William Matthew Flinders Petrie

Summary

William Matthew Flinders Petrie Encyclopædia Britannica, Ninth Edition (1888)

A unit of weight is the attractive force exerted between a unit of mass and some given body at a fixed distance,—this force being the weight of the unit in relation to the given body, or any other body of equal mass. [1] Usually the given body is the earth, and the distance a radius of the earth. For instance, the unit of weight in Britain is the attraction between the earth and the standard pound when that is placed at sea-level at London, in a vacuum. For astronomical comparisons the unit of mass is the sun, and a unit of weight is not needed.
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William Matthew Flinders Petrie Encyclopædia Britannica, Ninth Edition (1888)

Buildings will generally yield up their builder's foot or cubit when examined (Inductive Metrology, p. 9) . Vases may also be found bearing such relations to one another as to show their unit of volume. And coins have long been recognized as one of the great sources of metrology,—valuable for their wide and detailed range of information, though most unsatisfactory on account of the constant temptation to diminish their weight, a weakness which seldom allows us to reckon them as of the full standard.
Source: Wikisource

William Matthew Flinders Petrie Encyclopædia Britannica, Ninth Edition (1888)

A constant difficulty in studying works on metrology is the need of distinguishing the absolute facts of the case from the web of theory into which each writer has woven them,—often the names used, and sometimes the very existence of the units in question, being entirely an assumption of the writer. Therefore we shall here take the more pains to show what the actual authority is for each conclusion. Again, each writer has his own leaning: Böckh, to the study of water-volumes and weights, even deriving linear measures therefrom; Queipo, to the connexion with Arabic and Spanish measures
Source: Wikisource

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