## FANDOM

742 Pages

this is where all known calcs for Kinetic Energy measurements can be found.

## Blast Wave

this section is for feats that creates blast waves,  using G.I. Taylor’s Ideal blast wave formula.

E = (ρ/t^2)*(r/c)^5

• C = dimensionless constant (1-1.1)
• ρ = 1.225 kg/m^3 (Density of Air)
• t = seconds (The time needed for the shockwave to travel the radius.)

## Cloud Splitting

To find the Energy to split clouds for any feat, we use the following to find the factors for the equation.

• Height of the Clouds size (an Cumulonimbus cloud is 12000 meters high)
• the Density of the clouds. (average density is 1.003 Kg/m^3)
• the radius (Width of a Cloud/2)
• the Time. (estimate the time needed to take to do this via time frames)

Once you find that info, use the following equation to find the kinetic energy:

• After that, divide it by two to get the end result.

Here are some sources to better find the measurements you need.

## Force via Angular Degree

This is to find the force of something that flies up to a certain degree, to find that you need for find a few things.

• Distance between point A to B (meters)
• Angle in degrees.
• initial velocity (Link in m/s)
• Weight (kg)
• Kinetic energy (kg*m/s^2*.5)
• Momentum (kg*m/s)
• Force (momentum / m/s)

NOTE: here is the link for the Punch that lasts less than 60ms.

## Fluid Pressure and Cross Section

This part is where we will find the wind pressure of a feat that would be applied for another Kinetic Energy calculation method, first we would need to use the Bernoulli's principle, which states that the minimum pressure decrease required to move an object is given by the formula:

P1 + 0.5 * ρ * v12 + h1ρg = P2 + 0.5 * ρ * v22 + h2ρg

What I want to find here is the value of 'V', for this we have that, the pressure is always greater than the mass of the object moved.

Cross-sectional area of ​​cylinder, you can use this section to find the equation for various shapes.

## Kinetic Energy

This part is to talk about how to find the kinetic energy of a feat when it comes to how much force is pushed onto an object, here is the equation below.

This can be used for objects crashing into other objects, punches, kicks, etc..

KE=1/2*m*v^2

The units of the equation are as followed

• KE = Kinetic Energy
• m = mass (kg)
• v = velocity (m/s)

When Solved, to convert the KE to Joules is as follows (1J = 1kg m^2/s^2)

1. Find the wait of any object in question by grams (g), convert it to kilograms (kg) 1 kg = 1000 g
2. Find velocity which is speed = distance/time (m/s)
3. Then plug all those into the formula above.

This calculator is good for standard measurements such as weapons, guns, etc..

NOTE: This can be used for Tsunami, Sandstorm, Tornado, Volcanic Eruptions Feats as well

### Other Units for Conversion

In this section we will be talking about how to convert other sets of units such as Pressure to Kinetic Energy in a unique way. For this we will be using Pascals.

Sample Ivan Drago Feat.

• Force=Pressure(Pa)*Surface Area(cm^2)
• F=N
• Then find the Distance between impactor and the target (cm)
• Then find time which is the square root (2) *Distance*Mass/Force
• then find velocity (m/s) which is Force*Time/Mass
• after that, multply the mass with the velocity
• Finally add the Velocity and Mass of hand to the KE formula at the beginning to get results.

## Meteor

This is to calculate the meteor impact that is or would have happened to find the stat for DC.

This involved the following factors:

• Speed (over 11 km/s if in space, lower if from the atmosphere of the planet)
• Size
• Density of Projectile (average density of the meteor is 3500 kg/m^3)
• Density of Target
• Location of Impact
• TimeFrame

Optional (though not necessary)

• Trajectory
• Distance

You can use the following for reference or calculator simplification.

Or just go with the simple equation of:

• KE=0.5*Mass*Speed^2

NOTE: The Hemisphere usage without seeing it should be to multiply the diameter of the crater by .13 to get the depth.

• Here is the calc for finding the energy from the crater.

## Relativity

This is the page that talks about calculating relativistic mass.

### Explanation

This calculation is to talk about the energy in an object that moves at a certain velocity, relativistic speed is when an object that accelerates at or near the speed of light.

### Method 1

This link here a method to find the energy of relativistic mass.

• m = relativistic mass (1.2e30 kg = to .6 solar mass)
• m0 = rest mass (Targeted object's mass, ex 5kg)
• v = m's velocity (under speed of light "99,792,000 m/s")
• c = constant vacuum of speed of light. (300,000,000 m/s, or near SoL 299792458.044 m/s)

The value for velocity changes, this one is from plugging in the values to the 2.4e29 * √ (1 - v² / 300000000^2) but solved in a different manner.

### Method 2

Another method is finding the kinetic energy which is this:

KE = E - Eo

• m{rel} = γ*m^o
• m{re}/m^o = γ
• (γ-1)*mc^2
• 2.4*10^29 ratio, which is the Lorentz factor γ
• m is rest mass, ex. 5 kg
• c is constant vacuum of light speed