How is the magnitude of L calculated here?

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SUMMARY

The magnitude of angular momentum (L) is calculated using the vector equation L = r × mv, where r is the position vector, m is mass, and v is velocity. The formula for the magnitude is |L| = m |r| |v| sin(θ), with θ being the angle between the vectors. In this context, when the Earth moves in a straight line after the Sun disappears, the angular momentum remains constant and is expressed as |L| = m |v| d, where d is the Earth's orbital distance. Understanding the use of the sine function in the equation is crucial for grasping the conservation of angular momentum.

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Benjamin_harsh
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Homework Statement
How magnitude of L is calculated here?
Relevant Equations
How magnitude of L is calculated here?
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The green dot shows the position of the Earth at the instant the Sun disappears. The distance from the Sun, ##d##, is the Earth's orbital distance and the velocity ##v## is the Earth's orbital velocity.

When the Sun disappears the Earth heads off in a straight line at constant velocity as shown by the horizontal dashed line, so after some time ##t## it has moved a distance ##x = vt## as I've marked on the diagram. The question is now how the angular momentum can be conserved.

The answer is that angular momentum is given by the vector equation:

## \mathbf L = \mathbf r \times m\mathbf v ##

where ##\mathbf r## is the position vector, ##\mathbf v## is the velocity vector and ##\times## is the cross product. We are going to end up with the vector ##\mathbf L## pointing out of the page and the magnitude of ##L## is given by:

## |\mathbf L| = m\,|\mathbf r|\,|\mathbf v|\,\sin\theta \tag{1} ##

but looking at our diagram we see that:

## \sin\theta = \large\frac{d}{|\mathbf r|} ##

and if we substitute this into our equation (1) for the angular momentum we get:

## |\mathbf L| = m\,|\mathbf r|\,|\mathbf v|\,\large\frac{d}{|\mathbf r|}\normalsize = m\,|\mathbf v|\,d \tag{2} ##

And this equation tells us that the angular momentum is constant i.e. it depends only on the constant velocity ##\mathbf v## and the original orbital distance ##d##.

I didn't understand how ##|\mathbf L| = m\,|\mathbf r|\,|\mathbf v|\,\sin\theta## is written? Why ##sin## instead of ##cos## or ##tan##?

I only know one formula for angular momentum; ##L = mvr##.
 
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Benjamin_harsh said:
I didn't understand how |L|=m|r||v|sinθ is written?
Do you mean, how they get to that equation?
It follows from the nature of the cross product, ##|\vec x\times\vec y|=|x| |y||\sin(\theta)|##, where ##\theta## is the angle between the vectors.
 
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Benjamin_harsh said:
Problem Statement: How magnitude of L is calculated here?
Relevant Equations: How magnitude of L is calculated here?

I only know one formula for angular momentum; L=mvrL=mvrL = mvr.
This is only true in special cases.
The general form is L=m r x v where x is the vector cross product, which has
haruspex said:
$$|\vec x\times\vec y|=|x| |y||\sin(\theta)|$$
 
Why we have to use vectors here?

Can't we derive Earth's angular momentum without vectors?
 
Benjamin_harsh said:
Why we have to use vectors here?

Can't we derive Earth's angular momentum without vectors?
You will have to learn about vectors when you get to high school anyways.

You can do it with NOT THINKING about vectors but you are still imolicitly using L= mr x v
 

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