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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 , which is approximately 9.46 trillion km or 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 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 scale, especially in non-specialist contexts and publications. The unit most commonly used in professional is the (symbol: pc, about 3.26 light-years).


Definitions
As defined by the International Astronomical Union (IAU), 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 that both approximate) and the speed of light ().The speed of light is precisely by definition of the metre. Both of these values are included in the IAU (1976) System of Astronomical Constants, used since 1984." Selected Astronomical Constants " in Astronomical Almanac, p. 6. From this, the following conversions can be derived:
>
1 light-year  = metres (exactly)
trillion (short scale) kilometres ( trillion miles)
astronomical units

The abbreviation used by the IAU for light-year is "ly", International standards like (now superseded) have used "l.y."ISO 80000-3:2006 Quantities and Units – Space and TimeIEEE/ASTM SI 10-2010, American National Standard for Metric Practice and localized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 (not the Julian year) and a measured (not defined) speed of light were included in the IAU (1964) System of Astronomical Constants, used from 1968 to 1983. The product of 's J1900.0 mean tropical year of and a speed of light of produced a light-year of (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 's 1973 Astrophysical Quantities reference work, which 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 IAU system. A value of found in some modern sources is the product of a mean Gregorian year (365.2425 days or ) and the defined speed of light (). Another value, , 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:

  • "ly" for one light-year
  • "kly" or "klyr" Viollier 1994 for a kilolight-year (1,000 light-years)
  • "Mly" for a megalight-year (1,000,000 light-years)
  • "Gly" or "Glyr" Sanchez et al. 2022 for a gigalight-year ( light-years)


History
The light-year unit appeared a few years after the first successful measurement of the distance to a star other than the Sun, by in 1838. The star was 61 Cygni, and he used a designed by Joseph von Fraunhofer. The largest unit for expressing distances across space at that time was the astronomical unit, equal to the radius of the Earth's orbit at . In those terms, trigonometric calculations based on 61 Cygni's of 0.314 arcseconds, showed the distance to the star to be . Bessel added that light takes 10.3 years to traverse this distance. Bessel's statement that light employs 10.3 years to traverse the distance. He recognized that his readers would enjoy 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 () and 1862 (Foucault). It 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 . 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 is an odd name. In 1868 an English journal labelled the light-year as a unit used by the Germans. 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 , light-years are also popularly used to gauge the expanses of interstellar and intergalactic space.


Usage of term
Distances expressed in light-years include those between in the same general area, such as those belonging to the same or . 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 and the Sloan Great Wall run up into the billions of light-years.

+List of orders of magnitude for !Scale (ly) !Value !Item
10−9 Reflected sunlight from the 's surface takes 1.2–1.3 seconds to travel the distance to the Earth's surface (travelling roughly to kilometres).
10−6 One astronomical unit (the distance from the to the Earth). It takes approximately 499 seconds (8.32 minutes) for light to travel this distance.
The lands on Titan off and transmits images from its surface, 1.2 billion kilometres from Earth.
encounters at a distance of 4.7 billion kilometres, and the communication takes 4 hours 25 minutes to reach Earth.
10−3 The most distant , Voyager 1, was about 18 light-hours (130 au,19.4 billion km, 12.1 billion mi) away from the Earth . It will take about years to reach one light-year at its current speed of about 17 km/s (, 61 200 km/h) relative to the Sun. On 12 September 2013, NASA scientists announced that Voyager 1 had entered the interstellar medium of space on 25 August 2012, becoming the first manmade object to leave the .
Voyager 1 as of October 2018, nearly 20 light-hours (144 au, 21.6 billion km, 13.4 billion mi) from the Earth.
100 The is approximately two light-years in diameter. Its inner boundary is speculated to be at ≈ 0.8 ly, with its outer edge at ≈ 1.6 ly.
Approximate maximum distance at which an object can orbit the (/, ). Beyond this is the deep ex-solar gravitational interstellar medium.
The nearest known (other than the Sun), , is about 4.24 light-years away.
, the brightest star of the night sky. Twice as massive and 25 times more luminous than the Sun, it outshines more luminous stars due to its relative proximity.
Tau Ceti e, an extrasolar candidate for a habitable planet. 6.6 times as massive as the earth, it is in the middle of the habitable zone of star .
Gliese 581, a red-dwarf star with several detectable exoplanets.
, second in brightness in the terrestrial sky only to Sirius, a type A9 times more luminous than the Sun.
103 A0620-00, the second-nearest known , is about light-years away.
The of the is about light-years away.
The is about light-years across.
R136a1, in the Large Magellanic Cloud, the most luminous star known at 8.7 million times the of the Sun, has an apparent magnitude 12.77, just brighter than 3C 273.
106 The is approximately 2.5 million light-years away.
The Triangulum Galaxy (), at about 3 million light-years away, is the most distant object visible to the naked eye.
The nearest large , the , is about 59 million light-years away.
The lies at a distance of somewhere between 150 and 250 million light-years (the latter being the most recent estimate).
109 The Sloan Great Wall (not to be confused with Great Wall and Her–CrB GW) has been measured to be approximately one billion light-years distant.
3C 273, optically the brightest , of apparent magnitude 12.9, just dimmer than R136a1. 3C 273 is about 2.4 billion light-years away.
The comoving distance from the Earth to the edge of the visible universe is about 45.7 billion light-years in any direction; this is the comoving of the observable universe. This is larger than the age of the universe dictated by the cosmic background radiation; see here for why this is possible.


Related units
Distances between objects within a 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 , useful in astronomy, telecommunications and relativistic physics, is exactly metres or of a light-year. Units such as the light-minute, light-hour and light-day are sometimes used in 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-Travel Time and Distance by the Hayden Planetarium Accessed October 2010.

Light travels approximately one foot in a ; the term "light-foot" is sometimes used as an informal measure of time.

(2025). 9780691141275, Princeton University Press. .


See also
  • 1 petametre (examples of distances on the order of one light-year)
  • Einstein protocol
  • Hubble length
  • Orders of magnitude (length)


Notes

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