Òfin ìfàmọ́ra àgbáláayé Newton

Isiseero ogbologbo

$\mathbf{F} = \frac{\mathrm{d}}{\mathrm{d}t}(m \mathbf{v})$ Òfin Kejì Newton

History of classical mechanics · Timeline of classical mechanics Branches Statics · Dynamics / Kinetics · Kinematics · Applied mechanics · Celestial mechanics · Continuum mechanics · Statistical mechanics Formulations Ìṣiṣẹ́ẹ̀rọ Newton (Vectorial mechanics) Analytical mechanics: Lagrangian mechanics Hamiltonian mechanics Fundamental concepts Ààyè · Àsìkò · Velocity · Speed · Àkójọ · Acceleration · Gravity · Ipá · Impulse · Torque / Moment / Couple · Momentum · Angular momentum · Inertia · Moment of inertia · Reference frame · Energy · Kinetic energy · Potential energy · Mechanical work · Virtual work · D'Alembert's principle Core topics Rigid body · Rigid body dynamics · Euler's equations (rigid body dynamics) · Motion · Àwọn òfin ìṣípòpadà Newton · Òfin ìfàmọ́ra àgbáláayé Newton · Equations of motion · Inertial frame of reference · Non-inertial reference frame · Rotating reference frame · Fictitious force · Linear motion · Mechanics of planar particle motion · Displacement (vector) · Relative velocity · Friction · Simple harmonic motion · Harmonic oscillator · Vibration · Damping · Damping ratio · Rotational motion · Circular motion · Uniform circular motion · Non-uniform circular motion · Centripetal force · Centrifugal force · Centrifugal force (rotating reference frame) · Reactive centrifugal force · Coriolis force · Pendulum · Rotational speed · Angular acceleration · Angular velocity · Angular frequency · Angular displacement Scientists Isaac Newton · Jeremiah Horrocks · Leonhard Euler · Jean le Rond d'Alembert · Alexis Clairaut · Joseph Louis Lagrange · Pierre-Simon Laplace · William Rowan Hamilton · Siméon-Denis Poisson

The mechanisms of Newton's law of universal gravitation; a point mass m₁ attracts another point mass m₂ by a force F₂ which is proportional to the product of the two masses and inversely proportional to the square of the distance (r) between them. Regardless of masses or distance, the magnitudes of |F₁| and |F₂| will always be equal. G is the gravitational constant.

Òfin ìfàmọ́ra àgbáláayé ti Newton