Where is the Definition of Apsidal Vectors? Goldstein's Classical Mechanics Book

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SUMMARY

The term "apsidal vectors" is discussed in the context of central force problems and elliptical orbits in Goldstein's Classical Mechanics. The line of apsides connects the pericenter and apocenter of an elliptical orbit, serving as the major axis. The eccentricity vector, which has a magnitude equal to the eccentricity, points from the occupied focus to the pericenter. For further understanding, resources such as Wikipedia and celestial mechanics texts are recommended for additional context.

PREREQUISITES
  • Understanding of elliptical orbits in classical mechanics
  • Familiarity with central force problems
  • Knowledge of eccentricity vectors
  • Basic concepts of celestial mechanics
NEXT STEPS
  • Research the definition and properties of apsidal vectors in classical mechanics
  • Study the relationship between eccentricity vectors and orbital dynamics
  • Explore celestial mechanics texts for deeper insights into orbital trajectories
  • Review the Wikipedia page on the line of apsides for foundational knowledge
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Students of classical mechanics, astrophysicists, and anyone interested in the dynamics of elliptical orbits and central force problems will benefit from this discussion.

ehrenfest
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Homework Statement


My classical mechanics book (Goldstein) talks about apsidal vectors in the context of central force problems and elliptical orbits. I cannot find where the book defines this term and it is nowhere on the internet. Has anyone heard this term before?



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ehrenfest said:

Homework Statement


My classical mechanics book (Goldstein) talks about apsidal vectors in the context of central force problems and elliptical orbits. I cannot find where the book defines this term and it is nowhere on the internet. Has anyone heard this term before?

The line of apsides for an elliptical orbit joins the pericenter and apocenter of the orbit, i.e., it is the major axis. For open trajectories (parabolas and hyperbolas), it would still be the symmetry axis of the orbit. The eccentricity vector e, for example, has the magnitude of the eccentricity and points from the occupied focus to the pericenter. Here's a place to start: http://en.wikipedia.org/wiki/Apse_line ; Googling "apsidal vector" produces an avalanche, as does "line of apsides", but there are sites and books on the Web of some help. Celestial mechanics texts may also be useful to you.
 

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