A comet revolves around the sun

In summary, a comet revolves around the sun in a closed elliptical trajectory. The angle between the position vector (sun in the origin) and the velocity vector of the comet at its perihelion and aphelion is 90º. This solution was obtained by assuming dr(t)/dt = 0, which does not imply v(t) = 0.
  • #1
Calabi_Yau
35
1

Homework Statement



A comet revolves around the sun in a closed elliptical trajectory. Ignore any force acting upon it besides gravity. Prove that the angle between the position vector (sun in the origin) and the velocity vector of the comet at its perihelion and aphelion is 90º.

The Attempt at a Solution



I tried to approach this problem by writing down the motion equations for a body on an elliptical orbit under the action of gravity. But it is a second order differential equation, that I later found out has no analytic solution.

So I just thought: when the comet is nearest and furthest from the sun, position r(t) must have a maximum/minimum, hence dr(t)/dt = 0, at those points. That also works for the r(t)^2, so dr(t)^2/dt = 0 <=> r(t)[itex]\cdot[/itex]v(t) = 0 and this happens (since none of them is zero) only when they are both perpendicular.

However, by assuming dr(t)/dt = 0, I'm assuming that v(t) = 0 for some time t. But as we know that is never true, has the comet never stops moving. Is my solution valid? If so, why? If not, could you give me an hint? Does this all come down to the geomtry of the elipse ( because I never studied the equations that describe ellipses)?
 
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  • #2
I think you're getting mixed up between scalars and vectors. If ##\vec r(t)## is the position vector, what is its magnitude? What do you get when that is at an extreme value?
 
  • #3
After a few unsuccessful efforts to try to prove it by means of pure geometry, I learned a very useful theorem about ellipses, that the tangent of a point bissects the exterior angle. I just had to prove that. Then I found the answer where I least expected. I learned about Fermat's principle of least time, and with a little bit of thinking I had my proof.

I was really pleased with that, because those are the kind of answers I'm the most attracted to in physics.
 
  • #4
Glad you got there, but it's not clear to me whether you now understand what you did wrong here:
Calabi_Yau said:
when the comet is nearest and furthest from the sun, position r(t) must have a maximum/minimum, hence dr(t)/dt = 0, at those points. That also works for the r(t)^2, so dr(t)^2/dt = 0 <=> r(t)[itex]\cdot[/itex]v(t) = 0 and this happens (since none of them is zero) only when they are both perpendicular.

However, by assuming dr(t)/dt = 0, I'm assuming that v(t) = 0 for some time t
The first paragraph works if what you mean is:
when the comet is nearest and furthest from the sun, position ##r(t) = |\vec r(t)|## must have a maximum/minimum, hence dr(t)/dt = 0, at those points. That also works for the ##r(t)^2 = \vec r \cdot \vec r##, so dr(t)^2/dt = 0 <=> ##\vec r(t) \cdot \dot {\vec r}(t) = 0## and this happens (since none of them is zero) only when they are perpendicular.​
But what are you saying in the second paragraph? dr(t)/dt = 0 does not imply ##\vec v(t) = 0 ## nor ##|\vec v(t)| = 0 ##. ##\frac {d\vec r(t)}{dt} = 0## would imply that, but that's not what you assumed.
 
  • #5
Right, I see. I assumed [itex]\frac{dr.r}{dt}[/itex] = 0 does not imply dr(t)/dt = 0.

(Sorry for not writing with the proper symbols, but I am not very used to using those features)
 
  • #6
Calabi_Yau said:
Right, I see. I assumed [itex]\frac{dr.r}{dt}[/itex] = 0 does not imply dr(t)/dt = 0.

(Sorry for not writing with the proper symbols, but I am not very used to using those features)
If you don't want to be bothered with LaTex for vectors, you can just put the vector variables in bold.
 

1. How does a comet revolve around the sun?

A comet follows an elliptical orbit around the sun, with the sun at one of its foci. As it gets closer to the sun, the comet's speed increases due to the sun's gravitational pull. The comet then swings around the sun and heads back out into the outer reaches of the solar system.

2. What causes a comet to revolve around the sun?

The force of gravity between the sun and the comet is what causes the comet to revolve around the sun. The sun's gravitational pull keeps the comet in its orbit and determines the shape and speed of its path.

3. How long does it take for a comet to revolve around the sun?

The time it takes for a comet to complete one revolution around the sun varies depending on its orbit. Some comets have very long orbits, taking hundreds or even thousands of years to complete one revolution, while others have shorter orbits of a few years.

4. What is the difference between a comet's revolution and its rotation?

A comet's revolution refers to its orbit around the sun, while its rotation refers to its spinning motion around its own axis. Most comets do not have a noticeable rotation due to their irregular shape and low mass.

5. Can a comet's revolution around the sun change?

Yes, a comet's revolution can change due to various factors such as interactions with other objects in the solar system, gravitational influences from neighboring stars, and the release of gas and dust from the comet's surface. These changes can alter the comet's orbit and potentially cause it to collide with another object or be ejected from the solar system entirely.

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