Understanding the Orbit of Kapler's Law and its Relation to Potential Energy

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So the energy will be infinity and e will be infinity... please help me...It is difficult to give a concrete answer without the necessary context, but in general terms, if the energy and eccentricity are both infinity, it means the orbit is unbounded and the particles will move infinitely far away from each other.AND ONE MORE THING: if the potential is a/r^2 (>0) then then the two objects will attract each other, right? But in the Gravitational law (-Gm1m2/r^2) the potential is <0 and the objects will attract to each otherThis appears to be a contradiction, but it is likely that the potential in the problem is meant to be negative, as in the
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Cosmossos
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Hello,
In question 3(b) in the following file
http://phstudy.technion.ac.il/~wn114101/hw/wn2010_hw09.pdf

Why the orbit will be a straight line?
I think that when the particles are coming to r=0 the potential will be infinity, isn't that so?
So the energy will be infinity and e will be infinity... please help me...
thank you

AND ONE MORE THING: if the potential is a/r^2 (>0) then then the two objects will attract each other, right? But in the Gravitational law (-Gm1m2/r^2) the potential is <0 and the objects will attract to each other
 
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Cosmossos said:
Hello,
In question 3(b) in the following file
http://phstudy.technion.ac.il/~wn114101/hw/wn2010_hw09.pdf

Why the orbit will be a straight line?
The problem statement explicitly states the particles move "on the x direction" and "on the y direction". Presumably they mean on the x and y axes; it is not worded quite properly but I can't imagine it meaning anything else.

So, each particle moves in straight line simply because the problem statement says that they do. What would actually cause this to happen is not important.

I think that when the particles are coming to r=0 the potential will be infinity, isn't that so?
No, it would be negative infinity in this example.
 
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Related to Understanding the Orbit of Kapler's Law and its Relation to Potential Energy

What are Kapler's orbits?

Kapler's orbits, also known as Kepler's laws of planetary motion, are a set of three laws that describe the motion of planets around the sun.

What is the first law of Kapler's orbits?

The first law states that all planets move in elliptical orbits with the sun at one focus. This means that the distance between the planet and the sun changes throughout its orbit.

What is the second law of Kapler's orbits?

The second law, also known as the law of equal areas, states that a line connecting a planet to the sun will sweep out equal areas in equal amounts of time. This means that planets move faster when they are closer to the sun and slower when they are farther away.

What is the third law of Kapler's orbits?

The third law, also known as the harmonic law, states that the square of a planet's orbital period is proportional to the cube of its average distance from the sun. This means that the farther a planet is from the sun, the longer its orbital period will be.

Why are Kapler's orbits important?

Kapler's orbits are important because they provide a mathematical model for understanding the motion of planets in our solar system. They also helped to disprove the previous belief that planets move in perfect circles, and paved the way for future scientific discoveries and theories.

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