C. Clear, dry weather. A good way to remember is H for high pressure = H for happy weather; L for low pressure = L for lousy weather (Glad I had someone to tell me this)
Answer:
![\rho = 12580.7 kg/m^3](https://tex.z-dn.net/?f=%5Crho%20%3D%2012580.7%20kg%2Fm%5E3)
Explanation:
As we know that the satellite revolves around the planet then the centripetal force for the satellite is due to gravitational attraction force of the planet
So here we will have
![F = \frac{GMm}{(r + h)^2}](https://tex.z-dn.net/?f=F%20%3D%20%5Cfrac%7BGMm%7D%7B%28r%20%2B%20h%29%5E2%7D)
here we have
![F =\frac {mv^2}{(r+ h)}](https://tex.z-dn.net/?f=F%20%3D%5Cfrac%20%7Bmv%5E2%7D%7B%28r%2B%20h%29%7D)
![\frac{mv^2}{r + h} = \frac{GMm}{(r + h)^2}](https://tex.z-dn.net/?f=%5Cfrac%7Bmv%5E2%7D%7Br%20%2B%20h%7D%20%3D%20%5Cfrac%7BGMm%7D%7B%28r%20%2B%20h%29%5E2%7D)
here we have
![v = \sqrt{\frac{GM}{(r + h)}}](https://tex.z-dn.net/?f=v%20%3D%20%5Csqrt%7B%5Cfrac%7BGM%7D%7B%28r%20%2B%20h%29%7D%7D)
now we can find time period as
![T = \frac{2\pi (r + h)}{v}](https://tex.z-dn.net/?f=T%20%3D%20%5Cfrac%7B2%5Cpi%20%28r%20%2B%20h%29%7D%7Bv%7D)
![T = \frac{2\pi (2.05 \times 10^6 + 310 \times 10^3)}{\sqrt{\frac{GM}{(r + h)}}}](https://tex.z-dn.net/?f=T%20%3D%20%5Cfrac%7B2%5Cpi%20%282.05%20%5Ctimes%2010%5E6%20%2B%20310%20%5Ctimes%2010%5E3%29%7D%7B%5Csqrt%7B%5Cfrac%7BGM%7D%7B%28r%20%2B%20h%29%7D%7D%7D)
![1.15 \times 3600 = \frac{2\pi (2.05 \times 10^6 + 310 \times 10^3)}{\sqrt{\frac{(6.67 \times 10^{-11})(M)}{(2.05 \times 10^6 + 310 \times 10^3)}}}](https://tex.z-dn.net/?f=1.15%20%5Ctimes%203600%20%3D%20%5Cfrac%7B2%5Cpi%20%282.05%20%5Ctimes%2010%5E6%20%2B%20310%20%5Ctimes%2010%5E3%29%7D%7B%5Csqrt%7B%5Cfrac%7B%286.67%20%5Ctimes%2010%5E%7B-11%7D%29%28M%29%7D%7B%282.05%20%5Ctimes%2010%5E6%20%2B%20310%20%5Ctimes%2010%5E3%29%7D%7D%7D)
![M = 4.54 \times 10^{23} kg](https://tex.z-dn.net/?f=M%20%3D%204.54%20%5Ctimes%2010%5E%7B23%7D%20kg)
Now the density is given as
![\rho = \frac{M}{\frac{4}{3}\pi r^3}](https://tex.z-dn.net/?f=%5Crho%20%3D%20%5Cfrac%7BM%7D%7B%5Cfrac%7B4%7D%7B3%7D%5Cpi%20r%5E3%7D)
![\rho = \frac{4.54 \times 10^{23}}{\frac{4}[3}\pi(2.05 \times 10^6)^3}](https://tex.z-dn.net/?f=%5Crho%20%3D%20%5Cfrac%7B4.54%20%5Ctimes%2010%5E%7B23%7D%7D%7B%5Cfrac%7B4%7D%5B3%7D%5Cpi%282.05%20%5Ctimes%2010%5E6%29%5E3%7D)
![\rho = 12580.7 kg/m^3](https://tex.z-dn.net/?f=%5Crho%20%3D%2012580.7%20kg%2Fm%5E3)