Center of mass

The center of mass or center of inertia of an object is a point at which the object's mass can be assumed, for many purposes, to be concentrated. For example, an object can balance on a point only if its center of mass is directly above the point. Alternatively, if you hang an object from a string, the object's center of mass will be directly below the string. The path of an object in orbit depends only on its center of gravity. Most astronomical objects are radially symmetric, causing both the center of gravity and the center of mass to coincide at the center of the sphere.
In physics, the center of gravity (CoG) of an object is the average location of its weight. In a uniform gravitational field, it coincides with the object's center of mass. (In modern Britain the spelling centre is standard. Both spellings originated in England; center is now standard in America.)
Precisely, the center of mass of a group of points is defined as the weighted mean of the points' positions, where the weight applied to each point is the point's mass.
The concept of center of gravity was first introduced by the ancient Greek mathematician, physicist, and engineer Archimedes of Syracuse. Archimedes showed that the torque exerted on a lever by weights resting at various points along the lever is the same as what it would be if all of the weights were moved to a single point  their center of gravity. In work on floating bodies he demonstrated that the orientation of a floating object is the one that makes its center of gravity as low as possible. He developed mathematical techniques for finding the centers of gravity of objects of uniform density of various welldefined shapes, in particular a triangle, a hemisphere, and a frustum of a circular paraboloid.
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Aeronautical significance
The center of gravity is an important point on an aircraft, as it defines the amount of mass forward or behind the center of gravity that needs to be moved in order to pitch the plane up or down without applying any external forces. In conventional designs the CoG is often located very near the line 1/3rd back from the front of the wing. That is the line where most wings generate their lift, known as the center of pressure (CoP), so by balancing the plane at that point, the lift and weight balance out with no net torque. The CoG is sometimes moved slightly to the rear of this line in order to provide the plane with a natural "nose up" tendency when lift increases (like when applying more power).
If the balance of the plane is moved too far from the CoG, the control surfaces may have trouble controlling the plane. The actual force generated by the surfaces is typically quite small (a few pounds) but due to their location at the end of the tail (typically) they generate considerable torque to pitch the plane. If the CoG starts to move away from the CoP there will be an increasing amount of constant torque they have to counteract, and if it moves too far, it may be more than the controls can counter.
Motion of the center of mass
The following equations of motion assume that there is a system of particles governed by internal and external forces. An internal force is a force caused by the interaction of the particles within the system. An external force is a force that originates from outside the system, and acts on one or more particles within the system. The external force need not be due to a uniform field.
For any system with no external forces, the center of mass moves with constant velocity. This applies for all systems with classical internal forces, including magnetic fields, electric fields, chemical reactions, and so on. More formally, this is true for any internal forces that satisfy the weak form of Newton's Third Law.
The total momentum for any system of particles is given by
 <math>\mathbf{p}=M\mathbf{v}_\mathrm{cm}<math>
Where M indicates the total mass, and v_{cm} is the velocity of the center of mass. This velocity can be computed by taking the time derivative of the position of the center of mass.
An analogue to the famous Newton's Second Law is
 <math>\mathbf{F} = M\mathbf{a}_\mathrm{cm}<math>
Where F indicates the sum of all external forces on the system, and a_{cm} indicates the acceleration of the center of mass.
The angular momentum vector for a system is equal to the angular momentum of all the particles around the center of mass, plus the angular momentum of the center of mass, as if it were a single particle of mass <math>M<math>:
 <math>\mathbf{L}_\mathrm{sys} = \mathbf{L}_\mathrm{cm} + \mathbf{L}_\mathrm{around\mbox{ }cm}<math>
Examples
 Point A: position 2 m, mass 1 kg. Point B: position 4 m, mass 2 kg (assume positions are distances along a straight line from some origin). Center of mass:
 <math>\frac{2\mbox{ m} \times 1\mbox{ kg} + 4\mbox{ m} \times 2\mbox{ kg}}{1\mbox{ kg}+2\mbox{ kg}} = 3.33\mbox{ m}<math>
 Solid homogenous sphere (ideally divided in a high number of points of equal mass): each point averages with its opposite. Center of mass is at the center.
 Sphere with spherically symmetric density: center of mass is at the center. This approximately applies to the Earth: the density varies considerably, but it mainly depends on depth and less on the other two coordinates.
 Human being: It varies according to the body's position, but often it's somewhere inside the abdomen
 A sports car: engineers try hard to make the car as light as possible, and then add weight on the bottom. This way, the center of mass is nearer to the street, and the car handles better.
When talking about celestial bodies, the center of mass has a special relevance: when a moon orbits around planet, or a planet orbits around a star, both of them are actually orbiting around their center of mass, called the barycenter, see twobody problem. Some examples:
 EarthMoon system: the Moon's mass is 0.0123 that of Earth. Put Earth in position 0, mass 1 (here we use an arbitrary mass unit. It does not matter, provided that we use the same unit for the Moon). The Moon is at an average distance of 384400 km from the Earth. Then the center of mass is at:
 <math>\frac{0 \times 1 + 384400\mbox{ km} \times 0.0123}{1 + 0.0123} = 4671\mbox{ km}<math>
 from the Earth's center. Thus, as opposed to the Earth standing "still" and the Moon moving, both of them move around a point about 1700 km below the Earth's surface.
 SunEarth system: put Sun in position 0, mass=333,000 times the Earth. Earth in position 150,000,000 km, mass=1. Center of mass is 450 km from the Sun center. Here, the large mass difference between the two bodies makes the center of mass lie almost at the center of the Sun.
 SunJupiter system: put Sun in position 0, mass = 333,000 Earths. Jupiter in position 778,000,000 km, mass=318 Earths. Center of mass is 742,000 km from the Sun center, 96,000 km outside its surface. As Jupiter does its 11 year orbit, the Sun does a 1.5 million km orbit around the center of mass.
 To calculate the actual motion of the Sun, you would need to sum all the influences from all the planets, comets, asteroids, etc. of the solar system.
Note that the distance from the Sun's center to the center of mass of a twobody system consisting of the Sun and another celestial body, hence the size of the Sun's orbit around this center of mass, is approximately proportional to the product of the mass of that other body, and the distance between the two, even though gravity decreases with distance. That orbit is largest with Jupiter, its large mass more than compensates its smaller distance to the Sun than several other planets. If all the planets would align on the same side of the Sun, the combined center of mass would lie about 500,000 km outside the Sun surface.
See also
External links:
 Motion of the Center of Mass (http://www.kettering.edu/~drussell/Demos/COM/coma.html) shows that the motion of the center of mass of an object in free fall is the same as the motion of a point object.de:Massenmittelpunkt
fr:Centre de gravité ru:Центр масс sl:masno središče sv:Masscentrum