Whenever two Apollo astronauts were on the surface of the Moon, a third astronaut orbited the Moon. Assume the orbit to be circular and 680 km above the surface of the Moon, where the acceleration due to gravity is 0.867 m/s2. The radius of the Moon is 1.70 x10^6 m.(a) Determine the astronaut's orbital speed.(b) Determine the period of the orbit.

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Answer:

(a) Determine the astronaut's orbital speed

The velocity of the astronaut is 1436m/s.

(b) Determine the period of the orbit.  

The period of the orbit is 10413 seconds.

Explanation:

(a) Determine the astronaut's orbital speed

The orbital speed of astronaut can be found by means of the Universal law of gravity:        

[tex]F = G\frac{M \cdot m}{r^{2}}[/tex]   (1)

Then, replacing Newton's second law in equation 3 it is gotten:

[tex]m\cdot a  = G\frac{M \cdot m}{r^{2}}[/tex]  (2)

However, a is the centripetal acceleration since the astronaut describes a circular motion around the Moon:

[tex]a = \frac{v^{2}}{r}[/tex]  (3)

Replacing equation 3 in equation 2 it is gotten:

[tex]m\frac{v^{2}}{r} = G\frac{M \cdot m}{r^{2}}[/tex]

[tex]m \cdot v^{2} = G \frac{M \cdot m}{r^{2}}r[/tex]

[tex]m \cdot v^{2} = G \frac{M \cdot m}{r}[/tex]

[tex]v^{2} = G \frac{M \cdot m}{rm}[/tex]

[tex]v^{2} = G \frac{M}{r}[/tex]

[tex]v = \sqrt{\frac{G M}{r}}[/tex] (4)

   

Where v is the orbital speed, G is the gravitational constant, M is the mass of the Moon, and r is the orbital radius.        

Notice that the orbital radius will be given by the sum of the radius of the Moon and the height of the astronaut above the surface.

       

But it is necessary to express the height of the astronaut above the surface in units of meters before it can be used.

[tex]r = 680km \cdot \frac{1000m}{1km}[/tex] ⇒ [tex]680000m[/tex]

[tex]r = 1.70x10^{6}m+680000m[/tex]

       

[tex]r = 2380000m[/tex]

However it is neccesary to find the mass of Moon in order to use equation 4.

Then Newton's second law ([tex]F = ma[/tex]) will be replaced in equation (1):

[tex]ma = G\frac{Mm}{r^{2}}[/tex]

Then, M will be isolated

[tex]M = \frac{r^{2}a}{G}[/tex] (5)

Where r is the orbital radius of the astronaut and a is the acceleration due to gravity.

[tex]M = \frac{(2380000m)^{2}(0.867 m/s^{2})}{6.67x10^{-11}N.m^{2}/kg^{2}}[/tex] (5)

[tex]M = 7.36x10^{22}Kg[/tex]

[tex]v = \sqrt{\frac{(6.67x10^{-11}N.m^{2}/kg^{2})(7.36x10^{22}Kg)}{2380000m}}[/tex]

                         

[tex]v = 1436m/s[/tex]

                                 

Hence, the velocity of the astronaut is 1436m/s.  

                                 

(b) Determine the period of the orbit.        

The period of the orbit can be determined by the next equation:

[tex]v = \frac{2\pi r}{T}[/tex]  (6)

Where v is the orbital velocity, r is the orbital radius and T is the period of the orbit.

                       

Then, T can be isolated from equation 6.

[tex]T = \frac{2\pi r}{v}[/tex] (7)

[tex]T = \frac{2\pi (2380000m)}{1436m/s}[/tex]

         

[tex]T = 10413s[/tex]         

Hence, the period of the orbit is 10413 seconds.                                      

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