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| == Measurement == | == Measurement == | ||
| The '''metre''' (spelled "meter" in American English) is one of the seven ]. It is defined as the length of path traveled by light in vacuum during a time interval of 1/299,792,458 of a ]. | The '''metre''' (spelled "meter" in American English) is one of the seven ]. It is defined as the length of path traveled by light in vacuum during a time interval of 1/299,792,458 of a ]. | ||
| === History === | === History === | ||
| The metre was originally defined in ] by the ] as 1/10,000,000 of the distance along the ]'s surface from the North Pole to the Equator along the ] of ]. Uncertainty in the measurement of that distance lead the ] in ] to redefine the metre as the distance between two lines on a standard bar of ]-] kept at ]. | The metre was originally defined in ] by the ] as 1/10,000,000 of the distance along the ]'s surface from the North Pole to the Equator along the ] of ]. Uncertainty in the measurement of that distance lead the ] in ] to redefine the metre as the distance between two lines on a standard bar of ]-] kept at ]. | ||
| In ], as ] had become available, the 11th ] changed the definition of metre to be the length of 1,650,763.73 wavelengths in vacuum of the ]-] ] in the ] of ]-86. In ] the General Conference on Weights and Measures defined the metre as the distance traveled by light in a vacuum in 1/299,792,458 of a ] (that is, the ] in a vacuum was defined to be 299,792,458 metres per second). Since the speed of light is believed to be constant everywhere, a definition based on light is easier to maintain and more consistent than a measurement based on the circumference of the Earth or the length of a specific metal bar. Thus, should the bar be destroyed or lost, the standard meter can still be easily recreated in any laboratory. | In ], as ] had become available, the 11th ] changed the definition of metre to be the length of 1,650,763.73 wavelengths in vacuum of the ]-] ] in the ] of ]-86. In ] the General Conference on Weights and Measures defined the metre as the distance traveled by light in a vacuum in 1/299,792,458 of a ] (that is, the ] in a vacuum was defined to be 299,792,458 metres per second). Since the speed of light is believed to be constant everywhere, a definition based on light is easier to maintain and more consistent than a measurement based on the circumference of the Earth or the length of a specific metal bar. Thus, should the bar be destroyed or lost, the standard meter can still be easily recreated in any laboratory. | ||
| == Literature == | == Literature == | ||
| ⚫ | '''Metre''' is a term used in the ], usually indicated by the kind of feet and the number of them: for instance, "iambic pentameter", "dactylic tetrameter", etc. | ||
| ⚫ | '''Metre''' is a term used in the ], usually indicated by the kind of feet and the number of them: for instance, "iambic pentameter", "dactylic tetrameter", etc. See ]. | ||
| == Music == | == Music == | ||
| '''Metre''' refers to the measurement of a musical line into units such as '''beats''' and ], indicated in Western notation by a symbol called a ]. Properly, "metre" describes the whole concept of measuring rhythmic units, but it can also be used as a specific descriptor for a measurement of an individual piece as represented by the ] -- e.g., "This piece is in 4/4 metre" is equivalent to "This piece is in 4/4 time" or "This piece has a 4/4 ]." | '''Metre''' refers to the measurement of a musical line into units such as '''beats''' and ], indicated in Western notation by a symbol called a ]. Properly, "metre" describes the whole concept of measuring rhythmic units, but it can also be used as a specific descriptor for a measurement of an individual piece as represented by the ] -- e.g., "This piece is in 4/4 metre" is equivalent to "This piece is in 4/4 time" or "This piece has a 4/4 ]." | ||
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| ] | ] | ||
Revision as of 05:39, 12 November 2001
Measurement
The metre (spelled "meter" in American English) is one of the seven SI base units. It is defined as the length of path traveled by light in vacuum during a time interval of 1/299,792,458 of a second.
History
The metre was originally defined in 1791 by the French Academy of Sciences as 1/10,000,000 of the distance along the Earth's surface from the North Pole to the Equator along the meridian of Paris. Uncertainty in the measurement of that distance lead the International Bureau of Weights and Measures in 1889 to redefine the metre as the distance between two lines on a standard bar of platinum-iridium kept at Sevres.
In 1960, as lasers had become available, the 11th General Conference on Weights and Measures changed the definition of metre to be the length of 1,650,763.73 wavelengths in vacuum of the orange-red emission line in the spectrum of krypton-86. In 1983 the General Conference on Weights and Measures defined the metre as the distance traveled by light in a vacuum in 1/299,792,458 of a second (that is, the speed of light in a vacuum was defined to be 299,792,458 metres per second). Since the speed of light is believed to be constant everywhere, a definition based on light is easier to maintain and more consistent than a measurement based on the circumference of the Earth or the length of a specific metal bar. Thus, should the bar be destroyed or lost, the standard meter can still be easily recreated in any laboratory.
Literature
Metre is a term used in the scansion of poetry, usually indicated by the kind of feet and the number of them: for instance, "iambic pentameter", "dactylic tetrameter", etc. See meter in poetry.
Music
Metre refers to the measurement of a musical line into units such as beats and measures, indicated in Western notation by a symbol called a time signature. Properly, "metre" describes the whole concept of measuring rhythmic units, but it can also be used as a specific descriptor for a measurement of an individual piece as represented by the time signature -- e.g., "This piece is in 4/4 metre" is equivalent to "This piece is in 4/4 time" or "This piece has a 4/4 time signature."