Question
Question: A satellite of the moon revolves around it in radius n times the radius of the moon (R). Due to cosm...
A satellite of the moon revolves around it in radius n times the radius of the moon (R). Due to cosmic dust,it experiences a resistance f=av2. Find how long it will stay in the orbit.
(a). aRGMmn
(b). amGMR(n−1)
(c). amv(n−1)
(d). amvf2vl
Solution
- Hint: In this question, we first find the force due to air resistance as f=raGM by using v=rGM then we find word done using dw=fvdt that is dw=a(rGM)23dt . After that we find the total energy as E=−2rGMm then we use the work energy theorem that is dw=−dE
Complete step-by-step solution -
Here it is given that the resistance due to the cosmic dust is
f=av2---------------------- (1)
Where v is the velocity of the satellite and it is given as
v=rGM---------------------- (2)
Here G is the universal gravitational constant
M is the mass of the moon
And r is the distance of the satellite from the moon
Now substituting equation (2) in equation (1) we get
f=a(rGM)2
⇒f=raGM---------------------- (3)
Now we will find the small work done dw by the force f of cosmic dust resistances that is
dw=fdx
We can replace dx=vdtbecause velocity can be written as v=dtdx , so we will get
dw=fvdt-------------------- (4)
Now substituting equation (2) and equation (3) in equation (4) we get
dw=(raGM)(rGM)dt
⇒dw=a(rGM)23dt-------------------------- (5)
We know that the total energy is sum of potential and kinetic energy
Here kinetic energy is given as
21mv2
Putting v=rGMin this we get
KE=2rGMm
Here potential energy is given as
PE=−rGMm
So, total energy is given as
E=PE+KE
⇒E=−rGMm+2rGMm
⇒E=−2rGMm------------------------------- (6)
Now we find the change in energy that is
⇒dE=−d(2rGMm)
⇒dE=−(−2r2GMm)
⇒dE=2r2GMm-------------------------------- (7)
Now by applying the work energy theorem that the change in energy is equal to the word done, dw=−dE------------------------------------- (8)
Now substituting equation (5) and (7) in (8) we get
⇒−a(rGM)23dt=−2r2GMm
⇒(−raGM)(rGM)dt=−2r2GMm
Now canceling G, M on both side and taking r on one side and then taking integration on both side we get
⇒ma∫0tdt=21GM1ri∫rfr2−1dr
⇒ma∫0tdt=−21GM1nR∫Rr2−1dr
Now by solving this we get
t=amGMR(n−1)
Hence, option B is correct.
Note: For these types of questions we need to be familiar with the concepts of binding energy and satellites, orbital velocity, the minimum distance of approach, the expression for energy for satellites, the expression for the velocity of a satellite orbiting, and gravitational potential energy.