How long until the planets collide?

In summary: The problem involves finding the time it takes for these planets to collide, with the given information. The attempt at a solution includes drawing a free-body diagram, considering the position of the center of mass and the conservation of momentum. However, setting up the problem with a series of differential equations is proving to be challenging. Advice is requested.
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jgens
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Homework Statement



Two planets of masses [itex]m_1[/itex] and [itex]m_2[/itex] with radii [itex]r_1[/itex] and [itex]r_2[/itex] respectively are orbiting their common center of mass at some initial distance [itex]x_0[/itex] from each other with angular velocity [itex]\omega_0[/itex]. Find the amount of time it takes for these planets to collide.

Homework Equations



N/A

The Attempt at a Solution



So far, I've drawn my free-body diagram with the axes in the Center of Mass reference frame, figured that the position of the center of mass remains constant since no net external force acts, and that conservation of momentum applies since no net external torque acts either. However, I'm having difficulty setting the problem up (constructing a series of differential equations to solve) and would appreciate any advice.

Thanks!
 
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jgens said:
Find the amount of time it takes for these planets to collide.
Thanks!
Hello jgens
In the way you put it it is a potential equation. For colliding you need something diffusive. Rotational energy diminishing because of friction or any other diffusion. For instance if a speaker moves particles a comoving for some time, that is called sound. Since this comovement diffuses the sound deminishes and the particles are moving statistically erradic again.
greetings Janm
 

Related to How long until the planets collide?

What is orbital motion?

Orbital motion refers to the movement of an object around another object in space due to the force of gravity. This can be seen in the orbits of planets around the sun, moons around planets, and satellites around Earth.

What is the difference between a circular and elliptical orbit?

A circular orbit is when the object moves in a perfect circle around another object, while an elliptical orbit is when the object moves in an oval-shaped path around another object. In an elliptical orbit, the object is closer to the central object at one point in its orbit and farther away at another point.

How is orbital motion affected by the mass of objects?

The mass of objects affects orbital motion by determining the strength of the gravitational force between them. The larger the mass of the central object, the stronger the force of gravity and the faster the orbital speed of the other object needs to be to maintain its orbit.

What is Kepler's first law of planetary motion?

Kepler's first law states that all planets move in elliptical orbits with the sun at one focus. This means that the distance between a planet and the sun will vary throughout its orbit, with the closest point being the perihelion and the farthest point being the aphelion.

How do scientists calculate the orbital period of objects?

The orbital period of an object can be calculated using Kepler's third law, which states that the square of the orbital period is proportional to the cube of the semi-major axis of the orbit. This means that the further an object is from the central object, the longer its orbital period will be.

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