Kepler's 2nd.law and calculation

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Kepler's Second Law relates to the conservation of angular momentum, where the area swept out by a planet in its orbit is proportional to the time taken. The area of a triangle can be calculated using the formula 1/2 base x height, with the base defined as the arc length (dx) and height (h). For elliptical orbits, the relationship between radius (r), arc length (ds), and speed (v) is crucial, particularly at the ends of the major axis. However, at other points in the orbit, the angle between r and ds requires the inclusion of a sine or cosine factor for accurate area calculation. Understanding these nuances is essential for correctly applying Kepler's Second Law in various orbital scenarios.
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Hello,

While dealing with Kepler's 2nd.law, when calculating the area of the triangle which sweeps out:


Area of a triangle = 1/2 base x height

Now, we know dθ = dx/r (where dx = arc length, r=radius)

So, dx= rdθ

So, area of a triangle = 1/2 base(rdθ) x height(h)

Is this correct?

Thanks
 
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If dx is defined to be something like an "arc length in tangential direction", yes. It is not the actual arc length if the motion is not circular.
 
Keep in mind that Kepler's Second Law is just another way of saying that angular momentum is conserved. In other words, ##\omega r^2## is a constant. Keeping in mind that for a small section h = r, this is in agreement with what you wrote.
 
Thank you very much for letting me clear the confusion.
 
Hope I'm not going to regenerate the confusion, but for an elliptical orbit there are just two places where the triangle area is given by \frac{1}{2} r\ ds = \frac{1}{2} rv\ dt, and those are the two ends of the major axis. [I'm using ds as infinitesimal portion of arc length, r as distance from focus and v as speed of orbiting body.]

At every other point, r and ds are not perpendicular to each other, so a sine or cosine factor has to be inserted.
 
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