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Armand Hippolyte Louis Fizeau FRS FRSE MIF ( French pronunciation: [aʁmɑ̃ ipɔlit lwi fizo] ; 23 September 1819 – 18 September 1896) was a French physicist , who in 1849 measured the speed of light to within 5% accuracy. In 1851, he measured the speed of light in moving water in an experiment known as the Fizeau experiment .

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26-498: A light-year , alternatively spelled light year ( ly or lyr ), is a unit of length used to express astronomical distances and is equal to exactly 9 460 730 472 580 .8 km , which is approximately 5.88 trillion mi. As defined by the International Astronomical Union (IAU), a light-year is the distance that light travels in vacuum in one Julian year (365.25 days). Despite its inclusion of

52-407: A star system tend to be small fractions of a light-year, and are usually expressed in astronomical units . However, smaller units of length can similarly be formed usefully by multiplying units of time by the speed of light. For example, the light-second , useful in astronomy, telecommunications and relativistic physics, is exactly 299 792 458 metres or ⁠ 1 / 31 557 600 ⁠ of

78-409: A light-year. Units such as the light-minute, light-hour and light-day are sometimes used in popular science publications. The light-month, roughly one-twelfth of a light-year, is also used occasionally for approximate measures. The Hayden Planetarium specifies the light month more precisely as 30 days of light travel time. Light travels approximately one foot in a nanosecond ; the term "light-foot"

104-410: A rapidly rotating wheel with 720 teeth. The speed of the wheel was increased until, at 12.6 rotations per second, the returning light hit the next tooth and could not be seen. At 25.2 rotations per second, the light was again visible. This gives a result of 2 x 8633m x 25.2 x 720/s = 313,274,304 m/s , which is within 5% of the correct value ( 299,792,458 meters per second ). (See Fizeau's measurement of

130-403: A series of investigations on the interference of light and heat. In 1848, he predicted the redshifting of electromagnetic waves . In 1849, Fizeau calculated a value for the speed of light to a better precision than the previous value determined by Ole Rømer in 1676. He used a beam of light reflected from a mirror 8633 meters away. The beam passed through the gaps between the teeth of

156-524: Is abbreviated "lk", and links "lks", in old deeds and land surveys done for the government. Astronomical measure uses: In atomic physics, sub-atomic physics, and cosmology, the preferred unit of length is often related to a chosen fundamental physical constant, or combination thereof. This is often a characteristic radius or wavelength of a particle. Some common natural units of length are included in this table: Archaic units of distance include: In everyday conversation, and in informal literature, it

182-530: Is an odd name. In 1868 an English journal labelled the light-year as a unit used by the Germans. Eddington called the light-year an inconvenient and irrelevant unit, which had sometimes crept from popular use into technical investigations. Although modern astronomers often prefer to use the parsec , light-years are also popularly used to gauge the expanses of interstellar and intergalactic space. Distances expressed in light-years include those between stars in

208-533: Is common to see lengths measured in units of objects of which everyone knows the approximate width. Common examples are: Horse racing and other equestrian activities keep alive: Hippolyte Fizeau Fizeau was born in Paris to Louis and Beatrice Fizeau. He married into the de Jussieu botanical family. His earliest work was concerned with improvements in photographic processes. Following suggestions by François Arago , Léon Foucault and Fizeau collaborated in

234-468: Is sometimes used as an informal measure of time. Unit of length A unit of length refers to any arbitrarily chosen and accepted reference standard for measurement of length. The most common units in modern use are the metric units , used in every country globally. In the United States the U.S. customary units are also in use. British Imperial units are still used for some purposes in

260-598: Is the product of the J1900.0 mean tropical year and the defined speed of light. Abbreviations used for light-years and multiples of light-years are: The light-year unit appeared a few years after the first successful measurement of the distance to a star other than the Sun, by Friedrich Bessel in 1838. The star was 61 Cygni , and he used a 160-millimetre (6.2 in) heliometre designed by Joseph von Fraunhofer . The largest unit for expressing distances across space at that time

286-568: The Bureau des Longitudes in 1878. He died in France at Venteuil on 18 September 1896. "Fizeau" is one of the 72 names inscribed on the frieze below the first platform of the Eiffel Tower, all of whom were French scientists, mathematicians, engineers, or industrialists from the hundred years before the tower's public opening for the 1889 World's Fair . Of the 72, Fizeau is the only one who

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312-518: The Doppler–Fizeau effect. In 1853, Fizeau described the use of a capacitor (sometimes termed a "condenser") as a means to increase the efficiency of the induction coil . Later, he studied the thermal expansion of solids and applied the phenomenon of interference of light to the measurement of the dilatations of crystals . He became a member of the Académie des Sciences in 1860 and a member of

338-539: The IAU (1964) System of Astronomical Constants, used from 1968 to 1983. The product of Simon Newcomb 's J1900.0 mean tropical year of 31 556 925 .9747 ephemeris seconds and a speed of light of 299 792 .5 km/s produced a light-year of 9.460 530 × 10 m (rounded to the seven significant digits in the speed of light) found in several modern sources was probably derived from an old source such as C. W. Allen 's 1973 Astrophysical Quantities reference work, which

364-580: The IAU for light-year is "ly", International standards like ISO 80000:2006 (now superseded) have used "l.y." and localized abbreviations are frequent, such as "al" in French, Spanish, and Italian (from année-lumière , año luz and anno luce , respectively), "Lj" in German (from Lichtjahr ), etc. Before 1984, the tropical year (not the Julian year) and a measured (not defined) speed of light were included in

390-653: The United Kingdom and some other countries. The metric system is sub-divided into SI and non-SI units. The base unit in the International System of Units (SI) is the meter , defined as "the length of the path travelled by light in vacuum during a time interval of 1 ⁄ 299792458 seconds." It is approximately equal to 1.0936 yd . Other SI units are derived from the meter by adding prefixes , as in millimeter or kilometer, thus producing systematic decimal multiples and submultiples of

416-532: The base unit that span many orders of magnitude. For example, a kilometer is 1000 m . In the centimeter–gram–second system of units , the basic unit of length is the centimeter , or 1 ⁄ 100 of a meter. Other non-SI units are derived from decimal multiples of the meter. The basic unit of length in the imperial and U.S. customary systems is the yard , defined as exactly 0.9144 m by international treaty in 1959. Common imperial units and U.S. customary units of length include: In addition,

442-494: The following are used by sailors : Aviators use feet for altitude worldwide (except in Russia and China) and nautical miles for distance. Surveyors in the United States continue to use: The Australian building trades adopted the metric system in 1966 and the units used for measurement of length are meters (m) and millimeters (mm). Centimeters (cm) are avoided as they cause confusion when reading plans . For example,

468-408: The length two and a half meters is usually recorded as 2500 mm or 2.5 m; it would be considered non-standard to record this length as 250 cm. American surveyors use a decimal-based system of measurement devised by Edmund Gunter in 1620. The base unit is Gunter's chain of 66 feet (20 m) which is subdivided into 4 rods, each of 16.5 ft or 100 links of 0.66 feet. A link

494-510: The light-year is the product of the Julian year (365.25 days, as opposed to the 365.2425-day Gregorian year or the 365.24219-day Tropical year that both approximate) and the speed of light ( 299 792 458  m/s ). Both of these values are included in the IAU (1976) System of Astronomical Constants , used since 1984. From this, the following conversions can be derived: The abbreviation used by

520-438: The mental picture of the approximate transit time for light, but he refrained from using the light-year as a unit. He may have resisted expressing distances in light-years because it would reduce the accuracy of his parallax data due to multiplying with the uncertain parameter of the speed of light. The speed of light was not yet precisely known in 1838; the estimate of its value changed in 1849 ( Fizeau ) and 1862 ( Foucault ). It

546-493: The same general area, such as those belonging to the same spiral arm or globular cluster . Galaxies themselves span from a few thousand to a few hundred thousand light-years in diameter, and are separated from neighbouring galaxies and galaxy clusters by millions of light-years. Distances to objects such as quasars and the Sloan Great Wall run up into the billions of light-years. Distances between objects within

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572-456: The speed of light in air .) Fizeau made the first suggestion in 1864 that the "speed of a light wave be used as a length standard". In 1850 he measured the relative speeds of light in air and water , using a rotating mirror, however Foucault independently achieved the same result seven weeks earlier. Fizeau was involved in the discovery of the Doppler effect , which is known in French as

598-439: The word "year", the term should not be misinterpreted as a unit of time . The light-year is most often used when expressing distances to stars and other distances on a galactic scale, especially in non-specialist contexts and popular science publications. The unit most commonly used in professional astronomy is the parsec (symbol: pc, about 3.26 light-years). As defined by the International Astronomical Union (IAU),

624-431: Was not yet considered to be a fundamental constant of nature, and the propagation of light through the aether or space was still enigmatic. The light-year unit appeared in 1851 in a German popular astronomical article by Otto Ule . Ule explained the oddity of a distance unit name ending in "year" by comparing it to a walking hour ( Wegstunde ). A contemporary German popular astronomical book also noticed that light-year

650-489: Was the astronomical unit , equal to the radius of the Earth's orbit at 150 million kilometres (93 million miles). In those terms, trigonometric calculations based on 61 Cygni's parallax of 0.314 arcseconds, showed the distance to the star to be 660 000 astronomical units (9.9 × 10 km; 6.1 × 10 mi). Bessel added that light takes 10.3 years to traverse this distance. He recognized that his readers would enjoy

676-433: Was updated in 2000, including the IAU (1976) value cited above (truncated to 10 significant digits). Other high-precision values are not derived from a coherent IAU system. A value of 9.460 536 207 × 10 m found in some modern sources is the product of a mean Gregorian year (365.2425 days or 31 556 952  s ) and the defined speed of light ( 299 792 458  m/s ). Another value, 9.460 528 405 × 10 m ,

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