Light is
electromagnetic radiation of a
wavelength that's visible to the
eye (
visible light). In a
scientific context, the word "light" is sometimes used to refer to the entire
electromagnetic spectrum. Light is composed of an
elementary particle called a
photon.
Three primary properties of light are:
Light can exhibit properties of both
waves and
particles. This property is referred to as wave/particle duality. The study of light, known as
optics, is an important research area in modern
physics.
Speed of light
The speed of light in a
vacuum is fixed by definition to be exactly 299,792,458
m/s. The speed of light depends upon the medium in which it's traveling and the speed will be lower in a transparent medium. Although commonly called the "velocity of light", technically the word
velocity is a
vector quantity, having both magnitude and direction.
Speed refers only to the magnitude of the velocity vector. This fixed definition of the speed of light is a result of the modern attempt, in physics, to define the basic unit of length in terms of the speed of light, rather than defining the speed of light in terms of a length.
Different physicists have attempted to measure the speed of light throughout history.
Galileo attempted to measure the speed of light in the seventeenth century. A good early experiment to measure the speed of light was conducted by
Ole Rømer, a Danish physicist, in
1676. Using a telescope, Ole observed the motions of
Jupiter and one of its
moons,
Io. Noting discrepancies in the apparent period of Io's orbit, Rømer calculated that light takes about 18 minutes to traverse the diameter of Earth's orbit. Unfortunately this wasn't a value that was known at that time. If Ole had known the diameter of the Earth's orbit he'd have calculated a speed of 227,000,000 m/s.
Another, more accurate, measurement of the speed of light was performed in Europe by
Hippolyte Fizeau in
1849. Fizeau directed a beam of light at a mirror several kilometers away. A rotating cog wheel was placed in the path of the light beam as it traveled from the source, to the mirror and then returned to its origin. Fizeau found that at a certain rate of rotation, the beam would pass through one gap in the wheel on the way out and the next gap on the way back. Knowing the distance to the mirror, the number of teeth on the wheel, and the rate of rotation, Fizeau was able to calculate the speed of light as 313,000,000 m/s.
Léon Foucault used an experiment which used rotating mirrors to obtain a value of 298,000,000 m/s in
1862.
Albert A. Michelson conducted experiments on the speed of light from 1877 until his death in 1931. He refined Foucault's methods in 1926 using improved rotating
mirrors to measure the
time it took light to make a round trip from Mt. Wilson to Mt. San Antonio in
California. The precise measurements yielded a speed of 299,796,000 m/s.
Refraction
Light in a vacuum propagates at a maximum finite speed, defined above, and denoted by the symbol
c. While passing through any other transparent medium, the speed of light slows to some fraction of
c. The reduction of the speed of light traveling in a transparent medium is indicated by the
refractive index,
n, which is defined as:
»
As it originally stood, this theory didn't explain the simultaneous wave- and particle-like natures of light, though Planck would later work on theories that did. In 1918, Planck received the
Nobel Prize in Physics for his part in the founding of quantum theory.
Wave–particle duality
The modern theory that explains the nature of light includes the notion of
wave–particle duality, described by
Albert Einstein in the early 1900s, based on his study of the
photoelectric effect and Planck's results. Einstein asserted that the energy of a photon is proportional to its
frequency. More generally, the theory states that everything has both a particle nature and a wave nature, and various experiments can be done to bring out one or the other. The particle nature is more easily discerned if an object has a large mass, so it took until a bold proposition by
Louis de Broglie in 1924 to realise that
electrons also exhibited wave–particle duality. The wave nature of electrons was experimentally demonstrated by Davission and Germer in 1927. Einstein received the Nobel Prize in 1921 for his work with the wave–particle duality on photons (especially explaining the photoelectric effect thereby), and de Broglie followed in 1929 for his extension to other particles.
Quantum electrodynamics
The quantum mechanical theory of light and electromagnetic radiation continued to evolve through the 1920's and 1930's, and culminated with the development during the 1940's of the theory of
quantum electrodynamics, or QED. This so-called
quantum field theory is among the most comprehensive and experimentally successful theories ever formulated to explain a set of natural phenomena.
QED was developed primarily by physicists
Richard Feynman,
Freeman Dyson,
Julian Schwinger, and
Shin-Ichiro Tomonaga. Feynman, Schwinger, and Tomonaga shared the 1965 Nobel Prize in Physics for their contributions.
Light pressure
Light pushes on objects in its way, just as the wind would do. This pressure is most easily explainable in particle theory: photons hit and transfer their momentum. Light pressure can cause
asteroids to spin faster, acting on their irregular shapes as on the vanes of a
windmill. The possibility to make
solar sails that would accelerate spaceships in space is also under investigation.
Although the motion of the
Crookes radiometer was originally attributed to light pressure, this interpretation is incorrect; the characteristic Crookes rotation is the result of a partial vacuum. This shouldn't be confused with the
Nichols radiometer, in which the motion
is directly caused by light pressure.
Spirituality
The sensory perception of light plays a central role in spirituality (
vision,
enlightenment,
darshan,
Tabor Light), and the presence of light as opposed to its absence (
darkness) is a universal metaphor of
good and evil,
knowledge and
ignorance, and similar concepts.
External results
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