
A satellite which is geostationary in a particular orbit is taken to another orbit. Its distance from the center of the earth in a new orbit is 2 times than that of the earlier orbit. The time period in the 2nd orbit is given by-
(a) 4.8 hours
(b) \[48\sqrt 2 \] hours
(c) 24 hours
(d) \[24\sqrt 2 \] hours
Answer
177.9k+ views
Hint:
1. Kepler’s 3rd law of planetary motion gives direct proportionality relation between radius of the orbit and approximate time taken by the planet to complete 1 revolution.
2. Time period of revolution of the geostationary satellite is T= 24hrs Here, in question, there is no mention of Mass and other parameters so we should not think along gravitational force direction.
Formula Used:
According to Kepler’s 3rd law, for a given orbit around its Sun: $\dfrac{{{T^2}}}{{{R^3}}} = $ constant …… (1)
Where,
T is time period of revolution
R is radius of the circular orbit or path followed
Complete step by step answer:
Given:
1.Radius of the geostationary satellite: R where, R is radius of earth
Let, the time period of geostationary satellite: T
Let, New radius for the satellite: ${R_{new}} = 2R$ …… (a)
Let, new time period of the satellite in shifted orbit be: ${T_{new}}$
To find: New time period of revolution ${T_{new}}$
Step 1:
From equation (1) we know initially: $\dfrac{{{T^2}}}{{{R^3}}} = $ k …… (2)
where, k is constant
Step 2:
Similarly, Kepler’s 3rd law is valid for new orbit as well.
So, using equation (1) for new orbit we can again say: ${({T_{new}})^2} = k.{({R_{new}})^3}$ …… (3)
Step 3:
Dividing equation (2) by equation (3), we get-
$\dfrac{{{{(T)}^2}}}{{{{({T_{new}})}^2}}} = \dfrac{{k.{{(R)}^3}}}{{k.{{({R_{new}})}^3}}}$ …… (4)
Step 4:
From the hint we know, the time period of revolution is T=24 hours for geostationary satellites.
Using above fact, and substituting value from equation (a) in equation (4) we get-
$
\Rightarrow \dfrac{{{{(T)}^2}}}{{{{({T_{new}})}^2}}} = \dfrac{{k.{{(R)}^3}}}{{k.{{(2R)}^3}}} \\
\Rightarrow \dfrac{{{{(24)}^2}}}{{{{({T_{new}})}^2}}} = \dfrac{1}{8} \Rightarrow {(24)^2} \times 8 = {({T_{new}})^2} \\
\Rightarrow {T_{new}} = 24 \times 2\sqrt 2 \\
$
Final Answer
(b) \[48\sqrt 2 \] hours
Note: New time period is different than 24 hours. Hence the satellite is no more geo-stationary, for a satellite to be geo-stationary its time period should be the same as time taken for earth to rotate about its axis i.e 24hrs.
1. Kepler’s 3rd law of planetary motion gives direct proportionality relation between radius of the orbit and approximate time taken by the planet to complete 1 revolution.
2. Time period of revolution of the geostationary satellite is T= 24hrs Here, in question, there is no mention of Mass and other parameters so we should not think along gravitational force direction.
Formula Used:
According to Kepler’s 3rd law, for a given orbit around its Sun: $\dfrac{{{T^2}}}{{{R^3}}} = $ constant …… (1)
Where,
T is time period of revolution
R is radius of the circular orbit or path followed
Complete step by step answer:
Given:
1.Radius of the geostationary satellite: R where, R is radius of earth
Let, the time period of geostationary satellite: T
Let, New radius for the satellite: ${R_{new}} = 2R$ …… (a)
Let, new time period of the satellite in shifted orbit be: ${T_{new}}$
To find: New time period of revolution ${T_{new}}$
Step 1:
From equation (1) we know initially: $\dfrac{{{T^2}}}{{{R^3}}} = $ k …… (2)
where, k is constant
Step 2:
Similarly, Kepler’s 3rd law is valid for new orbit as well.
So, using equation (1) for new orbit we can again say: ${({T_{new}})^2} = k.{({R_{new}})^3}$ …… (3)
Step 3:
Dividing equation (2) by equation (3), we get-
$\dfrac{{{{(T)}^2}}}{{{{({T_{new}})}^2}}} = \dfrac{{k.{{(R)}^3}}}{{k.{{({R_{new}})}^3}}}$ …… (4)
Step 4:
From the hint we know, the time period of revolution is T=24 hours for geostationary satellites.
Using above fact, and substituting value from equation (a) in equation (4) we get-
$
\Rightarrow \dfrac{{{{(T)}^2}}}{{{{({T_{new}})}^2}}} = \dfrac{{k.{{(R)}^3}}}{{k.{{(2R)}^3}}} \\
\Rightarrow \dfrac{{{{(24)}^2}}}{{{{({T_{new}})}^2}}} = \dfrac{1}{8} \Rightarrow {(24)^2} \times 8 = {({T_{new}})^2} \\
\Rightarrow {T_{new}} = 24 \times 2\sqrt 2 \\
$
Final Answer
(b) \[48\sqrt 2 \] hours
Note: New time period is different than 24 hours. Hence the satellite is no more geo-stationary, for a satellite to be geo-stationary its time period should be the same as time taken for earth to rotate about its axis i.e 24hrs.
Recently Updated Pages
JEE Main Physics Mock Test 2025

JEE Main Maths Mock Test 2025: FREE Online Mock Test Series

JEE Main Chemistry Mock Test 2025

JEE Main Hydrocarbons Mock Test 2025-26: Free Practice Online

JEE Main 2025-26 Mock Test: Organic Compounds Containing Nitrogen

JEE Main 2025-26 Mock Test: Organic Compounds Containing Halogens

Trending doubts
JEE Main 2025 Session 2: Application Form (Out), Exam Dates (Released), Eligibility, & More

JEE Main 2025: Derivation of Equation of Trajectory in Physics

Displacement-Time Graph and Velocity-Time Graph for JEE

Learn About Angle Of Deviation In Prism: JEE Main Physics 2025

Degree of Dissociation and Its Formula With Solved Example for JEE

What is Hybridisation in Chemistry?

Other Pages
NCERT Solutions For Class 11 Physics Chapter 2 Motion In A Straight Line - 2025-26

NCERT Solutions For Class 11 Physics Chapter 1 Units and Measurements - 2025-26

JEE Advanced Marks vs Ranks 2025: Understanding Category-wise Qualifying Marks and Previous Year Cut-offs

Units And Measurements Class 11 Physics Chapter 1 CBSE Notes - 2025-26

NCERT Solutions For Class 11 Physics Chapter 3 Motion In A Plane - 2025-26

Motion in a Straight Line Class 11 Physics Chapter 2 CBSE Notes - 2025-26
