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Speed of light

 
Sci-Tech Dictionary: speed of light
 
(′spēd əv ′līt)

(electromagnetism) The speed of propagation of electromagnetic waves in a vacuum, which is a physical constant equal to exactly 299,792.458 kilometers per second. Also known as electromagnetic constant; velocity of light.


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All electromagnetic radiation, including light, radio transmission and electricity, travels at approximately 186,000 miles (300,000 kilometers) per second; more than seven times around the equator in one second. More precisely, the speed is 299,792,458 meters per second in a vacuum.

Never Fast Enough!

This inherent speed of Mother Nature is why computers work so fast. Within the tiny chip, electricity has to flow only a couple of millimeters, and, within an entire computer, only a few feet. Yet, as fast as that is, it is never fast enough. There is resistance in the lines, which slows down the current, and even though transistors switch in billionths of a second, scientific and multimedia applications are always exhausting the fastest computers.

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Hacker Slang: speed of light
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The absolutely fastest a particular algorithm or application could be implemented, given a set of constraints that are assumed to be unchangeable. For example, “This would take 60 microseconds without any processing whatsoever, so that's the speed of light.” However, as one brilliant hacker once commented: “Remember that the speed of light only is constant if you can't redesign the universe.


 
Dental Dictionary: speed of light
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n

A speed of 186,300 miles/sec.

 
Measures and Units: speed of light
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Essentially the speed of radio and other electromagnetic waves too, the speed of light depends on transmission medium. The maximum speed, labelled c and often referred to as the speed of light without qualification, occurs in a vacuum, it equals 299 792 458 m·s-1 (1.079 252 85~ × 109 km/h, 670.616 629~ × 106 m.p.h.), the first figure being precise since the 1983 re-definition of the metre. (That light has finite speed was accepted after Ole Rømer correctly forecast in 1679 that an eclipse of Io by Jupiter would be seen 10 minutes later than expected.)

Outside of electromagnetic radiations and accelerated atomic and sub-atomic particles, no speeds achieved by the physical creations of mankind are more than a minor fraction of such a speed.

197515th CGPM: ‘considering the excellent agreement among the results of wavelength measurements on the radiations of lasers locked on a molecular absorption line in the visible or infrared region, with an uncertainty estimated at ±4 × 10-9 which corresponds to the uncertainty of the realization of the metre, considering also the concordant measurements of the frequencies of several of these radiations, recommends the use of the resulting value for the speed of propagation of electromagnetic waves in vacuum c = 299 792 458 metres per second.’see note below

[Le Système International d'Unités (Sèvres, France: Bureau International de Poids et Mesures, 1985)]

 
Science Q&A: What is the speed of light?
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The figure is 186,282 miles (299,792 kilometers) per second.

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Science Dictionary: speed of light
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The distance light can travel in a unit of time through a given substance. Light travels through a vacuum at about 186,000 miles, or 300,000 kilometers, per second. (See E = mc2, electromagnetic waves, relativity, and twin paradox.)

  • A light year, or the distance light can travel in a year, is over five trillion miles.
  • Light from the sun takes about eight minutes to reach the Earth.
  • Light from the moon, and other electromagnetic radiation from the moon, takes about a second and a half to reach the Earth. In conversations between astronauts on the moon and their ground crews, there are lapses of about three seconds between exchanges, because of the time it takes for radio waves to make a round trip between the Earth and the moon.
  • The special theory of relativity states that the speed of light as measured by all observers is the same.
  •  
    Essay: Velocity of light
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    Most ancients, and even later scientists such as Johannes Kepler and René Descartes, believed the velocity of light to be infinite. Galileo thought otherwise and tried to measure light velocity with a method that had worked successfully for the measurement of the velocity of sound by Mersenne. Galileo and an assistant placed themselves on two hilltops some distance apart. Galileo flashed a light signal and the assistant responded by flashing a light signal in return as soon as he could see Galileo's light flash. Galileo then measured the time elapsed between the emission of his light signal and the return of the light signal from his assistant. Galileo soon realized that the elapsed time measured was independent of the distance to the assistant. Instead, the elapsed time was the time needed for the assistant to react to Galileo's signal.

    The Danish astronomer Ole Römer solved the problem by using a much longer distance over which to measure the velocity of light. He noticed that when Earth and Jupiter were on the same side of the Sun, the eclipses of Jupiter's satellites by the planet occurred a few minutes earlier than when the Sun was between Earth and Jupiter. Römer determined that it took 16 minutes longer for the light to travel when Earth was the farthest away from Jupiter than when Earth was closest. Römer deduced rightly that these 16 minutes were the time needed for the light to cover the distance between the closest and farthest positions of Jupiter. Römer calculated that the speed of light is 240,000 km (150,000 mi) per second.

    Precise measurements of the velocity of light were made in the 19th century using specially designed apparatuses. These relied on the wave phenomenon of interference, where the crests of light waves of the same frequency either enhance each other or cancel each other. With lasers, it is possible to have light waves with exact frequencies, making this method extremely accurate. As a result, the speed of light in a vacuum, which is always constant, is, along with the second, the basis of our system of measurement. Since 1983 the meter has been defined as the distance light travels in 1/299,792,458 second; the speed of light is exactly 299,792,458 meters per second. Furthermore, since the American inch is defined by Congress as 2.54 times the centimeter, the speed of light is exactly 186,292.03 miles per second.

     
    Wikipedia: Speed of light
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    Here, laser light in air is traveling at 99.97% the speed of light in a vacuum.[1]

    The speed of light normally refers the speed of light in a vacuum, and is an important physical constant in modern physics. Light travels at different speeds through different materials, but it travels fastest in vacuum and its speed does not vary with the color, intensity, or direction of travel.[2] Perhaps more surprisingly, the speed also does not depend on the motion of the light emitter or the observer. Therefore it makes sense to speak of the speed of light, which is the speed of light in vacuum and usually represented as c. The speed of light factors into much of modern physics, including special relativity, general relativity, and quantum mechanics.

    By everyday standards, light travels very rapidly - approximately 300,000 km each second, in vacuum or air. This is roughly a million times faster than sound, and fast enough to circle the Earth more than 7 times in one second. Such a rapid speed is very hard to measure without specialized techniques, and in ancient times the speed of light was the subject of speculation. The first effective measurements of the speed of light were made in the seventeenth century, and were progressively refined. Today, time intervals can be measured extremely precisely, to the point where the metre is now defined officially as the distance light travels in "vacuum" in 1299,792,458 of a second. As a consequence, according to NIST: "… the effect of this definition is to fix the speed of light in vacuum at exactly 299 792 458 m/s." (Further discussion is found later in the subsection Speed of light set by definition.)

    The speed of light plays a crucial role in both classical and modern physics. Maxwell in the 19th century provided the first explanation of the speed of light in relation to other physical constants.[3] In the early 20th century c assumed an even greater importance as a pivotal constant in Einstein's theory of special relativity, which holds that the speed of light has a special role connecting space and time in the structure of spacetime. As one result, the speed of light sets an absolute speed limit to how fast matter or information can move. As another result, energy and mass are connected by the speed of light in the famous mass-energy equation E = mc2. This relationship is a foundation of quantum mechanics, including nuclear energy. General relativity further explains gravity as an effect of curved space time, and in this theory all distances must be computed using c. Today, the speed of light continues to be a subject of research, both in theory and experiment.

    For many practical purposes, the speed of light is so great that it can be regarded to travel instantaneously. However, the finite speed of light becomes noticeable when very long distances, very short time intervals, or precise time measurements are involved. For instance, the speed of light is a critical factor in astronomy, modern electronics, and navigation systems such as global positioning systems.

    Notation and units

    Speed of light in different units
    metres per second 299,792,458 (exact)
    km per hour 1,079,252,848.8 (exact)
    miles per hour ≈ 671,000,000
    miles per second ≈ 186,000
    Approximate length of time for light to travel...
    One foot 0.98 nanoseconds
    One metre 3.3 nanoseconds
    One km 3.3 microseconds
    One mile 5.4 microseconds
    To Earth from geostationary orbit 0.12 seconds
    Around Earth's equator 0.13 seconds
    To Earth from the moon 1.3 seconds
    To Earth from the sun 8.3 minutes
    To Earth from Alpha Centauri 4.4 years
    Across the Milky Way 100,000 years

    The symbol "c" for "constant" or the Latin celeritas (meaning “swiftness”)[4] is used for the speed of light in free space, and in this article c is used exclusively this way. Some authors, however, use "c" for the speed of light in any material medium, and "c0" for the speed of light in free space.[5] This notation, which is endorsed in official SI literature,[6][7] produces consistency with other constants of free space such as μ0, ε0 and Z0.

    In branches of physics in which the speed of light plays an important part, such as in relativity, it is common to use a system of units known as natural units in which c is 1; thus no symbol for the speed of light is required.

    When physicists refer to the speed of light in "vacuum", most commonly they mean free space, which means classically a region void of all matter and fields. Such an ideal vacuum is unrealizable in practice: for example, interstellar space and terrestrial vacuums are only approximations. Therefore, measurements in real (imperfect) vacuums are related to those in "vacuum" using evolving corrections conforming to "best good practice" as defined by standards organizations and scientific and technical publications.[8] In this article, "vacuum" refers to the hypothetically perfect vacuum of free space unless otherwise specified.

    As light propagates down the telescope, the telescope moves requiring a tilt to the telescope that depends on the speed of light. The apparent angle of the star φ differs from its true angle θ, a phenomenon called stellar aberration

    Practical effect of the finite speed of light

    The speed of light plays an important part in many modern sciences and technologies. Radar systems measure the distance to a target by measuring the time taken for an echo of the light pulse to return. Similarly, a global positioning system (GPS) receiver measures its distance to satellites based on how long it takes for a radio signal to arrive from the satellite. The distances to the moon, planets, and spacecraft are determined by measuring the round-trip travel time.

    Another effect of the finite speed of light is stellar aberration. Suppose we look at a star with a telescope idealized as a narrow tube. The light enters the tube from a star at angle θ and travels at speed c taking a time h/c to reach the bottom of the tube, where our eye detects the light. Suppose observations are made from Earth, which is moving with a speed v. During the transit of the light, the tube moves a distance vh/c. Consequently, for the photon to reach the bottom of the tube, the tube must be inclined at an angle φ different from θ , resulting in an apparent position of the star at angle φ.

    In astronomy beyond the solar system, distances are often measured in light-years, the distance light travels in a year.

    In electronic systems, despite their small size, the speed of light can become a limiting factor in their maximum speed of operation.[9][10]

    Fundamental importance in physics

    Light as electromagnetic radiation

    Light is a form of electromagnetic radiation[11]. In classical electromagnetism, its speed is determined by the electromagnetic wave equation, which is derived from Maxwell's equations.

    In SI units the speed of all electromagnetic radiation in free space is related to the electric constant ε0 (also called the permittivity of free space) and the magnetic constant μ0 (also called the permeability of free space) by the equation c02=1/(ε0 μ0)[12] . As speed of light in free space is fixed by definition and the value of the magnetic constant is defined [13] to be 4π×10−7 H/m the value of the electric constant is now also fixed.

    In Gaussian units, the speed of light fixes the ratio between electrostatic and electromagnetic units.

    According to classical electromagnetism, the speed of electromagnetic radiation in free space is the same for all frequencies. This has been confirmed to a high degree of accuracy by experiment. [14][15] [16]

    A more complete theory of light and its interaction with matter is given by quantum electrodynamics in which c plays the role of a fundamental constant.

    Spacetime constant

    The speed of light is a fundamental constant of the spacetime in which we live. Light is measured to travel at the same speed in all inertial frames regardless of the motion of the source, although the observed frequency may change due to the Doppler effect.

    Experimental evidence has shown that the speed of light is independent of the motion of the source.[17][18] It has also been confirmed by the Michelson-Morley experiment and others that the two-way speed of light (for example from a source, to a mirror, and back again) is constant.[19][20] It is not, however, possible to measure the one-way speed of light (for example from a source to a distant detector) without some convention as to how clocks at the source and receiver should be synchronized.[21] Einstein (who was aware of this fact) postulated that the speed of light should be taken as constant in all cases, one-way and two-way. This postulate, together with the principle of relativity that all inertial frames are equivalent, forms the basis of Einstein's theory of special relativity, in which space and time are viewed as a four dimensional unification of space and time, known as spacetime,[22] with c playing the fundamental role of a conversion factor between the units of space and time, and mass and energy.[23]

    The finite speed of light in relativity leads to some counter-intuitive consequences, which include length contraction, time dilation and the relativity of simultaneity, this last item contradicting the classical notion that the duration of the time interval between two events is equal for all observers.

    In Einstein's general theory of relativity, spacetime is curved by the presence of matter and energy causing gravitation.[24] Disturbances in this curvature, including gravitational waves, propagate at the speed of light.[25][26]

    Causality and information transfer

    A light cone defines locations that are in causal contact and those that are not.

    According to the theory of special relativity, causality would be violated if information could travel faster than c in some reference frame, In some other reference frames, the information would be received before it had been sent, so the "effect" could be observed before the "cause". Such a violation of causality has never been recorded.[21]

    Information propagates to and from a point forming regions defined by a light cone. The interval AB in the diagram to the right is "time-like" (that is, there is a frame of reference in which event A and event B occur at the same location in space, separated only by their occurring at different times, and if A precedes B in that frame then A precedes B in all frames: there is no frame of reference in which event A and event B occur simultaneously). Thus, it is hypothetically possible for matter (or information) to travel from A to B, so there can be a causal relationship (with A the "cause" and B the "effect"). In other words, c represents the maximum speed at which matter, energy, or information can be transmitted.

    On the other hand, the interval AC in the diagram to the right is "space-like" (that is, there is a frame of reference in which event A and event C occur simultaneously, separated only in space; see simultaneity). However, there are also frames in which A precedes C (as shown) or in which C precedes A. Barring some way of traveling faster than light, it is not possible for any matter (or information) to travel from A to C or from C to A. Thus there is no causal connection between A and C.

    Speed of light in various systems

    Light in free space

    Free space is a reference state. Like absolute zero, it is an idealized state that only can be approximated in the physical world. Measurements in any real-world medium, such as air[27][28] or a medium perturbed by gravity must be corrected so as to relate to free space.

    Light in transparent media

    The refractive index of a transparent material indicates how much slower light propagates in that medium than in a vacuum. This slowing causes refraction. Classically, when an electromagnetic wave meets the surface of a dielectric material at an angle, the leading edge is slowed while the trailing edge continues normally. This causes the wave to change direction, as demonstrated by this prism (in the case of a prism splitting white light into a spectrum of colours, the refraction is known as dispersion).

    When a light pulse comprised of multiple frequencies passes through transparent materials, the speed of light is characterized by two speeds: the phase velocity and the group velocity. The phase velocity of light may be found from knowledge of the frequency-dependent refractive index:

     n=\sqrt{\epsilon_r\mu_r} = c_0 / v_p

    where εr is the material's relative permittivity, and μr is its relative permeability.

    The group velocity of the wave is the speed at which the envelope of the pulse travels through the medium, and is dependent on the frequency content of the pulse as well as the properties of the medium. A wave with different group and phase velocities is said to undergo dispersion. If the light passing through the medium is monochromatic, the phase velocity is often referred to as the "speed of light".

    When light enters materials its energy is absorbed. In the case of transparent materials (dielectrics) this energy is quickly re-radiated. However, this absorption and re-radiation introduces a delay. As light propagates through dielectric material it undergoes continuous absorption and re-radiation. Therefore when the speed of light in a medium is said to be less than c, this should be read as the speed of energy propagation at the macroscopic level. At an atomic level, electromagnetic waves always travel at c in the empty space between atoms. Two factors influence this slowing; stronger absorption leading to shorter path length between each re-radiation cycle and longer delays. The slowing is therefore the product of these two factors. This reduction in speed is also responsible for bending of light at an interface between two materials with different refractive indices, a phenomenon known as refraction.

    The refractive index in air is only slightly larger than one [1]. Denser media, such as water and glass, have refractive indices of between 1.3 and 1.5 for visible light. Diamond has a refractive index of about 2.4.

    History

    Until relatively recent times, whether the speed of light was infinite was unknown. The debate began in ancient Greece. Empedocles maintained that light was something in motion, and therefore there had to be some time elapsed in traveling. Aristotle said that, on the contrary, "light is due to the presence of something, but it is not a movement".[29] Euclid and Ptolemy advanced the emission theory of vision, which claimed light was emitted from the eye, thus enabling sight. Using that theory, Heron of Alexandria advanced the argument that the speed of light must be infinite, since distant objects such as stars appear immediately upon opening the eyes.

    Early Muslim philosophers initially agreed with the Aristotelian view of the speed of light being infinite. In 1021, Iraqi physicist Alhazen (Ibn al-Haytham) published the Book of Optics, in which he used experiments related to the camera obscura to support the intromission theory of vision, which claimed that light moves from an object into the eye.[30] This led to Alhazen proposing that light must therefore have a finite speed,[29][31][32] and that the speed of light is variable, with its speed decreasing in denser bodies.[32][33] He argued that light is a “substantial matter”, the propagation of which requires time "even if this is hidden to our senses".[34] This debate continued in Europe and the Middle East throughout the Middle Ages.

    Also in the 11th century, Abū Rayhān al-Bīrūnī agreed that light has a finite speed, and observed that the speed of light is much faster than the speed of sound.[35] In the 1270s, Witelo considered the possibility of light traveling at infinite speed in a vacuum but slowing down in denser bodies.[36] A comment on a verse in the Rigveda by the 14th century Indian scholar Sayana[37] may be interpreted as suggesting an estimate for the speed of light that is in good agreement with its actual speed. In 1574, the Ottoman astronomer and physicist Taqi al-Din concluded that the speed of light is constant, but variable in denser bodies, and suggested that it would take a long time for light from the stars which are millions of kilometres away to reach the Earth.[38]

    Early attempts to measure the speed of light

    In the early 17th century, Johannes Kepler believed that the speed of light was infinite since empty space presents no obstacle to it. Francis Bacon argued that the speed of light was not necessarily infinite, since something can travel too fast to be perceived. René Descartes argued that if the speed of light were finite, the Sun, Earth, and Moon would be noticeably out of alignment during a lunar eclipse. Since such misalignment had not been observed, Descartes concluded the speed of light was infinite. Descartes speculated that if the speed of light was found to be finite, his whole system of philosophy might be demolished.[29]

    In 1629, Isaac Beeckman proposed an experiment in which a person would observe the flash of a cannon reflecting off a mirror about one mile (1.6 km) away. In 1638, Galileo Galilei proposed an experiment, with an apparent claim to having performed it some years earlier, to measure the speed of light by observing the delay between uncovering a lantern and its perception some distance away. He concluded that the speed of light is ten times faster than the speed of sound, a figure now known to be much too slow.[32] Galileo's experiment was carried out by the Accademia del Cimento of Florence in 1667, with the lanterns separated by about one mile (1.6 km), but no delay was observed. Based on the modern value of the speed of light, the actual delay in this experiment would be about 11 microseconds. Robert Hooke explained the negative results as Galileo had by pointing out that such observations did not establish the infinite speed of light, but only that the speed must be very great.

    Astronomical techniques

    Rømer's observations of the occultations of Io from Earth.

    The first quantitative estimate of the speed of light was made in 1676 by Ole Christensen Rømer, who was studying the motions of Jupiter's moon, Io, with a telescope. It is possible to time the orbital revolution of Io because it enters and exits Jupiter's shadow at regular intervals (at points C and D in the diagram at right). Rømer observed that Io revolved around Jupiter once every 42.5 hours when Earth was closest to Jupiter (at H). He also observed that, as Earth and Jupiter moved apart, (as from L to K), Io's exit from the shadow would begin progressively later than predicted. He realized that these exit "signals" took longer to reach Earth as a result of the extra time it took for light to cross the extra distance between the moving planets. The opposite is the case when they are approaching (as from F to G). Rømer observed 40 orbits of Io when Earth was approaching Jupiter to be 22 minutes shorter than 40 orbits of Io when Earth was moving away from Jupiter.[39] On the basis of those observations, Rømer concluded that it took light 22 minutes to cross the distance the Earth traversed in 80 orbits of Io.[39] This means that in traveling from L to K and F to G, whereas the earth took 80 periods of Io's orbits (42.5 hours), the light only took 22 minutes. This corresponds to a ratio between the speed of light and the speed at which the Earth travels in its orbit around the sun of 9,300. The modern value of the ratio is about 10,100.

    Around the same time, the astronomical unit (roughly, the Earth-to-Sun distance) was estimated to be about 140 million kilometres (87 million miles). The astronomical unit and Rømer's time estimate were combined by Christiaan Huygens, who estimated the speed of light to be 1,000 Earth diameters per minute, based on having misinterpreted Rømer's value of 22 minutes to mean the time it would take light to cross the diameter of the orbit of the Earth.[39] This is about 220,000 kilometres per second (136,000 miles per second), 26% lower than the currently accepted value, but still very much faster than any physical phenomenon then known.

    Isaac Newton also accepted the finite speed. In his 1704 book Opticks he reports the value of 16.6 Earth diameters per second (210,000 kilometres per second. The same effect was subsequently observed by Rømer for a "spot" rotating with the surface of Jupiter. Later observations also showed the effect with the three other Galilean moons, where it was more difficult to observe, thus laying to rest some further objections that had been raised.

    In 1728, James Bradley deduced that starlight falling on the Earth should appear to come from a slight angle, which could be calculated by comparing the speed of the Earth in its orbit to the speed of light. This "aberration of light", as it is called, was observed to be about 1/200 of a degree. Bradley calculated the speed of light as about 298,000 kilometres per second (186,000 miles per second).

    Earth-bound techniques

    Diagram of the Fizeau apparatus.

    The first successful entirely earthbound measurement of the speed of light was carried out by Hippolyte Fizeau in 1849. Fizeau's experiment was conceptually similar to those proposed by Beeckman and Galileo. A beam of light was directed at a mirror 8 km away. On the way from the source to the mirror, the beam passed through a rotating cog wheel. At a certain rate of rotation, the beam could pass through one gap on the way out and another on the way back. But at slightly higher or lower rates, the beam would strike a tooth and not pass through the wheel. Knowing the distance to the mirror, the number of teeth on the wheel, and the rate of rotation, the speed of light could be calculated. Fizeau reported the speed of light as 313,000 kilometres per second. Leon Foucault improved on Fizeau's method by replacing the cogwheel with a rotating mirror. Foucault's estimate, published in 1862, was 298,000 kilometres per second.

    In 1861 Maxwell proposed a theory which linked the speed of light to the electromagnetic field.[3] In 1864 Maxwell compared known measurements of the speed of light with the ratio of electrostatic to electromagnetic units by Weber and Kohlrausch to support the connection between light and electromagnetic phenomena.[3] Maxwell’s equations allow the speed of light to be calculated, in much the same way as the speed of sound can be calculated in normal matter.

    A schematic representation of a Michelson interferometer, as used for the Michelson-Morley experiment. The point of reflection on the tilted beam splitter is shown as two separated points for clarity. Both beams travel equal length paths. If light speed is anisotropic, the interference pattern seen at the detector will vary with orientation of the apparatus.

    The 'luminiferous aether'

    After some proposals in the 17th and 18th century, Augustin Fresnel in 1818 argued that light moved through a rigid and stationary aether as a way to explain the existence of aberration and polarization. And because of James Clerk Maxwell's (1861) aether based concept of electromagnetism, the existence of the aether was widely accepted. In 1887, physicists Albert Michelson and Edward Morley designed an experiment to measure the velocity of the Earth through the aether.[40] As the Earth is in orbit round the sun, and the aether was assumed to be fixed, the Earth would be expected to be in motion with respect to the aether for at least some of the time.[41] As shown in the diagram of a Michelson interferometer, a half-silvered mirror was used to split a beam of monochromatic light into two beams traveling at right angles to one another. After leaving the splitter, each beam was reflected back and forth between mirrors several times then recombined to produce a pattern of constructive and destructive interference. Any slight change in speed of light along one arm of the interferometer compared with its speed along the other arm would then be observed as a change in the pattern of interference. The experiment gave a null result. Some interesting details of these experiments are found in Hollberg et al.[42] Later experiments confirmed this result to a much higher accuracy.[43][44]

    At the beginning the experiment was not understood as disproving the existence of the luminiferous aether, and so some hypothesis (like the Aether drag hypothesis or the Lorentz–Fitzgerald contraction) were made to explain the result within the framework of an aether. So it lasted until the beginning of the 20th century, when some physicists cast doubt on the existence of the aether. Eventually Einstein showed that the aether was not necessary. His theory of special relativity explains the null result of the Michelson–Morley experiment by postulating that the speed of light is always the same for all inertial observers. This means that the speed of light will always be the same in both arms of the interferometer, regardless of their orientation or state of inertial motion, thus no changes in the observed fringes would be expected when it was rotated. Einstein later published his general theory of relativity, which extended his special theory to include gravitation, and the concept of aether rapidly fell into disuse and it forms no part of physics today.

    Modern methods

    Electromagnetic standing waves in a cavity. Sinusoidal waves at the top have larger frequencies than below and are shifted upward for clarity. The conductive walls require the nodes of the standing wave to be at the wall surfaces, so the allowed wavelengths are: λ/2 = W, λ = W, 3λ/2 = W where W = width of cavity.

    During World War II, the development of the cavity resonance wavemeter for use in radar, together with precision timing methods, opened the way to laboratory-based measurements of the speed of light. In 1946, Louis Essen and A.C. Gordon-Smith used a microwave cavity of precisely known dimensions to establish the frequency for a variety of normal modes of microwaves. As the wavelength of the modes was known from the geometry of the cavity and from electromagnetic theory, knowledge of the associated frequencies enabled a calculation of the speed of light.

    The Essen-Gordon-Smith result, 299 792 ± 3 km/s, was substantially more precise than those found by optical techniques, and prompted much controversy. However, by 1950 repeated measurements by Essen established a result of 299 792.5 ± 1 km/s, which became the value adopted by the 12th General Assembly of the Radio-Scientific Union in 1957.

    An idealized interferometric determination of wavelength obtained by looking at interference fringes between two coherent beams recombined after traveling different distances. Top: Constructive interference (in phase); If the difference in path length is a multiple of a wavelength, the recombined beams support one another and reconstitute the original beam. Bottom: Destructive interference (out of phase); If the two paths differ by half a wavelength, the recombined beams are out of phase and cancel each other. The bottom panel in the figure suggests the path length has been increased by half a wavelength by moving the right-hand point of reflection further out.

    An alternative to the cavity resonator method to find the wavelength for determining the speed of light is to use a form of interferometer, indicated schematically in the figure.[45] A coherent light beam with a known frequency, as from a laser, is split to follow two paths and then recombined. By carefully changing the path length and observing the interference pattern, the wavelength of the light can be determined, which can be related to the speed of light.

    With modern electronics, particularly oscilloscopes with time resolutions of less than one nanosecond, the speed of light can now be directly measured by timing the delay of a light pulse from a laser or a LED in reflecting from a mirror, although this method is less precise than either the cavity resonator or the interferometric methods.[46][47][48]

    Speed of light set by definition

    For reasons stated in Resolution 1, [49] in 1983 the 17th Conférence Générale des Poids et Mesures defined the metre in terms of the distance traveled by light in a given time in perfect vacuum:[6]

    "The metre is the length of the path travelled by light in vacuum during a time interval of 1 ⁄ 299 792 458 of a second."

    A consequence of this definition is that the speed of light is a defined numerical value c = 299 792 458 m/s in "vacuum".

    Rather than measure a time-of-flight, one implementation of this definition is to use a recommended source with established frequency, and determine wavelength in terms of the metre using the defined numerical value of c as λ = c / f.[50]

    Because the second can be precisely realized, the new definition allows for a more precise definition of the metre, assuming an adequate realization of "vacuum" is available. The practical realization (or embodiment) of vacuum is obtained by measurement in a real medium (which may be simply a controlled volume of air[51]) and employing various corrections to reduce the measurements to what they are expected to be in free space. Practical realizations of the metre use recommended wavelengths of visible light in a laboratory vacuum with corrections being applied to take account of actual conditions such as diffraction, gravitation or imperfection in the vacuum.[52] With regard to the light source, as suggested by the BIPM: "it is not sufficient just to meet the specifications for the listed parameters. In addition, it is necessary to follow the best good practice concerning methods of stabilization as described in numerous scientific and technical publications."[50] Naturally, what constitutes "best good practice" evolves as measurement accuracy and reproducibility improve with advances in technique.

    Speed of light in astronomy

    The relative sizes and separation of the Earth–Moon system are shown to scale above. The beam of light is depicted traveling between the Earth and the Moon in the same time it actually takes light to scale the real distance between them: 1.255 seconds at its mean orbital distance (surface to surface). The light beam helps provide the sense of scale of the Earth-Moon system relative to the Sun, which is 8.28 light-minutes away (photosphere to Earth surface).

    The speed of light is particularly important in astronomy. Due to the vast distances involved it can take a very long time for light to travel from its source to Earth. For example, it takes 13 billion years for light to travel to Earth from the faraway galaxies viewed in the Hubble Ultra Deep Field images. Those photographs, taken today, capture images of the galaxies as they appeared 13 billion years ago (near the beginning of the universe). The fact that farther-away objects appear younger (due to the finite speed of light) is crucial in astronomy, allowing astronomers to infer the evolution of stars, galaxies, and the universe itself.

    Astronomical distances are sometimes measured in light-years, the distance light travels in one year. A light‑year is around 9 trillion km, 6 trillion miles, or 0.3 parsecs. Next to the Sun, the closest star to Earth, Proxima Centauri, is around 4.2 light‑years away.[53]

    Speed of light in cosmology

    Some scientists have questioned why the fundamental constants of nature, including the speed of light, have the values they do, and whether they are changing as the universe evolves.[54][55][56]

    Others have suggested that the speed of light may exhibit dispersion.[57] However, observations of astrophysical events at high redshifts can be used to place severe limits on the variation of the speed of light with frequency, as well as on the photon mass mγ. [58]

    Faster-than-light observations and experiments

    The blue glow in this "swimming pool" nuclear reactor is Čerenkov radiation, emitted as a result of electrons traveling faster than the speed of light in water.

    It is generally considered that it is impossible for any information or matter to travel faster than c, because it would travel backwards in time relative to some observers.[59] However, there are many physical situations in which speeds greater than c are encountered.

    Some of these situations involve entities that actually travel faster than c in a particular reference frame but none involves either matter, energy, or information traveling faster than the speed of light in vacuum.

    It is possible for the group velocity of light to exceed c[60][61] and in an experiment in 2000 laser beams traveled for extremely short distances through caesium atoms with a group velocity of 300 times c.[62] It is not, however, possible to use this technique to transfer information faster than c since the velocity of information transfer depends on the front velocity, which is always less than c.[63]

    If a laser is swept across a distant object, the spot of light can easily be made to move at a speed greater than c.[64] Similarly, a shadow projected onto a distant object can be made to move faster than c.[65] In neither case does any matter or information travel faster than light.

    In some interpretations of quantum mechanics, certain quantum effects may be transmitted at speeds greater than c. For example, the quantum states of two particles can be entangled. Until the particles are observed, they exist in a superposition of two quantum states. If the particles are separated and one of them is observed to determine its quantum state then the quantum state of the second particle is determined automatically and faster than a light signal could travel between the two particles. However, it is impossible to control which quantum state the first particle will take on when it is observed, so no information can be transmitted in this manner.

    Another prediction of faster-than-light speeds occurs for tunneling and is called the Hartman effect.[66][67] However, no information can be sent using these effects.[68]

    Closing speeds and proper speeds are examples of calculated speeds that may have value in excess of c but that do not represent the speed of an object as measured in a single inertial frame.

    So-called superluminal motion is seen in certain astronomical objects,[69] such as the jets of radio galaxies and quasars. However, these jets are not moving at speeds in excess of the speed of light: the apparent superluminal motion is a projection effect caused by objects moving near the speed of light and at a small angle to the line of sight.

    Čerenkov radiation

    It is possible for shock waves to be formed with electromagnetic radiation.[70][71] If a charged particle travels through an insulating medium faster than the speed of light in that medium then radiation is emitted which is analogous to a sonic boom and is known as Čerenkov radiation.

    Galaxies moving faster than light

    In models of the expanding universe, the further things are from Earth, the faster they move away from us. This movement is not considered to be a straightforward travel, like a rocket for example, but a movement due to the expansion of space itself. This expansion moves distant objects away from us faster and faster the further away they are. At a boundary called the Hubble sphere, the recessional velocity is the speed of light.

    See also

    References

    Footnotes

    1. ^ a b Michael De Podesta (2002). Understanding the Properites of Matter. CRC Press. p. 131. ISBN 0415257883. http://books.google.com/books?id=h8BNvnR050cC&pg=PA131&lpg=PA131. 
    2. ^ These ideal properties pertain exactly to ideal vacuum or free space, and apply only approximately to any realizable approximation to vacuum.
    3. ^ a b c See Maxwell p. 499 in A Dynamical Theory of the Electromagnetic Field (1864)
    4. ^ P. Gibbs (1997). "Why is c the symbol for the speed of light?". University of California, Riverside. http://math.ucr.edu/home/baez/physics/Relativity/SpeedOfLight/c.html. Retrieved on 2008-08-20. 
    5. ^ See, for example, some handbooks:
    6. ^ a b International Bureau of Weights and Measures (2006), The International System of Units (SI) (8th ed.), p. 112, ISBN 92-822-2213-6, http://www.bipm.org/utils/common/pdf/si_brochure_8_en.pdf 
    7. ^ B.N. Taylor (ed.), A. Thompson (ed.) (2008) (PDF). The International System of Units (SI): NIST Special Publication 330. Washington, DC: NIST. pp. 11, 33–34. http://physics.nist.gov/Pubs/SP330/sp330.pdf. 
    8. ^ Mise en pratique
    9. ^ Hall, S.H. and Hall, G.W. and McCall, J.A. (2000). High Speed Digital System Design: A Handbook of Interconnect Theory and Design Practices. Wiley New York. 
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    11. ^ http://www.geo.mtu.edu/rs/back/spectrum/
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    14. ^ |title=Severe limits on variations of the speed of light with frequency |author=Bradley E Shaefer |doi=10.1103/PhysRevLett.82.4964}}
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    30. ^ B. Steffens (2006). "Chapter Five – The Scholar of Cairo". Ibn al-Haytham: First Scientist. Morgan Reynolds. ISBN 1599350246. http://www.ibnalhaytham.net/custom.em?pid=673906. 
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    35. ^ O'Connor, John J.; Robertson, Edmund F., "Abu Arrayhan Muhammad ibn Ahmad al-Biruni", MacTutor History of Mathematics archive .
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    45. ^ A detailed discussion of the interferometer and its use for determining the speed of light can be found in J. M. Vaughan (1989). The Fabry-Perot interferometer. CRC Press. p. 47. ISBN 0852741383. http://books.google.com/books?id=mMLuISueDKYC&printsec=frontcover#PPA47,M1.  and pp. 384-391.
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    49. ^ Resolution 1
    50. ^ a b BIPM mise-en-pratique method b.
    51. ^ PE Ciddor (1996). "Refractive index of air: new equations for the visible and near infrared". Applied Optics 35: 1566-1573. http://cfa-www.harvard.edu/~jbattat/apollo/references/atmosphere/ciddor.pdf. 
    52. ^ Mise en pratique for the definition of the metre,and CIPM adopted Recommendation 1 (CI-1983) Appendix 1, p. 77 "provided that the given specifications and accepted good practice are followed; • that in all cases any necessary corrections be applied to take account of actual conditions such as diffraction, gravitation or imperfection in the vacuum; … "
    53. ^ Further discussion can be found at NASA StarChild
    54. ^ Weyl, H.: Annalen der Physik, vol. 359, Issue 18, pp.117-145 (1917); Weyl, H.: Annalen der Physik, vol. 364, Issue 10, pp.101-133 (1919)
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    58. ^ Bradley E Shaefer (1999). "Severe limits on variations of the speed of light with frequency". Phys. Rev. Lett. 82: 4964–4966. doi:10.1103/PhysRevLett.82.4964. http://arxiv.org/abs/astro-ph/9810479v1. 
    59. ^ E.F. Taylor, J.A. Wheeler (1992). Spacetime Physics. W. H. Freeman. pp. 74–75. ISBN 0716723271. 
    60. ^ G. Egan (2000). "Subluminal". http://gregegan.customer.netspace.net.au/APPLETS/20/20.html. Retrieved on 2007-02-06. 
    61. ^ L.J. Wang, A. Kuzmich, A. Dogariu (2000). "Gain-assisted superluminal light propagation". Nature 406 (406): 277. doi:10.1038/35018520. 
    62. ^ D. Whitehouse (2000). "Beam smashes light barrier". BBC News. http://news.bbc.co.uk/hi/english/sci/tech/newsid_841000/841690.stm. Retrieved on 2008-12-08. 
    63. ^ N. Brunner, V. Scarani, M. Wegmüller, M. Legré, N. Gisin (2004). "Direct Measurement of Superluminal Group Velocity and Signal Velocity in an Optical Fiber". Physical Review Letters 93 (20): 203902. doi:10.1103/PhysRevLett.93.203902. http://prola.aps.org/abstract/PRL/v93/i20/e203902. 
    64. ^ P. Gibbs (1997). "Is Faster-Than-Light Travel or Communication Possible?". University of California, Riverside. http://math.ucr.edu/home/baez/physics/Relativity/SpeedOfLight/FTL.html. Retrieved on 2008-08-20. 
    65. ^ M. Wertheim (2007). "The Shadow Goes". New York Times. http://www.nytimes.com/2007/06/20/opinion/20wertheim.html?_r=1&scp=1&sq=%27the%20shadow%20goes%27&st=cse&oref=slogin. 
    66. ^ Juan Gonzalo Muga, R. Sala Mayato, Iñigo L. Egusquiza, ed (2007). Time in Quantum Mechanics. Springer. p. 48. ISBN 3540734724. http://books.google.com/books?id=InKru6zHQWgC&pg=PA48. 
    67. ^ Hugo E. Hernández-Figueroa, Michel Zamboni-Rached, Erasmo Recami (2007). Localized Waves. Wiley-Interscience. p. 26. ISBN 0470108851. http://books.google.com/books?id=xxbXgL967PwC&pg=PA26. 
    68. ^ Klaas Wynne (2002). "Causality and the nature of information". Optics Communications 209: 84-100. http://bcp.phys.strath.ac.uk/the_group/r/uf/2002-OC-causality.pdf. 
    69. ^ M. Rees (1966). "The Appearance of Relativistically Expanding Radio Sources". Nature 211: 468. doi:10.1038/211468a0. 
    70. ^ P.A. Čerenkov (1934). "Visible Emission of Clean Liquids by Action of γ Radiation". Dokl. Akad. Nauk SSSR 2: 451. 
      Reprinted in "Selected Papers of Soviet Physicists". Usp. Fiz. Nauk 93: 385. 1967. 
    71. ^ A.N. Gorbunova (ed.), E.P. Čerenkov (1999), Pavel Alekseyevich Čerenkov: Chelovek i Otkrytie, Nauka, pp. 149–153 

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