The metre (meter in the US), symbol m, is the base unit of length in the International System of Units (SI). Originally intended to be one ten-millionth of the distance from the Earth's equator to the North Pole (at sea level), its definition has been periodically refined to reflect growing knowledge of metrology. Since 1983, it has been defined as "the length of the path travelled by light in vacuum during a time interval of 1 ⁄ 299,792,458 of a second".^[1]

History[link]

Name[link]

The first recorded proposal for a decimal-based unit of length was the universal measure unit proposed by the English philosopher John Wilkins in 1668.^[2] In 1675, the Italian scientist Tito Livio Burattini, in his work Misura Universale, used the words metro cattolico (lit. "catholic [i.e. universal] metre"), which was derived from the Greek μέτρον καθολικόν (métron katholikón), "a universal measure". This word gave rise to the French mètre which in 1797 was introduced into the English language.^[3]

Belfry, Dunkirk - the northern end of the meridian arc

Fortress of Montjuïc - the southerly end of the meridian arc

Meridional definition[link]

In 1668, Wilkins proposed using Christopher Wren's suggestion of a pendulum with a half-period of one second to measure a standard length that Christiaan Huygens had observed to be 38 Rhineland or 39¼ English inches (997 mm) in length.^[2] In the 18th century, there were two favoured approaches to the definition of the standard unit of length. One approach followed Wilkins in defining the metre as the length of a pendulum with a half-period of one second, a 'seconds pendulum'. The other approach suggested defining the metre as one ten-millionth of the length of the Earth's meridian along a quadrant, that is the distance from the equator to the North Pole. In 1791, the French Academy of Sciences selected the meridional definition over the pendular definition because the force of gravity varies slightly over the surface of the Earth, which affects the period of a pendulum.

To establish a universally accepted foundation for the definition of the metre, measurements of this meridian more accurate than those available at that time were imperative. The French Academy of Sciences commissioned an expedition led by Jean Baptiste Joseph Delambre and Pierre Méchain, lasting from 1792 to 1799, which measured the distance between the Dunkerque belfry and Montjuïc castle, Barcelona to estimate the length of the meridian arc through Dunkerque (assumed to be the same length as the Paris meridian). This portion of the meridian was to serve as the basis for the length of the half meridian, connecting the North Pole with the equator. The exact shape of the Earth is not a simple mathematical shape (sphere or oblate spheroid) at the level of precision required for defining a standard of length. The irregular and particular shape of the Earth (smoothed to sea level) is called a Geoid, which means "Earth-shaped".

However, in 1793, France adopted as its official unit of length a metre based on provisional results from the expedition. Although it was later determined that the first prototype metre bar was short by a fifth of a millimetre because of miscalculation of the flattening of the Earth, this length became the standard. The circumference of the Earth through the poles is therefore slightly more than forty million metres (40 007 863).^[4]

Prototype metre bar[link]

Creating the metre-alloy in 1874 at the Conservatoire des Arts et Métiers. Present Henri Tresca, George Matthey, Saint-Claire Deville and Debray

Historical International Prototype Metre bar, made of an alloy of platinum and iridium, that was the standard from 1889 to 1960.

In the 1870s and in light of modern precision, a series of international conferences was held to devise new metric standards. The Metre Convention (Convention du Mètre) of 1875 mandated the establishment of a permanent International Bureau of Weights and Measures (BIPM: Bureau International des Poids et Mesures) to be located in Sèvres, France. This new organisation would preserve the new prototype metre and kilogram standards when constructed, distribute national metric prototypes, and maintain comparisons between them and non-metric measurement standards. The organisation created a new prototype bar in 1889 at the first General Conference on Weights and Measures (CGPM: Conférence Générale des Poids et Mesures), establishing the International Prototype Metre as the distance between two lines on a standard bar composed of an alloy of ninety percent platinum and ten percent iridium, measured at the melting point of ice.^[5]

The original international prototype of the metre is still kept at the BIPM under the conditions specified in 1889. A discussion of measurements of a standard metre bar and the errors encountered in making the measurements is found in a NIST document.^[6]

Standard wavelength of krypton-86 emission[link]

In 1893, the standard metre was first measured with an interferometer by Albert A. Michelson, the inventor of the device and an advocate of using some particular wavelength of light as a standard of length. By 1925, interferometry was in regular use at the BIPM. However, the International Prototype Metre remained the standard until 1960, when the eleventh CGPM defined the metre in the new SI system as equal to 1,650,763.73 wavelengths of the orange-red emission line in the electromagnetic spectrum of the krypton-86 atom in a vacuum.^[7]

Speed of light[link]

To further reduce uncertainty, the seventeenth CGPM in 1983 replaced the definition of the metre with its current definition, thus fixing the length of the metre in terms of the second and the speed of light:

The metre is the length of the path travelled by light in vacuum during a time interval of 1  ⁄   299,792,458 of a second.^[1]

This definition fixed the speed of light in vacuum at exactly 299,792,458 metres per second. An intended by-product of the 17th CGPM’s definition was that it enabled scientists to compare their lasers accurately using frequency, resulting in wavelengths with one-fifth the uncertainty involved in the direct comparison of wavelengths because interferometer errors were eliminated. To further facilitate reproducibility from lab to lab, the 17th CGPM also made the iodine-stabilised helium–neon laser “a recommended radiation” for realising the metre.^[8] For purposes of delineating the metre, the BIPM currently considers the HeNe laser wavelength to be as follows: λ_HeNe = 632 991 212.58 fm with an estimated relative standard uncertainty (U ) of 2.1×10⁻¹¹.^[9][10] This uncertainty is currently one limiting factor in laboratory realisations of the metre, and it is several orders of magnitude poorer than that of the second, based upon the caesium fountain atomic clock (U = 5×10⁻¹⁶ ).^[11] Consequently, a realisation of the metre is usually delineated (not defined) today in labs as 1,579,800.762042(33) wavelengths of helium-neon laser light in vacuum, the error stated being only that of frequency determination.^[12] This bracket notation expressing the error is explained in the article on measurement uncertainty.

Practical realisation of the metre is subject to uncertainties in characterising the medium, in addition to various uncertainties of interferometry, and to uncertainties in measuring the frequency of the source.^[13] A commonly used medium is air, and NIST has set up an on-line calculator to convert wavelengths in vacuum to wavelengths in air.^[14] As described by NIST, in air the uncertainties in characterising the medium are dominated by errors in finding temperature and pressure, and errors in the theoretical formulas used are secondary.^[15] By implementing a refractive index correction such as this, an approximate realization of the metre can be implemented in air, for example, using the formulation of the metre as 1,579,800.762042(33) wavelengths of helium-neon laser light in vacuum, and converting the wavelengths in vacuum to wavelengths in air. Of course, air is only one possible medium to use in a realization of the metre, and any partial vacuum can be used, or some inert atmosphere like helium gas, provided the appropriate corrections for refractive index are implemented.^[16]

Length measurement in metres[link]

Although the metre is now defined as the path length travelled by light in a given time, actual laboratory length measurements in metres are determined by counting the number of wavelengths of laser light of one of the standard types that fit into the length,^[8][17] and converting the selected unit of wavelength to metres. Three major factors limit the accuracy attainable with laser interferometers for a length measurement:^[18][13]

• Uncertainty in vacuum wavelength of the source,
• Uncertainty in the refractive index of the medium,
• Least count resolution of the interferometer.

Of these, the last is peculiar to the interferometer itself. The conversion of a length in wavelengths to a length in metres is based upon the relation:

Failed to parse (Missing texvc executable; please see math/README to configure.): \lambda = \frac{c}{n f} \

which converts the unit of wavelength λ to metres using c, the speed of light in vacuum in m/s. Here n is the refractive index of the medium in which the measurement is made; and f is taken for the conversion here as the measured frequency of the source. Although conversion from wavelengths to metres introduces additional error in the overall length due to measurement error in determining the refractive index and the frequency, measurement of frequency is one of the most accurate measurements available.^[18]

Timeline of definition[link]

• 1790 May 8 – The French National Assembly decides that the length of the new metre would be equal to the length of a pendulum with a half-period of one second.
• 1791 March 30 – The French National Assembly accepts the proposal by the French Academy of Sciences that the new definition for the metre be equal to one ten-millionth of the length of the Earth's meridian along a quadrant through Paris, that is the distance from the equator to the north pole.
• 1795 – Provisional metre bar constructed of brass.
• 1799 December 10 – The French National Assembly specifies the platinum metre bar, constructed on 23 June 1799 and deposited in the National Archives, as the final standard.
• 1889 September 28 – The first General Conference on Weights and Measures (CGPM) defines the metre as the distance between two lines on a standard bar of an alloy of platinum with ten percent iridium, measured at the melting point of ice.
• 1927 October 6 – The seventh CGPM adjusts the definition of the metre to be the distance, at 0 °C, between the axes of the two central lines marked on the prototype bar of platinum-iridium, this bar being subject to one standard atmosphere of pressure and supported on two cylinders of at least one centimetre diameter, symmetrically placed in the same horizontal plane at a distance of 571 millimetres from each other.
• 1960 October 14 – The 11th CGPM defines the metre to be equal to 1,650,763.73 wavelengths in vacuum of the radiation corresponding to the transition between the 2p¹⁰ and 5d⁵ quantum levels of the krypton-86 atom.^[19]
• 1983 October 21 – The 17th CGPM defines the metre as equal to the length of the path travelled by light in vacuum during a time interval of ¹⁄_299,792,458 of a second.^[20]
• 2002  – The International Committee for Weights and Measures (CIPM) considers the metre to be a unit of proper length and thus recommends this definition be restricted to "lengths ℓ which are sufficiently short for the effects predicted by general relativity to be negligible with respect to the uncertainties of realisation".^[21]

SI prefixed forms of metre[link]

SI prefixes are often employed to denote decimal multiples and submultiples of the metre, as shown in the table below. As indicated in the table, some are commonly used, while others are not. Long distances are usually expressed in km, astronomical units (149.6 Gm), light-years (10 Pm), or parsecs (31 Pm), rather than in Mm, Gm, Tm, Pm, Em, Zm or Ym; "30 cm", "30 m", and "300 m" are more common than "3 dm", "3 dam", and "3 hm", respectively.

The term micron is often used instead of micrometre, but this practice is officially discouraged.^[23]

Spelling[link]

Metre is used as the standard spelling of the metric unit for length in all English-speaking nations except the USA, which uses meter.^[24]

The most recent official brochure, written in 2006, about the International System of Units (SI), Bureau international des poids et mesures, was written in French by the International Bureau of Weights and Measures. An English translation (using the spelling: metre) is included to make the SI standard "more widely accessible".^[25]

In 2008, the U.S. English translation published by the U.S. National Institute of Standards and Technology chose to use meter in accordance with the United States Government Printing Office Style Manual.^[26]

Measuring devices (such as parking meter, speedometer) are traditionally spelt "...meter" in all countries.^[27] The word "meter", signifying any such device, has the same derivation as the word "metre", denoting the unit of length this article is about.^[28]

Equivalents in other units[link]

Within this table, "inch" (and "yard") means "international inch" (and yard).^[29] though approximate conversions in the left-hand column hold for both international units and survey units.

"≈" means "is approximately equal to".

"≡" means "equals by definition" or equivalently, "is exactly equal to".

One metre is exactly equivalent to ¹⁰⁰⁰⁰⁄₂₅₄ inches and to ¹⁰⁰⁰⁰⁄₉₁₄₄ yards.

A simple mnemonic aid exists to assist with conversion, as three "3":

1 metre is nearly equivalent to 3 feet, 3 and 3/8 inches.^[30] This gives an over-estimate of 0.125 mm.

The ancient Egyptian cubit was about ½ m (surviving rods are 52.3–52.9 cm). Scottish and English definitions of ell (two cubits) were 0.941 m and 1.143 m, respectively. The ancient Paris toise (fathom) was slightly shorter than 2 m, and was standardized at exactly 2 m in the mesures usuelles system, such that 1 m was exactly ½ toise. The Russian verst was 1.0668 km. The Swedish mil was 10.688 km, but was changed to 10 km when Sweden converted to metric units.

See also[link]

• Conversion of units for comparisons with other units
• International System of Units
• ISO 1 – standard reference temperature for length measurements
• Length measurement
• Metre Convention
• Metric system
• Introduction to the metric system
• Metrication
• Orders of magnitude (length)
• SI prefix
• Speed of light

Notes[link]

References[link]

• 17th General Conference on Weights and Measures. (1983). Resolution 1. International Bureau of Weights and Measures.
• American Heritage Dictionary of the English Language. 3rd ed. (1992). Boston: Houghton Mifflin.
• Astin, A. V. & Karo, H. Arnold, (1959), Refinement of values for the yard and the pound, Washington DC: National Bureau of Standards, republished on National Geodetic Survey web site and the Federal Register (Doc. 59-5442, Filed, 30 June 1959, 8:45 a.m.)
• Barbrow, Louis E. & Judson, Lewis V. (1976). Weights and Measures of the United States: A brief history (Special Publication 447).. National Institute of Standards and Technology.
• Beers, J.S. & Penzes, W. B. (1992). NIST Length Scale Interferometer Measurement Assurance. (NISTIR 4998). National Institute of Standards and Technology.
• Bureau International des Poids et Mesures. (2006). The International System of Units (SI). Retrieved 18 August 2008.
  • HTML version. Retrieved 24 August 2008.
• Bureau International des Poids et Mesures. (n.d.). Resolutions of the CGPM (search facility). Retrieved 3 June 2006.
• Bureau International des Poids et Mesures. (n.d.). The BIPM and the evolution of the definition of the metre. Retrieved 3 June 2006.
• Cambridge Advanced Learner's Dictionary (2008). Cambridge University Press.
• Cardarelli, Francois (2003). Encydopaedia of scientific units, weights, and measures: their SI equivalences and origins, Springer-Verlag London Limited, ISBN 1-85233-682-X, page 5, table 2.1, data from Giacomo, P., Du platine a la lumiere, Bull. Bur. Nat. Metrologie, 102 (1995) 5–14.
• Humerfelt, Sigurd. (26 October 2010). How WGS 84 defines Earth. Retrieved 29 April 2011.
• Layer, H.P. (2008). Length—Evolution from Measurement Standard to a Fundamental Constant. Gaithersburg, MD: National Institute of Standards and Technology. Retrieved 18 August 2008.
• Merriam-Webster Online Dictionary. Retrieved 8 December 2009.
• Mohr, P., Taylor, B.N., and David B. Newell, D. (28 December 2007). CODATA Recommended Values of the Fundamental Physical Constants: 2006. Gaithersburg, MD: National Institute of Standards and Technology. Retrieved 18 August 2008.
• National Institute of Standards and Technology. (December 2003). The NIST Reference on Constants, Units, and Uncertainty: International System of Units (SI) (web site):
  • SI base units. Retrieved 18 August 2008.
  • Definitions of the SI base units. Retrieved 18 August 2008.
  • Historical context of the SI: Metre. Retrieved 26 May 2010.
• National Institute of Standards and Technology. (27 June 2011). NIST-F1 Cesium Fountain Atomic Clock. Author.
• National Physical Laboratory. (25 March 2010). Iodine-Stabilised Lasers. Author.
• National Research Council Canada. (5 February 2010). Maintaining the SI unit of length. Retrieved 4 December 2010.
• Naughtin, Pat. (2008). Spelling metre or meter. Author.
• Penzes, W. (29 December 2005). Time Line for the Definition of the Meter. Gaithersburg, MD: National Institute of Standards and Technology — Precision Engineering Division. Retrieved 4 December 2010.
• Taylor, B.N. and Thompson, A. (Eds.). (2008a). The International System of Units (SI). United States version of the English text of the eighth edition (2006) of the International Bureau of Weights and Measures publication Le Système International d’ Unités (SI) (Special Publication 330). Gaithersburg, MD: National Institute of Standards and Technology. Retrieved 18 August 2008.
• Taylor, B.N. and Thompson, A. (2008b). Guide for the Use of the International System of Units (Special Publication 811). Gaithersburg, MD: National Institute of Standards and Technology. Retrieved 23 August 2008.
• Tibo Qorl. (2005) The History of the Meter (Translated by Sibille Rouzaud). Retrieved 18 August 2008.
• Turner, J. (Deputy Director of the National Institute of Standards and Technology). (16 May 2008)."Interpretation of the International System of Units (the Metric System of Measurement) for the United States". Federal Register Vol. 73, No. 96, p. 28432-3.
• Wilkins, J. (c. 2007). An essay towards a real character, and a philosophical language.[Also available without images of original.] Metrication Matters. (Reprinted from title page and pp. 190–194 of original, 1668, London: Royal Society)
• Zagar, B.G. (1999). Laser interferometer displacement sensors in J.G. Webster (ed.). The Measurement, Instrumentation, and Sensors Handbook. CRC Press. isbn=0-8493-8347-1.
• "(Mise en Pratique) MEP 2003: Iodine (λ≈633nm)". BIPM. 2003. http://www.bipm.org/utils/common/pdf/mep/M-e-P_I2_633.pdf. 

Further reading[link]

• Alder, Ken. (2002). The Measure of All Things : The Seven-Year Odyssey and Hidden Error That Transformed the World. Free Press, New York ISBN 0-7432-1675-X

v t e SI units Base units Ampere · Candela · Kelvin · Kilogram · Metre · Mole · Second Derived units Becquerel · Coulomb · Degree Celsius · Farad · Gray · Henry · Hertz · Joule · Katal · Lumen · Lux · Newton · Ohm · Pascal · Radian · Siemens · Sievert · Steradian · Tesla · Volt · Watt · Weber Accepted for use with SI Dalton (Atomic mass unit) · Astronomical unit · Day · Decibel · Degree Celsius · Degree of arc · Electronvolt · Hectare · Hour · Litre · Minute · Minute of arc · Neper · Second of arc · Tonne Atomic units · Natural units See also SI prefixes · Systems of measurement · Conversion of units · New SI definitions · History of the metric system Book:International System of Units  · Category:SI base units

Atilla Taş (born 1975) is a Turkish singer. His first album Kırmızılım was released in 1998.

In October 2012, Taş's release of a cover of Gangnam Style called Yam Yam Style caused some Turkish social media outlets to claim that Taş was actually Greek and named "Athillas Thasos".^[1][2]

References[link]

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Ryo Miyaichi

Miyaichi with Feyenoord
Personal information
Full name	Ryo Miyaichi
Date of birth	(1992-12-14) 14 December 1992 (age 19)
Place of birth	Aichi, Japan
Height	1.83 m (6 ft 0 in)
Playing position	Winger
Club information
Current club	Arsenal
Number	31
Youth career
2001–2007	Sylphid FC
2008–2010	Chukyodai Chukyo High School
Senior career*
Years	Team	Apps†	(Gls)†
2011–	Arsenal	0	(0)
2011	→ Feyenoord (loan)	12	(3)
2012	→ Bolton Wanderers (loan)	12	(0)
National team‡
2010	Japan U19[1]	8	(1)
2012–	Japan	1	(0)
* Senior club appearances and goals counted for the domestic league only and correct as of 2 May 2012 (UTC). † Appearances (Goals). ‡ National team caps and goals correct as of 23 May 2012

Ryo Miyaichi (宮市 亮, Miyaichi Ryō ^?, born 14 December 1992) is a Japanese footballer who plays as a winger for Premier League side Arsenal.

Early life[link]

Miyaichi was born into a sporting family, with father Tatsuya being a former baseball player who played for and later managed the Toyota Motors baseball club, and brother Tsuyoshi also being a football player.^[2] Miyaichi started playing football in his elementary school years at Sylphid F.C. in Nagoya.^[3] He entered Chukyodai Chukyo High School and played for the school football club. In the 2010 season, the team advanced to the All Japan High School Soccer Tournament but were defeated in the first round; the match had also been televised across Japan.^[4][5]

Club career[link]

Arsenal[link]

Miyaichi first trialled for Arsenal in the summer of 2010, where he impressed the Arsenal manager. Arsène Wenger was convinced of Miyaichi's abilities and subsequently offered him a contract with Arsenal. On 31 January 2011, he joined the club and signed a professional contract. Wenger said: "We’re delighted that Ryo Miyaichi has joined us. He trialled with us in the summer and has raw ability which has attracted many clubs around the world".^[6]

Loan to Feyenoord[link]

Just after he signed for Arsenal, it was announced that he was set to join Feyenoord on loan. On 5 February, he played his first game for Feyenoord against Vitesse. He played the full 90 minutes and was named man of the match (the game ended 1–1).^[7] Miyaichi played against Heracles Almelo and scored the opening goal and created the second for Feyenoord.^[8] On April 17, 2011, Miyaichi scored two goals and contributed two assists in Feyenoord's 6–1 victory over Willem II, leading a revival after Feyenoord had conceded an early goal.^[9]

The Dutch media gave him the nickname "Ryodinho" after comparisons to Ronaldinho. He has also been branded the Japanese Messi.^[10]

2011–12 season[link]

As he returned to Arsenal after his loan spell at Feyenoord, Miyaichi joined up with the first team for pre-season training. He was included in the 23-man squad to tour Asia in the pre-season after impressing in training.

Miyaichi made his pre-season debut against Malaysia All-Stars XI, he started the match before being substituted for Robin van Persie in the 66th minute.^[11]

On 9 August 2011, Miyaichi was granted a work permit to play for Arsenal on the grounds of being an "exceptional talent" in view of evidence supplied by Wenger and the Japan Football Association, and was deemed free to represent Arsenal during the 2011–12 season.^[12][13] He was also included in Arsenal's 23-man Champions League squad for the fixture against Udinese.^[14] On 23 August 2011, Miyaichi featured in the Arsenal Reserves against Wigan Athletic Reserves and scored in the 83rd minute.

On 20 September 2011, Miyaichi made his first team debut against League Two side Shrewsbury Town in the League Cup third round as a 71st minute substitute. He also came on again in the League Cup as a substitute as Arsenal went on to win the match 2–1 against Bolton Wanderers.

During the reserve match against Fulham, on 7 November 2011, Miyaichi lasted 34 minutes before being forced off with an ankle injury, which would cause him to be out for 4–6 weeks. Despite being in the first team, Miyaichi admitted he still has a lot to learn.^[15]

Loan to Bolton Wanderers[link]

On 31 January 2012, Ryo joined Bolton Wanderers on loan until the end of the season.^[16] Shortly after arriving at Bolton, manager Owen Coyle spoke of his admiration for the young player, even though Miyaichi had yet to play in a competitive match for the team.^[17] He played a behind-closed-doors game on 7 February against Preston North End where he scored the only goal in a 1–0 win and made his full debut when coming on as a half-time substitute for Martin Petrov in Bolton's 2-1 home defeat to Wigan Athletic on 11 February.^[18] He made his first start, and scored his first goal, the following weekend in Bolton's 2-0 FA Cup win at Millwall.^[19] He played 78 minutes of the game before being substituted. He made his first Premier League start the following weekend in Bolton's 3–0 loss at Chelsea.^[20] He was voted February Player Of The Month by the Bolton fans after his debut.^[21]

International career[link]

Ryo has been involved in the Japan National Team from U-15 to U-19 level having played in the prestigious FIFA U-17 World Cup in 2009. He received his first call up to the senior team for the World Cup qualifier against Uzbekistan in February 2012, however he did not feature during the 90 minutes^[22].

He did however make his debut on 23 May 2012 in a friendly match against Azerbaijan coming on as a 60th minuite substitue in a game that ended 2-0 to the home side .^[23]

Career statistics[link]

Club[link]

As of 31 March 2012^[24][25]

International[link]

Statistics accurate as of 30 July 2010

National team Year Apps Goals Japan U15 2007 3 2 Japan U16 2008 3 1 Japan U17 2009 5 2 Japan U19 2010 8 1 Japan 2012 1 0 Total 1 0

International appearances and goals # Date Venue Opponent Result Goal Competition 1 23 May 2012 Shizuoka Stadium, Fukuroi Azerbaijan 2-0 0 Friendly[26]

References[link]

External links[link]

• Ryo Miyaichi career stats at Soccerbase
• Ryo Miyaichi – FIFA competition record
• Ryo Miyaichi – Arsenal F.C. official site

v t e Japan squad – 2009 FIFA U-17 World Cup 1 Kamita 2 Okamoto 3 Hiroki 4 Matsubara 5 Uchida 6 Takano 7 Usami 8 Miyayoshi 9 Sugimoto 10 Shibasaki 11 Takagi 12 Nakajima 13 Horigome 14 Kojima 15 Tada 16 Ogawa 17 Kanda 18 Watanabe 19 Kohno 20 Miyaichi 21 Matsuzawa Coach: Ikeuchi