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  2. Newton's laws of motion - Wikipedia

    en.wikipedia.org/wiki/Newton's_laws_of_motion

    In the absence of a net external force, the center of mass moves at a constant speed in a straight line. This applies, for example, to a collision between two bodies. [49] If the total external force is not zero, then the center of mass changes velocity as though it were a point body of mass . This follows from the fact that the internal forces ...

  3. Specific force - Wikipedia

    en.wikipedia.org/wiki/Specific_force

    Specific force (SF) is a mass-specific quantity defined as the quotient of force per unit mass. S F = F / m {\displaystyle \mathrm {SF} =F/m} It is a physical quantity of kind acceleration , with dimension of length per time squared and units of metre per second squared (m·s −2 ).

  4. Force - Wikipedia

    en.wikipedia.org/wiki/Force

    The SI unit of force is the newton (symbol N), which is the force required to accelerate a one kilogram mass at a rate of one meter per second squared, or kg·m·s −2.The corresponding CGS unit is the dyne, the force required to accelerate a one gram mass by one centimeter per second squared, or g·cm·s −2. A newton is thus equal to ...

  5. Mass versus weight - Wikipedia

    en.wikipedia.org/wiki/Mass_versus_weight

    Thus the kilogram-force is defined as precisely 9.80665 newtons. In reality, gravitational acceleration (symbol: g) varies slightly with latitude, elevation and subsurface density; these variations are typically only a few tenths of a percent. See also Gravimetry. Engineers and scientists understand the distinctions between mass, force, and weight.

  6. Torricelli's equation - Wikipedia

    en.wikipedia.org/wiki/Torricelli's_equation

    is the object's acceleration along the x axis, which is given as a constant. Δ x {\displaystyle \Delta x\,} is the object's change in position along the x axis, also called displacement . In this and all subsequent equations in this article, the subscript x {\displaystyle x} (as in v f x {\displaystyle {v_{f}}_{x}} ) is implied, but is not ...

  7. Centripetal force - Wikipedia

    en.wikipedia.org/wiki/Centripetal_force

    By Newton's second law, the cause of acceleration is a net force acting on the object, which is proportional to its mass m and its acceleration. The force, usually referred to as a centripetal force , has a magnitude [ 7 ] F c = m a c = m v 2 r {\displaystyle F_{c}=ma_{c}=m{\frac {v^{2}}{r}}} and is, like centripetal acceleration, directed ...

  8. Proper acceleration - Wikipedia

    en.wikipedia.org/wiki/Proper_acceleration

    The total (mechanical) force that is calculated to induce the proper acceleration on a mass at rest in a coordinate system that has a proper acceleration, via Newton's law F = ma, is called the proper force. As seen above, the proper force is equal to the opposing reaction force that is measured as an object's "operational weight" (i.e. its ...

  9. Orders of magnitude (acceleration) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude...

    Acceleration of Earth toward the sun due to sun's gravitational attraction 10 −1: 1 dm/s 2: lab 0.25 m/s 2: 0.026 g: Train acceleration for SJ X2 [citation needed] 10 0: 1 m/s 2: inertial 1.62 m/s 2: 0.1654 g: Standing on the Moon at its equator [citation needed] lab 4.3 m/s 2: 0.44 g: Car acceleration 0–100 km/h in 6.4 s with a Saab 9-5 ...

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