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1 millimeter [mm] = 0.1 centimeter [cm]
Celebrity Reflection cruise ship in the Port of Miami. It's length is 1047 ft or 319 m
The Golden Gate Bridge spanning the Golden Gate, the strait that provides an opening between the San Francisco Bay and the Pacific Ocean. Its total length is about 1.7 mi or 2.7 km.
Length describes the longest dimension of an object. For three-dimensional objects it is usually measured horizontally.
Distance, on the other hand, refers to the measure of how far the objects are from each other.
Measuring Length and Distance
Units
The basic unit for length and distance in the International System of Units (SI) is a meter. Derivatives of the meter, such as kilometers and centimeters, are also used in the metric system. Units such as inch, foot, and mile are used where the metric system is not accepted, such as in the USA and the UK.
Distances in Science
Sciences like Biology and Physics work with very small distances, therefore additional units are used. A micrometer is 1×10⁻⁶ of a meter. It is commonly used in biology to measure microorganisms, as well as for measuring infrared radiation wavelengths. It is also known as micron, and is represented by the sign µ. Nanometer (1×10⁻⁹ of a meter), picometer (1×10⁻¹² of a meter), femtometer (1×10⁻¹⁵ of a meter), and attometer (1×10⁻¹⁸ of a meter) are also used.
Sailing under the Golden Gate Bridge. The clearance below the bridge is 220 ft or 67.1 m at tide
Distances in Navigation
Navigation uses nautical miles. One nautical mile equals 1852 meters. Historically it was defined as one minute of arc along the meridian, or 1/(60×180) of a meridian. This allowed for simplified calculations of latitude, because every 60 nautical miles were one degree of latitude. When calculating speed using nautical miles, often knots are used as units. One knot equals the speed of one nautical mile per hour.
Distances in Astronomy
In astronomy, because of the great distances under consideration, additional units are used for convenience.
An astronomical unit (AU, au, a.u., or ua) equals 149,597,870,700 meters. There is a constant, the unit distance, of the value of one astronomical unit. It is denoted as A. Earth is about 1.00 AU from the Sun.
A light year (ly) equals 10,000,000,000,000 km, or 10¹³ km. It represents the distance that light travels in one Julian year in vacuum. It is used more often in popular culture than in astronomical calculations.
Parsec explanation
A parsec (pc) is about 30,856,775,814,671,900 meters, or approximately 3.09 × 10¹³ km. One parsec represents the distance from the Sun to an astronomical object, such as a planet, a star, a moon, or an asteroid, which has a parallax angle equal to an arcsecond. One arcsecond equals to 1/3600 of a degree, or about 4.8481368 µrad in radians. To calculate a parsec, the effect of parallax can be used, which is an apparent displacement of an object when it is viewed from two different points of view. Astronomers draw an imaginary line from the Earth (point E1) to the distant star or an astronomical object (point A2), line E1A2. Half a year later, when the Sun is on the opposite side of the Earth, they draw another imaginary line from the current position of the Earth (point E2) to the new apparent position of the distant star (point A1), line E2A1. They then also connect the two positions of the Earth, making line E1E2. The sun is in the middle of this line, at a point S. The distance of lines E1S and E2S each equal 1 AU. When one draws a line perpendicular to E1E2, going through S, it will also pass through the intersection of E1A2 and E2A1, point I. The distance from the sun to this point, that is, the line SI, is equal to 1 pc, if the angle formed by the lines A1I and A2I is two arcseconds. Please see the diagram below for a better visualization. There, angle P is one arcsecond.
On this picture:
- A1, A2: apparent positions of a distant star
- E1, E2: positions of the Earth
- S: position of the Sun
- I: the intersection point
- IS = 1 parsec
- ∠P or ∠XIA2: parallax angle
- ∠P = 1 arcsecond
A league is an obsolete unit in most countries. It is still in use in some areas, such as Yucatan and rural Mexico. It is defined as a distance that a person can walk in one hour. A nautical league is defined as three nautical miles, which is about 5.6 km. A league was widely used in literature, such as in “Twenty Thousand Leagues Under the Sea” by Jules Verne.
A cubit is the length from the tip of the middle finger to the elbow. This unit was widely used from the Antiquity though to Early Modern Times.
A yard is used in the imperial system and it equals three feet or 0.9144 meters. In some countries like Canada it is only used when measuring fabric, as well as sports grounds, such as swimming pools and cricket pitches.
Defining the Meter
The meter was originally defined to be 1/10,000,000 of the distance between the North Pole and the Equator. It was later redefined as a length of a prototype meter bar, created from platinum and iridium alloy. It was further redefined 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. Later it was redefined once more using the speed of light. This definition is used today and states that one meter equals to the length of the path travelled by light in vacuum in 1/299,792,458 of a second.
Calculations
In geometry, distance between two points A and B with the coordinates A(x₁, y₁) and B(x₂, y₂) is calculated using the formula:
In physics distance is a scalar value and never negative. It can be measured by an odometer. Distance is measured along the object’s travel trajectory. It must not be confused with displacement, which is a vector that measures a straight line that is the shortest distance between the departure and the arrival points of an object.
Circular distance is a distance travelled by a circular object, such as a wheel. It can be calculated using frequency, or the radius of the wheel.
This article was written by Kateryna Yuri
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Do you have difficulty translating a measurement unit into another language? Help is available! Post your question in TCTerms and you will get an answer from experienced technical translators in minutes.
Calculations for the Length and Distance Converter converter are made using the math from unitconversion.org.
Page 2
1 millimeter [mm] = 0.1 centimeter [cm]
Celebrity Reflection cruise ship in the Port of Miami. It's length is 1047 ft or 319 m
The Golden Gate Bridge spanning the Golden Gate, the strait that provides an opening between the San Francisco Bay and the Pacific Ocean. Its total length is about 1.7 mi or 2.7 km.
Length describes the longest dimension of an object. For three-dimensional objects it is usually measured horizontally.
Distance, on the other hand, refers to the measure of how far the objects are from each other.
Measuring Length and Distance
Units
The basic unit for length and distance in the International System of Units (SI) is a meter. Derivatives of the meter, such as kilometers and centimeters, are also used in the metric system. Units such as inch, foot, and mile are used where the metric system is not accepted, such as in the USA and the UK.
Distances in Science
Sciences like Biology and Physics work with very small distances, therefore additional units are used. A micrometer is 1×10⁻⁶ of a meter. It is commonly used in biology to measure microorganisms, as well as for measuring infrared radiation wavelengths. It is also known as micron, and is represented by the sign µ. Nanometer (1×10⁻⁹ of a meter), picometer (1×10⁻¹² of a meter), femtometer (1×10⁻¹⁵ of a meter), and attometer (1×10⁻¹⁸ of a meter) are also used.
Sailing under the Golden Gate Bridge. The clearance below the bridge is 220 ft or 67.1 m at tide
Distances in Navigation
Navigation uses nautical miles. One nautical mile equals 1852 meters. Historically it was defined as one minute of arc along the meridian, or 1/(60×180) of a meridian. This allowed for simplified calculations of latitude, because every 60 nautical miles were one degree of latitude. When calculating speed using nautical miles, often knots are used as units. One knot equals the speed of one nautical mile per hour.
Distances in Astronomy
In astronomy, because of the great distances under consideration, additional units are used for convenience.
An astronomical unit (AU, au, a.u., or ua) equals 149,597,870,700 meters. There is a constant, the unit distance, of the value of one astronomical unit. It is denoted as A. Earth is about 1.00 AU from the Sun.
A light year (ly) equals 10,000,000,000,000 km, or 10¹³ km. It represents the distance that light travels in one Julian year in vacuum. It is used more often in popular culture than in astronomical calculations.
Parsec explanation
A parsec (pc) is about 30,856,775,814,671,900 meters, or approximately 3.09 × 10¹³ km. One parsec represents the distance from the Sun to an astronomical object, such as a planet, a star, a moon, or an asteroid, which has a parallax angle equal to an arcsecond. One arcsecond equals to 1/3600 of a degree, or about 4.8481368 µrad in radians. To calculate a parsec, the effect of parallax can be used, which is an apparent displacement of an object when it is viewed from two different points of view. Astronomers draw an imaginary line from the Earth (point E1) to the distant star or an astronomical object (point A2), line E1A2. Half a year later, when the Sun is on the opposite side of the Earth, they draw another imaginary line from the current position of the Earth (point E2) to the new apparent position of the distant star (point A1), line E2A1. They then also connect the two positions of the Earth, making line E1E2. The sun is in the middle of this line, at a point S. The distance of lines E1S and E2S each equal 1 AU. When one draws a line perpendicular to E1E2, going through S, it will also pass through the intersection of E1A2 and E2A1, point I. The distance from the sun to this point, that is, the line SI, is equal to 1 pc, if the angle formed by the lines A1I and A2I is two arcseconds. Please see the diagram below for a better visualization. There, angle P is one arcsecond.
On this picture:
- A1, A2: apparent positions of a distant star
- E1, E2: positions of the Earth
- S: position of the Sun
- I: the intersection point
- IS = 1 parsec
- ∠P or ∠XIA2: parallax angle
- ∠P = 1 arcsecond
A league is an obsolete unit in most countries. It is still in use in some areas, such as Yucatan and rural Mexico. It is defined as a distance that a person can walk in one hour. A nautical league is defined as three nautical miles, which is about 5.6 km. A league was widely used in literature, such as in “Twenty Thousand Leagues Under the Sea” by Jules Verne.
A cubit is the length from the tip of the middle finger to the elbow. This unit was widely used from the Antiquity though to Early Modern Times.
A yard is used in the imperial system and it equals three feet or 0.9144 meters. In some countries like Canada it is only used when measuring fabric, as well as sports grounds, such as swimming pools and cricket pitches.
Defining the Meter
The meter was originally defined to be 1/10,000,000 of the distance between the North Pole and the Equator. It was later redefined as a length of a prototype meter bar, created from platinum and iridium alloy. It was further redefined 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. Later it was redefined once more using the speed of light. This definition is used today and states that one meter equals to the length of the path travelled by light in vacuum in 1/299,792,458 of a second.
Calculations
In geometry, distance between two points A and B with the coordinates A(x₁, y₁) and B(x₂, y₂) is calculated using the formula:
In physics distance is a scalar value and never negative. It can be measured by an odometer. Distance is measured along the object’s travel trajectory. It must not be confused with displacement, which is a vector that measures a straight line that is the shortest distance between the departure and the arrival points of an object.
Circular distance is a distance travelled by a circular object, such as a wheel. It can be calculated using frequency, or the radius of the wheel.
This article was written by Kateryna Yuri
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Do you have difficulty translating a measurement unit into another language? Help is available! Post your question in TCTerms and you will get an answer from experienced technical translators in minutes.
Calculations for the Length and Distance Converter converter are made using the math from unitconversion.org.
Page 3
1 миллиметр [мм] = 0,1 сантиметр [см]
Круизный теплоход Celebrity Reflection в порту в Майами. Его длина составляет 319 метров или 1047 футов.
Мост Золотые Ворота, пересекающий пролив Золотые Ворота. Этот пролив соединяет залив Сан-Франциско и Тихий океан. Длина моста составляет 2,7 километра или 1,7 мили.
Длина — это наибольшее измерение тела. В трехмерном пространстве длина обычно измеряется горизонтально.
Расстояние — это величина, определяющая насколько два тела удалены друг от друга.
Измерение расстояния и длины
Единицы расстояния и длины
В системе СИ длина измеряется в метрах. Производные величины, такие как километр (1000 метров) и сантиметр (1/100 метра), также широко используются в метрической системе. В странах, где не пользуются метрической системой, например в США и Великобритании, используют такие единицы как дюймы, футы и мили.
Расстояние в физике и биологии
В биологии и физике часто измеряют длину намного менее одного миллиметра. Для этого принята специальная величина, микроме́тр. Один микроме́тр равен 1×10⁻⁶ метра. В биологии в микрометрах измеряют величину микроорганизмов и клеток, а в физике — длину инфракрасного электромагнитного излучения. Микроме́тр также называют микроном и иногда, особенно в англоязычной литературе, обозначают греческой буквой µ. Широко используются и другие производные метра: нанометры (1×10⁻⁹ метра), пикометры (1×10⁻¹² метра), фемтометры (1×10⁻¹⁵ метра и аттометры (1×10⁻¹⁸ метра).
Парусник проходит под мостом Золотые Ворота. Максимальная высота проходящего под ним судна может быть до 67,1 метра или 220 футов во время прилива.
Расстояние в навигации
В судоходстве используют морские мили. Одна морская миля равна 1852 метрам. Первоначально она измерялась как дуга в одну минуту по меридиану, то есть 1/(60×180) меридиана. Это облегчало вычисления широты, так как 60 морских миль равнялись одному градусу широты. Когда расстояние измеряется в морских милях, скорость часто измеряют в морских узлах. Один морской узел равен скорости движения в одну морскую милю в час.
Расстояние в астрономии
В астрономии измеряют большие расстояния, поэтому для облегчения вычислений приняты специальные величины.
Астрономическая единица (а. е., au) равна 149 597 870 700 метрам. Величина одной астрономической единицы — константа, то есть, постоянная величина. Принято считать, что Земля находится от Солнца на расстоянии одной астрономической единицы.
Световой год равен 10 000 000 000 000 или 10¹³ километрам. Это расстояние, которое проходит свет в вакууме за один Юлианский год. Эта величина используется в научно-популярной литературе чаще, чем в физике и астрономии.
Объяснение понятия «парсек»
Парсек приблизительно равен 30 856 775 814 671 900 метрам или примерно 3,09 × 10¹³ километрам. Один парсек — это расстояние от Солнца до другого астрономического объекта, например планеты, звезды, луны, или астероида, с углом в одну угловую секунду. Одна угловая секунда — 1/3600 градуса, или примерно 4,8481368 мкрад в радианах. Парсек можно вычислить используя параллакс — эффект видимого изменения положения тела, в зависимости от точки наблюдения. При измерениях прокладывают отрезок E1A2 (на иллюстрации) от Земли (точка E1) до звезды или другого астрономического объекта (точка A2). Шесть месяцев спустя, когда Солнце находится на другой стороне Земли, прокладывают новый отрезок E2A1 от нового положения Земли (точка E2) до нового положения в пространстве того же самого астрономического объекта (точка A1). При этом Солнце будет находиться на пересечении этих двух отрезков, в точке S. Длина каждого из отрезков E1S и E2S равна одной астрономической единице. Если отложить отрезок через точку S, перпендикулярный E1E2, он пройдет через точку пересечения отрезков E1A2 и E2A1, I. Расстояние от Солнца до точки I — отрезок SI, он равен одному парсеку, когда угол между отрезками A1I и A2I — две угловые секунды.
На рисунке:
- A1, A2: видимое положение звезды
- E1, E2: положение Земли
- S: положение Солнца
- I: точка пересечения
- IS = 1 парсек
- ∠P or ∠XIA2: угол параллакса
- ∠P = 1 угловая секунда
Лига — устаревшая единица длины, использовавшаяся раньше во многих странах. В некоторых местах ее до сих пор применяют, например, на полуострове Юкатан и в сельских районах Мексики. Это расстояние, которое человек проходит за час. Морская лига — три морских мили, примерно 5,6 километра. Лье — единица примерно равная лиге. В английском языке и лье, и лиги называются одинаково, league. В литературе лье иногда встречается в названии книг, как например «20 000 лье под водой» — известный роман Жюля Верна.
Локоть — старинная величина, равная расстоянию от кончика среднего пальца до локтя. Эта величина была широко распространена в античном мире, в средневековье, и до нового времени.
Ярд используется в британской имперской системе мер и равен трем футам или 0,9144 метра. В некоторых странах, например в Канаде, где принята метрическая система, ярды используют для измерения ткани и длины бассейнов и спортивных полей и площадок, например, полей для гольфа и футбола.
Определение метра
Определение метра несколько раз менялось. Изначально метр определяли как 1/10 000 000 расстояния от Северного полюса до экватора. Позже метр равнялся длине платиноиридиевого эталона. Позднее метр приравнивали к длине волны оранжевой линии электромагнитного спектра атома криптона ⁸⁶Kr в вакууме, умноженной на 1 650 763,73. Сегодня метр определяют как расстояние, пройденное светом в вакууме за 1/299 792 458 секунды.
Вычисления
В геометрии расстояние между двумя точками, А и В, с координатами A(x₁, y₁) и B(x₂, y₂) вычисляют по формуле:
В физике длина — всегда положительная скалярная величина. Ее можно измерить при помощи специального прибора, одометра. Расстояние измеряется по траектории движения тела. Важно не путать расстояние с перемещением — вектором, измеряемым по прямой от точки начала пути до точки конца пути. Перемещение и длина одинаковы по величине только если тело двигалось по прямой.
При известной частоте оборота колеса или его радиуса можно вычислить расстояние, пройденное этим колесом. Такие вычисления полезны, например, в велоспорте.
Автор статьи: Kateryna Yuri
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Вы затрудняетесь в переводе единицы измерения с одного языка на другой? Коллеги готовы вам помочь. Опубликуйте вопрос в TCTerms и в течение нескольких минут вы получите ответ.
Расчеты для перевода единиц в конвертере «Конвертер длины и расстояния» выполняются с помощью функций unitconversion.org.
Page 4
1 milimetru [mm] = 0,1 centimetru [cm]
Celebrity Reflection cruise ship in the Port of Miami. It's length is 1047 ft or 319 m
The Golden Gate Bridge spanning the Golden Gate, the strait that provides an opening between the San Francisco Bay and the Pacific Ocean. Its total length is about 1.7 mi or 2.7 km.
Lungimea desemnează cea mai lungă dimensiune a unui obiect. În cazul obiectelor tridimensionale, ea este măsurată, de regulă, orizontal.
Distanţa, pe de altă parte, ne precizează cât de departe se află obiectele unele de altele.
Măsurarea lungimii şi a distanţei
Unităţi de măsură
În Sistemul Internaţional de Unităţi (SI), unitatea fundamentală pentru lungime şi distanţă este metrul. Unităţile derivate ale metrului, de exemplu kilometrul sau centimetrul, sunt, de asemenea, utilizate în sistemul metric. Unităţi precum ţolul (inch-ul), piciorul sau mila sunt utilizate în ţări în care sistemul metric nu este acceptat, de exemplu în SUA şi Marea Britanie.
Distanţele în Ştiinţă
Ştiinţe precum Biologia şi Fizica operează cu distanţe foarte mici şi, de aceea, sunt utilizate unităţi de măsură suplimentare. Un micrometru este egal cu 1×10⁻⁶ dintr-un metru. Este des utilizat în biologie, pentru măsurarea microorganismelor sau pentru lungimile de undă ale radiaţiei infraroşii. Micrometrul este cunoscut şi sub numele de micron şi este simbolizat prin litera µ. De asemenea, sunt utilizaţi şi nanometrul (1×10⁻⁹ dintr-un metru), picometrul (1×10⁻¹² dintr-un metru), femtometrul (1×10⁻¹⁵ dintr-un metru) şi attometrul (1×10⁻¹⁸ dintr-un metru).
Sailing under the Golden Gate Bridge. The clearance below the bridge is 220 ft or 67.1 m at tide
Distanţele în navigaţie
Navigation uses nautical miles. One nautical mile equals 1852 meters. Historically it was defined as one minute of arc along the meridian, or 1/(60×180) of a meridian. This allowed for simplified calculations of latitude, because every 60 nautical miles were one degree of latitude. When calculating speed using nautical miles, often knots are used as units. One knot equals the speed of one nautical mile per hour.
Distanţele în astronomie
În astronomie sunt utilizate unităţi de măsură suplimentare, din cauza distanţelor mari ce sunt implicate.
An astronomical unit (AU, au, a.u., or ua) equals 149,597,870,700 meters. There is a constant, the unit distance, of the value of one astronomical unit. It is denoted as A. Earth is about 1.00 AU from the Sun.
Un an-lumină (a.l.) este egal cu 10.000.000.000.000 km sau cu 10¹³ km şi reprezintă distanţa parcursă de lumină în vid într-un an iulian. Anul-lumină este folosit mai des în cultura populară şi mai rar în calculele astronomice.
Parsec explanation
A parsec (pc) is about 30,856,775,814,671,900 meters, or approximately 3.09 × 10¹³ km. One parsec represents the distance from the Sun to an astronomical object, such as a planet, a star, a moon, or an asteroid, which has a parallax angle equal to an arcsecond. One arcsecond equals to 1/3600 of a degree, or about 4.8481368 µrad in radians. To calculate a parsec, the effect of parallax can be used, which is an apparent displacement of an object when it is viewed from two different points of view. Astronomers draw an imaginary line from the Earth (point E1) to the distant star or an astronomical object (point A2), line E1A2. Half a year later, when the Sun is on the opposite side of the Earth, they draw another imaginary line from the current position of the Earth (point E2) to the new apparent position of the distant star (point A1), line E2A1. They then also connect the two positions of the Earth, making line E1E2. The sun is in the middle of this line, at a point S. The distance of lines E1S and E2S each equal 1 AU. When one draws a line perpendicular to E1E2, going through S, it will also pass through the intersection of E1A2 and E2A1, point I. The distance from the sun to this point, that is, the line SI, is equal to 1 pc, if the angle formed by the lines A1I and A2I is two arcseconds. Please see the diagram below for a better visualization. There, angle P is one arcsecond.
În această imagine:
- A1, A2: apparent positions of a distant star
- E1, E2: poziţiile Pământului
- S: poziţia Soarelui
- I: punctul de intersecţie
- IS = 1 parsec
- ∠P or ∠XIA2: parallax angle
- ∠P = 1 arcsecond
Leghea este o unitate de măsură ieşită din uz în majoritatea ţărilor. Mai este folosită în unele zone, de exemplu în Yucatan sau în satele din Mexic. Leghea este definită ca distanţa pe care o poate parcurge un om, pe jos, într-o oră. O leghe marină este egală cu trei mile marine, ceea ce înseamnă circa 5,6 km. Ca unitate de măsură, leghea a fost mult folosită în literatură, spre exemplu în "Douăzeci de mii de leghe sub mări" de Jules Verne.
Cotul este distanţa de la vârful degetului mijlociu până la cot. Această unitate de măsură a fost mult folosită încă din Antichitate până în Epoca Modernă Timpurie.
Yard-ul este întrebuinţat în Sistemul Britanic de Unităţi; el este egal cu trei picioare sau cu 0,9144 metri. În unele ţări, precum Canada, este utilizat doar la măsurarea ţesăturilor sau a terenurilor sportive, de exemplu la măsurarea bazinelor de înot sau a terenurilor de cricket.
Definirea metrului
The meter was originally defined to be 1/10,000,000 of the distance between the North Pole and the Equator. It was later redefined as a length of a prototype meter bar, created from platinum and iridium alloy. It was further redefined 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. Later it was redefined once more using the speed of light. This definition is used today and states that one meter equals to the length of the path travelled by light in vacuum in 1/299,792,458 of a second.
Calculations
În geometrie, distanţa dintre două puncte A şi B, având coordonatele A(x₁, y₁) şi B(x₂, y₂), este calculată cu ajutorul formulei:
In physics distance is a scalar value and never negative. It can be measured by an odometer. Distance is measured along the object’s travel trajectory. It must not be confused with displacement, which is a vector that measures a straight line that is the shortest distance between the departure and the arrival points of an object.
Circular distance is a distance travelled by a circular object, such as a wheel. It can be calculated using frequency, or the radius of the wheel.
Acest articol a fost scris de către Kateryna Yuri.
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Aveţi dificultăţi în traducerea unităţilor de măsură într-o altă limbă? Puteţi primi ajutor! Scrieţi întrebarea dvs în TCTerms şi veţi primi răspuns de la traducători experimentaţi, specializaţi în domeniul tehnic, în câteva minute.
Calculele pentru convertorul Lungime şi distanţă sunt realizate folosind funcţiile matematice din unitconversion.org.
Page 5
1 millimeter [mm] = 0.1 centimeter [cm]
Celebrity Reflection cruise ship in the Port of Miami. It's length is 1047 ft or 319 m
The Golden Gate Bridge spanning the Golden Gate, the strait that provides an opening between the San Francisco Bay and the Pacific Ocean. Its total length is about 1.7 mi or 2.7 km.
Length describes the longest dimension of an object. For three-dimensional objects it is usually measured horizontally.
Distance, on the other hand, refers to the measure of how far the objects are from each other.
Measuring Length and Distance
Units
The basic unit for length and distance in the International System of Units (SI) is a meter. Derivatives of the meter, such as kilometers and centimeters, are also used in the metric system. Units such as inch, foot, and mile are used where the metric system is not accepted, such as in the USA and the UK.
Distances in Science
Sciences like Biology and Physics work with very small distances, therefore additional units are used. A micrometer is 1×10⁻⁶ of a meter. It is commonly used in biology to measure microorganisms, as well as for measuring infrared radiation wavelengths. It is also known as micron, and is represented by the sign µ. Nanometer (1×10⁻⁹ of a meter), picometer (1×10⁻¹² of a meter), femtometer (1×10⁻¹⁵ of a meter), and attometer (1×10⁻¹⁸ of a meter) are also used.
Sailing under the Golden Gate Bridge. The clearance below the bridge is 220 ft or 67.1 m at tide
Distances in Navigation
Navigation uses nautical miles. One nautical mile equals 1852 meters. Historically it was defined as one minute of arc along the meridian, or 1/(60×180) of a meridian. This allowed for simplified calculations of latitude, because every 60 nautical miles were one degree of latitude. When calculating speed using nautical miles, often knots are used as units. One knot equals the speed of one nautical mile per hour.
Distances in Astronomy
In astronomy, because of the great distances under consideration, additional units are used for convenience.
An astronomical unit (AU, au, a.u., or ua) equals 149,597,870,700 meters. There is a constant, the unit distance, of the value of one astronomical unit. It is denoted as A. Earth is about 1.00 AU from the Sun.
A light year (ly) equals 10,000,000,000,000 km, or 10¹³ km. It represents the distance that light travels in one Julian year in vacuum. It is used more often in popular culture than in astronomical calculations.
Parsec explanation
A parsec (pc) is about 30,856,775,814,671,900 meters, or approximately 3.09 × 10¹³ km. One parsec represents the distance from the Sun to an astronomical object, such as a planet, a star, a moon, or an asteroid, which has a parallax angle equal to an arcsecond. One arcsecond equals to 1/3600 of a degree, or about 4.8481368 µrad in radians. To calculate a parsec, the effect of parallax can be used, which is an apparent displacement of an object when it is viewed from two different points of view. Astronomers draw an imaginary line from the Earth (point E1) to the distant star or an astronomical object (point A2), line E1A2. Half a year later, when the Sun is on the opposite side of the Earth, they draw another imaginary line from the current position of the Earth (point E2) to the new apparent position of the distant star (point A1), line E2A1. They then also connect the two positions of the Earth, making line E1E2. The sun is in the middle of this line, at a point S. The distance of lines E1S and E2S each equal 1 AU. When one draws a line perpendicular to E1E2, going through S, it will also pass through the intersection of E1A2 and E2A1, point I. The distance from the sun to this point, that is, the line SI, is equal to 1 pc, if the angle formed by the lines A1I and A2I is two arcseconds. Please see the diagram below for a better visualization. There, angle P is one arcsecond.
On this picture:
- A1, A2: apparent positions of a distant star
- E1, E2: positions of the Earth
- S: position of the Sun
- I: the intersection point
- IS = 1 parsec
- ∠P or ∠XIA2: parallax angle
- ∠P = 1 arcsecond
A league is an obsolete unit in most countries. It is still in use in some areas, such as Yucatan and rural Mexico. It is defined as a distance that a person can walk in one hour. A nautical league is defined as three nautical miles, which is about 5.6 km. A league was widely used in literature, such as in “Twenty Thousand Leagues Under the Sea” by Jules Verne.
A cubit is the length from the tip of the middle finger to the elbow. This unit was widely used from the Antiquity though to Early Modern Times.
A yard is used in the imperial system and it equals three feet or 0.9144 meters. In some countries like Canada it is only used when measuring fabric, as well as sports grounds, such as swimming pools and cricket pitches.
Defining the Meter
The meter was originally defined to be 1/10,000,000 of the distance between the North Pole and the Equator. It was later redefined as a length of a prototype meter bar, created from platinum and iridium alloy. It was further redefined 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. Later it was redefined once more using the speed of light. This definition is used today and states that one meter equals to the length of the path travelled by light in vacuum in 1/299,792,458 of a second.
Calculations
In geometry, distance between two points A and B with the coordinates A(x₁, y₁) and B(x₂, y₂) is calculated using the formula:
In physics distance is a scalar value and never negative. It can be measured by an odometer. Distance is measured along the object’s travel trajectory. It must not be confused with displacement, which is a vector that measures a straight line that is the shortest distance between the departure and the arrival points of an object.
Circular distance is a distance travelled by a circular object, such as a wheel. It can be calculated using frequency, or the radius of the wheel.
This article was written by Kateryna Yuri
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Do you have difficulty translating a measurement unit into another language? Help is available! Post your question in TCTerms and you will get an answer from experienced technical translators in minutes.
Calculations for the Length and Distance Converter converter are made using the math from unitconversion.org.
Page 6
1 Millimeter [mm] = 0,1 Zentimeter [cm]
Kreuzschiff Celebrity Reflection im Hafen von Miami. Seine Länge beträgt 1047 Fuß oder 319 m
Die Golden Gate Bridge über dem Golden Gate, der Meerstraße zwischen San Francisco Bay und dem pazifischen Ozean. Die Gesamtlänge beträgt etwa 1,7 mi oder 2,7 km.
Die Länge beschreibt die längste Größendimension eines Objekts. Bei dreidimensionalen Objekten ist es in der Regel die horizontale Messung.
Distanz ist demgegenüber der Abstand, den zwei Objekte zueinander haben.
Länge und Distanz messen
Einheiten
Die Basiseinheit für Länge und Distanz im internationalen Einheitensystem (Système International d'Unités, SI) ist ein Meter. Ableitungen des Meters wie Kilometer und Zentimeter werden ebenfalls im metrischen System verwendet. Einheiten wie Zoll, Fuß und Meile werden in Ländern verwendet, in denen das metrische System nicht akzeptiert wird, wie den USA und Großbritannien.
Distanzen in der Wissenschaft
Wissenschaften wie Biologie und Physik arbeiten mit sehr geringen Distanzen oder Längen. Dafür werden zusätzliche Einheiten verwendet. Ein Mikrometer beträgt 1×10⁻⁶ Meter. Die Einheit wird in der Biologie verwendet, um Mikroorganismen sowie auch die Wellenlänge von Infrarotstrahlung zu messen. Es ist auch als Mikron bekannt und wird durch das Zeichen µ repräsentiert. Nanometer (1×10⁻⁹ Meter), Pikometer (1×10⁻¹² Meter), Femtometer (1×10⁻¹⁵ Meter) und Attometer (1×10⁻¹⁸ Meter) werden ebenfalls genutzt.
Segler unter der Golden Gate Bridge. Die Durchfahrthöhe unter der Brücke beträgt 220 ft oder 67,1 m bei Flut
Distanzen in der Navigation
In der Navigation wird die Seemeile verwendet. Eine Seemeile entspricht 1852 Meter. Historisch gesehen entsprach sie einer Bogenminute entlang des Meridians oder 1/(60×180) eines Meridians. Dadurch waren vereinfachte Berechnungen der Breite möglich, da 60 Seemeilen einem Breitengrad entsprechen. Bei der Berechnung von Geschwindigkeit mit Seemeilen wird die Einheit Knoten verwendet. Ein Knoten entspricht der Geschwindigkeit einer Seemeile pro Stunde.
Distanzen in der Astronomie
In der Astronomie werden ebenfalls zusätzliche Einheiten aufgrund der enormen Distanzen verwendet.
Eine astronomische Einheit (AU, au, a.u. oder ua) entspricht 149.597.870.700 Meter. Es gibt eine Konstante, die Einheitsdistanz mit der Größe einer astronomischen Einheit. Sie wird mit A angegeben. Erde hat eine Distanz von etwa 1,00 AU zur Sonne.
Ein Lichtjahr (ly) entspricht 10.000.000.000.000 km bzw. 10¹³ km. Sie entspricht der Distanz, die Licht in einem julianischen Jahr in einem Vakuum zurücklegt. Es wird häufiger von der Allgemeinheit als in astronomischen Berechnungen verwendet.
Parsec-Erklärung
Ein Parsec (pc) beträgt 30.856.775.814.671.900 Meter bzw. etwa 3,09 × 10¹³ km. Ein Parsec repräsentiert die Distanz von der Sonne zu einem astronomischen Objekt wie einem Planeten, einem Stern, einem Mond oder einem Asteroiden und hat einen Parallaxenwinkel gleich einer Bogensekunde. Eine Bogensekunde entspricht 1/3600 Grad oder 4,8481368 µrad im Bogenmaß. Um ein Parsec zu berechnen, kann der Parallaxeneffekt verwendet werden, der eine augenscheinliche Verschiebung eines Objekts ist, wenn es aus zwei unterschiedlichen Perspektiven betrachtet wird. Astronomen ziehen eine imaginäre Linie von der Erde (Punkt E1) zu einem Stern oder einem astronomischen Objekt (Punkt A2), Linie E1A2. Nach einem halben Jahr, wenn die Sonne auf der gegenüberliegenden Seite der Erde steht, ziehen sie eine zweite imaginäre Linie von der aktuellen Position von der Erde (Punkt E2) zu der neuen augenscheinlichen Position des entfernten Stern (Punkt A1), Linie E2A1. Dann verbinden sie die zwei Positionen der Erde, was Linie E1E2 ergibt. Die Sonne ist in der Mitte der Linie, an einem Punkt S. Die Distanzen der Linien E1S und E2S entsprechen jeweils 1 AU. Wenn eine Linie rechtwinklig zu E1E2 durch S gezogen wird, geht sie außerdem durch den Schnittpunkt von E1A2 und E2A1, Punkt I. Die Distanz von der Sonne zu diesem Punkt, das heißt Linie SI, entspricht 1 pc, wenn der Winkel der Linie A1I und A2I zwei Bogensekunden entspricht. Das Diagramm zeigt dies. Hier entspricht Winkel P einer Bogensekunde.
In diesem Bild:
- A1, A2: augenscheinliche Position eines entfernten Sterns.
- E1, E2: Positionen der Erde
- S: Position der Sonne
- I: Schnittpunkt
- IS = 1 Parsec
- ∠P oder ∠XIA2: Parallaxenwinkel
- ∠P = 1 Bogensekunde
Eine Leuge (engl. league, lea) ist eine in den meisten Ländern nicht mehr gebräuchliche Längeneinheit. Sie wird noch in einigen Gebieten verwendet, beispielsweise im Yucatán und ländlichen Mexiko. Sie wurde als Distanz definiert, die eine Person in einer Stunde zu Fuß gehen kann. Eine Seeleuge sind drei Seemeilen und etwa 5,6 km. Eine Leuge wurde häufig in der Literatur verwendet, beispielsweise im französischen und englischen Titel von Jules Vernes „20.000 Meilen unter dem Meer“: „Vingt mille lieues sous les mers“ und „Twenty Thousand Leagues Under the Sea“.
Ein Cubit ist die Länge von der Spitze des Mittelfingers zum Ellbogen. Diese Einheit wurde weithin seit der Antike bis in die frühe Neuzeit verwendet.
Ein Yard wird im britischen System verwendet und entspricht drei Fuß oder 0,9144 Meter. In einigen Ländern wie Kanada wird sie nur zum Abmessen von Stoff und Sporteinrichtungen wie Schwimmbahnen und Cricket-Plätzen eingesetzt.
Definition des Meters
Der Meter betrug ursprünglich 1/10000000 der Distanz zwischen dem Nordpol und dem Äquator. Er wurde später als Prototypmeterleiste neu definiert, die aus einer Platinum- und Iridiumlegierung hergestellt war. Er wurde zudem als 1.650.763,73-Faches der Wellenlänge der von Atomen des Nuklids 86Kr ausgesandten Strahlung in einem Vakuum definiert. Später wurde er anhand der Lichtgeschwindigkeit erneut definiert. Diese Definition ist heute gültig und besagt, dass ein Meter gleich der Länge von in einem Vakuum zurückgelegten Weges von Licht in einem Zeitintervall von 1/299792458 Sekunden ist.
Berechnungen
In der Geometrie wird eine Distanz zwischen zwei Punkten A und B mit den Koordinaten A(x₁, y₁) und B(x₂, y₂) anhand folgender Formel berechnet:
In der Physik ist Distanz eine skalare Göße, die niemals negativ ist. Sie kann anhand eines Wegmessers gemessen werden. Die Distanz wird entlang der Bewegungsbahn des Objekts gemessen. Sie darf nicht mit dem Versatz verwechselt werden, der ein Vektor ist und eine gerade Linie beschreibt, die die küzeste Distanz zwischen den Ausgangs- und Endpunkten eines Objekts ist.
Die kreisförmige Distanz ist der von einem kreisförmigen Objekt wie einem Reifen zurückgelegte Weg. Er kann anhand von Frequenz oder dem Radius des Reifens berechnet werden.
Dieser Artikel wurde von Kateryna Yuri verfasst.
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Haben Sie Schwierigkeiten, eine Messung in eine andere Sprache zu übersetzen? Hier erhalten Sie Hilfe! Stellen Sie Ihre Frage bei TCTerms und Sie erhalten von erfahrenen technischen Übersetzern binnen Minuten eine Antwort.
Berechnungen für den Umrechner Länge und Distanz werden anhand der mathematischen Funktionen von unitconversion.org erstellt.
Page 7
1 millimeter [mm] = 0,1 centimeter [cm]
Celebrity Reflection cruise ship in the Port of Miami. It's length is 1047 ft or 319 m
The Golden Gate Bridge spanning the Golden Gate, the strait that provides an opening between the San Francisco Bay and the Pacific Ocean. Its total length is about 1.7 mi or 2.7 km.
Length describes the longest dimension of an object. For three-dimensional objects it is usually measured horizontally.
Distance, on the other hand, refers to the measure of how far the objects are from each other.
Measuring Length and Distance
Units
The basic unit for length and distance in the International System of Units (SI) is a meter. Derivatives of the meter, such as kilometers and centimeters, are also used in the metric system. Units such as inch, foot, and mile are used where the metric system is not accepted, such as in the USA and the UK.
Distances in Science
Sciences like Biology and Physics work with very small distances, therefore additional units are used. A micrometer is 1×10⁻⁶ of a meter. It is commonly used in biology to measure microorganisms, as well as for measuring infrared radiation wavelengths. It is also known as micron, and is represented by the sign µ. Nanometer (1×10⁻⁹ of a meter), picometer (1×10⁻¹² of a meter), femtometer (1×10⁻¹⁵ of a meter), and attometer (1×10⁻¹⁸ of a meter) are also used.
Sailing under the Golden Gate Bridge. The clearance below the bridge is 220 ft or 67.1 m at tide
Distances in Navigation
Navigation uses nautical miles. One nautical mile equals 1852 meters. Historically it was defined as one minute of arc along the meridian, or 1/(60×180) of a meridian. This allowed for simplified calculations of latitude, because every 60 nautical miles were one degree of latitude. When calculating speed using nautical miles, often knots are used as units. One knot equals the speed of one nautical mile per hour.
Distances in Astronomy
In astronomy, because of the great distances under consideration, additional units are used for convenience.
An astronomical unit (AU, au, a.u., or ua) equals 149,597,870,700 meters. There is a constant, the unit distance, of the value of one astronomical unit. It is denoted as A. Earth is about 1.00 AU from the Sun.
A light year (ly) equals 10,000,000,000,000 km, or 10¹³ km. It represents the distance that light travels in one Julian year in vacuum. It is used more often in popular culture than in astronomical calculations.
Parsec explanation
A parsec (pc) is about 30,856,775,814,671,900 meters, or approximately 3.09 × 10¹³ km. One parsec represents the distance from the Sun to an astronomical object, such as a planet, a star, a moon, or an asteroid, which has a parallax angle equal to an arcsecond. One arcsecond equals to 1/3600 of a degree, or about 4.8481368 µrad in radians. To calculate a parsec, the effect of parallax can be used, which is an apparent displacement of an object when it is viewed from two different points of view. Astronomers draw an imaginary line from the Earth (point E1) to the distant star or an astronomical object (point A2), line E1A2. Half a year later, when the Sun is on the opposite side of the Earth, they draw another imaginary line from the current position of the Earth (point E2) to the new apparent position of the distant star (point A1), line E2A1. They then also connect the two positions of the Earth, making line E1E2. The sun is in the middle of this line, at a point S. The distance of lines E1S and E2S each equal 1 AU. When one draws a line perpendicular to E1E2, going through S, it will also pass through the intersection of E1A2 and E2A1, point I. The distance from the sun to this point, that is, the line SI, is equal to 1 pc, if the angle formed by the lines A1I and A2I is two arcseconds. Please see the diagram below for a better visualization. There, angle P is one arcsecond.
On this picture:
- A1, A2: apparent positions of a distant star
- E1, E2: positions of the Earth
- S: position of the Sun
- I: the intersection point
- IS = 1 parsec
- ∠P or ∠XIA2: parallax angle
- ∠P = 1 arcsecond
A league is an obsolete unit in most countries. It is still in use in some areas, such as Yucatan and rural Mexico. It is defined as a distance that a person can walk in one hour. A nautical league is defined as three nautical miles, which is about 5.6 km. A league was widely used in literature, such as in “Twenty Thousand Leagues Under the Sea” by Jules Verne.
A cubit is the length from the tip of the middle finger to the elbow. This unit was widely used from the Antiquity though to Early Modern Times.
A yard is used in the imperial system and it equals three feet or 0.9144 meters. In some countries like Canada it is only used when measuring fabric, as well as sports grounds, such as swimming pools and cricket pitches.
Defining the Meter
The meter was originally defined to be 1/10,000,000 of the distance between the North Pole and the Equator. It was later redefined as a length of a prototype meter bar, created from platinum and iridium alloy. It was further redefined 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. Later it was redefined once more using the speed of light. This definition is used today and states that one meter equals to the length of the path travelled by light in vacuum in 1/299,792,458 of a second.
Calculations
In geometry, distance between two points A and B with the coordinates A(x₁, y₁) and B(x₂, y₂) is calculated using the formula:
In physics distance is a scalar value and never negative. It can be measured by an odometer. Distance is measured along the object’s travel trajectory. It must not be confused with displacement, which is a vector that measures a straight line that is the shortest distance between the departure and the arrival points of an object.
Circular distance is a distance travelled by a circular object, such as a wheel. It can be calculated using frequency, or the radius of the wheel.
Artikel ini ditulis oleh Kateryna Yuri.
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
Anda kesulitan menerjemahkan satuan pengukuran ke bahasa lainnya? Bantuan tersedia! Posting pertanyaan Anda di TCTerms dan Anda akan mendapatkan jawaban dari penerjemah teknis berpengalaman dalam hitungan menit.
Perhitungan untuk pengonversi Panjang dan Jarak dilakukan menggunakan matematika dari unitconversion.org.
Page 8
1 millimetro [mm] = 0,1 centimetro [cm]
Celebrity Reflection cruise ship in the Port of Miami. It's length is 1047 ft or 319 m
The Golden Gate Bridge spanning the Golden Gate, the strait that provides an opening between the San Francisco Bay and the Pacific Ocean. Its total length is about 1.7 mi or 2.7 km.
Length describes the longest dimension of an object. For three-dimensional objects it is usually measured horizontally.
Distance, on the other hand, refers to the measure of how far the objects are from each other.
Misurazione della lunghezza e della distanza
Unità
The basic unit for length and distance in the International System of Units (SI) is a meter. Derivatives of the meter, such as kilometers and centimeters, are also used in the metric system. Units such as inch, foot, and mile are used where the metric system is not accepted, such as in the USA and the UK.
Distances in Science
Sciences like Biology and Physics work with very small distances, therefore additional units are used. A micrometer is 1×10⁻⁶ of a meter. It is commonly used in biology to measure microorganisms, as well as for measuring infrared radiation wavelengths. It is also known as micron, and is represented by the sign µ. Nanometer (1×10⁻⁹ of a meter), picometer (1×10⁻¹² of a meter), femtometer (1×10⁻¹⁵ of a meter), and attometer (1×10⁻¹⁸ of a meter) are also used.
Sailing under the Golden Gate Bridge. The clearance below the bridge is 220 ft or 67.1 m at tide
Distances in Navigation
Navigation uses nautical miles. One nautical mile equals 1852 meters. Historically it was defined as one minute of arc along the meridian, or 1/(60×180) of a meridian. This allowed for simplified calculations of latitude, because every 60 nautical miles were one degree of latitude. When calculating speed using nautical miles, often knots are used as units. One knot equals the speed of one nautical mile per hour.
Distances in Astronomy
In astronomy, because of the great distances under consideration, additional units are used for convenience.
An astronomical unit (AU, au, a.u., or ua) equals 149,597,870,700 meters. There is a constant, the unit distance, of the value of one astronomical unit. It is denoted as A. Earth is about 1.00 AU from the Sun.
A light year (ly) equals 10,000,000,000,000 km, or 10¹³ km. It represents the distance that light travels in one Julian year in vacuum. It is used more often in popular culture than in astronomical calculations.
Parsec explanation
A parsec (pc) is about 30,856,775,814,671,900 meters, or approximately 3.09 × 10¹³ km. One parsec represents the distance from the Sun to an astronomical object, such as a planet, a star, a moon, or an asteroid, which has a parallax angle equal to an arcsecond. One arcsecond equals to 1/3600 of a degree, or about 4.8481368 µrad in radians. To calculate a parsec, the effect of parallax can be used, which is an apparent displacement of an object when it is viewed from two different points of view. Astronomers draw an imaginary line from the Earth (point E1) to the distant star or an astronomical object (point A2), line E1A2. Half a year later, when the Sun is on the opposite side of the Earth, they draw another imaginary line from the current position of the Earth (point E2) to the new apparent position of the distant star (point A1), line E2A1. They then also connect the two positions of the Earth, making line E1E2. The sun is in the middle of this line, at a point S. The distance of lines E1S and E2S each equal 1 AU. When one draws a line perpendicular to E1E2, going through S, it will also pass through the intersection of E1A2 and E2A1, point I. The distance from the sun to this point, that is, the line SI, is equal to 1 pc, if the angle formed by the lines A1I and A2I is two arcseconds. Please see the diagram below for a better visualization. There, angle P is one arcsecond.
In questa immagine:
- A1, A2: apparent positions of a distant star
- E1, E2: positions of the Earth
- S: position of the Sun
- I: the intersection point
- IS = 1 parsec
- ∠P or ∠XIA2: parallax angle
- ∠P = 1 arcsecond
A league is an obsolete unit in most countries. It is still in use in some areas, such as Yucatan and rural Mexico. It is defined as a distance that a person can walk in one hour. A nautical league is defined as three nautical miles, which is about 5.6 km. A league was widely used in literature, such as in “Twenty Thousand Leagues Under the Sea” by Jules Verne.
A cubit is the length from the tip of the middle finger to the elbow. This unit was widely used from the Antiquity though to Early Modern Times.
A yard is used in the imperial system and it equals three feet or 0.9144 meters. In some countries like Canada it is only used when measuring fabric, as well as sports grounds, such as swimming pools and cricket pitches.
Defining the Meter
The meter was originally defined to be 1/10,000,000 of the distance between the North Pole and the Equator. It was later redefined as a length of a prototype meter bar, created from platinum and iridium alloy. It was further redefined 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. Later it was redefined once more using the speed of light. This definition is used today and states that one meter equals to the length of the path travelled by light in vacuum in 1/299,792,458 of a second.
Calcoli
In geometry, distance between two points A and B with the coordinates A(x₁, y₁) and B(x₂, y₂) is calculated using the formula:
In physics distance is a scalar value and never negative. It can be measured by an odometer. Distance is measured along the object’s travel trajectory. It must not be confused with displacement, which is a vector that measures a straight line that is the shortest distance between the departure and the arrival points of an object.
Circular distance is a distance travelled by a circular object, such as a wheel. It can be calculated using frequency, or the radius of the wheel.
Questo articolo è stato scritto da Kateryna Yuri.
Unit Converter articles were edited and illustrated by Anatoly Zolotkov
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I calcoli per il convertitore di Lunghezza e distanza vengono eseguiti usando le funzioni matematiche da unitconversion.org.
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