Find the speed of a satellite at a distance R from Earth

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SUMMARY

The discussion focuses on calculating the speed of a satellite at a distance R from the Earth's surface, utilizing gravitational force equations. Key equations include the orbital velocity formula \( v = \sqrt{gR} \) and escape velocity \( v = \sqrt{2gR} \). Participants clarify that for a circular orbit, the centripetal force must equal gravitational force, leading to the conclusion that the correct orbital speed is \( v = \sqrt{GM/R} \). The total mechanical energy of the satellite is also discussed, emphasizing that it can be negative due to the gravitational potential energy being defined as zero at infinity.

PREREQUISITES
  • Understanding of gravitational force and its formula \( F = \frac{GMm}{r^2} \)
  • Knowledge of orbital mechanics, specifically circular motion and centripetal force
  • Familiarity with kinetic and potential energy concepts in physics
  • Basic proficiency in algebra and solving equations involving square roots
NEXT STEPS
  • Study the derivation of gravitational force and its implications on satellite motion
  • Learn about the differences between circular, elliptical, parabolic, and hyperbolic orbits
  • Explore the concept of mechanical energy in gravitational fields and its significance
  • Investigate the relationship between escape velocity and orbital velocity
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and gravitational forces, as well as educators looking for examples of satellite motion calculations.

Helly123
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Homework Statement


Gravitational force exerted on mass m is GMm/r^2

2. Relevant equations
Orbital velocity at distance R from Earth = ##\sqrt gR##
Escape velocity = ##\sqrt 2gR##
gR = GM/R
Fc = mV^2/R
F =m.a

The Attempt at a Solution


1) express acceleration of gravity in terms of G, M , and R
F = m.a
a = F/m = GM/r^2

2) velocity of satellite at distance R from Earth's surface
I thought v = ##\sqrt gR##
But it is wrong.
I thought it is mv^2/R = GMm/R

3) mechanical energy for satellite in terms of G, m, R and EP at distance r infinity = 0
So, left EK. But i have to find the v first

Can i get a clue?
 
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Hi,
Whaat is the problem statement ? And what are considered known variables ?
 
BvU said:
Hi,
Whaat is the problem statement ? And what are considered known variables ?
Hi Sir.
The problem statement only that above. Variable is m, R, force of gravitational.
 
Helly123 said:

Homework Statement


Gravitational force exerted on mass m is GMm/r^2

2. Relevant equations
Orbital velocity at distance R from Earth = ##\sqrt gR##
Escape velocity = ##\sqrt 2gR##
gR = GM/R
Fc = mV^2/R
F =m.a

The Attempt at a Solution


1) express acceleration of gravity in terms of G, M , and R
F = m.a
a = F/m = GM/r^2

2) velocity of satellite at distance R from Earth's surface
I thought v = ##\sqrt gR##
But it is wrong.
I thought it is mv^2/R = GMm/R

3) mechanical energy for satellite in terms of G, m, R and EP at distance r infinity = 0
So, left EK. But i have to find the v first

Can i get a clue?
##\sqrt{2gR}## and ##\sqrt{gR}##
 
Helly123 said:
Hi Sir.
The problem statement only that above. Variable is m, R, force of gravitational.

But a satellite can have any speed at a point that is at a distance R from the center of the earth. If the trajectory must be circular (as I suspect is the intention in this exercise), then that makes things very different.
 
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BvU said:
But a satellite can have any speed at a point that is at a distance R from the center of the earth. If the trajectory must be circular (as I suspect is the intention in this exercise), then that makes things very different.
Orbital velocity is a circular motion right?
 
Helly123 said:
Orbital velocity is a circular motion right?
Not all orbits are circular, no. They can be circular, elliptical, parabolic or hyperbolic.

However, many orbits are approximately circular. If the problem stated in the title of this thread is to be answered given values for only G, M, m and r then, like @BvU, I suspect that the person who posed the question expected you to assume a circular orbit.
Helly123 said:
I thought it is ##\frac{mv^2}{R} = \frac{GMm}{R}##
Equating the required centripetal force for a circular trajectory of radius R with the actual centripetal force provided by gravity. Almost correct. You should check both formulas [at least one is wrong]. Then solve for v.
 
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jbriggs444 said:
Not all orbits are circular, no. They can be circular, elliptical, parabolic or hyperbolic.

However, many orbits are approximately circular. If the problem stated in the title of this thread is to be answered given values for only G, M, m and r then, like @BvU, I suspect that the person who posed the question expected you to assume a circular orbit.

Equating the required centripetal force for a circular trajectory of radius R with the actual centripetal force provided by gravity. Almost correct. You should check both formulas [at least one is wrong]. Then solve for v.
I missed it.
mv^2/R = GMm/R^2
V = ##\sqrt{GM/R}##
However, it is still wrong
 
Helly123 said:
I missed it.
mv^2/R = GMm/R^2
V = ##\sqrt{GM/R}##
However, it is still wrong
The answer is ##\sqrt{gR/2}## for number 2. Number 2 including 3, it says to be expressed in terms of r, G
 
  • #10
You are leaving us with not much to go on. The original post does not contain the problem statement. No subsequent post does either.
 
  • #11
jbriggs444 said:
You are leaving us with not much to go on. The original post does not contain the problem statement. No subsequent post does either.
I am sorry.. but i have added it. That is what it says
 
  • #12
The problem statement might ask the speed of satellite at distance R from the surface of Earth (R is the radius of Earth).
 
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  • #13
ehild said:
The problem statement might ask the speed of satellite at distance R from the surface of Earth (R is the radius of Earth).
Which means the total R is 2R?
 
  • #14
Better to use two different symbols for two different variables. The phrase 'Which means the total R is 2R?' looks really weird to me (but I understand what you mean).

Why not work it out ?
 
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  • #15
So, r = 2R
r is distance from satellite to Earth's center
Btw, mechanical energy is Ek. The answer is -mGR/4
How can Ek be negative?
 
  • #16
When object has centripetal force mv^2/r,
The radius r is measured in regards to what? If satellite, is due to Earth's center or Earth's surface?
 
  • #17
Helly123 said:
When object has centripetal force mv^2/r,
The radius r is measured in regards to what? If satellite, is due to Earth's center or Earth's surface?
What is the centripetal force in general? When a particle moves along a circle of radius r?
 
  • #18
ehild said:
What is the centripetal force in general? When a particle moves along a circle of radius r?
Ok it is in regard to the center
 
  • #19
Helly123 said:
Ok it is in regard to the center
Yes. And where is the center of the orbit?
 
  • #20
ehild said:
Yes. And where is the center of the orbit?
Earth's center?
Why Ek can be negative? Do you know it?
 
  • #21
If you mean Ek kinetic energy, it can not be ó negative.
For a bound orbit, the total mechanical energy is negative, and the satellite does not reach infinity. What is the total mechanical energy on the orbit of radius r? On an orbit of radius 2R? What happens if r increases to infinity?
 
  • #22
ehild said:
If you mean Ek kinetic energy, it can not be ó negative.
For a bound orbit, the total mechanical energy is negative, and the satellite does not reach infinity. What is the total mechanical energy on the orbit of radius r? On an orbit of radius 2R? What happens if r increases to infinity?
Satellite does not reach infinity?
If r increases to infinity, gravitational force = 0, Fc = 0 ?
 
  • #23
The total mechanical energy does not change.
The problem states that the potential energy is zero at infinity. That means the satellite is not under the influence of other planets (Sun for example) even at far away from the Earth. What is the gravitational potential of the Earth at distance r ? What is the total mechanical energy Ep+Ek of the satellite along an orbit of radius r? The kinetic energy is 1/2 mv2. It can not be negative. The satellite can reach infinity if the speed exceeds the escape velocity. You calculated the speed on an orbit of radius 2R . How is it related to the escape velocity?
 
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  • #24
ehild said:
The total mechanical energy does not change.
The problem states that the potential energy is zero at infinity. That means the satellite is not under the influence of other planets (Sun for example) even at far away from the Earth. What is the gravitational potential of the Earth at distance r ? What is the total mechanical energy Ep+Ek of the satellite along an orbit of radius r? The kinetic energy is 1/2 mv2. It can not be negative. The satellite can reach infinity if the speed exceeds the escape velocity. You calculated the speed on an orbit of radius 2R . How is it related to the escape velocity?
Ok.
Escape velocity
1/2mv^2 = EP of Earth
1/2mv^2 = GMm/R
v = ##\sqrt{2GM/R}## = ##\sqrt{2gR}##
R = Earth's radius

Ep of Earth at distance r
= GMm/r = mgR^2/2R = mgR/2

Kinetic energy during orbitting is obtained by using escape velocity?
 
  • #25
Helly123 said:
Ok.
Escape velocity
1/2mv^2 = EP of earth
1/2mv^2 = GMm/R
v = ##\sqrt{2GM/R}## = ##\sqrt{2gR}##
R = Earth's radius

Ep of Earth at distance r
= GMm/r = mgR^2/2R = mgR/2

Kinetic energy during orbitting is obtained by using escape velocity?
No, it is calculated from the speed along the orbit, you have already.
What is the sign of the potential energy? The force points towards the center.
 
  • #26
ehild said:
No, it is calculated from the speed along the orbit, you have already.
What is the sign of the potential energy? The force points towards the center.
ehild said:
No, it is calculated from the speed along the orbit, you have already.
What is the sign of the potential energy? The force points towards the center.
is it negative? But why?
 
  • #27
Helly123 said:
is it negative? But why?
Where is the reference point where potential energy is zero?
 
  • #28
jbriggs444 said:
Where is the reference point where potential energy is zero?
In the center of the earth? Isn't it?
 
  • #29
Helly123 said:
In the center of the earth? Isn't it?
Using a reference point at the center of the earth, the potential energy of a satellite would be positive. The conventional reference point is infinitely far away instead.

You can read that from the formula for potential energy. If the potential energy is given by$$PE=-\frac{GMm}{r}$$then the potential energy is zero when r is infinite.

The choice of reference point is purely arbitrary. Only differences in potential energy are physically meaningful. Placing the reference point at infinity simplifies the above potential energy formula by eliminating the need to add a "+ C" at the end.
 
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  • #30
Helly123 said:
is it negative? But why?
Bodies released from rest, move in the direction so as their potential energy decrease.
It was said in the problem that the potential energy of the satellite is zero at infinity.
If it is in rest, the total mechanical energy is zero at infinity. Adding just a little push towards the Earth, it will move towards the Earth and its potential energy decreases. The potential energy decreases from zero, so it must be negative Ep=-GmM/r.
 
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