Calculating perihelion |
We'll note right up front that Bagley managed to find an authoritative reference and somehow transcribe its content correctly (for the most part) while still meeting the infamous Demand Media minimum word count. Since the answer is actually quite straightforward when expressed as a formula, Soren had to convert it to words – lots of 'em – to meet MWC. Even so, he never actually gets around to explaining why his answer works. If he had, he would have said something to the effect of
"Perihelion and aphelion occur at the foci of an elliptical orbit. Perihelion occurs at the focus nearer the sun; aphelion occurs at the farther focus. The two points' distances from the sun can be calculated using the geometry of the ellipse."But Soren most likely didn't understand that. So instead, he just rattled off the process (as he understood it):
- Determine the semi-major axis of the orbit.
- Determine the eccentricity of the orbit.
- Subtract the ellipse's eccentricity from the number 1.
- Multiply the result of Step 3 by the result of Step 1.
"[divide] the length of the ellipse's major-axis [sic] by the distance between the ellipse's two foci..."...which, unfortunately, is wrong. The eccentricity of an ellipse is the ratio of c, the distance from the center to a focus; and a, the distance between the focus and the end of the semi-minor axis. A, then, is the hypotenuse of a triangle with sides c and b, where b is the semi-minor axis (see image above). Using the Pythagorean Theorem, then, the value Bagley actually needed is the square root of b² + c².
¹ aka "rocks for jocks"
² Leaf Group sent this one to one of their rewrite team. We might get to that one later...
² Leaf Group sent this one to one of their rewrite team. We might get to that one later...
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MM - ASTRONOMY
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