Answer:
[tex]-4.941*10^8J.[/tex]
Explanation:
To solve this exercise it is necessary to take into account the concepts related to gravitational potential energy, as well as the concept of perigee and apogee of a celestial body.
By conservation of energy we know that,
[tex]\Delta U = \Delta_{perogee}-\Delta_{Apogee}[/tex]
Where,
[tex]U= \frac{-GmM_e}{r}[/tex]
Replacing
[tex]\Delta U = \frac{-GmM_e}{r_p}- \frac{-GmM_e}{r_a}[/tex]
[tex]\Delta U = GmM_e (\frac{1}{r_A}-\frac{1}{r_p})[/tex]
Our values are given by,
[tex]m = 85.5Kg[/tex]
[tex]M_e = 5.97*10^{24}Kg[/tex]
[tex]r_A = 7330Km[/tex]
[tex]r_p = 6610Km[/tex]
[tex]G = 6.67*10^{-11}Nm^2/Kg^2[/tex]
Replacing at the equation,
[tex]\Delta U = (6.67*10^{-11})(85.5)(5.97*10^{24}) (\frac{1}{7330}-\frac{1}{6610})[/tex]
[tex]\Delta U = -4.941*10^8J[/tex]
Therefore the Energy necessary for Sputnik I as it moved from apogee to perigee was [tex]-4.941*10^8J.[/tex]