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(Top)
 


1 Laws of Motion  



1.1  Classical mechanics  





1.2  Quantum mechanics  







2 Kinematics  



2.1  Planar motion  





2.2  Spherical motion  





2.3  Spatial motion  







3 List of "imperceptible" human motions  



3.1  Universe  





3.2  Galaxy  





3.3  Sun  





3.4  Solar System  





3.5  Earth  





3.6  Continents  





3.7  Internal body  





3.8  Cells  





3.9  Particles  





3.10  Subatomic particles  







4 Light  





5 Types of motion  





6 See also  





7 References  














Motion: Difference between revisions






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[[Image:Leaving Yongsan Station.jpg|300px|thumb|right|Motion involves a change in position, such as in this perspective of rapidly leaving [[Yongsan Station]].]]

[[Image:Leaving Yongsan Station.jpg|300px|thumb|right|Motion involves a change in position, such as in this perspective of rapidly leaving [[Yongsan Station]].]]



==Laws of Motion==

Gamgam style yo oy Nicolas bob bob

{{main|Mechanics}}

In physics, motion in the universe is described through two sets of apparently contradictory [[scientific law|laws]] of [[mechanics]]. Motions of all large scale and familiar objects in the universe (such as [[projectile]]s, [[planet]]s, [[Cell (biology)|cell]]s, and [[human]]s) are described by [[classical mechanics]]. Whereas the motion of very small [[atom]]ic and [[subatomic particle|sub-atomic]] objects is described by [[quantum mechanic]]s.


===Classical mechanics===

{{main|Classical mechanics}}

{{Classical mechanics}}

{{Classical mechanics}}

Classical mechanics is used for describing the motion of [[macroscopic]] objects, from [[projectiles]] to parts of [[machinery]], as well as [[astronomical objects]], such as [[spacecraft]], [[planets]], [[star]]s, and [[galaxies]]. It produces very accurate results within these domains, and is one of the oldest and largest subjects in [[science]], [[engineering]], and [[technology]].

Classical mechanics is used for describing the motion of [[macroscopic]] objects, from [[projectiles]] to parts of [[machinery]], as well as [[astronomical objects]], such as [[spacecraft]], [[planets]], [[star]]s, and [[galaxies]]. It produces very accurate results within these domains, and is one of the oldest and largest subjects in [[science]], [[engineering]], and [[technology]].


Revision as of 00:59, 23 January 2013

Inphysics, motion is a change in position of an object with respect to time and its reference point. Motion is typically described in terms of velocity, acceleration, displacement, and time.[1] Motion is observed by attaching a frame of reference to a body and measuring its change in position relative to another reference frame.

A body which does not move is said to be at rest, motionless, immobile, stationary, or to have constant (time-invariant) position. An object's motion cannot change unless it is acted upon by a force, as described by Newton's first law. An object's momentum is directly related to the object's mass and velocity, and the total momentum of all objects in a closed system (one not affected by external forces) does not change with time, as described by the law of conservation of momentum.

As there is no absolute frame of reference, absolute motion cannot be determined.[2] Thus, everything in the universe can be considered to be moving.[3]

More generally, the term motion signifies a continuous change in the configuration of a physical system. For example, one can talk about motion of a wave or a quantum particle (or any other field) where the configuration consists of probabilities of occupying specific positions.

Motion involves a change in position, such as in this perspective of rapidly leaving Yongsan Station.

Laws of Motion

In physics, motion in the universe is described through two sets of apparently contradictory lawsofmechanics. Motions of all large scale and familiar objects in the universe (such as projectiles, planets, cells, and humans) are described by classical mechanics. Whereas the motion of very small atomic and sub-atomic objects is described by quantum mechanics.

Classical mechanics

Classical mechanics 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, engineering, and technology.

Classical mechanics is fundamentally based on Newton's Laws of Motion. These laws describe the relationship between the forces acting on a body and the motion of that body. They were first compiled by Sir Isaac Newton in his work Philosophiæ Naturalis Principia Mathematica, first published on July 5, 1687. His three laws are:

  1. In the absence of a net external force, a body either is at rest or moves with constant velocity.
  2. The net external force on a body is equal to the mass of that body times its acceleration; F = ma. Alternatively, the acceleration is directly proportional to the force causing it, and inversely proportional to the mass.
  3. Whenever one body exerts a force F onto a second body, the second body exerts the force −F on the first body. F and −F are equal in magnitude and opposite in sense.[4]

Newton's three laws of motion, along with his law of universal gravitation, explain Kepler's laws of planetary motion, which were the first to accurately provide a mathematical model or understanding orbiting bodies in outer space. This explanation unified the motion of celestial bodies and motion of objects on earth.

Classical mechanics was later further enhanced by Albert Einstein's special relativity and general relativity. Special relativity explains the motion of objects with a high velocity, approaching the speed of light; general relativity is employed to handle gravitation motion at a deeper level.

Quantum mechanics

Quantum mechanics is a set of principles describing physical reality at the atomic level of matter (molecules and atoms) and the subatomic (electrons, protons, and even smaller particles). These descriptions include the simultaneous wave-like and particle-like behavior of both matter and radiation energy, this described in the wave–particle duality.

In contrast to classical mechanics, where accurate measurements and predictions can be calculated about location and velocity, in the quantum mechanics of a subatomic particle, one can never specify its state, such as its simultaneous location and velocity, with complete certainty (this is called the Heisenberg uncertainty principle).

In addition to describing the motion of atomic level phenomena, quantum mechanics is useful in understanding some large scale phenomenon such as superfluidity, superconductivity, and biological systems, including the function of smell receptors and the structures of proteins.

Kinematics

Kinematics applies geometry to the analysis of movement, or motion, of a mechanical system. Rest and motion is a very relative term as far as the frames of reference is concerned. So, while proceeding with any of the problems in kinematics one should be very careful about the frame of reference. [5] The rotation and sliding movement central a mechanical system is modeled mathematically as Euclidean, or rigid, transformations. The set of rigid transformations in three dimensional space forms a Lie group, denoted as SE(3).

Planar motion

While all motion in a mechanical system occurs in three dimensional space, planar motion can be analyzed using plane geometry, if all point trajectories are parallel to a plane. In this case the system is called a planar mechanism (or robot). The kinematic analysis of planar mechanisms uses the subset of SE(3) consisting of planar rotations and translations, denoted SE(2).

The group SE(2) is three dimensional, which means that every position of a body in the plane is defined by three parameters. The parameters are often the x and y coordinates of the origin of a coordinate frame in M measured from the origin of a coordinate frame in F, and the angle measured from the x-axis in F to the x-axis in M. This is described saying a body in the plane has three degrees-of-freedom. SE(2) is the configuration space for a planar body, and a planar motion is a curve in this space.

Spherical motion

It is possible to construct a mechanical system such that the point trajectories in all components lie in concentric spherical shells around a fixed point. An example is the gimbaled gyroscope. These devices are called spherical mechanisms.[6] Spherical mechanisms are constructed by connecting links with hinged joints such that the axes of each hinge passes through the same point. This point becomes center of the concentric spherical shells. The movement of these mechanisms is characterized by the group SO(3) of rotations in three dimensional space. Other examples of spherical mechanisms are the automotive differential and the robotic wrist.

Select this link for an animation of a Spherical deployable mechanism.

The rotation group SO(3) is three dimensional. An example of the three parameters that specify a spatial rotation are the roll, pitch and yaw angles used to define the orientation of an aircraft. SO(3) is the configuration space for a rotating body, and a spherical motion is a curve in this space.

Spatial motion

Amechanical system in which a body moves through a general spatial movement is called a spatial mechanism. An example is the RSSR linkage, which can be viewed as a four-bar linkage in which the hinged joints of the coupler link are replaced by rod ends, also called spherical joints or ball joints. The rod ends allow the input and output cranks of the RSSR linkage to be misaligned to the point that they lie in different planes, which causes the coupler link to move in a general spatial movement. Robot arms, Stewart platforms, and humanoid robotic systems are also examples of spatial mechanisms.

Select this link for an animation of Bennett's linkage, which is a spatial mechanism constructed from four hinged joints.

The group SE(3) is six dimensional, which means the position of a body in space is defined by six parameters. Three of the parameters define the origin of the moving reference frame relative to the fixed frame. Three other parameters define the orientation of the moving frame relative to the fixed frame. SE(3) is the configuration space for a body moving in space, and a spatial motion is a curve in this space.

List of "imperceptible" human motions

Humans, like all known things in the universe, are in constant motion,[7] however, aside from obvious movements of the various external body parts and locomotion, humans are in motion in a variety of ways which are more difficult to perceive. Many of these "imperceptible motions" are only perceivable with the help of special tools and careful observation. The larger scales of "imperceptible motions" are difficult for humans to perceive for two reasons: 1) Newton's laws of motion (particularly Inertia) which prevent humans from feeling motions of a mass to which they are connected, and 2) the lack of an obvious frame of reference which would allow individuals to easily see that they are moving.[8] The smaller scales of these motions are too small for humanstosense.

Universe

Galaxy

Sun

Solar System

Earth

Continents

Internal body

Cells

The cells of the human body have many structures which move throughout them.

Particles

Subatomic particles

Light

Light propagates at 299,792,458 m/s, often approximated as 300,000 kilometres per second or 186,000 miles per second. The speed of light (orc) is the speed of all massless particles and associated fields in a vacuum, and it is the upper limit on the speed at which energy, matter, and information can travel.

Types of motion

See also

References

  • ^ Wåhlin, L. 1997. "THE DEADBEAT UNIVERSE", Chapter 9. Colutron Research Corporation ISBN 0-933407-03-3
  • ^ De Grasse Tyson, N., Liu, C., & Irion, R. 2000. One Universe: At home in the cosmos. p.20–21. Joseph Henry Press. ISBN 0-309-06488-0
  • ^ Newton's "Axioms or Laws of Motion" can be found in the "Principia" on page 19 of volume 1 of the 1729 translation.
  • ^ O. Bottema & B. Roth (1990). Theoretical Kinematics. Dover Publications. reface. ISBN 0-486-66346-9. {{cite book}}: Unknown parameter |nopp= ignored (|no-pp= suggested) (help)
  • ^ J. M. McCarthy and G. S. Soh, 2010, Geometric Design of Linkages, Springer, New York.
  • ^ De Grasse Tyson, N., Liu, C., & Irion, R. 2000. One Universe: At home in the cosmos. p.8–9. Joseph Henry Press. ISBN 0-309-06488-0
  • ^ Safkan, Y. 2007 "f the term 'absolute motion' has no meaning, then why do we say that the earth moves around the sun and not vice versa?" Ask the Experts. PhysicsLink
  • ^ Hubble, Edwin, "A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae" (1929) Proceedings of the National Academy of Sciences of the United States of America, Volume 15, Issue 3, pp. 168–173 (Full article, PDF)
  • ^ Kogut, A.; Lineweaver, C.; Smoot, G. F.; Bennett, C. L.; Banday, A.; Boggess, N. W.; Cheng, E. S.; de Amici, G.; Fixsen, D. J.; Hinshaw, G.; Jackson, P. D.; Janssen, M.; Keegstra, P.; Loewenstein, K.; Lubin, P.; Mather, J. C.; Tenorio, L.; Weiss, R.; Wilkinson, D. T.; Wright, E. L. (1993). "Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps". Astrophysical Journal. 419: 1. arXiv:astro-ph/9312056. Bibcode:1993ApJ...419....1K. doi:10.1086/173453.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  • ^ Imamura, Jim (August 10, 2006). "Mass of the Milky Way Galaxy". University of Oregon. Archived from the original on 2007-03-01. Retrieved 2007-05-10.
  • ^ Ask and Astrophysicist. NASA Goodard Space Flight Center.
  • ^ Williams, David R. (September 1, 2004). "Earth Fact Sheet". NASA. Retrieved 2007-03-17.
  • ^ Staff. "GPS Time Series". NASA JPL. Retrieved 2007-04-02.
  • ^ Huang, Zhen Shao. "Speed of the Continental Plates". The Physics Factbook. Retrieved 2007-11-09.
  • ^ Meschede, M.; Udo Barckhausen, U. (November 20, 2000). "Plate Tectonic Evolution of the Cocos-Nazca Spreading Center". Proceedings of the Ocean Drilling Program. Texas A&M University. Retrieved 2007-04-02.{{cite web}}: CS1 maint: multiple names: authors list (link)
  • ^ Penny, P. 2003. Hemodynamic: Blood Velocity
  • ^ LEWIS WEXLER, DEREK H. BERGEL, IVOR T. GABE, GEOFFREY S. MAKIN, & CHRISTOPHER J. MILLS (1 September 1968GGHKHJ,H,kamnalaa mancha haru khatam). "Velocity of Blood Flow in Normal Human Venae Cavae". Circulation Research. 23 (3): 349–59. PMID 5676450. Retrieved 2007-11-14. {{cite journal}}: Check date values in: |date= (help); line feed character in |date= at position 46 (help)CS1 maint: multiple names: authors list (link)
  • ^ Bowen, R. 2006. Gastrointestinal Transit: How Long Does It Take? Colorado State University.
  • ^ M. Fischer, U. K. Franzeck, I. Herrig, U. Costanzo, S. Wen, M. Schiesser, U. Hoffmann and A. Bollinger (1 January 1996). "Flow velocity of single lymphatic capillaries in human skin". Am J Physiol Heart Circ Physiology. 270 (1): H358–H363. PMID 8769772. Retrieved 2007-11-14.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  • ^ Cytoplasmic Streaming: Encyclopædia Britannica
  • ^ Microtubules Motors: Rensselaer Polytechnic Institute.
  • ^ Hill, David; Holzwarth, George; Bonin, Keith (2002). "Velocity and Drag Forces on motor-protein-driven Vesicles in Cells". American Physical Society, the 69th Annual Meeting of the Southeastern. abstract. #EA.002. Bibcode:2002APS..SES.EA002H.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  • ^ Temperature and BEC. Physics 2000: Colorado State University Physics Department
  • ^ Ask a scientist archive. Argonne National Laboratory, United States Department of Energy
  • ^ Chapter 2, Nuclear Science- A guide to the nuclear science wall chart. Berkley National Laboratory.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Motion&oldid=534414044"

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    This page was last edited on 23 January 2013, at 00:59 (UTC).

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