Sabtu, 30 Mei 2009

Pendidikan Mekanika Klasik

Classical mechanics

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Angga Fuja W., Arip Nurahman, Dzikri Rahmat R., Deden Anugrah H., Cecepullah, Bambang Achdiat,

Rizkiana Putra M., Iqbal R., Purwanto, Yogaswara A., Rulli Alfian at all

Department of Physics
Faculty of Sciences and Mathematics, Indonesia University of Education

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Aeronautics and Astronautics Engineering
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Classical mechanics (commonly confused with Newtonian mechanics, which is a subfield thereof) is used for describing the motion of macroscopic objects, from projectiles to parts of machinery, as well as astronomical objects, such as spacecraft, planets, stars, and galaxies. It produces very accurate results within these domains, and is one of the oldest and largest subjects in science and technology.

Besides this, many related specialties exist, dealing with gases, liquids, and solids, and so on. Classical mechanics is enhanced by special relativity for objects moving with high velocity, approaching the speed of light; general relativity is employed to handle gravitation at a deeper level; and quantum mechanics handles the wave-particle duality of atoms and molecules.

In physics, classical mechanics is one of the two major sub-fields of study in the science of mechanics, which is concerned with the set of physical laws governing and mathematically describing the motions of bodies and aggregates of bodies. The other sub-field is quantum mechanics.

The term classical mechanics was coined in the early 20th century to describe the system of mathematical physics begun by Isaac Newton and many contemporary 17th century workers, building upon the earlier astronomical theories of Johannes Kepler, which in turn were based on the precise observations of Tycho Brahe and the studies of terrestrial projectile motionGalileo, but before the development of quantum physics and relativity. Therefore, some sources exclude so-called "relativistic physics" from that category. However, a number of modern sources do include Einstein's mechanics, which in their view represents classical mechanics in its most developed and most accurate form. The initial stage in the development of classical mechanics is often referred to as Newtonian mechanics, and is associated with the physical concepts employed by and the mathematical methods invented by Newton himself, in parallel with Leibniz, and others. This is further described in the following sections. More abstract and general methods include Lagrangian mechanics and Hamiltonian mechanics. While the terms classical mechanics and Newtonian mechanics are usually considered equivalent (if relativity is excluded), much of the content of classical mechanics was created in the 18th and 19th centuries and extends considerably beyond (particularly in its use of analytical mathematics) the work of Newton. of

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The SI derived units with kg, m and s
displacement m
speed m s−1
acceleration m s−2
jerk m s−3
specific energy m² s−2
absorbed dose rate m² s−3
moment of inertia kg m²
momentum kg m s−1
angular momentum kg m² s−1
force kg m s−2
torque kg m² s−2
energy kg m² s−2
power kg m² s−3
pressure kg m−1 s−2
surface tension kg s−2
irradiance kg s−3
kinematic viscosity m² s−1
dynamic viscosity kg m−1 s


Classical Mechanics

an introductory course




Richard Fitzpatrick


Associate Professor of Physics


The University of Texas at Austin





Arip Nurahman
Guru dan Dosen Profesional

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