Light-second

The light-second is a unit of length useful in astronomy, telecommunications and relativistic physics. It is defined as the distance that light travels in free space in one second, and is equal to exactly 299,792,458 metres (983,571,056 ft).

Light-second
Unit oflength
Conversions
1 light-second in ...... is equal to ...
   SI units   299792458 m
   astronomical units   0.0020040 AU
 3.1688×10−8 ly
 9.7156×10−9 pc
   imperial/US units   186282 mi

Just as the second forms the basis for other units of time, the light-second can form the basis for other units of length, ranging from the light-nanosecond (299.8 mm or just under one international foot) to the light-minute, light-hour and light-day, which are sometimes used in popular science publications. The more commonly used light-year is also currently defined to be equal to precisely 31,557,600 light-seconds, since the definition of a year is based on a Julian year (not the Gregorian year) of exactly 365.25 days, each of exactly 86400 SI seconds.[1]

Use in telecommunications

Communications signals on Earth rarely travel at precisely the speed of light in free space. Distances in fractions of a light-second are useful for planning telecommunications networks.

  • One light-nanosecond is almost 300 millimetres (299.8 mm, 5 mm less than one foot[2]), which limits the speed of data transfer between different parts of a large computer.
  • One light-microsecond is about 300 metres.
  • The mean distance, over land, between opposite sides of the Earth is 66.8 light-milliseconds.
  • Communications satellites are typically 1.337 light-milliseconds (low earth orbit) to 119.4 light-milliseconds (geostationary orbit) from the surface of the Earth. Hence there will always be a delay of at least a quarter of a second in a communication via geostationary satellite (119.4ms times 2); this delay is just perceptible in a transoceanic telephone conversation routed by satellite. The answer will also be delayed with a quarter of a second and this is clearly noticeable during interviews or discussions on TV when sent over satellite.

Use in astronomy
The yellow shell indicating one light-day distance from the Sun compares in size with the positions of Voyager 1 and Pioneer 10 (red and green arrows respectively). It is larger than the heliosphere's termination shock (blue shell) but smaller than Comet Hale-Bopp's orbit (faint orange ellipse below). Click on the image for a larger view and links to other scales.
The faint yellow sphere centred on the Sun has a radius of one light-minute. For comparison, sizes of Rigel (the blue star in the top left) and Aldebaran (the red star in the top right) are shown to scale. The large yellow ellipse represents Mercury's orbit.

The light-second is a convenient unit for measuring distances in the inner Solar System, since it corresponds very closely to the radiometric data used to determine them. (The match is not exact for an Earth-based observer because of a very small correction for the effects of relativity.) The value of the astronomical unit (roughly the distance between Earth and the Sun) in light-seconds is a fundamental measurement for the calculation of modern ephemerides (tables of planetary positions). It is usually quoted as "light-time for unit distance" in tables of astronomical constants, and its currently accepted value is 499.004786385(20) s.[3][4]

  • The mean diameter of Earth is about 0.0425 light-seconds.
  • The average distance between Earth and the Moon (the lunar distance) is about 1.282 light-seconds.
  • The diameter of the Sun is about 4.643 light-seconds.
  • The average distance between Earth and the Sun (the astronomical unit) is 499.0 light-seconds.

Multiples of the light-second can be defined, although apart from the light-year, they are more used in popular science publications than in research works. For example, a light-minute is 60 light-seconds, and the average distance between Earth and the Sun is 8.317 light-minutes.

Unit Definition Distance Example
  m km miles  
light-second   299792458 m2.998×105 km1.863×105 mi average distance from the Earth to the Moon is about 1.282 light-seconds
light-minute 60 light-seconds 17987547480 m1.799×107 km1.118×107 mi average distance from the Earth to the Sun is 8.317 light-minutes
light-hour 60 light-minutes
= 3600 light-seconds		 1079252848800 m1.079×109 km6.706×108 mi semi-major axis of Pluto's orbit is about 5.473 light-hours
light-day 24 light-hours
= 86400 light-seconds		 25902068371200 m2.590×1010 km1.609×1010 mi Sedna is currently 0.52 light-days from the Sun; on an orbit that varies from a perihelion of 0.44 light-days to an aphelion of 5.41 light-days
light-week 7 light-days
= 604800 light-seconds		 181314478598400 m1.813×1011 km1.127×1011 mi The Oort cloud is thought to extend between 41 and 82 light-weeks out from the Sun
light-year 365.25 light-days
= 31557600 light-seconds		 9460730472580800 m9.461×1012 km5.879×1012 mi Proxima Centauri is the nearest star to the Sun, about 4.24 light years away

See also

References
  1. IAU Recommendations concerning Units Archived 2007-02-16 at the Wayback Machine
  2. David Mermin suggested one light-nanosecond might be called a phoot at page 22 of It's About Time (2005), Princeton University Press
  3. Standish, E. M. (1998). "JPL Planetary and Lunar Ephemerides, DE405/LE405" (PDF). JPL IOM 312.F-98-048. Archived from the original (PDF) on 2012-02-20..
  4. McCarthy, Dennis D.; Petit, Gérard, eds. (2004). "IERS Conventions (2003)". IERS Technical Note No. 32. Frankfurt: Bundesamts für Kartographie und Geodäsie. ISBN 3-89888-884-3.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.