Two satellites revolve round the earth with orbital radii 4R and 16R, if the time period of first satellite is T then that of the other is (a) 4 T (b) 42/3 T (c) 8 T (d) None of these
Answers
According to Kepler's Third law:
T² ∝ R³
Given that, two satellites revolve round the earth with orbital radii 4R and 16R, if the time period of first satellite is T.
For first satellite:
(T1)² = (4R)³
T1 = (4R)³/² ...........(1st equation)
For second satellite
(T2)² = (16R)³
T2 = (16)³/² ...........(2nd equation)
We have to find T2. So, divide (1st equation) and (2nd equation)
T1/T2 = [(4R)³/²]/[(16R)³/²]
T1/T2 = [(4R)/(16R)]³/²
T1/T2 = (1/4)³/²
(T1)²/(T2)² = (1/4)³
(T1)²/(T2)² = 1/64
T1/T2 = √1/64
T1/T2 = 1/8
T2 = 8 × T1
As, the time period for first satellite is T. So, T1 = T
T2 = 8T
Option c) 8T
Kepler's Third Law:
The square of time period of revolution of planet around sun is directly proportional to square of cube of length of semi-major axis. i.e. T² ∝ R³
Given:
- Two satellites revolve around the earth with orbital radii 4R & 16R
- Time period for first satellite T
To find:
- Time period of other sattelite
Solution:
Using Kepler's third law
T² ∝ R³
Let
- Time taken for first satellite be T1
- Time taken for second satellite be T2
Now,
First satellite
(T1)² = (4R)³
→ T1 = √(4R)³. ….…(Eq 1)
Second satellite
(T2)² = (16R)³
T2 = √(16R)³. .….…(Eq 2)
To find T2 dividing both the equations
→ T1/T2 = [√(4R)³]/[√(16R)³]
→ T1/T2 = √[4R/16R]³
→ T1/T2 = √1/64
→ T1/T2 = 1/8
Substituting T1 = T ( °.° Given )
→ T/T2 = 1/8
Cross Multiplying
→ T2 = 8T. ( Option C)
Hence, option (c) is answer