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Classical physics

Gravity

Based on meticulous mathematical evaluation of astronomical observations, Kepler discovered in the early 17th century laws that for the first time correctly described the motion of planets around the Sun. Kepler's laws are: 1. the planetary orbits are ellipses; 2. the line joining Sun and planet sweeps equal areas in equal time; and 3. the square of the orbital period is proportional to the cube of the orbit’s semi-major axis. It took about 100 years until the genius of Newton presented a comprehensive physical explanation with his laws of motion and gravitation [1] . It then became evident that Kepler’s second law is a consequence of the conservation of angular momentum and the third law reflects the equilibrium of gravitational and centrifugal forces. Kepler’s and Newton’s discoveries allow accurate calculation and prediction of celestial orbits and events, as well as of trajectories of artificial satellites and space vehicles. However, despite the formulas’ astounding accuracy and immense usefulness, puzzling questions of why and how matter (or mass) causes gravity remain unanswered.

Classical mechanics

Newton formulated the relation between a body’s mass and its movement in his famous three laws of motion. Simplified, they describe: 1. inertia - without a force, a body is either at rest or moves with constant velocity; 2. force - equals mass times acceleration (or change of momentum); and 3. reaction - every force occurs together with an equal force in opposite direction. These simple and most powerful laws revolutionized physics [2] . Many physical quantities, including work, power, kinetic and potential energy, are directly related to Newton's laws [3] . Kinematics and dynamics explain many natural phenomena, including microscopic motions and oscillations and waves, and provide analytical tools in many areas of physics, including acoustics, thermodynamics, and even atomic, nuclear and particle physics .

Oscillations and waves

In an oscillation, physical quantities change periodically. A sine function describes the displacement motion of a simple harmonic oscillator. Amplitude, velocity (first time derivative) and acceleration (second time derivative) equally follow harmonic changes (described by sine and cosine functions) [4] . Any number of sine functions with different frequencies, amplitudes, and phases can be combined by superposition to result in any periodic functions. Reversely, any periodic function can be decomposed into basic sine/cosine functions by Fourier transformation [5] . Waves are oscillations that move forward in space. The momentary amplitude is not only a function of time but also of distance [6] . The wave’s speed of propagation depends on the stiffness (resistance to deformation) and the density of the medium through which it travels. The momentary displacement caused by a wave can be transversal (perpendicular to the direction of the wave’s propagation) or longitudinal (in direction of the wave’s propagation) [7] . Reflexion, refraction, diffraction, and interference are phenomena associated with waves [8] . Electromagnetic waves propagate also in vacuum, i.e. in 'free space' without the presence of any carrier medium (see also Speed of light). An even weirder type of waves are de Broglie’s matter waves.

Thermodynamics

The ideal gas law defines the relation between pressure, volume, and temperature of a gas, i.e., the product of pressure and volume (a mechanical work quantity) is proportional to the absolute temperature, where the gas constant is the proportionality factor. The law, originally derived from empirical evidence, is central to thermodynamics and physical chemistry [9] . Statistics and probability theory explain thermodynamic properties with the erratic motion of atoms and molecules [10] . A multitude of engineering formulas and tables based on thermodynamics are used in the design of combustion engines and turbines, thermal power plants, and heating, air conditioning and refrigeration systems.


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