Scaling The Solar System By A Factor ##\alpha##

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Homework Help Overview

The problem involves scaling a model of the solar system by a factor of ##\alpha##, focusing on how this scaling affects the velocity and period of circular orbits. The context is rooted in gravitational physics and orbital mechanics.

Discussion Character

  • Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the relationship between velocity and the scaling factor, with one asserting that ##v \propto \alpha## is correct. Questions arise regarding the treatment of the radius ##r## in the second part of the problem and its implications for the period ##T##.

Discussion Status

The discussion is ongoing, with participants exploring the implications of their reasoning. Some guidance has been offered regarding the relationship between the radius and the scaling factor, but there is no explicit consensus on the correct interpretation of the period's dependence on ##\alpha##.

Contextual Notes

There appears to be some confusion regarding the application of the scaling factor to the radius in different parts of the problem, leading to differing conclusions about the period's dependence on ##\alpha##.

XanMan
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I am given the solution to the first part of the problem, however not the second part - would appreciate for someone to double check my work! Cheers.

1. Homework Statement

If a scale model of the solar system is made using materials of the same respective average density as the sun and planets, but reducing all linear dimension by a factor ##\alpha##, how will the velocity and period scale with ##\alpha##? Assume a circular orbit in your calculations.

Homework Equations


[/B]
$$F = \cfrac{GMm}{r^2}
$$F = \cfrac{mv^2}{r}

The Attempt at a Solution



Starting off with the basic relationship required:
$$\cfrac{GMm}{r^2} = \cfrac{mv^2}{r}$$

Then: ##v^2 = \cfrac{GM}{r} \propto \cfrac{G \rho R^3}{r}##, where ##R## is the radius of the Sun.

In general: $$v^2 \propto \cfrac{R^3}{r}$$

Re-scaling the solar system by ##\alpha##:

$$v^2 \propto \cfrac{\alpha^3 R^3}{\alpha r}$$

i) Therefore ##v \propto \alpha##

Now, ##v = \cfrac{2 \pi r}{T}##. Thus:
$$\cfrac{2 \pi r}{T} \propto \alpha$$

ii) Therefore ##T \propto \cfrac{1}{\alpha}##
 
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Well, apparently ##v\propto\alpha## is the right answer. If that is so, then I don't understand why you don't let ##r\propto\alpha## in part ii).

Oh, and a belated :welcome: !
 
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BvU said:
Well, apparently ##v\propto\alpha## is the right answer. If that is so, then I don't understand why you don't let ##r\propto\alpha## in part ii).

Oh, and a belated :welcome: !

Thank you! I'm not quite sure what you mean exactly. With some reasoning I could have also said that since ##v \propto \alpha##, then ##r \propto \alpha##. It thus follows that ##T \propto \cfrac{1}{\alpha}##.
 
What I mean is

In part 1 you use ##r' = \alpha r## to find ##v'= \alpha v##
Why don't you do that in part ii) ? to find that ##T'= {2\pi r'\over v'} = ..##
 
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BvU said:
What I mean is

In part 1 you use ##r' = \alpha r## to find ##v'= \alpha v##
Why don't you do that in part ii) ? to find that ##T'= {2\pi r'\over v'} = ..##

In which case ##T' = T## - thus ##T## is independent of ##\alpha##? What is wrong in my reasoning that results in me obtaining ##T \propto \cfrac{1}{\alpha}##?
 
You left ##r## as is. In part i) you inserted ##\alpha r##:
XanMan said:
Re-scaling the solar system by α:$$v^2 \propto \cfrac{\alpha^3 R^3}{\alpha r}$$

[edit] By the way: I had seen this part ii) result before, here
 
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Ah, how silly of me! Looked at the result you forwarded as well - got it now. Thank you so much and all the best for the new year!
 

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