Solving Planet A's Semi-Major Axis Ratio To Planet B's

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SUMMARY

The discussion centers on calculating the ratio of the semi-major axis of Planet A to that of Planet B, given that Planet A never appears more than 16 degrees from the star they both orbit. The solution involves using trigonometric principles, specifically the sine function, to establish the relationship between the radii of the orbits. For circular orbits, the radius is equivalent to the semi-major axis, simplifying the calculation. The complexity increases when considering elliptical orbits, where the alignment of perihelion directions affects the observed angular size.

PREREQUISITES
  • Understanding of basic trigonometry, specifically sine functions.
  • Familiarity with orbital mechanics, particularly circular and elliptical orbits.
  • Knowledge of celestial geometry and angular measurements.
  • Concept of semi-major axis in the context of planetary orbits.
NEXT STEPS
  • Study the principles of celestial mechanics and orbital dynamics.
  • Learn about the mathematical treatment of elliptical orbits.
  • Explore the application of trigonometry in astronomy, particularly in angular measurements.
  • Investigate the effects of perihelion alignment on orbital calculations.
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in understanding planetary motion and orbital mechanics.

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Homework Statement


You are one of the first astronomers in a civilization on Planet B in another solar system. With your unaided eye, you follow planet A in the same solar system and note that it never gets further away than 16 degrees from the star (around which both planets orbit).

What is the ratio of the size of Planet A's semi-major axis
to that of Planet B?


Homework Equations





The Attempt at a Solution



I seem to have trouble visualizing this scenario and so I don't know how to approach the problem...
 
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Sketch a star and the orbits of two planets in circular motion. With such a small angle, we must be on the planet of the larger circle; mark its position anywhere on the circle. Mark the points where the inner planet will appear furthest away from the star. With a bit of trigonometry you should be able to find the answer.
 
Would it be sin(16) = Ra/Rb
I know that gives that the ratio of the radius' but I'm not to sure how to find the semi-major axis
 
For circular orbits, the radius IS the semi-major axis.
Perhaps the use of the term implies you are to consider elliptical orbits. I suspect that would result in the same answer.
 
Delphi51 said:
For circular orbits, the radius IS the semi-major axis.
Perhaps the use of the term implies you are to consider elliptical orbits. I suspect that would result in the same answer.

It gets quite a bit more complicated when the orbits are elliptical and the perihelion directions are not aligned (the major axes are not collinear). Mutual distance plays a big role in the observed angular size, and the "width" of the orbit varies with viewing angle.
 

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