Kepler's 2nd.law and calculation

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In summary, Kepler's Second Law states that angular momentum is conserved, expressed as ##\omega r^2## being a constant. This is reflected in the equation for the area of a triangle swept out by a body in orbit, which is given by 1/2 base x height. However, for an elliptical orbit, there are only two points where this equation holds true, as at every other point, a sine or cosine factor must be included to account for the non-perpendicularity of r and ds.
  • #1
shounakbhatta
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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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  • #2
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.
 
  • #3
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.
 
  • #4
Thank you very much for letting me clear the confusion.
 
  • #5
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 [itex]\frac{1}{2} r\ ds = \frac{1}{2} rv\ dt[/itex], 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.
 

What is Kepler's 2nd law?

Kepler's 2nd law, also known as the law of equal areas, states that a line that connects a planet to the sun sweeps out equal areas in equal time intervals. This means that a planet moves faster when it is closer to the sun and slower when it is farther away.

How is Kepler's 2nd law calculated?

Kepler's 2nd law can be calculated using the formula A = (1/2)bh, where A is the area swept out by the planet, b is the base of the triangle formed by the planet's position, and h is the height of the triangle. This formula can be used to calculate the area for different time intervals and confirm the law.

What is the significance of Kepler's 2nd law?

Kepler's 2nd law is significant because it helps us understand the motion of planets in our solar system and beyond. It also played a crucial role in the development of Isaac Newton's laws of motion and the law of universal gravitation.

How does Kepler's 2nd law relate to the orbit of a planet?

Kepler's 2nd law relates to the orbit of a planet by describing the speed at which a planet moves along its elliptical orbit around the sun. This law states that a planet will move faster when it is closer to the sun and slower when it is farther away, resulting in an equal area being swept out in equal time intervals.

Can Kepler's 2nd law be applied to other objects in space?

Yes, Kepler's 2nd law can be applied to other objects in space that follow an elliptical orbit around a central body. This includes comets, moons, and other celestial bodies. However, it may not be applicable to objects with highly irregular orbits or those influenced by external forces.

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