Comet Orbit Around the Sun: Calculating Speed

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A comet follows an elliptical orbit around the Sun, with its closest approach at 4.5 x 10^10 m and a speed of 8.9 x 10^4 m/s. To calculate its speed at a distance of 6 x 10^12 m, the conservation of mechanical energy principle is applied, where the total energy remains constant. Gravitational potential energy can be calculated without knowing the comet's mass by using a variable "m." By setting the initial total energy equal to the final total energy, the speed at the specified distance can be determined. Understanding these principles is essential for solving the problem effectively.
jamagner
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A comet is in an elliptical orbit around the Sun. Its closest approach to the Sun is a distance of 4.5 1010 m (inside the orbit of Mercury), at which point its speed is 8.9 104 m/s. Its farthest distance from the Sun is far beyond the orbit of Pluto. What is its speed when it is 6 1012 m from the Sun? (This is the approximate distance of Pluto from the Sun.)

i have no clue how to find the speed given only the distances and the other speed
 
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Hint: What's conserved?
 
see that's what i don't know...my guess would be kinetic energy is conserved but i don't really know...i suck at physics i never know what's going on
 
Mechanical energy (kinetic energy + gravitational potential energy) is conserved.
 
so how do i use this in an equation can i set it up as a proportion
 
Initial total energy = final total energy. You'll need to know how to calculate gravitational PE.
 
What if you don't know the mass of the comet, because don't you need this to use the gravitational PE?
 
sriceb01 said:
What if you don't know the mass of the comet, because don't you need this to use the gravitational PE?
You don't need the actual mass. Just call it "m" and see what happens.
 

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