Kepler's 2nd.law and calculation

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The discussion focuses on the application of Kepler's Second Law in calculating the area swept by a triangle during orbital motion. The formula for the area of a triangle is correctly represented as 1/2 base times height, where the base is defined as rdθ, with dx representing the arc length. The conversation emphasizes that Kepler's Second Law reflects the conservation of angular momentum, specifically stating that ωr² remains constant. Additionally, it clarifies that for elliptical orbits, the area calculation requires adjustments for non-perpendicular relationships between r and ds.

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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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