List Of Discredited Substances
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List Of Discredited Substances
This is a list of substances or materials generally considered discredited. A substance can be discredited in one of three ways: #It was widely believed to exist at one time but no longer is. Such substances are often part of an obsolete scientific theory. #It was once believed to have drastically different properties from those accepted now. It was widely claimed and believed to possess significant properties that are no longer attributed to it. #It is currently believed to exist as part of a theory that has not met the theoretical and experimental requirements of mainstream science. In particular, such a theory must be predictive. Substances whose existence is discredited Substances whose properties are discredited This is not to be construed as implying that these items––are discredited. What is listed are fire, water, metal, etc. as universal principles or fundamentals. * Classical elements and Chinese elements discredited by atomic theory and nuclear physics. ...
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Obsolete Scientific Theory
This list includes well-known general theories in science and pre-scientific natural philosophy and natural history that have since been superseded by other scientific theories. Many discarded explanations were once supported by a scientific consensus, but replaced after more empirical information became available that identified flaws and prompted new theories which better explain the available data. Pre-modern explanations originated before the scientific method, with varying degrees of empirical support. Some scientific theories are discarded in their entirety, such as the replacement of the phlogiston theory by energy and thermodynamics. Some theories known to be incomplete or in some ways incorrect are still used. For example, Newtonian classical mechanics is accurate enough for practical calculations at everyday distances and velocities, and it is still taught in schools. The more complicated relativistic mechanics must be used for long distances and velocities nearing th ...
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Heat
In thermodynamics, heat is energy in transfer between a thermodynamic system and its surroundings by such mechanisms as thermal conduction, electromagnetic radiation, and friction, which are microscopic in nature, involving sub-atomic, atomic, or molecular particles, or small surface irregularities, as distinct from the macroscopic modes of energy transfer, which are thermodynamic work and transfer of matter. For a closed system (transfer of matter excluded), the heat involved in a process is the difference in internal energy between the final and initial states of a system, after subtracting the work done in the process. For a closed system, this is the formulation of the first law of thermodynamics. Calorimetry is measurement of quantity of energy transferred as heat by its effect on the states of interacting bodies, for example, by the amount of ice melted or by change in temperature of a body. In the International System of Units (SI), the unit of measurement for he ...
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Molecular Biology
Molecular biology is a branch of biology that seeks to understand the molecule, molecular basis of biological activity in and between Cell (biology), cells, including biomolecule, biomolecular synthesis, modification, mechanisms, and interactions. Though cells and other microscopic structures had been observed in living organisms as early as the 18th century, a detailed understanding of the mechanisms and interactions governing their behavior did not emerge until the 20th century, when technologies used in physics and chemistry had advanced sufficiently to permit their application in the biological sciences. The term 'molecular biology' was first used in 1945 by the English physicist William Astbury, who described it as an approach focused on discerning the underpinnings of biological phenomena—i.e. uncovering the physical and chemical structures and properties of biological molecules, as well as their interactions with other molecules and how these interactions explain observ ...
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Life
Life, also known as biota, refers to matter that has biological processes, such as Cell signaling, signaling and self-sustaining processes. It is defined descriptively by the capacity for homeostasis, Structure#Biological, organisation, metabolism, Cell growth, growth, adaptation, response to stimulus (physiology), stimuli, and reproduction. All life over time eventually reaches a state of death, and none is Immortality, immortal. Many philosophical definitions of living systems have been proposed, such as self-organizing systems. Viruses in particular make definition difficult as they replicate only in Host (biology), host cells. Life exists all over the Earth in air, water, and soil, with many ecosystems forming the biosphere. Some of these are harsh environments occupied only by extremophiles. Life has been studied since ancient times, with theories such as Empedocles's materialism asserting that it was composed of Classical element, four eternal elements, and Aristotle's ...
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Henri Bergson
Henri-Louis Bergson (; ; 18 October 1859 â€“ 4 January 1941) was a French philosopher who was influential in the traditions of analytic philosophy and continental philosophy, especially during the first half of the 20th century until the Second World War, but also after 1966 when Gilles Deleuze published ''Le Bergsonisme''. Bergson is known for his arguments that processes of immediate experience and Intuition (knowledge), intuition are more significant than abstract rationalism and science for understanding reality. Bergson was awarded the 1927 Nobel Prize in Literature "in recognition of his rich and vitalizing ideas and the brilliant skill with which they have been presented". In 1930, France awarded him its highest honour, the Grand-Croix de la Legion d'honneur. Bergson's great popularity created a controversy in France, where his views were seen as opposing the Secularism in France, secular and scientific attitude adopted by the French Third Republic, Republic's offici ...
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Élan Vital
''Élan vital'' () is a term coined by French philosopher Henri Bergson in his 1907 book '' Creative Evolution'', in which he addresses the question of self-organisation and spontaneous morphogenesis of things in an increasingly complex manner. ''Élan vital'' was translated in the English edition as "vital impetus", but is usually translated by his detractors as "vital force". It is a hypothetical explanation for evolution and development of organisms, which Bergson linked closely with consciousness – the intuitive perception of experience and the flow of inner time. Precursors Distant anticipations of Bergson can be found in the work of the pre-Christian Stoic philosopher Posidonius, who postulated a "vital force" emanated by the sun to all living creatures on the Earth's surface, and in that of Zeno of Elea. The concept of ''élan vital'' is also similar to Baruch Spinoza's concept of conatus as well as Arthur Schopenhauer's concept of the will-to-live and the Sanskrit '' ...
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Iron
Iron is a chemical element; it has symbol Fe () and atomic number 26. It is a metal that belongs to the first transition series and group 8 of the periodic table. It is, by mass, the most common element on Earth, forming much of Earth's outer and inner core. It is the fourth most abundant element in the Earth's crust, being mainly deposited by meteorites in its metallic state. Extracting usable metal from iron ores requires kilns or furnaces capable of reaching , about 500 Â°C (900 Â°F) higher than that required to smelt copper. Humans started to master that process in Eurasia during the 2nd millennium BC and the use of iron tools and weapons began to displace copper alloys – in some regions, only around 1200 BC. That event is considered the transition from the Bronze Age to the Iron Age. In the modern world, iron alloys, such as steel, stainless steel, cast iron and special steels, are by far the most common industrial metals, due to their mechan ...
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Bengt Edlén
Bengt Edlén (2 November 1906, Gusum – 10 February 1993, Lund) was a Swedish professor of physics and astronomer who specialized in spectroscopy. He was the first who identified the unknown coronal spectral lines in the Solar corona, Corona, which was used to calculate the temperature of the corona. Biography Bengt Edlén was born on 2 November 1906 in Gusum, Sweden. He graduated from high school in Norrköping in 1926 and entered the Uppsala University the same year. He was awarded his bachelor's degree after three semester and graduated with a PhD in 1934 with his thesis about the spectra and energy of the elements in the beginning of the periodic system. He received international fame after finding unidentified spectral lines in the Sun's stellar spectrum, spectrum which were speculatively believed to originate from a hitherto unidentified chemical element termed coronium. Edlén later showed that those lines are from multiply ionized iron (Fe-XIV). His discovery was ...
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Walter Grotrian
Walter Robert Wilhelm Grotrian (21 April 1890 in Aachen; † 3 March 1954 in Potsdam) was a German astronomer and astrophysicist. In 1928 he introduced the Grotrian diagram in atomic spectroscopy, showing the allowed transitions between atomic energy levels Grotrian studied the emission line from the solar corona in the green region of the spectrum; this emission line could not be attributed to any known chemical element and was thought to be a new element (which scientists named "coronium"). Grotrian and Bengt Edlén from Sweden demonstrated that the two observed emission lines arise from iron atoms that have lost about half their 26 electrons.ESO: The Glory of a Nearby Star


Named after Grotrian

*The impact crater
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Solar Corona
In astronomy, a corona (: coronas or coronae) is the outermost layer of a star's Stellar atmosphere, atmosphere. It is a hot but relatively luminosity, dim region of Plasma (physics), plasma populated by intermittent coronal structures such as solar prominence, prominences, coronal loops, and helmet streamers. The Sun's corona lies above the chromosphere and extends millions of kilometres into outer space. Coronal light is typically obscured by diffuse sky radiation and Glare (vision), glare from the solar disk, but can be easily seen by the naked eye during a total solar eclipse or with a specialized coronagraph. Spectroscopic measurements indicate strong ionization in the corona and a plasma temperature in excess of , much hotter than the surface of the Sun, known as the photosphere. is, in turn, derived . History In 1724, French-Italian astronomer Giacomo F. Maraldi recognized that the aura visible during a solar eclipse belongs to the Sun, not to the Moon. In 1809, Span ...
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William Harkness
William Harkness (December 17, 1837 – February 28, 1903) was an astronomer. He was born at Ecclefechan, Scotland, a son of James (1803–78) and Jane (née Wield) Harkness. His father was a pastor and moved the family to the United States. Harkness served in the military, traveled extensively, and headed research missions developing techniques and equipment for astronomical study. Harkness died at his home in Jersey City on February 28, 1903, at the age of 65. Biography Raised in Fishkill Landing, New York, Harkness was educated at Lafayette College (September 1854 – January 1856), graduated from the University of Rochester (1858) where he was a brother of Delta Kappa Epsilon, and then studied medicine in New York City. In 1862, Harkness graduated from the New York Homeopathic Medical College. In August 1862, he served as volunteer surgeon for the Union Army at the Second Battle of Bull Run. From 1862 to 1865, Harkness was an "aid in astronomy" at the United States Na ...
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Charles Augustus Young
Charles Augustus Young (December 15, 1834 – January 4, 1908) one of the foremost solar spectroscopist astronomers in the United States. He observed solar eclipses and worked on spectroscopy of the Sun. He observed a solar flare with a spectroscope on 3 August 1872, and also noted that it coincided with a magnetic storm on Earth. Young graduated from Dartmouth College in 1853. For two years, he taught classes at Phillips Academy in Andover, Massachusetts, Andover, Massachusetts. The following year, he studied at the theological seminary in Andover, while also continuing to teach. In 1857, he became the Professor of Mathematics and Natural Philosophy at Case Western Reserve University, Western Reserve College, now known as Case Western Reserve University, devoting nine years. Young's name is inscribed on the Loomis Observatory, which is the oldest observatory in the United States still remaining in its original location. In 1862, he served in the 85th Ohio Infantry, 85th ...
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