Derive expression for orbital velocity?
Answer
558.6k+ views
Hint: Derive the orbital velocity, as we concern ourselves with the following two concepts:
Gravitational Force: it is very important to keep the universe functioning. Is a force that exists among all material objects in the universe. For any two objects or particles having nonzero mass, the force of gravity tends to attract them toward each other.
Centripetal Force: Is a force that makes a body follow a curved path. Its direction is always orthogonal to the motion of the body and towards the fixed point of the instantaneous center of curvature of the path. Isaac Newton described it as “a force by which bodies are drawn or impelled, or in any way tend, toward a point as to a center.
Complete step by step solution:
For the derivation, let us consider a satellite of mass $ m $ revolving around the Earth in a circular orbit of the radius $ r $ at a height $ h $ from the surface of the Earth. Suppose $ M $ and $ R $ are the mass and radius of the Earth respectively, then $ r = R + h $ .
To revolve the satellite, centripetal force of $ \dfrac{{m{v_0}^2}}{r} $ is needed which is provided by the gravitational force $ G\dfrac{{Mm}}{{{r^2}}} $ between the satellite and the Earth.
So, equating both the equations, we get
$ \dfrac{{m{v_0}^2}}{r} = G\dfrac{{Mm}}{{{r^2}}} $
$ {v_0}^2 = \dfrac{{GM}}{r} = \dfrac{{GM}}{{R + h}} $
Simplifying the above equation further, we get
$ {v_0} = \sqrt {\dfrac{{GM}}{{R + h}}} $ ……. $ (1) $
But $ GM = g{R^2} $ , Where $ g $ is the acceleration due to gravity.
Therefore,
$ {V_0} = \sqrt {\dfrac{{g{R^2}}}{{R + h}}} $
From the above equation, we get
$ {v_0} = R\sqrt {\dfrac{g}{{R + h}}} $
Let $ g $ ’ be the acceleration due to gravity (at a height h from the surface)
$ g' = \dfrac{{GM}}{{{{\left( {R + h} \right)}^2}}} $
Solve it. We get,
$ \dfrac{{GM}}{{\left( {R + h} \right)}} = g'\left( {R + h} \right) = g'r $ …. $ (2) $
Substituting $ (2) $ in $ (1) $ , we get
$ {v_0} = \sqrt {g'r} = \sqrt {g'\left( {R + h} \right)} $
Note:
Satellites, the object is not to escape Earth’s gravity. But balance it. Orbital velocity is velocity needed to achieve balance between the gravity’s pull on satellite and inertia of the satellite’s motion- the satellite’s tendency to keep going.
Gravitational Force: it is very important to keep the universe functioning. Is a force that exists among all material objects in the universe. For any two objects or particles having nonzero mass, the force of gravity tends to attract them toward each other.
Centripetal Force: Is a force that makes a body follow a curved path. Its direction is always orthogonal to the motion of the body and towards the fixed point of the instantaneous center of curvature of the path. Isaac Newton described it as “a force by which bodies are drawn or impelled, or in any way tend, toward a point as to a center.
Complete step by step solution:
For the derivation, let us consider a satellite of mass $ m $ revolving around the Earth in a circular orbit of the radius $ r $ at a height $ h $ from the surface of the Earth. Suppose $ M $ and $ R $ are the mass and radius of the Earth respectively, then $ r = R + h $ .
To revolve the satellite, centripetal force of $ \dfrac{{m{v_0}^2}}{r} $ is needed which is provided by the gravitational force $ G\dfrac{{Mm}}{{{r^2}}} $ between the satellite and the Earth.
So, equating both the equations, we get
$ \dfrac{{m{v_0}^2}}{r} = G\dfrac{{Mm}}{{{r^2}}} $
$ {v_0}^2 = \dfrac{{GM}}{r} = \dfrac{{GM}}{{R + h}} $
Simplifying the above equation further, we get
$ {v_0} = \sqrt {\dfrac{{GM}}{{R + h}}} $ ……. $ (1) $
But $ GM = g{R^2} $ , Where $ g $ is the acceleration due to gravity.
Therefore,
$ {V_0} = \sqrt {\dfrac{{g{R^2}}}{{R + h}}} $
From the above equation, we get
$ {v_0} = R\sqrt {\dfrac{g}{{R + h}}} $
Let $ g $ ’ be the acceleration due to gravity (at a height h from the surface)
$ g' = \dfrac{{GM}}{{{{\left( {R + h} \right)}^2}}} $
Solve it. We get,
$ \dfrac{{GM}}{{\left( {R + h} \right)}} = g'\left( {R + h} \right) = g'r $ …. $ (2) $
Substituting $ (2) $ in $ (1) $ , we get
$ {v_0} = \sqrt {g'r} = \sqrt {g'\left( {R + h} \right)} $
Note:
Satellites, the object is not to escape Earth’s gravity. But balance it. Orbital velocity is velocity needed to achieve balance between the gravity’s pull on satellite and inertia of the satellite’s motion- the satellite’s tendency to keep going.
Recently Updated Pages
Three beakers labelled as A B and C each containing 25 mL of water were taken A small amount of NaOH anhydrous CuSO4 and NaCl were added to the beakers A B and C respectively It was observed that there was an increase in the temperature of the solutions contained in beakers A and B whereas in case of beaker C the temperature of the solution falls Which one of the following statements isarecorrect i In beakers A and B exothermic process has occurred ii In beakers A and B endothermic process has occurred iii In beaker C exothermic process has occurred iv In beaker C endothermic process has occurred

Master Class 11 Social Science: Engaging Questions & Answers for Success

Master Class 11 Physics: Engaging Questions & Answers for Success

Master Class 11 Maths: Engaging Questions & Answers for Success

Master Class 11 Economics: Engaging Questions & Answers for Success

Master Class 11 Computer Science: Engaging Questions & Answers for Success

Trending doubts
One Metric ton is equal to kg A 10000 B 1000 C 100 class 11 physics CBSE

There are 720 permutations of the digits 1 2 3 4 5 class 11 maths CBSE

State and prove Bernoullis theorem class 11 physics CBSE

Draw a diagram of a plant cell and label at least eight class 11 biology CBSE

Difference Between Prokaryotic Cells and Eukaryotic Cells

1 Quintal is equal to a 110 kg b 10 kg c 100kg d 1000 class 11 physics CBSE

