Answer:
![-4.941*10^8J.](https://tex.z-dn.net/?f=-4.941%2A10%5E8J.)
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,
![\Delta U = \Delta_{perogee}-\Delta_{Apogee}](https://tex.z-dn.net/?f=%5CDelta%20U%20%3D%20%5CDelta_%7Bperogee%7D-%5CDelta_%7BApogee%7D)
Where,
![U= \frac{-GmM_e}{r}](https://tex.z-dn.net/?f=U%3D%20%5Cfrac%7B-GmM_e%7D%7Br%7D)
Replacing
![\Delta U = \frac{-GmM_e}{r_p}- \frac{-GmM_e}{r_a}](https://tex.z-dn.net/?f=%5CDelta%20U%20%3D%20%5Cfrac%7B-GmM_e%7D%7Br_p%7D-%20%5Cfrac%7B-GmM_e%7D%7Br_a%7D)
![\Delta U = GmM_e (\frac{1}{r_A}-\frac{1}{r_p})](https://tex.z-dn.net/?f=%5CDelta%20U%20%3D%20GmM_e%20%28%5Cfrac%7B1%7D%7Br_A%7D-%5Cfrac%7B1%7D%7Br_p%7D%29)
Our values are given by,
![m = 85.5Kg](https://tex.z-dn.net/?f=m%20%3D%2085.5Kg)
![M_e = 5.97*10^{24}Kg](https://tex.z-dn.net/?f=M_e%20%3D%205.97%2A10%5E%7B24%7DKg)
![r_A = 7330Km](https://tex.z-dn.net/?f=r_A%20%3D%207330Km)
![r_p = 6610Km](https://tex.z-dn.net/?f=r_p%20%3D%206610Km)
![G = 6.67*10^{-11}Nm^2/Kg^2](https://tex.z-dn.net/?f=G%20%3D%206.67%2A10%5E%7B-11%7DNm%5E2%2FKg%5E2)
Replacing at the equation,
![\Delta U = (6.67*10^{-11})(85.5)(5.97*10^{24}) (\frac{1}{7330}-\frac{1}{6610})](https://tex.z-dn.net/?f=%5CDelta%20U%20%3D%20%286.67%2A10%5E%7B-11%7D%29%2885.5%29%285.97%2A10%5E%7B24%7D%29%20%28%5Cfrac%7B1%7D%7B7330%7D-%5Cfrac%7B1%7D%7B6610%7D%29)
![\Delta U = -4.941*10^8J](https://tex.z-dn.net/?f=%5CDelta%20U%20%3D%20-4.941%2A10%5E8J)
Therefore the Energy necessary for Sputnik I as it moved from apogee to perigee was ![-4.941*10^8J.](https://tex.z-dn.net/?f=-4.941%2A10%5E8J.)
To solve the problem it is necessary to refer to the definition of entropy.
Entropy is defined aso
![\Delta S = \frac{\Delta Q}{T}](https://tex.z-dn.net/?f=%5CDelta%20S%20%3D%20%5Cfrac%7B%5CDelta%20Q%7D%7BT%7D)
Where,
Heat exchange
T = Temperature
Since the heat exchange is conserved and it is an isothermal process where the temperature remains constant the change in entropy remains the same, ie
(Reamins same)
Therefore the correct answer is C.
Correct answer choice is:
B. 50 percent
Explanation:
France Capitulates to Nazi Germany. On June 22, 1940, the French state approved a cease-fire with Nazi Germany just six weeks after the Nazis began their incursion of Western Europe.
Paris began preparing for combat in September 1939, when Nazi Germany overran Poland, but the combat appeared far beyond until May 10, 1940, when the Germans invaded France and immediately took the French troops. The French administration left Paris on June 10, and the Germans controlled the capital on June 14.
KE depends on velocity. It is easier to answer this question in terms of the earth.
The closer the object (earth/comet) is to the sun, the faster it moves. that means that the fastest moving point would be as the comet/earth passes through point C.
The slowest speed would be the furthest away from the sun which is point A.
Answer: The faster the planet moves the greater the Kinetic Energy.
The Slower the planet moves, the less the KE.
Point A is where it is slowest with the lowest amount of energy.
Discussion
The formula for KE is KE = 1/2mv^2. The mass of the comet or earth is a constant. It doesn't change no matter which point the comet passes through. If v goes down KE will go down. If v goes up, KE goes up.
Different fractions of the moon