ATAR Notes: Forum
VCE Stuff => VCE Science => VCE Mathematics/Science/Technology => VCE Subjects + Help => VCE Physics => Topic started by: IntoTheNewWorld on June 08, 2009, 10:57:05 am
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Gravity questions annoy me =[
Any help on this question (attached) greatly appreciated =]
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I cbs working it out properly, but you could probably do it like this:
+ find g of mercury from the g of mars (g mars = 1/16 g mercury)
+g=GM/r^2 (we know the mass of the sun, so rearrange to find the the radius of mars' orbit)
+Mercury's orbit's radius = 1/4 of the orbit of mars (so then you've got the second part of the question done)
+g=4((pi)^2)r/T^2 (rearrange to find the value of T^2 for each one)
+Then sub the values of T^2 into your ratio
There's probably an easier way to do this, but I don't really have the time to sit down and look at it properly.
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Whoops, misread the question.
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R^3/T^2 = GM/4pi
So T^2/R^3 = 4pi/GM
Something like that.
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thx Appianway =], it's simpler than I thought =0
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No problem... sorry for misreading the question at first!
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LOL i wasted my time working this out the hard way so i'll give you the easy way first
By Kepler's Third Law(rearranged) we got
T^2 4pi^2
___ = ______
R^3 GM
sub M in as the Sun and you're sweet you got
2.2959E-19s^2m^-3
units will be seconds^2*meters^-3
what's interesting is that the ratio for this for every planet rotating around the sun is theoretically the same.
p.s. yea hardway is what appian said first*