Is a Comet's Momentum Conserved When Passing Near the Sun?

In summary, the momentum of the comet is nearly conserved because the interaction with the sun is similar to an elastic collision.
  • #1
levi2613
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Homework Statement


Which of the following is a true statement concerning a comet passing near the sun? (Mass of comet and mass loss are negligible)

1. The momentum of the comet is nearly conserved because the interaction with the sun is similar to an elastic collision.
2. The momentum of the comet is nearly conserved because the interaction with the sun is similar to an inelastic collision.
3. The mechanical energy (kinetic plus potential) of the comet is nearly conserved because the interaction with the sun is similar to an elastic collision.
4. The mechanical energy (kinetic plus potential) of the comet is nearly conserved because the interaction with the sun is similar to an inelastic collision.

The Attempt at a Solution


The correct answer is C. I understand that the momentum of just the comet is not conserved, but rather the system's as a whole is, so that knocks out A and B. And since it is clearly not inelastic, it can't be D either.

My question: NASA often uses this "slingshot" effect to accelerate objects without the use of fuel. If the object comes around the other side with more velocity than when it started, its KE must increase... where does that come from? The only potential energy I see is from the gravitational force of the sun. So I don't see how at equidistant points from the sun, one before the "collision" and one after, the KE could increase but the PE would be the same.

Thank you so much!
 
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  • #2
The slingshot effect you mention I believe comes from the fact that the planet they use to slingshot around is not standing still. The movement of the planet gives you the extra KE needed.

In fact you could calculate this...

Suppose you have a large planet (Jupiter for example) with mass M, moving with speed V, to the left.
Then suppose you have a spacecraft of mass m, moving with speed v, to the right. (So the planet and spacecraft are moving towards each other).
After the spacecraft has passed Jupiter (so it is now moving to the left aswell, it 'bounced' off the planet) it has a speed w (to the left) and the planet has a speed W.
The relation between their momentum and KE would be:
[tex]mv - MV = P = -mw - MW[/tex]
[tex]1/2 mv^2 + 1/2MV^2 = KE = 1/2mw^2 + 1/2MW^2[/tex]

Working this out further:
[tex]m(w^2 - v^2) = M(V^2 - W^2)[/tex]
[tex]m(w-v)(w+v) = M(V-W)(V+W)[/tex]

And
[tex]m(w+v) = M(V-W)[/tex]

This leads to:
[tex]w-v = V+W[/tex]

Note finally that W has changed only a tiny little bit due to the planet's very large mass, so we can say:
[tex]V+W = 2V[/tex]

So finally:
[tex]w = v + 2V[/tex]

I hope this is right :)
 
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  • #3
Thank you for taking the time to answer...

I can actually follow along with the math pretty well. And I intuitively understand how the spaceship would pick up speed... What I can't reconcile is that the total mechanical energy of the spaceship would be conserved. If it picks up twice the speed of the planet, its KE is multiplied by 4. Since the total mechanical energy = KE + PE, it would seem that the PE would have to drop dramatically. But the only potential energy I see is the gravitational enery, which would be the same at equidistant points before and after the collision. So if the potential energy is the same, but the KE has increased by a factor of 4, where's the conservation??

Thank you!
 
  • #4
I guess that in the question above they assumed the sun to be standing still, not moving (there is no mention of the comet picking up speed). I can't think of any other answer lol...
 

FAQ: Is a Comet's Momentum Conserved When Passing Near the Sun?

What is an elastic collision with the sun?

An elastic collision with the sun refers to when an object, such as a comet or asteroid, enters the sun's gravitational field and bounces off of it without any loss of kinetic energy or change in direction.

How does an elastic collision with the sun differ from other types of collisions?

An elastic collision with the sun is unique because it involves an object interacting with the immense gravitational force of the sun without being pulled in or destroyed. In other types of collisions, such as inelastic or partially inelastic collisions, the objects involved typically experience a loss of energy or change in direction.

What factors influence the outcome of an elastic collision with the sun?

The outcome of an elastic collision with the sun is primarily determined by the mass and velocity of the object, as well as the strength of the sun's gravitational field. The angle and trajectory of the object's approach can also play a role in the outcome.

Can an elastic collision with the sun cause any effects on the sun itself?

In most cases, an elastic collision with the sun will not have a significant impact on the sun itself. However, in rare cases where a very large or dense object collides with the sun, it may cause a temporary disturbance in the sun's surface or magnetic field.

How does studying elastic collisions with the sun contribute to our understanding of the solar system?

Studying elastic collisions with the sun can provide valuable information about the composition and behavior of objects in our solar system. It can also help us better understand the dynamics of the sun's gravitational field and how it interacts with other objects in space.

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