What Is the Relative Velocity of Two Colliding Planets?

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SUMMARY

The discussion focuses on calculating the relative velocity of two colliding hypothetical planets with masses of 2.5 × 1023 kg and 7.8 × 1023 kg, and radii of 3.2 × 106 m and 7.1 × 106 m, respectively. Using the gravitational constant G = 6.67259 × 10−11 Nm2/kg2, the relative velocity at a center-to-center separation of 4.5 × 108 m is calculated to be 475.54 m/s. The discussion emphasizes the importance of considering the center of mass frame to ensure zero net momentum, which affects the velocities of the planets.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation
  • Familiarity with kinetic and potential energy equations
  • Knowledge of center of mass calculations
  • Basic algebra for solving equations
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  • Study the concept of gravitational forces using Newton's law of gravitation
  • Learn about the conservation of momentum in collision scenarios
  • Explore the center of mass frame and its applications in physics
  • Investigate the relationship between kinetic energy and gravitational potential energy
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Students and educators in physics, astrophysicists, and anyone interested in celestial mechanics and gravitational interactions between massive bodies.

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Homework Statement



Given: G = 6.67259 × 10^−11 Nm2/kg2
Two hypothetical planets of masses 2.5 × 10^23 kg and 7.8×10^23 kg and radii 3.2×10^6 m
and 7.1×10^6 m, respectively, are at rest when
they are an infinite distance apart. Because
of their gravitational attraction, they head
toward each other on a collision course.

When their center-to-center separation is
4.5 × 10^8 m, find their relative velocity. An-
swer in units of m/s.

Homework Equations


The Attempt at a Solution



F=GMm/r^2
M=7.8e23 kg
m=2.5e23 kg
Ki+Ui=Kf+Uf
r=4.5e8+3.2e6 +7.1e6=460300000m
0+0=.5mv^2+(-GMm/r)
.5v^2=GM/r
v=475.54 m/sIs this answer correct?
 
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I just tried to take the velocity from above and added the following:
v=at
475.54=at
F=ma
F=GMm/r^2
a=F/m
475.54/a=t

then I took the t value and tried to solve the velocity for the M mass. Then I found the difference between the two velocities. However, this is not right...any help is greatly appreciated!
 
In the frame where the origin is the center of mass of the two planets (which is where you should be working), the two planets don't move with equal velocity. They have to have 0 net momentum as well. m*v=M*V.
 

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