Speed of a comet around the sun.

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SUMMARY

The discussion focuses on calculating the speed of a comet in an elliptical orbit around the Sun, specifically at a distance of 6e12 m, which approximates Pluto's distance. The comet's closest approach to the Sun is 4.5e10 m with a speed of 9.6e4 m/s. To determine the speed at a greater distance, the conservation of energy principle is applied, allowing for the calculation without needing the comet's mass. The analogy of a ball thrown into the air is used to illustrate the concept of energy conservation in orbital mechanics.

PREREQUISITES
  • Understanding of elliptical orbits in celestial mechanics
  • Familiarity with the conservation of energy principle
  • Basic knowledge of kinetic and potential energy equations
  • Ability to apply mathematical reasoning to physics problems
NEXT STEPS
  • Study the conservation of mechanical energy in orbital dynamics
  • Learn about Kepler's laws of planetary motion
  • Explore the equations of motion for elliptical orbits
  • Investigate the relationship between distance and speed in gravitational fields
USEFUL FOR

Students studying physics, particularly those focusing on celestial mechanics, as well as educators and anyone interested in understanding the dynamics of comets and their orbits around the Sun.

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Homework Statement



A comet is in an elliptical orbit around the Sun. Its closest approach to the Sun is a distance of 4.5e10 m (inside the orbit of Mercury), at which point its speed is 9.6e4 m/s. Its farthest distance from the Sun is far beyond the orbit of Pluto. What is its speed when it is 6e12 m from the Sun? (This is the approximate distance of Pluto from the Sun.)


Homework Equations





The Attempt at a Solution



I don't know where to start with this. All I'm told is its speed at the "bottom" of its orbit, and then I'm told to calculate its speed at the "top" of it orbit. I am not given the mass of the comet so I can't find it's Potential or Kinetic Energy which is what this section is over. To my knowledge there is no direct relationship between distance in an orbit and a bodies speed. Perhaps I'm overlooking something brutally obvious.
 
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you need to use potential energy. because you know its speed at a certain distance, mass becomes a common factor and you no longer need it. So you have the speed at a certain distance, and you need to find its speed at a further distance.

analogy:

a ball of mass m is thrown into the air and has an instantaneous speed right before it hits the ground of 35 metres per second. What is its speed when it is a distance of 15 metres from the ground.

You can use energy to find this answer, and it is exactly the same concept. good luck
 

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