- #1
XanMan
- 14
- 1
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.
[/B]
$$F = \cfrac{GMm}{r^2}
$$F = \cfrac{mv^2}{r}
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}##
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}##