All Exams Test series for 1 year @ ₹349 only
Question

Mass of uniform circular ring is M and its radius is R. Find the maximum intensity of gravitation field on the axis of the ring

The correct answer is \(\frac{2}{{3\sqrt 3 }}\frac{{GM}}{{{R^2}}}\)

Understanding Gravitational Field on the Ring Axis

The question asks for the maximum gravitational field intensity on the axis of a uniform circular ring. A uniform circular ring of mass M and radius R creates a gravitational field at points along its axis. The field varies depending on the distance from the center of the ring.

Gravitational Field Formula on the Axis

For a uniform circular ring of mass M and radius R, the gravitational field intensity \(E(x)\) at a point on its axis at a distance \(x\) from the center is given by the formula:

$$ E(x) = \frac{GMx}{(R^2 + x^2)^{3/2}} $$

Here:

  • \(G\) is the gravitational constant.
  • \(M\) is the total mass of the ring.
  • \(R\) is the radius of the ring.
  • \(x\) is the distance of the point from the center of the ring along the axis.

We need to find the value of \(x\) for which \(E(x)\) is maximum and then calculate this maximum value.

Finding the Maximum Gravitational Field Intensity

To find the maximum value of \(E(x)\), we need to differentiate the function \(E(x)\) with respect to \(x\) and set the derivative equal to zero. This process helps us find the critical points where the function reaches its maximum or minimum value.

The formula is \(E(x) = GMx (R^2 + x^2)^{-3/2}\).

Let's differentiate \(E(x)\) with respect to \(x\) using the product rule \((uv)' = u'v + uv'\):

Let \(u = GMx\) and \(v = (R^2 + x^2)^{-3/2}\).

$$ \frac{dE}{dx} = \frac{d}{dx} \left( GMx (R^2 + x^2)^{-3/2} \right) $$

$$ \frac{dE}{dx} = GM \left[ \frac{d}{dx}(x) \cdot (R^2 + x^2)^{-3/2} + x \cdot \frac{d}{dx}(R^2 + x^2)^{-3/2} \right] $$

$$ \frac{dE}{dx} = GM \left[ 1 \cdot (R^2 + x^2)^{-3/2} + x \cdot \left(-\frac{3}{2}\right) (R^2 + x^2)^{-3/2 - 1} \cdot \frac{d}{dx}(R^2 + x^2) \right] $$

$$ \frac{dE}{dx} = GM \left[ (R^2 + x^2)^{-3/2} - \frac{3}{2}x (R^2 + x^2)^{-5/2} \cdot (2x) \right] $$

$$ \frac{dE}{dx} = GM \left[ (R^2 + x^2)^{-3/2} - 3x^2 (R^2 + x^2)^{-5/2} \right] $$

Factor out \((R^2 + x^2)^{-5/2}\):

$$ \frac{dE}{dx} = GM (R^2 + x^2)^{-5/2} \left[ (R^2 + x^2)^{(-3/2) - (-5/2)} - 3x^2 \right] $$

$$ \frac{dE}{dx} = GM (R^2 + x^2)^{-5/2} \left[ (R^2 + x^2)^{1} - 3x^2 \right] $$

$$ \frac{dE}{dx} = GM (R^2 + x^2)^{-5/2} (R^2 + x^2 - 3x^2) $$

$$ \frac{dE}{dx} = GM (R^2 + x^2)^{-5/2} (R^2 - 2x^2) $$

Set the derivative to zero to find the value of \(x\) for maximum intensity:

$$ GM (R^2 + x^2)^{-5/2} (R^2 - 2x^2) = 0 $$

Since \(GM\) and \((R^2 + x^2)^{-5/2}\) are non-zero for any \(x\) along the axis (except potentially at infinity, which isn't where the max occurs), the term causing the derivative to be zero must be \((R^2 - 2x^2)\).

$$ R^2 - 2x^2 = 0 $$

$$ 2x^2 = R^2 $$

$$ x^2 = \frac{R^2}{2} $$

$$ x = \pm \frac{R}{\sqrt{2}} $$

Since \(x\) represents a distance along the axis from the center, we consider the magnitude \(x = \frac{R}{\sqrt{2}}\). The maximum gravitational field intensity occurs at a distance of \(R/\sqrt{2}\) on either side of the center along the axis.

Calculating the Maximum Intensity Value

Now, substitute \(x = \frac{R}{\sqrt{2}}\) back into the formula for \(E(x)\):

$$ E_{max} = E\left(x = \frac{R}{\sqrt{2}}\right) = \frac{GM \left(\frac{R}{\sqrt{2}}\right)}{\left(R^2 + \left(\frac{R}{\sqrt{2}}\right)^2\right)^{3/2}} $$

$$ E_{max} = \frac{\frac{GMR}{\sqrt{2}}}{\left(R^2 + \frac{R^2}{2}\right)^{3/2}} $$

$$ E_{max} = \frac{\frac{GMR}{\sqrt{2}}}{\left(\frac{3R^2}{2}\right)^{3/2}} $$

$$ E_{max} = \frac{\frac{GMR}{\sqrt{2}}}{\left(\frac{3}{2}\right)^{3/2} (R^2)^{3/2}} $$

$$ E_{max} = \frac{\frac{GMR}{\sqrt{2}}}{\left(\frac{3\sqrt{3}}{2\sqrt{2}}\right) R^3} $$

$$ E_{max} = \frac{GMR}{\sqrt{2}} \cdot \frac{2\sqrt{2}}{3\sqrt{3} R^3} $$

Cancel out terms:

$$ E_{max} = \frac{2GM}{3\sqrt{3} R^2} $$

This is the maximum gravitational field intensity on the axis of the uniform circular ring.

Comparing with Options

Let's compare our calculated maximum intensity with the given options:

Calculated Value Option 1 Option 2 Option 3 Option 4
\(\frac{2GM}{3\sqrt{3} R^2}\) \(\frac{2}{3\sqrt 3}\frac{GM}{R^2}\) \(\frac{GM}{R^2}\) \(\frac{2GM}{R^2}\) \(\frac{3}{2\sqrt 2}\frac{GM}{R^2}\)

Our calculated value matches Option 1.

Revision Table: Gravitational Field Concepts

Concept Formula Description
Gravitational Field at center of ring (x=0) \(E(0) = 0\) Due to symmetry, field contributions from opposite points on the ring cancel out.
Gravitational Field far from ring (\(x >> R\)) \(E(x) \approx \frac{GM}{x^2}\) Behaves like a point mass at large distances.
Distance of maximum intensity \(x = \frac{R}{\sqrt{2}}\) Found by setting \(\frac{dE}{dx} = 0\).
Maximum Gravitational Intensity \(E_{max} = \frac{2GM}{3\sqrt{3} R^2}\) Value of E(x) at \(x = R/\sqrt{2}\).

Additional Information: Gravitational Potential

Besides the gravitational field, another important concept is the gravitational potential. The gravitational potential \(V(x)\) on the axis of a uniform circular ring at a distance \(x\) from the center is given by:

$$ V(x) = -\frac{GM}{\sqrt{R^2 + x^2}} $$

The gravitational field is related to the negative gradient of the potential:

$$ E(x) = -\frac{dV}{dx} $$

Let's verify this for the ring:

$$ V(x) = -GM (R^2 + x^2)^{-1/2} $$

$$ -\frac{dV}{dx} = - \frac{d}{dx} \left( -GM (R^2 + x^2)^{-1/2} \right) $$

$$ -\frac{dV}{dx} = GM \frac{d}{dx} (R^2 + x^2)^{-1/2} $$

$$ -\frac{dV}{dx} = GM \left( -\frac{1}{2} (R^2 + x^2)^{-3/2} \cdot 2x \right) $$

$$ -\frac{dV}{dx} = GM \left( -x (R^2 + x^2)^{-3/2} \right) $$

$$ -\frac{dV}{dx} = -\frac{GMx}{(R^2 + x^2)^{3/2}} $$

Wait, there's a sign difference. Gravitational field is generally defined as pointing towards the mass. On the positive x-axis, the field is in the positive x direction for positive x, so the field is \(\vec{E}(x) = E(x) \hat{i}\) where \(E(x)\) is the magnitude. The relation is \(\vec{E} = -\nabla V\). In 1D along the axis, this is \(E_x = -\frac{dV}{dx}\). Let's recheck the derivative:

$$ \frac{dV}{dx} = -GM \left( -\frac{1}{2} \right) (R^2 + x^2)^{-3/2} (2x) = GMx (R^2 + x^2)^{-3/2} $$

So, \(E_x = -\frac{dV}{dx} = -GMx (R^2 + x^2)^{-3/2}\). The magnitude is \(|E_x| = \frac{GM|x|}{(R^2 + x^2)^{3/2}}\). For \(x > 0\), the magnitude is \(\frac{GMx}{(R^2 + x^2)^{3/2}}\), which matches our field formula used for the maximum intensity calculation.

The gravitational potential is minimum where the field is maximum or minimum magnitude (excluding points at infinity). The potential is related to the work done by gravity.

Was this answer helpful?

Important Questions from Gravitational potential energy

  1. Statement I: A body weighs less on a hill top than on earth's surface even though its mass remains unchanged.

    Statement II: The acceleration due to gravity of the earth decreases with height.
  2. The work done to raise a mass $m$ from the surface of the Earth to a height $h$, which is equal to twice the radius of the Earth $R$, is:
  3. Mass of the earth is M and its radius is R. An object of mass m is placed on the surface of earth. Find the work done in lifting the object through a height \(\frac{R}{2}\) above the surface of earth.

  4. A solid sphere of constant density p has mass M and radius R. What is the gravitational potential difference between a point P which is at distance \(\frac{R}{2}\) from the central and its surface?

    (i.e. Vp - Vsurface)

  5. Which term is used for celestial bodies that revolve around the sun in highly elliptical orbit ?

Need Expert Advice?

Start Your Preparation with Prepp Mobile App

Download the app from Google Play & App Store
Download the app from Google Play & App Store
Prepp Mobile App