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dani123
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Homework Statement
As the Earth revolves around the sun, if not only travels a certain distance every second, it also causes an imaginary line between the Earth and the sun to pass through a certain area every second. During one complete trip around the sun, the total area would be approximately equal to ∏R2. The time it would take to do this would be the period, T. Determine the rate at which the area is swept by an imaginary line joining the sun and the Earth as the Earth orbits the sun. Use the Earth's period of 365 days and the mean orbital radius of 1.50x1011.
Homework Equations
I have made a list of equations that are relevant for this entire module on universal gravitation. So although there are many of them does not mean that they all apply in this circumstance. The ones relevant to this question will be placed in bold.
Kepler's 3rd law: (Ta/Tb)2=(Ra/Rb)3
motion of planets must conform to circular motion equation: Fc=4∏2mR/T2
From Kepler's 3rd law: R3/T2=K or T2=R3/K
Gravitational force of attraction between the sun and its orbiting planets: F=(4∏2Ks)*m/R2=Gmsm/R2
Gravitational force of attraction between the Earth and its orbiting satelittes: F=(4∏2Ke)m/R2=Gmem/R2
Newton's Universal Law of Gravitation: F=Gm1m2/d2
value of universal gravitation constant is: G=6.67x10-11N*m2/kg2
weight of object on or near Earth: weight=Fg=mog, where g=9.8 N/kg
Fg=Gmome/Re2
g=Gme/(Re)2
determine the mass of the Earth: me=g(Re)2/G
speed of satellite as it orbits the Earth: v=√GMe/R, where R=Re+h
period of the Earth-orbiting satellite: T=2∏√R3/GMe
Field strength in units N/kg: g=F/m
Determine mass of planet when given orbital period and mean orbital radius: Mp=4∏2Rp3/GTp2
The Attempt at a Solution
I highlighted the above equation because I think I am supposed to use this equation for this problem. But I honestly don't understand what this question is actually looking for, so if someone could let me know where I should even begin it would be greatly appreciated! Thank you so much in advance!