Q4. Multiple Correct Two objects of mass m and 4 m are at rest at an infinite separation. They move towards each other under mutual attraction. If G is the universal gravitational constant. Then at separation r . (1) The sum of energy of the two objects is negative. (2) Their relative velocity of approach is in magnitude (3) The sum of kinetic energy of the objects is . (4) The sum of angular momenta of both the objects is zero about any point.

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Published July 22, 2025
Physics
Gravitation
Conservation of Energy & Momentum
Centre of Mass & Relative Motion

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Detailed Explanation

Concepts you need

  1. Gravitational Potential Energy (GPE) between two masses m1m_1 and m2m_2 separated by distance rr is U=Gm1m2rU = -\frac{G m_1 m_2}{r} Here the zero level of potential energy is taken at r=r=\infty.

  2. Conservation of Mechanical Energy Initial Energy=Final Kinetic Energy+Final Potential Energy\text{Initial Energy} = \text{Final Kinetic Energy} + \text{Final Potential Energy}

  3. Conservation of Linear Momentum (because no external force acts on the whole two-mass system). If they start from rest, the centre of mass (CM) stays at rest, hence mv=4mVv=4Vm v = 4m V \qquad \Rightarrow \qquad v = 4V where vv is the speed of the lighter mass and VV is the speed of the heavier one.

  4. Relative Speed of approach is simply the sum of the individual speeds when they head straight toward each other: vrel=v+Vv_{\text{rel}} = v + V

  5. Angular Momentum about any point is zero because

    • their motion is strictly along the line joining them, and
    • the net external torque is zero.

Logical chain to solve

  1. Write momentum relation v=4Vv = 4V from the CM being at rest.
  2. Write energy conservation using the above velocity relation; solve for VV (or vv).
  3. Compute
    • relative speed vrelv_{\text{rel}},
    • total kinetic energy KK,
    • check sign of total mechanical energy E=K+UE = K + U,
    • reason about angular momentum.
  4. Compare each computed/ deduced quantity with the statements (1)–(4).

Simple Explanation (ELI5)

What’s happening here?

Imagine two ice-skaters standing very far apart on a super-slippery lake. One skater is light (mass mm) and the other is heavier (mass 4m4m). At first they are both standing still. Suddenly they feel a magical rope pulling them toward each other (this rope is like gravity).

Because the rope only pulls straight along the line connecting them, they will simply glide toward each other – no turns, no curves.

Key ideas:

  1. Energy can change form but the total stays the same. At the start, there is no kinetic energy (nobody is moving) and the gravitational energy is zero because they are infinitely far apart. As they move closer, gravitational energy becomes negative, and the lost energy turns into their motion energy (kinetic).
  2. Momentum of the pair stays zero. They begin with zero total momentum, so the light skater must move faster than the heavy one to keep the momenta equal and opposite.
  3. Because they glide along one straight line, they never spin about any point – so the system has no angular momentum.

These simple facts let us write easy equations to find their speeds, kinetic energy, and check which of the given statements are right.

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Step-by-Step Solution

Step-by-step calculation

Let

  • Masses: m1=mm_1 = m, m2=4mm_2 = 4m
  • Speeds when separated by distance rr: vv (for mm), VV (for 4m4m)
  • Initial separation: \infty (both at rest)

1. Conservation of Linear Momentum

Total initial momentum is zero, so at any time m v = 4m V \;\; \Longrightarrow \;\; v = 4V \tag{1}


2. Conservation of Mechanical Energy

Initial mechanical energy Ei=0E_i = 0 (no kinetic, zero potential at \infty).

Final energy K=12mv2+12(4m)V2K = \frac12 m v^2 + \frac12 (4m) V^2 U=Gm(4m)r=4Gm2rU = -\frac{G m (4m)}{r} = -\frac{4 G m^2}{r}

Set Ei=EfE_i = E_f: 0=K+U0 = K + U Substitute v=4Vv = 4V into KK: K=12m(4V)2+2mV2=8mV2+2mV2=10mV2K = \frac12 m (4V)^2 + 2 m V^2 = 8 m V^2 + 2 m V^2 = 10 m V^2 So 10 m V^2 - \frac{4 G m^2}{r} = 0 \;\; \Longrightarrow \;\; V^2 = \frac{2 G m}{5 r} \tag{2} From (1): v2=16V2=16(2Gm5r)=32Gm5rv^2 = 16 V^2 = 16\left(\frac{2 G m}{5 r}\right) = \frac{32 G m}{5 r}


3. Relative Speed of Approach

vrel=v+V=4V+V=5Vv_{\text{rel}} = v + V = 4V + V = 5V Square it: vrel2=25V2=25(2Gm5r)=10Gmrv_{\text{rel}}^2 = 25 V^2 = 25\left(\frac{2 G m}{5 r}\right) = \frac{10 G m}{r} Hence vrel=10Gmrv_{\text{rel}} = \sqrt{\frac{10 G m}{r}}


4. Total Kinetic Energy

Using V2V^2 from (2): K=10mV2=10m(2Gm5r)=4Gm2rK = 10 m V^2 = 10 m \left(\frac{2 G m}{5 r}\right) = \frac{4 G m^2}{r}


5. Total Mechanical Energy

E=K+U=4Gm2r4Gm2r=0E = K + U = \frac{4 G m^2}{r} - \frac{4 G m^2}{r} = 0 So the sum of energies is zero, not negative.


6. Angular Momentum

Since both masses move directly along the line joining them, the position and momentum vectors are collinear, giving zero angular momentum about any reference point.


Checking Statements

  1. "Sum of energy is negative" ⟹ False (it is zero).
  2. "Relative velocity magnitude ..." ⟹ True; it equals 10Gmr\sqrt{\frac{10 G m}{r}}.
  3. "Sum of kinetic energy is …" ⟹ True; it is 4Gm2r\frac{4 G m^2}{r}.
  4. "Sum of angular momenta is zero about any point" ⟹ True.

Hence, statements (2), (3), (4) are correct.

Examples

Example 1

Planets orbiting the Sun: while they are not moving directly toward the Sun, the gravitational potential energy constantly converts to and from kinetic energy as they speed up toward perihelion and slow down toward aphelion.

Example 2

Binary star systems where one star is much more massive than the other; the lighter star moves faster to conserve momentum, mirroring the ‘m’ and ‘4m’ masses.

Example 3

Collapsing dust clouds in space: as particles fall inward under gravity, potential energy drops and kinetic energy rises, but the CM stays fixed if no external forces act.

Example 4

Two magnets sliding on an air-track toward each other under attraction; their centre of mass remains stationary and total angular momentum is zero if they move along the track line.

Visual Representation

References

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