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American physicist (1852–1931)
Michelson, who was born at Strelno (now Strzelno in Poland), came to America with his parents when he was two years old. He graduated from the US Naval Academy in 1873 and remained there to teach physics and chemistry. Some five years later he began his work on measuring the speed of light and to this end he traveled to Europe to study optics at the Collège de France, Heidelberg, and Berlin. When he returned to America he left the navy to become professor of physics at the Case School, Cleveland. In 1882 he estimated the speed of light as 186,320 miles per second. This was the most accurate value then available and remained so for another ten years, when Michelson made an even more accurate measurement.
In the course of this work Michelson developed an interferometer, an instrument that can divide a beam of light in two, send the beams in different directions, and then unite them again. If the two beams traveled the same distance at different speeds (or different distances at the same speed) then, on being brought together again, the waves would be out of step and produce interference fringes on a screen. Michelson used the interferometer to test whether light travelng in the same direction as the Earth moves more slowly than light traveling at right angles to the Earth's surface. This was effectively testing the presence of the ‘ether’ – a substance that was supposed to exist in all space beyond the Earth's atmosphere. Because the ether was thought to be motionless and the Earth moved through it, it followed that light traveling in the same direction as the Earth would be more impeded than light going at right angles to it.
Michelson first conducted this experiment in 1881 in Berlin and got a negative result, that is there were no interference fringes and thus no evidence that the two beams were traveling at different speeds. He repeated the procedure several times under increasingly elaborate conditions until, in 1887, with Edward Morley (1838–1923), the experiment was made under near perfect conditions at the Case School. Again the ether could not be detected and physicists had seriously to consider that the ether did not exist. This result questioned much orthodox physical theory, and it remained for Einstein to develop the special theory of relativity to explain the constancy of the speed of light. Michelson was awarded the 1907 Nobel Prize in physics for this work.
Others, however, continued to report that they had found a measurable difference. Thus Dayton Miller (1866–1941), professor of physics at the Case School of Applied Science, Cleveland, Ohio took his equipment in 1925 to the 6000-ft summit of Mount Wilson in California. He claimed to have detected a difference of 6 miles per second for light travelling at right angles to the Earth's orbit. It was later established, however, that Miller's results were caused by different temperature conditions.
Michelson also applied interference techniques to astronomical measurements and was able to measure the diameters of various heavenly bodies by contrasting the light emitted from both sides. He also continued to make increasingly more accurate estimates of the speed of light and he suggested that the wavelength of light waves should be used as the length standard rather than the platinum–iridium meter in Paris. This suggestion was taken up in 1960 when light waves from the inert gas krypton became the standard measure.
The American physicist Albert Abraham Michelson (1852-1931) is important for his determination of the velocity of light and the study of optical interference.
Albert Michelson was born on Dec. 19, 1852, in German Poland. The family emigrated to the United States in 1854. He took the competitive examinations for congressional appointment to the U.S. Naval Academy. Although he qualified for the appointment, the place was awarded to another boy. Young Michelson traveled to Washington, was unsuccessful in getting President Grant to appoint him to the academy, but then persuaded the commandant to accept him.
Michelson graduated from the Naval Academy in 1873. Two years later he was appointed instructor in physics and chemistry there. He resigned his commission in 1880 and spent 2 years studying in Berlin, Heidelberg, and Paris. He was then appointed to the Case School of Applied Science at Cleveland, Ohio, as professor of physics. In 1889 he moved to Clark University as professor of physics, and in 1892 he was invited to head the department of physics at the new University of Chicago, a position which he held until 1931.
With few exceptions, all of Michelson's work bore directly on problems involved in the study of light; he was thus specialized to a degree that was unique among Americans at the end of the 19th century. While serving at Annapolis, he hit upon a slight but vital modification to a method then being used to measure the speed of light. With his simple device, consisting essentially of two plane mirrors, one fixed and one revolving at the rate of about 130 turns per second from which light was to be reflected, Michelson succeeded in obtaining a measure closer than any that had been obtained to the presently accepted figure - 186,508 miles per second.
Michelson performed his most famous experiment at Cleveland in collaboration with the chemist Edward W. Morley. Light waves were regarded as undulations of the ether which filled all space. If a light source were moving through the ether, the speed of the light would be different for each direction in which it was emitted. In the Michelson-Morley experiment two beams of light, sent out and reflected back at right angles to each other, took the same amount of time. Thus the notion of a stationary ether had to be discarded.
Even though his own work helped touch off a revolution in physics, Michelson never realized the fundamental nature of the change. Basically a brilliant experimenter, he saw the future development of physics only as one of further precision and newer instruments which would bring the accuracy of scientific measurements to the ultimate degree. He never understood the more mathematical and theoretical approach which came to dominate physics toward the end of his life.
Michelson's contributions were numerous. He developed, as a by-product of his interference experiments, the first spectroscope having sufficiently high resolution to disclose direct optical evidence of molecular motion; gave the scientific world a new fundamental standard of length when he calibrated the international meter in terms of wavelengths of cadmium; and, using a variation of his interferometer, became the first man to measure the diameter of a star. He received the Nobel Prize in 1907, the first American to be so honored. He died on May 9, 1931, while at work on a still more refined measurement of the velocity of light.
Further Reading
A good account of the major work of Michelson's life is in Bernard Jaffe, Michelson and the Speed of Light (1960). There is a useful biographical memoir of Michelson by Robert A. Millikan in National Academy of Sciences, Biographical Memoirs, vol. 19 (1938), and another profile of his life and work is in Royal Society of London, Obituary Notices of Fellows of the Royal Society, vol. 1 (1932-1935). The Nobel Foundation, Nobel Lectures: Physics, 1901-1921 (1964), has a biographical sketch.
(1852-1931), scientist. Although Albert Michelson was born in a Polish village to a Jewish father and a gentile mother, he became both a symbol and a star of American science as it stood in his time. He was three when his family immigrated to a California mining town, itself a symbol of American restlessness and hustle. Michelson graduated from the U.S. Naval Academy in 1873, ranking first among his classmates in optics. Unlike most Americans in the frenzied materialism of the Gilded Age, Michelson was attracted to science and found his métier in the sort of work most congenial to American scientists of his day: instrumentation and measurement. The ardent collection of discrete facts, rather than patient, long-range investigative projects, dominated American science in those years.
Michelson was a young physics instructor at Annapolis in 1877 when his department head urged him to open his lecture demonstrations with the French physicist Foucault's apparatus for measuring the speed of light. Michelson thereupon conceived an ingenious improvement on Foucault's device, simplifying it and significantly improving its accuracy. From then on, through almost half a century of university teaching, Michelson would pursue the holy grail of ultimate precision in measuring that fundamental physical constant. Early in the quest he confronted the problem of how light traveled. Scientists at the time generally accepted the theory that light traveled in the form of waves transmitted by a hypothetical substance they called the "ether," supposedly stationary and filling the entire universe. Michelson accepted that hypothesis and set out to determine the motion of the earth relative to the postulated ether.
In 1887, collaborating with a chemist friend, Edward W. Morley, Michelson carried out an ingenious experiment with a negative result: the speed of light was the same regardless of its direction relative to the earth's motion in space. The ether, if it existed, evidently had no effect, at least at the earth's surface. This startling finding did not, as legend has had it, directly inspire Einstein's theory of relativity (which ruled out ether), though it did lead others to ideas that in turn played a part in that theory, and it gave experimental support to the theory, once formulated. Michelson himself, weak in mathematics like most American physicists of the period, continued to believe in the ether and grudgingly accepted Einstein's theory only after many years, on the pragmatic grounds that it accounted for certain measurable phenomena.
Although he neither claimed nor craved a share in Einstein's glory, Michelson found consolation and pride in the instrument he had developed for the classic experiment: the interferometer. He refined and improved it brilliantly over the years, adapting it to a dazzling array of scientific measurements. It became one of the basic instruments of physical science, in a class with telescopes, microscopes, and thermometers. It was for his instruments and measurements, not for any contribution to relativity, that Michelson in 1907 became the first American to win a Nobel Prize in science. The honor was a sign of American science's coming of age. Ironically, that meant going beyond the very kind of science that Michelson had so famously represented.
Bibliography:
Dorothy M. Livingston, The Master of Light (1979); Loyd S. Swenson, Jr., The Ethereal Aether: A History of the Michelson-Morley-Miller Aether Drift Experiments, 1880-1930 (1972).
Author:
Robert V. Bruce
See also Science and Technology.
Bibliography
See biography by his daughter, D. M. Livingston (1973).
| Albert Abraham Michelson | |
|---|---|
| Born | December 19, 1852 Strzelno, Kingdom of Prussia |
| Died | May 9, 1931 (aged 78) Pasadena, California |
| Nationality | United States |
| Fields | Physics |
| Institutions | Case Western Reserve University Clark University University of Chicago |
| Alma mater | United States Naval Academy University of Berlin |
| Doctoral advisor | Hermann Helmholtz |
| Doctoral students | Robert Millikan |
| Known for | Speed of light Michelson-Morley experiment |
| Notable awards | Nobel Prize for Physics (1907) Copley Medal (1907) Henry Draper Medal (1916) |
| Signature |
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Albert Abraham Michelson (December 19, 1852 – May 9, 1931) was an American physicist known for his work on the measurement of the speed of light and especially for the Michelson-Morley experiment. In 1907 he received the Nobel Prize in Physics. He became the first American to receive the Nobel Prize in sciences.
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Michelson was born in Strzelno, Provinz Posen in the Kingdom of Prussia (now Poland) into a Jewish family.[1] He moved to the US with his parents in 1855, at the age of two. He grew up in the mining towns of Murphy's Camp, California and Virginia City, Nevada, where his father was a merchant. Despite his family being Jewish by birth, his family were non-religious. Michelson was later said to be a lifelong agnostic.[2] He spent his high school years in San Francisco in the home of his aunt, Henriette Levy (née Michelson), who was the mother of author Harriet Lane Levy.[3]
President Ulysses S. Grant awarded Michelson a special appointment to the U.S. Naval Academy in 1869.[4] During his four years as a midshipman at the Academy, Michelson excelled in optics, heat, climatology and drawing. After graduating in 1873 and two years at sea, he returned to the Naval Academy in 1875 to become an instructor in physics and chemistry until 1879. In 1879, he was posted to the Nautical Almanac Office, Washington (part of the United States Naval Observatory[5][6][7]), to work with Simon Newcomb. In the following year he obtained leave of absence to continue his studies in Europe. He visited the Universities of Berlin and Heidelberg, and the Collège de France and École Polytechnique in Paris.
Michelson was fascinated with the sciences, and the problem of measuring the speed of light in particular. While at Annapolis, he conducted his first experiments of the speed of light, as part of a class demonstration in 1877. His Annapolis experiment was refined, and in 1879, he measured the speed of light in air to be 299,864±51 kilometres per second, and estimated the speed of light in vacuum as 299,940 km/s, or 186,380 mi/s[8][9][10]. After two years of studies in Europe, he resigned from the Navy in 1881. In 1883 he accepted a position as professor of physics at the Case School of Applied Science in Cleveland, Ohio and concentrated on developing an improved interferometer. In 1887 he and Edward Morley carried out the famous Michelson-Morley experiment which seemed to rule out the existence of the aether. He later moved on to use astronomical interferometers in the measurement of stellar diameters and in measuring the separations of binary stars.
In 1889 Michelson became a professor at Clark University at Worcester, Massachusetts and in 1892 was appointed professor and the first head of the department of physics at the newly organized University of Chicago.
In 1899, he married Edna Stanton. They raised one son and three daughters.
In 1907, Michelson had the honor of being the first American to receive a Nobel Prize in Physics "for his optical precision instruments and the spectroscopic and metrological investigations carried out with their aid". He also won the Copley Medal in 1907, the Henry Draper Medal in 1916 and the Gold Medal of the Royal Astronomical Society in 1923. A crater on the Moon is named after him.
Michelson died in Pasadena, California at the age of 78. The University of Chicago Residence Halls remembered Michelson and his achievements by dedicating 'Michelson House' in his honor. Case Western Reserve has dedicated a Michelson House to him, and the chemistry academic building at the United States Naval Academy also bears his name. Clark University named a theatre after him.[11] Michelson Laboratory at Naval Air Weapons Station China Lake in Ridgecrest, California is named for him. There is a display in the publicly accessible area of the Lab which includes facsimiles of Michelson's Nobel Prize medal, the prize document, and examples of his diffraction gratings.
As early as 1877, while still serving as an officer in the United States Navy, Michelson started planning a refinement of the rotating-mirror method of Léon Foucault for measuring the speed of light, using improved optics and a longer baseline. He conducted some preliminary measurements using largely improvised equipment in 1878, about the same time that his work came to the attention of Simon Newcomb, director of the Nautical Almanac Office who was already advanced in planning his own study. Michelson published his result of 299,910±50 km/s in 1879 before joining Newcomb in Washington DC to assist with his measurements there. Thus began a long professional collaboration and friendship between the two.
Simon Newcomb, with his more adequately funded project, obtained a value of 299,860±30 km/s, just at the extreme edge of consistency with Michelson's. Michelson continued to "refine" his method and in 1883 published a measurement of 299,853±60 km/s, rather closer to that of his mentor.
In 1906, a novel electrical method was used by E. B. Rosa and N. E. Dorsey of the National Bureau of Standards to obtain a value for the speed of light of 299,781±10 km/s. Though this result has subsequently been shown to be severely biased by the poor electrical standards in use at the time, it seems to have set a fashion for rather lower measured values.
From 1920, Michelson started planning a definitive measurement from the Mount Wilson Observatory, using a baseline to Lookout Mountain, a prominent bump on the south ridge of Mount San Antonio (Old Baldy), some 22 miles distant.
In 1922, the U.S. Coast and Geodetic Survey began two years of painstaking measurement of the baseline using the recently available invar tapes. With the baseline length established in 1924, measurements were carried out over the next two years to obtain the published value of 299,796±4 km/s.[12]
Famous as the measurement is, it was beset by problems, not least of which was the haze created by the smoke from forest fires which blurred the mirror image. It is also probable that the intensively detailed work of the geodetic survey, with an estimated error of less than one part in 1 million, was compromised by a shift in the baseline arising from the Santa Barbara earthquake of June 29, 1925, which was an estimated magnitude of 6.3 on the Richter scale.
The now-famous Michelson-Morley Experiment also influenced the affirmation attempts of peer Albert Einstein's theory of general relativity and special relativity, using similar optical instrumentation. These instruments and related collaborations included the participations of fellow physicists Dayton Miller, Hendrick Lorentz, and Robert Shankland.
The period after 1927 marked the advent of new measurements of the speed of light using novel electro-optic devices, all substantially lower than Michelson's 1926 value.
Michelson sought another measurement, but this time in an evacuated tube to avoid difficulties in interpreting the image owing to atmospheric effects. In 1930, he began a collaboration with Francis G. Pease and Fred Pearson to perform a measurement in a 1.6 km tube at Pasadena, California. Michelson died with only 36 of the 233 measurement series completed and the experiment was subsequently beset by geological instability and condensation problems before the result of 299,774±11 km/s, consistent with the prevailing electro-optic values, was published posthumously in 1935.
In 1887 he collaborated with colleague Edward Williams Morley of Western Reserve College, now part of Case Western Reserve University, in the Michelson-Morley experiment. Their experiment for the expected motion of the Earth relative to the aether, the hypothetical medium in which light was supposed to travel, resulted in a null result. Surprised, Michelson repeated the experiment with greater and greater precision over the next years, but continued to find no ability to measure the aether. The Michelson-Morley results were immensely influential in the physics community, leading Hendrik Lorentz to devise his now-famous Lorentz contraction equations as a means of explaining the null result.
There has been some historical controversy over whether Albert Einstein was aware of the Michelson-Morley results when he developed his theory of special relativity, which pronounced the aether to be "superfluous". Regardless of Einstein's specific knowledge, the experiment is today considered the canonical experiment in regards to showing the lack of a detectable aether.[13][14]
From 1920 and into 1921 Michelson and Francis G. Pease became the first individuals to measure the diameter of a star other than the Sun. They used an astronomical interferometer at the Mount Wilson Observatory to measure the diameter of the super-giant star Betelgeuse. A periscope arrangement was used to obtain a densified pupil in the interferometer, a method later investigated in detail by Antoine Émile Henry Labeyrie for use in "Hypertelescopes". The measurement of stellar diameters and the separations of binary stars took up an increasing amount of Michelson's life after this.
A century later, the specific interferometer instrumentation design produced by Albert Michelson has become the principle means to conduct astronomical interferometry. The "Michelson Interferometer" design is found on modern operational observatories such as VLTI, CHARA – and the U.S. Navy's NPOI.
In an episode of the television series Bonanza (Look to the Stars, broadcast March 18, 1962), Ben Cartwright (Lorne Greene) helps the 16-year-old Albert Abraham Michelson (portrayed by 25-year-old Douglas Lambert (1936–1986)) obtain an appointment to the U.S. Naval Academy, despite the opposition of the bigoted town schoolteacher (played by William Schallert). Bonanza was set in and around Virginia City, Nevada, where Michelson lived with his parents prior to leaving for the Naval Academy. In a voice-over at the end of the episode, Greene mentions Michelson's 1907 Nobel Prize.
The home in which Michelson lived as a child in Murphys Camp, California is now a tasting room for Twisted Oak Winery.
New Beast Theater Works in collaboration with High Concept Laboratories produced a "semi-opera" about Michelson, his obsessive work style and its effect on his family life which ran from February 11 to February 26, 2011 in Chicago at The Building Stage. Michelson was portrayed by Jon Stutzman. The play was directed by Davaid Maral with music composed by Joshua Dumas.
Michelson was a member of the Royal Society, the National Academy of Sciences, the American Physical Society and the American Association for the Advancement of Science.
The Computer Measurement Group gives an annual A. A. Michelson Award.
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