Angle Between Velocity and Acceleration in Central Force Motion
Physics • Mechanics • 2025Non-Uniform Circular Motion under Central Force
Problem Statement
A particle of mass m moves under a central force $F = -\frac{k}{r^2}$. At position $r = R$, it has tangential velocity $v_0$. Find the angle between the velocity and acceleration vectors as a function of $r$.
Given Data
- Mass of particle: m
- Central force: $F = -\frac{k}{r^2}$ (attractive)
- Initial position: $r = R$
- Initial tangential velocity: $v_0$
- No initial radial velocity
Concepts & Approach
We use:
- Central force properties — angular momentum conservation
- Polar coordinates
- Velocity and acceleration components in polar form
- Dot product to find the angle
Step-by-Step Solution
Step 1: Angular Momentum Conservation
For a central force, angular momentum is conserved:
$$L = m r^2 \dfrac{d\theta}{dt}$$ At $r=R$, $v_0$ is purely tangential, so $$\left.\dfrac{d\theta}{dt}\right|_{r=R} = \dfrac{v_0}{R}$$ Thus $L = m R v_0$. Therefore at any $r$:
$m r^2 \dfrac{d\theta}{dt} = m R v_0$, so $\dfrac{d\theta}{dt} = \dfrac{R v_0}{r^2}$.
Step 2: Velocity Components in Polar Coordinates
Velocity:
$\mathbf{v} = \dfrac{dr}{dt}\,\hat{r} + r\dfrac{d\theta}{dt}\,\hat{\theta}$. So $v_r = \dfrac{dr}{dt}$ and $v_\theta = r\dfrac{d\theta}{dt} = \dfrac{R v_0}{r}$.
Step 3: Energy Conservation to Find Radial Velocity
Total energy:
$$E = \dfrac{1}{2} m \left[\left(\dfrac{dr}{dt}\right)^2 + r^2 \left(\dfrac{d\theta}{dt}\right)^2 \right] - \dfrac{k}{r}.$$ At $r=R$, $E = \dfrac{1}{2} m v_0^2 - \dfrac{k}{R}$.
At general $r$, substituting $r^2(d\theta/dt)^2 = (R v_0 / r)^2$:
$$\left(\dfrac{dr}{dt}\right)^2 = v_0^2 - \dfrac{R^2 v_0^2}{r^2} + \dfrac{2k}{m} \left( \dfrac{1}{r} - \dfrac{1}{R} \right).$$
Step 4: Acceleration Components in Polar Coordinates
General polar acceleration:
$\mathbf{a} = \left(\dfrac{d^2 r}{dt^2} - r\left(\dfrac{d\theta}{dt}\right)^2 \right) \hat{r} + \left( 2\dfrac{dr}{dt}\dfrac{d\theta}{dt} + r\dfrac{d^2 \theta}{dt^2} \right) \hat{\theta}$.
For central force motion, $\dfrac{d^2\theta}{dt^2} = 0$. From Newton:
$a_r = -\dfrac{k}{m r^2}$ and $a_\theta = 0$.
Step 5: Angle Between Velocity and Acceleration
The angle $\phi$ satisfies $\cos \phi = \dfrac{\mathbf{v} \cdot \mathbf{a}}{|\mathbf{v}|\,|\mathbf{a}|}$. Since $a_\theta = 0$:
$$\mathbf{v} \cdot \mathbf{a} = v_r a_r = \dfrac{dr}{dt} \left( -\dfrac{k}{m r^2} \right)$$ Magnitudes: $|\mathbf{v}| = \sqrt{ \left( \dfrac{dr}{dt} \right)^2 + \dfrac{R^2 v_0^2}{r^2} }$, $|\mathbf{a}| = \dfrac{k}{m r^2}$. Hence:
$$\cos \phi = - \dfrac{ \dfrac{dr}{dt} }{ \sqrt{ \left( \dfrac{dr}{dt} \right)^2 + \dfrac{R^2 v_0^2}{r^2} } }.$$
Step 6: Express in Terms of $r$ Only
Using the expression for $(dr/dt)^2$ from Step 3:
$$\cos \phi = - \dfrac{ \sqrt{\, v_0^2 \left(1 - \dfrac{R^2}{r^2} \right) + \dfrac{2k}{m} \left( \dfrac{1}{r} - \dfrac{1}{R} \right) \,} }{ \sqrt{\, v_0^2 + \dfrac{2k}{m} \left( \dfrac{1}{r} - \dfrac{1}{R} \right) \,} }.$$
Final Answer
$$\boxed{ \displaystyle \cos \phi = - \frac{ \sqrt{\, v_0^2 \left(1 - \dfrac{R^2}{r^2} \right) + \dfrac{2k}{m} \left( \dfrac{1}{r} - \dfrac{1}{R} \right) \,} }{ \sqrt{\, v_0^2 + \dfrac{2k}{m} \left( \dfrac{1}{r} - \dfrac{1}{R} \right) \,} } }$$
Physical Interpretation
- Negative cosine indicates $\phi > 90^\circ$ — acceleration has a component opposing velocity due to the attractive central force.
- Energy dependence: the expression depends on kinetic and potential energy terms.
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Special cases:
- At $r = R$, $dr/dt = 0$, so $\phi = 90^\circ$.
- As $r \to \infty$, the angle approaches a constant depending on energy/escape conditions.
- For circular orbits, the angle remains $90^\circ$.
- Dynamic behavior: $\phi$ changes as the particle moves radially.
Tags: #Physics #CentralForce #OrbitalMechanics #PolarCoordinates #NewtonianMechanics #ClassicalDynamics