Files
blog/content/Formulas.md
2026-03-31 02:07:49 -05:00

3.0 KiB
Raw Blame History

#public

Work and energy

Formula equation Usage
Gravitational Potential Energy (U_g) U_g=mgh Changes in height
Kinetic Energy K=\frac{1}{2}mv^2 Energy of motion
Work-Energy Theorem \Delta E_{mec} = \Delta K+\Delta U=W_{other}* calculating the effects of friction
Variable Symbol SI Unit Notes
Mass m kg Convert from grams (g) if necessary.
Height / Distance h,d m Measures vertical or horizontal displacement.
Velocity / Speed v m/s Convert from km/h by dividing by 3.6.+3
Gravity g m/s2 Earth's standard is approximately 9.8 m/s2.
Energy / Work U_g,K,W J 1 Joule = 1 kg⋅m2/s2.

Center Of Mass (CM)

Formula equation Usage
Position of COM X x_{com}=\frac{1}{M}\sum_{i=1}^{n}M_ix_i find COM X
Position of COM Y y_{com}=\frac{1}{M}\sum_{i=1}^{n}M_iy_i find COM Y
velocity of COM v_{com}=\frac{\sum m_iv_i}{M} find the Velocity of COM
Variable Symbol SI Unit Notes
Position (X or Y) x_{com},y_{com} m Coordinates on the Cartesian plane.+ 1
Total Mass M kg The sum of all individual masses (m1+m2+…)
Velocity of CM vcom m/s The speed at which the entire system's balance point moves

Linear Momentum and impulse

Formula equation Usage
Linear Momentum p = mv find linear momentum
Impulse J=\Delta p=F_{avg}\Delta t=\int F(t)dt change in momentum. Also area under Force-time graph
Conservation Law P_{initial}=P_{final} if net external force is 0, totoal momentum is constant
Elastic Collisions (1D) v_{1f}=(\frac{m_1-m_2}{m_1+m_2})v_i+(\frac{2m_2}{m_1+m_2})v_2i momentum and kinetic energy are conserved
completely inelastic collisions m_1v_{1i}+m_2v_{2i}=(m_1+m_2)v_f find situation where the objects stick together
Variable Symbol SI Unit Notes
Momentum p kg⋅m/s Calculated as mass × velocity.
Impulse J N⋅s Also equivalent to kg⋅m/ s.
Force F N 1 Newton = 1 kg⋅m/s2.+2
Time t,$\Delta$t s The duration of the force application.+1