Section 3: Work, Energy and Collisions Flashcards
If given L (the length of the cord in its relaxed state), 𝓶 (the mass of the jumper), the elastic constant K and the height (y) of the bridge from the jumper’s legs. How could one find distance (h) the jumper will be from the ground at the lowest point of the jump ?
We can start by setting up our Conservation of Energy Equation:
U₁ + K₁ = U₂ + K₂
We can eliminate K₁ since our initial velocity is 0, we can Convert K₂ into elastic energy since it is under elasticity after point L, we will then set the spring distance to (d) and solve for it first:
𝓶𝑔(y) = 𝓶𝑔(y - L - d) + ½Kd² → 𝓶𝑔(L + d) = ½Kd²
We can now solve for d using quadratic equation:
0 = ½Kd² - 𝓶𝑔d - 𝓶𝑔L
We can then use h = y - [L + d] to solve for the distance from the ground.
A small block with mass 𝓶 slides without friction around the loop-the-loop apparatus shown in the diagram. It is released from rest from point A (where its height is 4R higher than the bottom of the circular section, which has a radius R. At point B, it is at the same height as the center of the circle.
Find Velocity at point B
We can start by stating our Conservation of Energy equation:
U₁ + K₁ = U₂ + K₂
At point A we are at the full height 4R and at point B we are at R and our initial K cancels due to lack of initial velocity:
𝓶𝑔(4R) = 𝓶𝑔(R) + ½𝓶𝓥² → 𝓥 = √(𝑔[6R])
(A) What is the net force on Block A
(B) What is the acceleration of the system ?
(A) ΣFₐ = [𝓶ₐ𝑔 - T]
(B) 𝑔[𝓶ₐ - 𝓶𝔟]/[𝓶ₐ + 𝓶𝔟]
For objects near the surface of the Earth, the universal law of gravitation can be simplified to F = mg, where g = 9.81m/s².
(A) If the mass of the Earth were doubled while at the same time its radius remained constant, by what factor would this change its acceleration due to gravity at it’s surface?
(B) If the radius of Earth doubles ?
(A) Since our formula is GmM/R², we know the acceleration due to gravity will double
(B) Given the same formula, we know the radius will cause the acceleration to lower by 1/4th
What is the Equation to period of revolution (T) according to Keppler’s Law ?
T² = (4π²r³)/(GM)
The satellite has mass m and the Earth has mass M and radius R. In order to be geosynchronous, the satellite must be at a certain height H above the Earth’s surface.
How do you solve for H ?
We start knowing the equation to Period of Revolution given our known variables and replacing our r variable with the R and H values:
T² = (4π²r³)/(GM) → T² = (4π²[R +H]³)/(GM)
Now we can manipulate this equation to get the value of H:
T² = (4π²[R +H]³)/(GM) → H = ³√( T²GM/4π² ) - R
A box with a mass 𝓶 = 63kg is being pulled by a constant force F = 155N at an angle θ = 33°. The initial speed of the box is zero m/s.
What is an expression for the Work done on the Block ?
What is speed of block at d = 3.850m ?
(A) The work done can be found using Fcosθd
(B) Since we have 2 equations for work, we can set them equal and solve for Velocity:
Fcosθd = ½mv² → v = √(Fcosθd / ½m)
What is the conversion from Rotational Velocity (ω) to Linear Velocity (𝓥) ?
𝓥 = rω
What is equation of an angle (θ) relative to arch length (s) and radius (r) ?
θ = s/r
s = arch length
r = radius
If a Bird can Distinguish θ = 3x10⁻⁴rad from 100m away
(A) How many degrees is this
(B) How long is this in arc length ?
(A) θ = 3x10⁻⁴rad (180/π) = 0.0172°
(B) Since we know θ = s/r → rθ = s
[100m][3x10⁻⁴rad] = 0.03m
Two satellites orbit with radius of 4.23x10⁷m and 2.0° of seperation.
What is the arc length ?
First convert degrees to radians:
θ = 2.0° (π/180) = 0.0349rad
then use θ = s/r → rθ = s
[0.0349rad][4.23x10⁷m] = 1.48x10⁶m
What is the equation to Tangent acceleration from Rotational Variables ?
a_t = rα
What is the equation to Centripetal Acceleration from Rotational Variables ?
a_r = rω²
If an object moves 1 revolution in 4.0s around a 1.2m center at constant velocity. What is the Linear Velocity and Linear acceleration ?
Velocity = rω
ω = 1.0rev/4.0s = 2π/4.0s = 1.6rev/s
𝓥 = rω = [1.6rev/s][1.2m] = 1.92m/s
Acceleration = a_r = rω²; a_t = rα
a_t = 0
a_r = [1.2m][1.6rev/s]² = 3.1m/s²
What is equation to Torque (Շ) ?
Շ = r⟂F
where F is perpendicular to the moment of inertia.