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Wiktionary
conservation of mass

n. (context physics chemistry English) A conservation law of classical physics that states that the total mass of a closed system remains constant regardless of the chemical or physical changes that take place within it.

WordNet
conservation of mass

n. a fundamental principle of classical physics that matter cannot be created or destroyed in an isolated system [syn: conservation of matter, law of conservation of mass, law of conservation of matter]

Wikipedia
Conservation of mass

The law of conservation of mass or principle of mass conservation states that for any system closed to all transfers of matter and energy, the mass of the system must remain constant over time, as system mass cannot change quantity if it is not added or removed. Hence, the quantity of mass is "conserved" over time. The law implies that mass can neither be created nor destroyed, although it may be rearranged in space, or the entities associated with it may be changed in form, as for example when light or physical work is transformed into particles that contribute the same mass to the system as the light or work had contributed. The law implies (requires) that during any chemical reaction, nuclear reaction, or radioactive decay in an isolated system, the total mass of the reactants or starting materials must be equal to the mass of the products.

The concept of mass conservation is widely used in many fields such as chemistry, mechanics, and fluid dynamics. Historically, mass conservation was discovered in chemical reactions by Antoine Lavoisier in the late 18th century, and was of crucial importance in the progress from alchemy to the modern natural science of chemistry.

The closely related concept of matter conservation was found to hold good in chemistry to such high approximation that it failed only for the high energies treated by the later refinements of relativity theory, but otherwise remains useful and sufficiently accurate for most chemical calculations, even in modern practice.

In special relativity, needed for accuracy when large energy transfers between systems is involved, the difference between thermodynamically closed and isolated systems becomes important, since conservation of mass is strictly and perfectly upheld only for so-called isolated systems, i.e. those completely isolated from all exchanges with the environment. In this circumstance, the mass–energy equivalence theorem states that mass conservation is equivalent to total energy conservation, which is the first law of thermodynamics. By contrast, for a thermodynamically closed system (i.e., one which is closed to exchanges of matter, but open to exchanges of non-material energy, such as heat and work, with the surroundings) mass is (usually) only approximately conserved. The input or output of non-material energy must change the mass of the system in relativity theory, although the change is usually small, since relatively large amounts of such energy (by comparison with ordinary experience) carry only a small amount of mass (again by ordinary standards of measurement).

In special relativity, mass is not converted to energy, since mass and energy cannot be destroyed, and energy in all of its forms always retains its equivalent amount of mass throughout any transformation to a different type of energy within a system (or translocation into or out of a system). Certain types of matter (a different concept) may be created or destroyed, but in all of these processes, the energy and mass associated with such matter remains unchanged in quantity (although type of energy associated with the matter may change form).

In general relativity, mass (and energy) conservation in expanding volumes of space is a complex concept, subject to different definitions, and neither mass nor energy is as strictly and simply conserved as is the case in special relativity and in Minkowski space. For a discussion, see mass in general relativity.

Usage examples of "conservation of mass".

The two Doctors Berlin, now instant celebrities, were explaining the situation in terms of conservation of angular momentum (the primes who appeared in cars or planes were already moving at a high rate of speed) and conservation of mass and energy in a closed system (twice as many people, but only the same number of cars, planes, bicycles, and so on).

It was just something to even up the bookkeeping and save the law of conservation of mass energy.

No physical laws are violated, as the conservation of mass-energy is balanced at a higher level.

This became known as the conservation of mass, and it was a revolutionary concept.

Hunt voiced their reactions by asking how some of the fundamental laws of physics-conservation of mass-energy and momentum, for example-could be reconciled with the notion of particles being able to vanish spontaneously whenever they chose.

Second Law of yours with the Law of the Conservation of Mass and Energy?

And as to the famous heat death of the universe which you allude to, just how do you adjust, rectify, and justify this Second Law of yours with the Law of the Conservation of Mass and Energy?

There is the question of the true nature of Reality, the question of the conservation of mass-energy during Reality Change and so on.