How Do Velocities Change in a Two-Dimensional Elastic Collision?

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Two shuffleboard disks of equal mass, one orange and the other yellow, are involved in an elastic, glancing collision. The yellow disk is initially at rest and is struck by the orange disk moving with a speed of 5.00 m/s. After the collision, the orange disk moves along a direction that makes an angle of 37.0 degrees with its initial direction of motion. The velocities of the two disks are perpendicular after the collision. Determine the final speed of each disk.

I have no idea where to start. I know I need to conservation of momentum and/or maybe conservation of energy, but I can't figure out how to set it up. Please help me out. Thanks.
 
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To solve this problem, we can use the principles of conservation of momentum and conservation of energy.

First, let's set up some variables:
- m = mass of each disk (since they are equal, we can use the same value for both disks)
- v1 = initial velocity of the orange disk (5.00 m/s)
- v2 = initial velocity of the yellow disk (0 m/s)
- v1f = final velocity of the orange disk
- v2f = final velocity of the yellow disk
- θ = angle between the initial direction of motion of the orange disk and its final direction of motion (37.0 degrees)

Now, let's apply the conservation of momentum principle:
m * v1 + m * v2 = m * v1f + m * v2f

Since the yellow disk is initially at rest, its initial velocity (v2) is equal to 0. Therefore, we can simplify the equation to:
m * v1 = m * v1f + m * v2f

Next, we can use the conservation of energy principle, which states that the total kinetic energy before the collision is equal to the total kinetic energy after the collision. The kinetic energy of an object can be calculated using the formula KE = (1/2) * m * v^2.

So, the total kinetic energy before the collision is:
KE1 = (1/2) * m * v1^2

And the total kinetic energy after the collision is:
KE2 = (1/2) * m * v1f^2 + (1/2) * m * v2f^2

Since this is an elastic collision, the total kinetic energy before and after the collision should be equal. Therefore, we can set up the following equation:
KE1 = KE2

Substituting the values for KE1 and KE2, we get:
(1/2) * m * v1^2 = (1/2) * m * v1f^2 + (1/2) * m * v2f^2

Simplifying and rearranging the equation, we get:
v1^2 = v1f^2 + v2f^2

Now, we can use the fact that the velocities of the two disks are perpendicular after the collision to solve for v1f and v2f. This means that we can use the