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

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Homework Help Overview

The problem involves determining the ratio of the semi-major axes of two planets orbiting a star, based on the angular distance observed from one planet to another. The context is set in an astronomical scenario where one planet observes another within the same solar system.

Discussion Character

  • Exploratory, Assumption checking, Conceptual clarification

Approaches and Questions Raised

  • Participants discuss visualizing the scenario and the implications of the observed angle. There are attempts to apply trigonometric relationships to find the ratio of the semi-major axes, with some questioning the relevance of circular versus elliptical orbits.

Discussion Status

The discussion is ongoing, with participants exploring different interpretations of the problem. Some guidance has been offered regarding the relationship between radius and semi-major axis in circular orbits, while concerns about elliptical orbits and their complexities have also been raised.

Contextual Notes

There is a mention of potential complications arising from elliptical orbits and the alignment of perihelion directions, which may affect the observed angular size and the interpretation of the problem.

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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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