Is it possible for one celestial body to trail another indefinetly?

  • Context: Undergrad 
  • Thread starter Thread starter MickN
  • Start date Start date
  • Tags Tags
    Body
Click For Summary
SUMMARY

In celestial mechanics, it is impossible for one body to trail another indefinitely under the influence of gravity without orbiting or crashing into it. When two bodies, with one significantly less massive than the other, are in mutual gravitational attraction, the smaller body will always accelerate towards the larger one. However, introducing a third massive body allows for configurations where the smaller body can trail the larger one while both orbit the central mass, specifically at the Lagrangian points L4 and L5, which are stable solutions.

PREREQUISITES
  • Understanding of gravitational forces and acceleration
  • Familiarity with celestial mechanics and orbital dynamics
  • Knowledge of Lagrangian points in astrodynamics
  • Basic concepts of mass and gravitational influence
NEXT STEPS
  • Research the properties and significance of Lagrangian points in orbital mechanics
  • Study the dynamics of three-body problems in celestial mechanics
  • Explore the effects of gravitational interactions in multi-body systems
  • Learn about the stability of orbits and perturbation theory in astrodynamics
USEFUL FOR

Astronomers, astrophysicists, and students of celestial mechanics interested in gravitational interactions and orbital stability.

MickN
Messages
8
Reaction score
0
In other words, are there any circumstances in which one object, captured by the gravity of another, would simply trail behind it indefinitely, instead of revolving around it or crashing into it? Is it possible? It seems reasonable to me that under certain circumstances it could happen, but someone tells me it's impossible, and that, except in the case of one object breaking up into several (like a commit breaking up), it can't happen.

Thanks
 
Astronomy news on Phys.org
As long as there are just two bodies under each other's gravitational influence, it's not possible.
Take a simplified scenario, where one of the bodies is much less massive(m) than the other(M), so that only the massive one attracts the light one. The m body will always feel the force of gravity, constantly accelerating towards M. To preserve the intial setup where both are at rest with respect to each other, you'd have to constantly keep pushing the body M away at the same rate as it pulls in the body m.

If you introduce a third massive body, that both M and m are orbiting, then you can get a class of solutions that is close to what you're asking for. Namely, M and m can follow one another as they orbit the central mass. In this case, the body m is at all times under the gravitational influence of M, as well as the central mass, so it can be said that it is trailing M.

These solutions are called the Lagrangian points.
300px-Lagrange_very_massive.svg.png

(the blue blob representing M, the red dot m)
Of these five points, only L4 and L5 are stable.

To reiterate, if by trailing you mean being affected by the gravity of another body but neither obiting it nor changing the distance to it, then L4 and L5 should do.

By the way, a comet(or any other body) breaking into parts will not stay in a static configuration indefinitely. Either the parts will move towards each other under mutual gravitational attraction, or move away from each other affected by whatever force caused the breakup in the first place(tidal forces for example).
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 86 ·
3
Replies
86
Views
9K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 21 ·
Replies
21
Views
6K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
17
Views
4K
  • · Replies 26 ·
Replies
26
Views
3K
  • · Replies 36 ·
2
Replies
36
Views
8K
Replies
13
Views
2K