Word
Gems
What is a
man but the sum of his thoughts?
Chemistry
& Physics:
Light:
Wikipedia Encyclopedia
- from http://en.wikipedia.org/wiki/Light
Light
From Wikipedia, the free encyclopedia.
Light often means the portion of the electromagnetic spectrum
visible to the human eye, but can also refer to other forms of electromagnetic radiation.
The three basic dimensions of light (and of all electromagnetic radiation) are brilliance
(or amplitude), color (or frequency), and polarization
(or angle of vibration). Due to wave-particle duality, light
simultaneously exhibits properties of both waves and particles.
- Particle
Theory
- First proposed by Isaac Newton in the seventeenth century
- Argues that light is made up of tiny particles of matter (corpuscles)
- Corpuscles are emitted in all directions
- Supports the fact that light is reflected
- Argues that light speeds up upon entering a denser medium because gravitational pull is
greater
- Greatly discounted by wave theory
- Wave (or
Ray) Theory
- First proposed by Christian Huygens in the
seventeenth century
- Argues that light is emitted as a series of waves only
- Waves are emitted in all directions
- Waves not affected by gravity, so they slow down upon entering a denser medium
- Greatly discounted the corpuscular theory
- Can interfere with each other like sound waves (noted in eighteenth
century by Thomas Young)
- Waves can be polarized
- Assumes that light needs a medium for transmission like sound
- Quantum
(or Wave-particle duality)
Theory
- Combines previous three theories
- Pioneered at end of the nineteenth century
- Max Planck proposed that light waves are made of packets of energy known as quanta or photons in 1900
- Light behaves as both particles and waves
Visible light is that portion of the spectrum between the wavelengths of about
400 nanometers
(abbreviated nm) and 800 nm (in air). Light can also be characterized by its
frequency. The frequency and wavelength of light obey the relation
(see speed of light)
- v = ?f,
where ? is the wavelength, f is the frequency, v is the
speed of the light. If the light is travelling in a vacuum, then v = c,
thus
- c = ?f,
where c is the speed of light. We can express v as
where n is a constant (the refractive index) which is a
property of the material through which the light is passing.
All light propagates at a finite speed. Even moving observers always measure the same
value of c, the speed of light in vacuum, as c
= 299,792,458 metres
per second;
however, when light passes through a transparent substance such as air, water or glass,
its speed is reduced, and it suffers refraction. Thus, n=1 in a
vacuum and n>1 in matter. It is a violation of the technical
terminology of physics to speak of the "velocity of
light;" velocity is reserved for a different use.
The speed of light has been measured many times, by many physicists. The best early
measurement is Olaus Roemer's (a Danish physicist),
in 1676. He
had developed a method for measuring light. He observed and noted the motions of Jupiter and one of its moons with a telescope. It was
possible to time the revolution of the moon because it was eclipsed
by Jupiter at regular intervals. Roemer discovered that
the moon revolved around Jupiter once every 42-1/2 hours when Earth was closest to Jupiter. The problem
was that when Earth and Jupiter were not as close, the moon's revolution seemed to be
more. It was clear that light took longer to reach Earth when it was farther away from
Jupiter. The speed of light was calculated by analyzing the distance between the two planets at
various times. Roemer reached a speed of 227,000 kilometers per second (approximately
141,050 miles
per second).
Albert A. Michelson improved
on Roemer's work in 1926. He used 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 186,285 miles/second (299,796 kilometers/second).
In daily use, the figures are rounded off to 186,000 mi/sec and 300,000 km/sec.
The study of light and the interaction of light and matter is termed optics. The observation and
study of optical phenomena such as rainbows
offers many clues as to the nature of light as well as much enjoyment.
The different wavelengths are interpreted by the human brain as colors, ranging from red at the
longest wavelengths (lowest frequencies) to violet at the shortest wavelengths (highest
frequencies). The intervening frequencies are seen as orange, yellow, green, blue, and,
conventionally, indigo. The frequencies of the spectrum
immediately outside the range the human eye is able to perceive are called ultraviolet
(UV) at the high frequency end and infrared (IR) at the low. Though
humans cannot see IR, we do perceive it by receptors in the skin as heat. Cameras that can pick up IR
and convert it to visible light are called night-vision cameras. UV radiation is
not perceived by humans at all except in a very delayed fashion, as overexposure of the
skin to UV light causes sunburn, or skin cancer. Some
animals, such as bees,
can see UV radiation while others, such as pit viper snakes, can see IR using pits in their
heads.
The following quantities and units are used to measure light.
- brightness
(or temperature)
- illuminance or illumination (SI unit: lux)
- luminous flux (SI unit: lumen)
- luminous intensity (SI unit: candela)
See also: Photometry

The only characteristic of the wave not seen here (because of need for the passage of
time) is frequency.
See also: Huygens' principle, Color temperature, Illumination,
International
Commission on Illumination, Wave-particle duality, Light pollution, photic sneeze reflex
|