To solve the problem of two particles with masses 20 kg and 10 kg moving towards each other under the influence of gravitational forces, we can use the principles of conservation of energy and Newton's law of universal gravitation. Let's break it down step by step.
Understanding the Forces at Play
According to Newton's law of universal gravitation, the gravitational force \( F \) between two masses \( m_1 \) and \( m_2 \) separated by a distance \( r \) is given by:
F = G \frac{m_1 m_2}{r^2}
where \( G \) is the gravitational constant, approximately \( 6.674 \times 10^{-11} \, \text{N m}^2/\text{kg}^2 \).
Initial and Final Conditions
Initially, the two particles are 1.0 m apart. We want to find their speeds when they are 0.5 m apart. The gravitational potential energy (U) at a distance \( r \) is given by:
U = -G \frac{m_1 m_2}{r}
Calculating Initial Potential Energy
At the initial separation of 1.0 m:
- Mass \( m_1 = 20 \, \text{kg} \)
- Mass \( m_2 = 10 \, \text{kg} \)
- Distance \( r = 1.0 \, \text{m} \)
The initial potential energy \( U_i \) is:
U_i = -G \frac{20 \times 10}{1} = -200G
Calculating Final Potential Energy
At the final separation of 0.5 m:
The final potential energy \( U_f \) is:
U_f = -G \frac{20 \times 10}{0.5} = -400G
Energy Conservation Principle
The total mechanical energy in the system is conserved. Thus, the change in potential energy will equal the change in kinetic energy:
U_i - U_f = K_f - K_i
Initially, both particles are at rest, so \( K_i = 0 \). Therefore:
-200G + 400G = K_f
This simplifies to:
K_f = 200G
Finding Kinetic Energy
The kinetic energy \( K \) of a particle is given by:
K = \frac{1}{2}mv^2
Let \( v_1 \) be the speed of the 20 kg mass and \( v_2 \) be the speed of the 10 kg mass. The total kinetic energy is:
K_f = \frac{1}{2} m_1 v_1^2 + \frac{1}{2} m_2 v_2^2
Substituting the values:
200G = \frac{1}{2} (20)v_1^2 + \frac{1}{2} (10)v_2^2
This simplifies to:
200G = 10v_1^2 + 5v_2^2
Using Conservation of Momentum
Since no external forces are acting on the system, the momentum is conserved. The initial momentum is zero, so:
m_1 v_1 + m_2 v_2 = 0
Substituting the masses gives:
20v_1 + 10v_2 = 0
From this, we can express \( v_2 \) in terms of \( v_1 \):
v_2 = -2v_1
Substituting Back into Kinetic Energy Equation
Now, substitute \( v_2 \) into the kinetic energy equation:
200G = 10v_1^2 + 5(-2v_1)^2
This expands to:
200G = 10v_1^2 + 20v_1^2
Combining terms gives:
200G = 30v_1^2
Solving for \( v_1^2 \) yields:
v_1^2 = \frac{200G}{30} = \frac{20G}{3}
Thus, the speed of the 20 kg mass is:
v_1 = \sqrt{\frac{20G}{3}}
Finding the Speed of the Second Particle
Now, substituting back to find \( v_2 \):
v_2 = -2\sqrt{\frac{20G}{3}} = -\frac{4\sqrt{20G}}{\sqrt{3}}
Final Speeds
In summary, the speeds of the particles when the separation decreases to 0.5 m are:
- Speed of the 20 kg particle: v_1 = \sqrt{\frac{20G}{3}} \, \text{m/s}
- Speed of the 10 kg particle: v_2 = -\frac{4\sqrt{20G}}{\sqrt{3}} \, \text{m/s}
These equations give you the speeds of both particles as they move towards each other due to