How Does the Mass of a Moon Affect Its Orbital Speed Around a Planet?

  • Context: Undergrad 
  • Thread starter Thread starter Hasan Ribin
  • Start date Start date
  • Tags Tags
    Mass Speed
Click For Summary
SUMMARY

The mass of a moon significantly affects its orbital speed around a planet, particularly when considering the gravitational interactions between the two bodies. The formula for acceleration is given by GMplanet/L², where G is the gravitational constant, Mplanet is the mass of the planet, and L is the distance between the moon and the planet. Additionally, the orbital speed is determined by centripetal acceleration, expressed as v²/R, where R is the distance from the center of mass. Changes in the moon's mass will alter the center of mass, thereby affecting the distance R and consequently the orbital dynamics.

PREREQUISITES
  • Understanding of gravitational forces and Newton's laws of motion
  • Familiarity with orbital mechanics and centripetal acceleration
  • Knowledge of the gravitational constant (G) and its application
  • Basic mathematical skills for manipulating formulas related to motion
NEXT STEPS
  • Study the implications of the two-body problem in celestial mechanics
  • Learn about the concept of center of mass and its calculation in multi-body systems
  • Explore the effects of varying mass on orbital stability and dynamics
  • Investigate the mathematical derivations of Kepler's laws of planetary motion
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in understanding the dynamics of celestial bodies and their orbits.

Hasan Ribin
Messages
3
Reaction score
0
Hi. Tell me pls how does the mass of moons effect their speed around planets?
I know that in case of satellites their speeds depend on planet Mass and ٌ R+h only (R is a radius of the planet and h is satellite's height from the planet surface), but in that case we do not measure satellites' mass because of its insignificance.. But if a satellite for instance has the same mass as the Moon, we should take into account its gravitational effect to the planet as well I guess.. Please help (and if it is possible - with necessary formula). Thanks ))

P.S.: Sorry for English.. Long time without practice :)

I've also added that question http://http://answers.yahoo.com/question/index?qid=20110525032837AAL59Xi" , maybe someone wishes to answer on the site
 
Last edited by a moderator:
Physics news on Phys.org
Welcome to PF!

Hi Hasan! Welcome to PF! :smile:

The acceleration of the moon depends only on the distance L between the moon and the planet: GMplanet/L2.

The speed of the moon depends on the distance R of the moon from the centre of mass (assuming a circular orbit): centripetal acceleration = v2/R.

The rest of the calculation I'll leave to you. :wink:
 
Thanks ))

The acceleration of the moon depends only on the distance L between the moon and the planet: GMplanet/L2.

Yeah.. that is what I tried to talk about but.. You mean that if we reduce the Moon's mass, say, to 3.5 × 10^22 kg but the distance between the Earth's and the Moon's mass centers leave the same there will be no changes regarding its velocity during moving around the planet? I mean the orbital period of the Moon will remain about 27 days?

I thought it is right only for planet sattelites or planets within solar system because their mass is negligible relative to the sun or other globes they are moving around.. But what if the mass of a sattelite or a moon is insignificantly different from the globe it is moving around? Say, the Moon and the Earth.. (or if we significantly in- decrease the Moon mass )?
 
Hi Hasan! :smile:
Hasan Ribin said:
You mean that if we reduce the Moon's mass, say, to 3.5 × 10^22 kg but the distance between the Earth's and the Moon's mass centers leave the same there will be no changes regarding its velocity during moving around the planet? I mean the orbital period of the Moon will remain about 27 days?

No, because the speed depends on both L and R, and if you change the mass of the moon, then the position of the centre of mass changes, ie R changes.
 
if you change the mass of the moon, then the position of the centre of mass changes, ie R changes.

Ok, thank you very much, now I see.. Dear, would you explain this stuff as well please? How does the position change, I guess that the more mass moves the Moon closer to the center of mass, is there anything that this prosess depend on also? How to calculate it?
 

Similar threads

Replies
1
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
9
Views
4K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
17
Views
4K
  • · Replies 5 ·
Replies
5
Views
8K
  • · Replies 1 ·
Replies
1
Views
3K