right hand in the direction of rotation, your thumb points along ω\boldsymbol{\omega}. So one disk rotates clockwise when viewed from above, and its ω\boldsymbol{\omega} points downward; the other rotates anticlockwise, and its ω\boldsymbol{\omega} points upward. The figure makes it clear that ω\boldsymbol{\omega} is not a "spin" that lives on the rim — it is an axial vector that lies along the axis of rotation, with its sense determined by the rotation sense.

Panel (b) moves from the axis to a single point on the rotating body. It shows a zz-axis with ω\boldsymbol{\omega} drawn along it. A point PP is located on the body. The centre CC is the foot of the perpendicular from PP to the axis — so CC lies on the axis, and the line CPCP is perpendicular to the axis. The distance CPCP is labelled r⊥r_\perp (the perpendicular distance from the axis to the point). The vector from the origin OO (some fixed point on the axis) to PP is r\mathbf{r}. A dashed circle is drawn in the plane perpendicular to the axis, centred at CC and passing through PP — this is the circular path that PP follows as the body rotates. Finally, the velocity v\mathbf{v} is shown as a vector tangent to this circle at PP.

The physical idea is that every point in a rigid body rotating with angular velocity ω\boldsymbol{\omega} moves in a circle around the axis. The linear velocity of a point is not simply ωr\omega r; it depends on the perpendicular distance from the axis, not on the distance from the origin.

v=ω×r\mathbf{v} = \boldsymbol{\omega} \times \mathbf{r}

Here ω\boldsymbol{\omega} is the angular velocity vector (direction along the axis, magnitude ω\omega), r\mathbf{r} is the position vector of the point from any origin on the axis, and v\mathbf{v} is the instantaneous linear velocity of that point. The cross product ensures three things: (1) v\mathbf{v} is perpendicular to both ω\boldsymbol{\omega} and r\mathbf{r}; (2) its magnitude is v=ω rsin⁡θv = \omega \, r \sin\theta, where θ\theta is the angle between ω\boldsymbol{\omega} and r\mathbf{r}. But since ω\boldsymbol{\omega} is along the axis and r\mathbf{r} makes an angle θ\theta with it, rsin⁡θr \sin\theta is exactly the perpendicular distance r⊥r_\perp from the axis to the point. So v=ω r⊥v = \omega \, r_\perp, which matches the geometry of the dashed circle in panel (b). (3) The direction of v\mathbf{v} is tangent to the circle, as shown. …