Two-body Kepler problem where the Sun is at rest in a coordinate system orbited by another body

Click For Summary
SUMMARY

The discussion centers on the two-body Kepler problem with the Sun at rest in a coordinate system orbited by another body. It concludes that the coordinate system is non-inertial due to the Sun being affected by gravitational forces, specifically Newton's third law. The barycentric frame, where both bodies orbit their common center of mass, is identified as inertial. The conversation emphasizes the importance of understanding reduced mass and relative coordinates for accurate solutions in binary star systems.

PREREQUISITES
  • Understanding of Newton's laws of motion, particularly Newton's third law
  • Familiarity with the concepts of inertial and non-inertial reference frames
  • Knowledge of the barycentric frame of reference in celestial mechanics
  • Basic principles of the two-body problem in orbital mechanics
NEXT STEPS
  • Study the concept of reduced mass in two-body problems
  • Learn about the barycentric coordinates and their applications in celestial mechanics
  • Explore Newton's laws of motion in the context of gravitational interactions
  • Investigate the mathematical formulation of the two-body problem and its solutions
USEFUL FOR

Astronomy students, physicists, and anyone interested in celestial mechanics and orbital dynamics will benefit from this discussion.

DrToby
Messages
5
Reaction score
1
The two-body Kepler problem where the Sun is at rest in a coordinate system orbited by another body: is the coordinate system an inertial reference system or not? Please no yes/no answers. A bit of elaboration is appreciated towards why and which principles apply.
 
Physics news on Phys.org
If the Sun is at rest, you are using the Sun's rest frame. Is the Sun affected by any forces that might make it accelerate?
 
Suppose the other body has the same mass as the sun, as in e.g. a binary star system. Would you expect either body to be at rest in an inertial coordinate system?
 
  • Like
Likes   Reactions: Ibix
The Sun is orbited by another mass. The origin of a coordinate system is placed at the center of the Sun. The Sun pulls on the mass with a given force. According to Newtons third law the Sun is pulled towards the mass with an equal force. Hence the coordinate system is accelerated and hence it must be a non-inertial coordinate system. An inertial coordinate system is defined as a system for which Newtons 1. law is valid. Is all this reasoning correct?
 
DrToby said:
An inertial coordinate system
Called the Center Of Mass frame of reference. The same trick is used to reduce many two body problems to modified "one body" ones
 
DrToby said:
Is all this reasoning correct?
Yes.

The barycentre is the point about which both Sun and planet orbit. The barycentric frame is inertial, and the barycentre is one of the foci of the ellipses of both bodies' orbits.
 
Thank you for confirmation. Nice to find people to discuss stuff with.
 
  • Like
Likes   Reactions: hutchphd
The problem you describe is not what you want . It is an approximation for very disparate masses. The usual exact solution involves reduced mass and relative coordinates, and the sun is not at rest in the chosen coordinate system. It would be good to read carefully all previous answers as well as any good freshman text.
 

Similar threads

  • · Replies 3 ·
Replies
3
Views
2K
Replies
1
Views
2K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 86 ·
3
Replies
86
Views
8K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 13 ·
Replies
13
Views
3K
  • · Replies 7 ·
Replies
7
Views
3K