Orbital Speed: Earth vs Moon - How Does Altitude Affect Orbital Velocity?

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Discussion Overview

The discussion revolves around the relationship between altitude and orbital velocity for objects orbiting the Earth and the Moon. Participants explore how the gravitational differences between the two bodies affect the required speeds for maintaining circular orbits at specified altitudes.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested, Mathematical reasoning

Main Points Raised

  • Some participants suggest that the orbital speed at a given altitude above the Moon would be less than that above the Earth due to the Moon's lower gravitational force.
  • Others argue that orbital velocity depends on the radius of the orbit and the mass of the celestial body, indicating that the Moon's lower mass would result in a lower required speed.
  • A participant presents a mathematical approach using Newton's laws and gravitational equations to derive the orbital speed, asserting that it would be less for the Moon.
  • There is a clarification about the definition of altitude, with some insisting it should refer to the distance above the center of mass rather than above the surface, while others maintain that altitude typically refers to height above a reference surface.
  • One participant provides specific values for the Moon's mass and radius, suggesting that the orbital velocity at a small altitude is reduced by about a factor of 2 compared to Earth.
  • Another participant challenges the assertion that distance above the surface does not affect orbital dynamics, arguing that it is crucial for understanding orbital mechanics.
  • A detailed mathematical ratio of orbital velocities for the Earth and Moon is presented, indicating that the ratio increases with altitude, with specific calculations provided for different altitudes.

Areas of Agreement / Disagreement

Participants express disagreement regarding the definition of altitude and its implications for orbital dynamics. While some agree on the mathematical relationships involved, there is no consensus on the impact of altitude definitions on the understanding of orbital mechanics.

Contextual Notes

Participants reference specific gravitational values and ratios, but there are unresolved assumptions regarding the definitions of altitude and the implications for orbital calculations. The discussion includes corrections and refinements of earlier claims without reaching a definitive conclusion.

robotnut
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Just can't get my head around this one. If at 100Km high above Earth the orbital speed to maintain altitude is X, then what would the speed be for the same object around the moon?
Since gravity of the moon is smaller then earth's? I assume the orbital speed would need to be less?
 
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orbital velocity might be less as the orbital velocity depends on the radius of the orbit in which they move and the mass of moon is less than Earth .
 
Considering this mass orbiting around the Earth or around the moon means its covering a uniform circular motion.
Studying the sum of forces =0, where the forces are:
F=(G.M.m)/d^2 :Gravitational force done by the Earth on the object which is the centripetal force.
F1 :Centrifugal force which is also equal in magnitude to the centripetal force, but opposite direction.
applying Newtons 2nd law and knowing that the centripetal force is also given by the following fomula F=(m.V^2)/d
then [(G.M.m)/d^2]=[(m.V^2)/d]
calculate v and you will notice that it will be less than the speed on the earth.
 
robotnut said:
...If at 100Km high above Earth the orbital speed to maintain altitude is X...

To avoid any confusion, we should all agree that these altitudes are above the center of the Earth and Moon, respectively; not above their surfaces.
 
That is contrary to the meaning of the term "altitude", which invariably means height above some reference surface.
 
This seems like a straightforward question. For a circular orbit (which is the only kind where you get a constant speed), we just set the gravitational field equal to the centripetal acceleration

[tex]\dfrac{v^2}{r} = \dfrac{GM}{r^2}[/tex]

[tex]v = \sqrt{\dfrac{GM}{r}}[/tex]

So if you're at some altitude h, just set the distance from the center equal to the radius of the planet R, plus the altitude

[tex]v = \sqrt{\dfrac{GM}{R + h}}[/tex]

The required speed is independent of the mass (this is for precisely the same reason as why all objects fall at the same acceleration without air resistance). Just set h to 100 km, and you can calculate the orbital speed for the Earth and the moon by substituting the appropriate values for the radius and mass of the Earth and the moon.
 
arunma said:
The required speed is independent of the mass
of the orbiting body, of course (I know that's what you meant, just thought a clarification couldn't hurt)

If I remember correctly, the moon's mass is 1/6 that of Earth, and it's radius is about 1/3 of the Earth's, so I guess the orbital velocity at a given (small) altitude is reduced by about a factor of 2...
 
The Moon's surface gravity is about 1/6 that of the Earth. The Moon's mass however is about 1/81 Earth masses.
 
diazona said:
of the orbiting body, of course (I know that's what you meant, just thought a clarification couldn't hurt)

You're quite right, thanks!
 
  • #10
D H said:
That is contrary to the meaning of the term "altitude", which invariably means height above some reference surface.
Yes, I know. But what I'm asking is that we all refer to the distance above center of mass, because it removes an unnecessary complication, and avoids the need for secondary calculations such as...

diazona said:
If I remember correctly, the moon's mass is 1/6 that of Earth, and it's radius is about 1/3 of the Earth's, so I guess the orbital velocity at a given (small) altitude is reduced by about a factor of 2...

Distance above the surface does not effect orbital dynamics, and I believe this would help the OP gain the understanding he seeks.
 
  • #11
LURCH said:
D H said:
That is contrary to the meaning of the term "altitude", which invariably means height above some reference surface.
Yes, I know. But what I'm asking is that we all refer to the distance above center of mass, because it removes an unnecessary complication, and avoids the need for secondary calculations such as...
diazona said:
If I remember correctly, the moon's mass is 1/6 that of Earth, and it's radius is about 1/3 of the Earth's, so I guess the orbital velocity at a given (small) altitude is reduced by about a factor of 2...
Distance above the surface does not effect orbital dynamics, and I believe this would help the OP gain the understanding he seeks.
Whatever makes you think that? Distance above the surface most definitely does affect orbital dynamics. Moreover, distance below the surface most definitely hinders orbital mechanics. A satellite could not orbit the Earth at the orbital radius corresponding to an orbital altitude of 100 km above the surface of the Moon because that orbital radius is well inside the Earth. A satellite can however orbit 200 km above the surface of the Earth or the Moon.

The problem with diazona's analysis was incorrect values for the Moon's mass and radius. So, let's do it correctly.

The orbital velocity for a circular orbit at altitude h is

[tex]v=\sqrt{\frac{GM}{R+h}}[/tex]

The ratio of the orbital velocities for orbits at the same altitude about the Earth and Moon is thus

[tex] \frac{v_e}{v_m} = \sqrt{\frac{M_e}{M_m}\,\frac{R_m+h}{R_e+h}}<br /> \approx \sqrt{\frac{Me}{Mm}\,\frac{R_m}{R_e}}\,\left(1+\frac h 2\,\frac{R_e-R_m}{R_eR_m}\right)[/tex]

Using the correct numbers, Mm/Me=0.0123 and Rm/Re=0.273, yields ve/vm=4.71 for h=0, increasing as altitude increases. The ratio is 5.15 for h=500 km, at which point the approximation is still valid to within about 1%.
 

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