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Motion (physics)
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In physics, motion is a change in position of an object over time. Motion is described in terms of displacement, distance, velocity, acceleration, time, and speed. Motion of a body is observed by attaching a frame of reference to an observer and measuring the change in position of the body relative to that frame.
If the position of a body is not changing with respect to a given frame of reference (reference point), the body 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. Momentum is a quantity which is used for measuring the motion of an object. An object's momentum is directly related to the object's mass and velocity, and the total momentum of all objects in an isolated 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.[1] Thus, everything in the universe can be considered to be moving.[2]:20–21
Motion applies to objects, bodies, and matter particles, to radiation, radiation fields and radiation particles, and to space, its curvature and space-time. One can also speak of motion of shapes and boundaries. So, the term motion, in general, signifies a continuous change in the configuration of a physical system. For example, one can talk about motion of a wave or about motion of a quantum particle, 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.
Contents
[hide]
1 Laws of motion
1.1 Classical mechanics
1.2 Quantum mechanics
2 List of "imperceptible" human motions
2.1 Universe
2.2 Galaxy
2.3 Sun and solar system
2.4 Earth
2.5 Continents
2.6 Internal body
2.7 Cells
2.8 Particles
2.9 Subatomic particles
3 Light
4 Types of motion
5 Fundamental motions
6 See also
7 References
8 External links
Laws of motion[edit]
Main article: Mechanics
In physics, motion is described through two sets of apparently contradictory laws of mechanics. 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.
First law: In an inertial reference frame, an object either remains at rest or continues to move at a constant velocity, unless acted upon by a net force.
Second law: In an inertial reference frame, the vector sum of the forces F on an object is equal to the mass m of that object multiplied by the acceleration a of the object: F = ma.
Third law: When one body exerts a force on a second body, the second body simultaneously exerts a force equal in magnitude and opposite in direction on the first body.
Classical mechanics[edit]
Part of a series of articles about
Classical mechanics
F → = m a → {\displaystyle {\vec {F}}=m{\vec {a}}}
Second law of motion
History
Timeline
Branches[show]
Applied
Celestial
Continuum
Dynamics
Kinematics
Kinetics
Statics
Statistical
Fundamentals[show]
Acceleration
Angular momentum
Couple
D'Alembert's principle
Energy
kinetic
potential
Force
Frame of reference
Inertial frame of reference
Impulse
Inertia / Moment of inertia
Mass

Mechanical power
Mechanical work

Moment
Momentum
Space
Speed
Time
Torque
Velocity
Virtual work
Formulations[show]
Newton's laws of motion
Analytical mechanics
Lagrangian mechanics
Hamiltonian mechanics
Routhian mechanics
Hamilton–Jacobi equation
Appell's equation of motion
Udwadia–Kalaba equation
Koopman–von Neumann mechanics
Core topics[show]
Damping (ratio)
Displacement
Equations of motion
Euler's laws of motion
Fictitious force
Friction
Harmonic oscillator
Inertial / Non-inertial reference frame
Mechanics of planar particle motion
Motion (linear)
Newton's law of universal gravitation
Newton's laws of motion
Relative velocity
Rigid body
dynamics
Euler's equations
Simple harmonic motion
Vibration
Rotation[show]
Circular motion
Rotating reference frame
Centripetal force
Centrifugal force
reactive
Coriolis force
Pendulum
Tangential speed
Rotational speed
Angular acceleration / displacement / frequency / velocity
Scientists[show]
Galileo
Huygens
Newton
Kepler
Horrocks
Halley
Euler
d'Alembert
Clairaut
Lagrange
Laplace
Hamilton
Poisson
Daniel Bernoulli
Johann Bernoulli
Cauchy
v
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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 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. Newton's three laws are:
A body either is at rest or moves with constant velocity, until and unless an outer force is applied to it.
An object will travel in one direction only until an outer force changes its direction.
Whenever one body exerts a force F onto a second body, (in some cases, which is standing still) the second body exerts the force −F on the first body. F and −F are equal in magnitude and opposite in sense. So, the body which exerts F will go backwards.[3]
Newton's three laws of motion were the first to accurately provide a mathematical model for understanding orbiting bodies in outer space. This explanation unified the motion of celestial bodies and motion of objects on earth.
Classical mechanics was further enhanced by Albert Einstein's special relativity and general relativity. Special relativity is concerned with the motion of objects with a high velocity, approaching the speed of light; general relativity is employed to handle gravitational motion at a deeper level.
Uniform Motion:
This section is incomplete. This is because the information in the last sentence of this section does not provide sufficient and complete information. (October 2017)
When an object moves with a constant speed at a particular direction at regular intervals of time it's known as the uniform motion. For example: a bike moving in a straight line with a constant speed.
EQUATIONS OF UNIFORM MOTION:
If v = final velocity, u = initial velocity, a = acceleration, t = time, s = displacement, then :
v = u + a t {\displaystyle \mathbf {v} =\mathbf {u} +\mathbf {a} \mathbf {t} }
v 2 = u 2 + 2 a s {\displaystyle \mathbf {v} ^{2}=\mathbf {u} ^{2}+2\mathbf {a} \mathbf {s} }
s = u t + a t 2 2 {\displaystyle \mathbf {s} =\mathbf {u} \mathbf {t} +{\frac {\mathbf {a} \mathbf {t} ^{2}}{2}}}
Quantum mechanics[edit]
Main article: Quantum mechanics
Quantum mechanics is a set of principles describing physical reality at the atomic level of matter (molecules and atoms) and the subatomic particles (electrons, protons, neutrons, and even smaller elementary particles such as quarks). These descriptions include the simultaneous wave-like and particle-like behavior of both matter and radiation energy as described in the wave–particle duality.[citation needed]
In classical mechanics, accurate measurements and predictions of the state of objects can be calculated, such as location and velocity. In the quantum mechanics, due to the Heisenberg uncertainty principle, the complete state of a subatomic particle, such as its location and velocity, cannot be simultaneously determined.[citation needed]
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.[citation needed]
List of "imperceptible" human motions[edit]
Humans, like all known things in the universe, are in constant motion;[2]:8–9 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: Newton's laws of motion (particularly the third) which prevents the feeling of motion on a mass to which the observer is connected, and the lack of an obvious frame of reference which would allow individuals to easily see that they are moving.[4] The smaller scales of these motions are too small to be detected conventionally with human senses.
Universe[edit]
Spacetime (the fabric of the universe) is expanding meaning everything in the universe is stretching like a rubber band. This motion is the most obscure as it is not physical motion as such, but rather a change in the very nature of the universe. The primary source of verification of this expansion was provided by Edwin Hubble who demonstrated that all galaxies and distant astronomical objects were moving away from Earth, known as Hubble's law, predicted by a universal expansion.[5]
Galaxy[edit]
The Milky Way Galaxy is moving through space and many astronomers believe the velocity of this motion to be approximately 600 kilometres per second (1,340,000 mph) relative to the observed locations of other nearby galaxies. Another reference frame is provided by the Cosmic microwave background. This frame of reference indicates that the Milky Way is moving at around 582 kilometres per second (1,300,000 mph).[6][not in citation given]
Sun and solar system[edit]
The Milky Way is rotating around its dense galactic center, thus the sun is moving in a circle within the galaxy's gravity. Away from the central bulge, or outer rim, the typical stellar velocity is between 210 and 240 kilometres per second (470,000 and 540,000 mph).[7] All planets and their moons move with the sun. Thus, the solar system is moving.
Earth[edit]
The Earth is rotating or spinning around its axis. This is evidenced by day and night, at the equator the earth has an eastward velocity of 0.4651 kilometres per second (1,040 mph).[8] The Earth is also orbiting around the Sun in an orbital revolution. A complete orbit around the sun takes one year, or about 365 days; it averages a speed of about 30 kilometres per second (67,000 mph).[9]
Continents[edit]
The Theory of Plate tectonics tells us that the continents are drifting on convection currents within the mantle causing them to move across the surface of the planet at the slow speed of approximately 2.54 centimetres (1 in) per year.[10][11] However, the velocities of plates range widely. The fastest-moving plates are the oceanic plates, with the Cocos Plate advancing at a rate of 75 millimetres (3.0 in) per year[12] and the Pacific Plate moving 52–69 millimetres (2.0–2.7 in) per year. At the other extreme, the slowest-moving plate is the Eurasian Plate, progressing at a typical rate of about 21 millimetres (0.83 in) per year.
Internal body[edit]
The human heart is constantly contracting to move blood throughout the body. Through larger veins and arteries in the body, blood has been found to travel at approximately 0.33 m/s. Though considerable variation exists, and peak flows in the venae cavae have been found between 0.1 and 0.45 metres per second (0.33 and 1.48 ft/s).[13] additionally, the smooth muscles of hollow internal organs are moving. The most familiar would be the occurrence of peristalsis which is where digested food is forced throughout the digestive tract. Though different foods travel through the body at different rates, an average speed through the human small intestine is 3.48 kilometres per hour (2.16 mph).[14] The human lymphatic system is also constantly causing movements of excess fluids, lipids, and immune system related products around the body. The lymph fluid has been found to move through a lymph capillary of the skin at approximately 0.0000097 m/s.[15]
Cells[edit]
The cells of the human body have many structures which move throughout them. Cytoplasmic streaming is a way which cells move molecular substances throughout the cytoplasm,[16] various motor proteins work as molecular motors within a cell and move along the surface of various cellular substrates such as microtubules, and motor proteins are typically powered by the hydrolysis of adenosine triphosphate (ATP), and convert chemical energy into mechanical work.[17] Vesicles propelled by motor proteins have been found to have a velocity of approximately 0.00000152 m/s.[18]
Particles[edit]
According to the laws of thermodynamics, all particles of matter are in constant random motion as long as the temperature is above absolute zero. Thus the molecules and atoms which make up the human body are vibrating, colliding, and moving. This motion can be detected as temperature; higher temperatures, which represent greater kinetic energy in the particles, feel warm to humans who sense the thermal energy transferring from the object being touched to their nerves. Similarly, when lower temperature objects are touched, the senses perceive the transfer of heat away from the body as feeling cold.[19]
Subatomic particles[edit]
Within each atom, electrons exist in an area around the nucleus. This area is called the electron cloud. According to Bohr's model of the atom, electrons have a high velocity, and the larger the nucleus they are orbiting the faster they would need to move. If electrons 'move' about the electron cloud in strict paths the same way planets orbit the sun, then electrons would be required to do so at speeds which far exceed the speed of light. However, there is no reason that one must confine one's self to this strict conceptualization, that electrons move in paths the same way macroscopic objects do. Rather one can conceptualize electrons to be 'particles' that capriciously exist within the bounds of the electron cloud.[20] Inside the atomic nucleus, the protons and neutrons are also probably moving around due to the electrical repulsion of the protons and the presence of angular momentum of both particles.[21]
Light[edit]
Main article: Speed of light
Light propagates at 299,792,458 m/s, often approximated as 299,792 kilometres per second (186,282 mi/s) in a vacuum. The speed of light (or c) is also 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, information or causation can travel; the speed of light is the limit of speed for all physical systems.
In addition, the speed of light is an invariant quantity: it has the same value, irrespective of the position or speed of the observer. This property makes the speed of light c a natural measurement unit for speed.
Types of motion[edit]
Simple harmonic motion – (e.g., that of a pendulum).
Linear motion – motion which follows a straight linear path, and whose displacement is exactly the same as its trajectory.
Reciprocal motion (e.g. vibration)
Random motion (e.g. vibration)
Brownian motion (i.e. the random movement of particles)
Circular motion (e.g. the orbits of planets)
Rotary motion – a motion about a fixed point. (e.g. Ferris wheel).
Curvilinear motion – It is defined as the motion along a curved path that may be planar or in three dimensions.
Rotational motion
Rolling motion - (as of the wheel of a bicycle)
Oscillation - (swinging from side to side)
Vibratory motion
Combination (or simultaneous) motions - Combination of two or more above listed motions
Projectile motion - uniform horizontal motion + vertical accelerated motion
Fundamental motions[edit]
Linear motion
Circular motion
Oscillation
Wave
Momentum
Relative motion
See also[edit]
Physics portal
Simple machines
Kinematic chain
Power
Machine
Motion (geometry)
Displacement
Translatory motion
References[edit]
Jump up ^ Wahlin, Lars (1997). "9.1 Relative and absolute motion". The Deadbeat Universe (PDF). Boulder, CO: Coultron Research. pp. 121–129. ISBN 0-933407-03-3. Retrieved 25 January 2013.
^ Jump up to: a b Tyson, Neil de Grasse; Charles Tsun-Chu Liu; Robert Irion (2000). The universe : at home in the cosmos. Washington, DC: National Academy Press. ISBN 0-309-06488-0.
Jump up ^ Newton's "Axioms or Laws of Motion" can be found in the "Principia" on page 19 of volume 1 of the 1729 translation.
Jump up ^ Safkan, Yasar. "Question: If 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. PhysLink.com. Retrieved 25 January 2014.
Jump up ^ 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)
Jump up ^ 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.
Jump up ^ 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.
Jump up ^ Ask an Astrophysicist. NASA Goodard Space Flight Center.
Jump up ^ Williams, David R. (September 1, 2004). "Earth Fact Sheet". NASA. Retrieved 2007-03-17.
Jump up ^ Staff. "GPS Time Series". NASA JPL. Retrieved 2007-04-02.
Jump up ^ Huang, Zhen Shao (2001). Glenn Elert, ed. "Speed of the Continental Plates". The Physics Facebook. Retrieved 2016-12-29.
Jump up ^ 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.
Jump up ^ Wexler, L.; D H Bergel; I T Gabe; G S Makin; C J Mills (1 September 1968). "Velocity of Blood Flow in Normal Human Venae Cavae". Circulation Research. 23 (3): 349–359. doi:10.1161/01.RES.23.3.349.
Jump up ^ Bowen, R (27 May 2006). "Gastrointestinal Transit: How Long Does It Take?". Pathophysiology of the digestive system. Colorado State University. Retrieved 25 January 2014.
Jump up ^ M. Fischer; U. K. Franzeck; I. Herrig; U. Costanzo; S. Wen; M. Schiesser; U. Hoffmann; A. Bollinger (1 January 1996). "Flow velocity of single lymphatic capillaries in human skin". Am J Physiol Heart Circ Physiol. 270 (1): H358–H363. PMID 8769772. Retrieved 2007-11-14.
Jump up ^ "cytoplasmic streaming - biology". Encyclopædia Britannica.
Jump up ^ "Microtubule Motors". rpi.edu. Archived from the original on 2007-11-30.
Jump up ^ 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.
Jump up ^ Temperature and BEC. Archived 2007-11-10 at the Wayback Machine. Physics 2000: Colorado State University Physics Department
Jump up ^ "Classroom Resources - Argonne National Laboratory". anl.gov.
Jump up ^ Chapter 2, Nuclear Science- A guide to the nuclear science wall chart. Berkley National Laboratory.
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Kretanje – Bosnian
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bs
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Moviment – Catalan
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ca
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Mudiant – Welsh
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Liikumine – Estonian
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Higidura – Basque
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Movemento – Galician
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gl
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Gibanje – Croatian
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hr
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values:
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Movo – Ido
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https://id.wikipedia.org/wiki/Gerak
Gerak – Indonesian
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id
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Movimento – Portuguese
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pt
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Kuyuy – Quechua
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qu
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values:
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Movimentu – Sardinian
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sc
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Gibanje – Slovenian
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sl
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Gibanje – Serbo-Croatian
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Gerak – Sundanese
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su
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Mosyon – Tagalog
tl
tl
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values: All languages (initial selection from common choices by you and others)

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