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 of | length |
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 presently defined to be equal to precisely 31557600 light-seconds, since the definition of a year is based on a Julian year (not Gregorian year) of exactly 365.25 days, each of exactly 86400 SI seconds.^{[1]}
Contents
Use in telecommunicationsEdit
Communications signals on Earth rarely travel at precisely the speed of light in free space.^{[citation needed]} 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^{[citation needed]} (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 astronomyEdit
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-second.
- The average distance between Earth and the Moon 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 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 (exact values) | km | miles | |||
light-second | 299792458 m | 2.998×10^{5} km | 1.863×10^{5} mi | average distance from the Earth to the Moon is about 1.282 light-seconds | |
---|---|---|---|---|---|
light-minute | 60 light-seconds | 1.798754748×10^{10} m | 1.799×10^{7} km | 1.118×10^{7} mi | average distance from the Earth to the Sun is 8.317 light-minutes |
light-hour | 60 light-minutes = 3600 light-seconds |
1.0792528488×10^{12} m | 1.079×10^{9} km | 6.706×10^{8} mi | semi-major axis of Pluto's orbit is about 5.473 light-hours |
light-day | 24 light-hours = 86400 light-seconds |
2.59020683712×10^{13} m | 2.590×10^{10} km | 1.609×10^{10} 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 |
1.813144785984×10^{14} m | 1.813×10^{11} km | 1.127×10^{11} 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 |
9.4607304725808×10^{15} m | 9.461×10^{12} km | 5.879×10^{12} mi | Proxima Centauri is the nearest star to the Sun, about 4.24 light years away |
See alsoEdit
ReferencesEdit
- ^ IAU Recommendations concerning Units Archived 2007-02-16 at the Wayback Machine
- ^ David Mermin suggested one light-nanosecond might be called a phoot at page 22 of It's About Time (2005), Princeton University Press
- ^ 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..
- ^ McCarthy, Dennis D.; Petit, Gérard, eds. (2004). "IERS Technical Note No. 32". Frankfurt: Bundesamts für Kartographie und Geodäsie. ISBN 3-89888-884-3.
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