Charles M. Huffer
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Charles M. Huffer
Charles Morse Huffer (June 28, 1894 – March 9, 1981) was an American astronomer and instructor. Biography He was born in Edinburgh, Indiana, the first son of Presbyterian minister Charles Huffer and his wife Nellie Morse. His grandfather, Frank Lyford Morse, was a professor of mathematics at Hanover College, and his father also had a strong interest in mathematics. Charles attended Albion College in Michigan, where he studied mathematics and graduated with an A.B. degree in 1916. Professor E. Roscoe Sleight at Albion arranged a graduate scholarship for Huffer to attend the University of Illinois. While studying at the University of Illinois he attended an astronomy course taught by Joel Stebbins, the director of the University observatory. The class size was small and the two got to know each other, which would lead to future collaboration. The director of Lick Observatory, W. W. Campbell, wrote to Stebbins letting him know he needed a volunteer for a position at an observator ...
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Washburn Observatory
The Washburn Observatory ( obs. code: 753) is an astronomical observatory located at 1401 Observatory Drive on the University of Wisconsin–Madison campus in Madison, Wisconsin, United States. Completed in 1881, it was a major research facility for about 50 years. Today, it is home to the UW-Madison College of Letters and Science Honors Program, while the telescope remains in use by students in introductory astronomy courses and the general public during open houses and viewings. History The observatory is named after the former Wisconsin governor, Cadwallader C. Washburn. In 1876, the Wisconsin State Legislature passed "An Act to permanently provide for deficiencies in the University fund income" to which Washburn added a provision that allocated a sum of $3000 USD per year over three years for the establishment of astronomy instruction and a corresponding observatory. This money was not to come from state funds, but was to be raised with property tax. On September 18, 1877, J ...
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Complex Variables
Complex analysis, traditionally known as the theory of functions of a complex variable, is the branch of mathematical analysis that investigates functions of complex numbers. It is helpful in many branches of mathematics, including algebraic geometry, number theory, analytic combinatorics, applied mathematics; as well as in physics, including the branches of hydrodynamics, thermodynamics, and particularly quantum mechanics. By extension, use of complex analysis also has applications in engineering fields such as nuclear, aerospace, mechanical and electrical engineering. As a differentiable function of a complex variable is equal to its Taylor series (that is, it is analytic), complex analysis is particularly concerned with analytic functions of a complex variable (that is, holomorphic functions). History Complex analysis is one of the classical branches in mathematics, with roots in the 18th century and just prior. Important mathematicians associated with com ...
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Professor Emeritus
''Emeritus'' (; female: ''emerita'') is an adjective used to designate a retired chair, professor, pastor, bishop, pope, director, president, prime minister, rabbi, emperor, or other person who has been "permitted to retain as an honorary title the rank of the last office held". In some cases, the term is conferred automatically upon all persons who retire at a given rank, but in others, it remains a mark of distinguished service awarded selectively on retirement. It is also used when a person of distinction in a profession retires or hands over the position, enabling their former rank to be retained in their title, e.g., "professor emeritus". The term ''emeritus'' does not necessarily signify that a person has relinquished all the duties of their former position, and they may continue to exercise some of them. In the description of deceased professors emeritus listed at U.S. universities, the title ''emeritus'' is replaced by indicating the years of their appointmentsThe Protoc ...
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Olin J
Olin may refer to: People Organizations * OLIN, American landscape architecture firm * Olin Business School at Washington University in St. Louis * Olin College, an undergraduate engineering college in Massachusetts * Olin Corporation, a chemical corporation with a history of producing chemicals and ammunition * Olin Edirne, the former name of Turkish basketball team Eskişehir Basket * F. W. Olin Foundation, a foundation endowed by Franklin W. Olin * John M. Olin Foundation, a foundation endowed by John M. Olin * Preston and Olin Institute, a defunct Methodist boys' school now a part of Virginia Tech Places * Olin, Iowa, a small city in the United States * Olin, North Carolina, an unincorporated community in the United States * Olin, Poland * Olin's Covered Bridge, the only bridge in Ashtabula county, Ohio named for a family * Olin Observatory, an astronomical observatory in New London, Connecticut * Olin Sang Ruby Union Institute, a Jewish overnight summer camp in Wisconsin F ...
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American Astronomical Society
The American Astronomical Society (AAS, sometimes spoken as "double-A-S") is an American society of professional astronomers and other interested individuals, headquartered in Washington, DC. The primary objective of the AAS is to promote the advancement of astronomy and closely related branches of science, while the secondary purpose includes enhancing astronomy education and providing a political voice for its members through lobbying and grassroots activities. Its current mission is to enhance and share humanity's scientific understanding of the universe as a diverse and inclusive astronomical community. History The society was founded in 1899 through the efforts of George Ellery Hale. The constitution of the group was written by Hale, George Comstock, Edward Morley, Simon Newcomb and Edward Charles Pickering. These men, plus four others, were the first Executive Council of the society; Newcomb was the first president. The initial membership was 114. The AAS name of the so ...
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Eclipsing Binary
A binary star is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars in the night sky that are seen as a single object to the naked eye are often resolved using a telescope as separate stars, in which case they are called ''visual binaries''. Many visual binaries have long orbital periods of several centuries or millennia and therefore have orbits which are uncertain or poorly known. They may also be detected by indirect techniques, such as spectroscopy (''spectroscopic binaries'') or astrometry (''astrometric binaries''). If a binary star happens to orbit in a plane along our line of sight, its components will eclipse and transit each other; these pairs are called ''eclipsing binaries'', or, together with other binaries that change brightness as they orbit, ''photometric binaries''. If components in binary star systems are close enough they can gravitationally distort their mutual outer stellar atmospheres. In some cases, these ...
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Badger Army Ammunition Plant
The Badger Army Ammunition Plant (BAAP or Badger) or Badger Ordnance Works (B.O.W.) is an excess, non- BRAC, United States Army facility located near Sauk City, Wisconsin. It manufactured nitrocellulose-based propellants during World War II, the Korean War, and the Vietnam War. It was a large munitions factory during World War II. As of 2013, the facility was in the end stages of demolition and remediation in preparation for property transfer. History Construction On 29 October 1941, U.S. Representative William H. Stevenson announced the construction of a powder and acid works to be built by Hercules Powder Company.Michael J. Goc, ''Powder, People, and Place: Badger Ordnance Works and the Sauk Prairie'', Friendship, WI: New Past Press, 2002. On 19 November 1941, despite protests from those living on Sauk Prairie, President Franklin D. Roosevelt authorized $65,000,000 to build the plant. By 1 March 1942, the farmers who lived there had left their farms. Construction of Badge ...
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Navigation
Navigation is a field of study that focuses on the process of monitoring and controlling the movement of a craft or vehicle from one place to another.Bowditch, 2003:799. The field of navigation includes four general categories: land navigation, marine navigation, aeronautic navigation, and space navigation. It is also the term of art used for the specialized knowledge used by navigators to perform navigation tasks. All navigational techniques involve locating the navigator's position compared to known locations or patterns. Navigation, in a broader sense, can refer to any skill or study that involves the determination of position and direction. In this sense, navigation includes orienteering and pedestrian navigation. History In the European medieval period, navigation was considered part of the set of '' seven mechanical arts'', none of which were used for long voyages across open ocean. Polynesian navigation is probably the earliest form of open-ocean navigation; it was ...
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World War II
World War II or the Second World War, often abbreviated as WWII or WW2, was a world war that lasted from 1939 to 1945. It involved the vast majority of the world's countries—including all of the great powers—forming two opposing military alliances: the Allies and the Axis powers. World War II was a total war that directly involved more than 100 million personnel from more than 30 countries. The major participants in the war threw their entire economic, industrial, and scientific capabilities behind the war effort, blurring the distinction between civilian and military resources. Aircraft played a major role in the conflict, enabling the strategic bombing of population centres and deploying the only two nuclear weapons ever used in war. World War II was by far the deadliest conflict in human history; it resulted in 70 to 85 million fatalities, mostly among civilians. Tens of millions died due to genocides (including the Holocaust), starvation, ma ...
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B-type Star
A B-type main-sequence star (B V) is a main-sequence (hydrogen-burning) star of spectral type B and luminosity class V. These stars have from 2 to 16 times the mass of the Sun and surface temperatures between 10,000 and 30,000 K. B-type stars are extremely luminous and blue. Their spectra have neutral helium, which are most prominent at the B2 subclass, and moderate hydrogen lines. Examples include Regulus and Algol A. This class of stars was introduced with the Harvard sequence of stellar spectra and published in the ''Revised Harvard photometry'' catalogue. The definition of type B-type stars was the presence of non-ionized helium lines with the absence of singly ionized helium in the blue-violet portion of the spectrum. All of the spectral classes, including the B type, were subdivided with a numerical suffix that indicated the degree to which they approached the next classification. Thus B2 is 1/5 of the way from type B (or B0) to type A. Later, however, more refined s ...
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Color Index
In astronomy, the color index is a simple numerical expression that determines the color of an object, which in the case of a star gives its temperature. The lower the color index, the more blue (or hotter) the object is. Conversely, the larger the color index, the more red (or cooler) the object is. This is a consequence of the logarithmic magnitude scale, in which brighter objects have smaller (more negative) magnitudes than dimmer ones. For comparison, the whitish Sun has a B−V index of , whereas the bluish Rigel has a B−V of −0.03 (its B magnitude is 0.09 and its V magnitude is 0.12, B−V = −0.03). Traditionally, the color index uses Vega as a zero point. To measure the index, one observes the magnitude of an object successively through two different filters, such as U and B, or B and V, where U is sensitive to ultraviolet rays, B is sensitive to blue light, and V is sensitive to visible (green-yellow) light (see also: UBV system). The set of passbands or filter ...
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Extinction (astronomy)
In astronomy, extinction is the absorption and scattering of electromagnetic radiation by dust and gas between an emitting astronomical object and the observer. Interstellar extinction was first documented as such in 1930 by Robert Julius Trumpler. However, its effects had been noted in 1847 by Friedrich Georg Wilhelm von Struve, and its effect on the colors of stars had been observed by a number of individuals who did not connect it with the general presence of galactic dust. For stars that lie near the plane of the Milky Way and are within a few thousand parsecs of the Earth, extinction in the visual band of frequencies (photometric system) is roughly 1.8  magnitudes per kiloparsec. For Earth-bound observers, extinction arises both from the interstellar medium (ISM) and the Earth's atmosphere; it may also arise from circumstellar dust around an observed object. Strong extinction in earth's atmosphere of some wavelength regions (such as X-ray, ultraviolet, and infrared ...
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