Friday, 1 May 2015

Speed of light

The speed of light in vacuum, commonly denoted c, is a universal physical constant important in many areas of physics. Its value is exactly 299792458792458 metres per second, as the length of the metre is defined from this constant and the international standard for time. According to special relativityc is the maximum speed at which all matter and information in the universe can travel. It is the speed at which all massless particles and changes of the associated fields (including electromagnetic radiation such as light and gravitational waves) travel in vacuum. Such particles and waves travel at c regardless of the motion of the source or the inertial frame of reference of the observer. In the theory of relativityc interrelates space and time, and also appears in the famous equation of mass–energy equivalence E = mc2.
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The speed at which light propagates through transparent materials, such as glass or air, is less than c. The ratio between c and the speed v at which light travels in a material is called the refractive index n of the material (n = c / v). For example, for visible light the refractive index of glass is typically around 1.5, meaning that light in glass travels at c / 1.5 ≈ 200000 km/s; the refractive index of air for visible light is about 1.0003, so the speed of light in air is about 299700700 km/s or 90 km/s slower than c.
     Actually when you see an object it the space literally you are seeing the past of object. The time of the object depends on how far the object is and how much time the light from the object is. 
Eg: Sunlight takes about 8 minutes 17 seconds to travel the average distance from the surface of the Sun to the Earth. Then the sun you are seeing is literally 8mins and 17 sec in the past

The distance from the Sun to the Earth is shown as 150 million kilometers, an approximate average. Sizes to scale.
Sunlight takes about 8 minutes 17 seconds to travel the average distance from the surface of the Sun to the Earth.

Exact values
metres per second299792458
Planck length per Planck time
(i.e., Planck units)
1
Approximate values (to three significant digits)
kilometres per hour1080 million (1.08×109)
miles per second186000
miles per hour671 million (6.71×108)
astronomical units per day173[Note 1]
Approximate light signal travel times
DistanceTime
one foot1.0 ns
one metre3.3 ns
from geostationary orbit to Earth119 ms
the length of Earth's equator134 ms
from Moon to Earth1.3 s
from Sun to Earth (1 AU)8.3 min
one light year1.0 year
one parsec3.26 years
from nearest star to Sun (1.3 pc)4.2 years
from the nearest galaxy (the Canis Major Dwarf Galaxy) to Earth25000 years
across the Milky Way100000 years
from the Andromeda Galaxy to Earth2.5 million years
from Earth to the edge of the observable universe46.5 billion years

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