Calculating Relative Acceleration and Velocity with Newton's Law of Gravity

In summary, two particles with masses m and M attract each other according to Newton's law of gravity. They start at rest at an infinite distance apart, with their centre of mass staying steady during the motion. Using conservation of momentum and energy, it can be shown that their relative velocity of approach is v(rel) = square root(2G(M+m)/a), where a is the distance between the particles and G is the universal gravitational constant. By solving equations for v and V, the relative speed v_{rel} can be determined.
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starbaj12
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Two particles having masses of m and M respectively, attract each other according to Newton's law of gravity. Initially they are at rest at an infinite distance apart. Find their relative acceleration and show that their relative velocity of approach is

v(rel) = square root(2G(M+m)/a)

I do not even know where to start on this problem, if any could give me help that would be great.

Thank you
 
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Momentum and energy are conserved!
 
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starbaj12 said:
Two particles having masses of m and M respectively, attract each other according to Newton's law of gravity. Initially they are at rest at an infinite distance apart. Find their relative acceleration and show that their relative velocity of approach is

v(rel) = square root(2G(M+m)/a)

I do not even know where to start on this problem, if any could give me help that would be great.

Thank you

The particles are initially at rest so their angular momentum is zero, they will move towards each other along the straight line connecting them.
As there are no external forces acting on this system of particles, their centre of mass stays steady during the motion. You can place the origin of the frame of reference there. That is

[tex]mv+MV=0\mbox{ } \rightarrow \mbox{ }V=-\frac{M}{m}v[/tex]

The energy of the system is conserved, and it is zero, as the particles started from rest at infinite distance apart.
At distance 'a' the mutual potential energy is

[tex]U_{pot}= - G\frac{mM}{a^2}[/tex].

[tex] \frac{1}{2}mv^2+\frac{1}{2}MV^2-G\frac{mM}{a^2}=0[/tex]

You have two equations for v and V. Solve, and determine their relative speed [tex]v_{rel}=|v-V|[/tex].

ehild
 
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FAQ: Calculating Relative Acceleration and Velocity with Newton's Law of Gravity

What is Newton's Law of Gravity?

Newton's Law of Gravity is a fundamental law of physics that describes the gravitational force between two objects. It states that the force of attraction between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

How do you calculate relative acceleration with Newton's Law of Gravity?

To calculate relative acceleration using Newton's Law of Gravity, you will need to know the masses of the two objects and the distance between them. Then, you can use the formula a = (G * m1 * m2) / r^2, where G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between them.

How do you calculate relative velocity with Newton's Law of Gravity?

To calculate relative velocity using Newton's Law of Gravity, you will need to know the masses of the two objects, the distance between them, and the initial velocities of the objects. Then, you can use the formula v = √(2 * G * (m1 + m2) / r), where G is the gravitational constant, m1 and m2 are the masses of the objects, and r is the distance between them.

What is the gravitational constant?

The gravitational constant, denoted by G, is a fundamental constant in physics that is used to calculate the gravitational force between two objects. It has a value of approximately 6.67 x 10^-11 N * m^2 / kg^2.

What are the units of measurement for relative acceleration and velocity?

The units of measurement for relative acceleration are meters per second squared (m/s^2) or gravitational units (g). The units for relative velocity are meters per second (m/s) or kilometers per hour (km/h).

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