Mechanics Flashcards
Conditions for Static Equilibrium
The sum of both the forces and the moments acting on the body must be equal to zero.
Kepler’s 1st Law
All planets move in elliptical orbits with the Sun at one focus.
Kepler’s 2nd Law
A line joining any planet to the Sun sweeps out equal areas in equal times.
Kepler’s 3rd Law
The square of the period of any planet is proportional to the cube of semi-major axis of its orbit.
Conservative Force
Is a force with the property that the total work done in moving a particle between two points is independent of the path taken. Equivalently, if a particle travels in a closed loop, the total work done by a conservative force is zero.
Newton’s 1st Law
An object at rest stays at rest unless acted on by an external force.
Newton’s 2nd Law
F = ma
Newton’s 3rd Law
F_BA = - F_AB
4 Fundamental Forces
- Gravitational interaction
- Electromagnetic interaction
- Weak interaction
- Strong nuclear interaction (hadronic force)
Mechanical Energy
The sum of the kinetic and potential energies of a system
Total Energy of a System
The energy of a system consists of: mechanical energy, thermal energy, chemical energy and other types of energy - such as sound radiation and electromagnetic radiation.
Binding Energy
The energy required to separate a bound system into its constituent parts is called its binding energy. The binding energy is dM*c^2
Law of Conservation of Momentum
If the net external force acting on a system remains zero, the total momentum of the system is conserved.
Impulse
The impulse of a force is the integral of the force over the time interval during which the force acts
Elastic Collisions
The sum of the kinetic energies is the same before and after the collision.