Difference between revisions of "Cosmology"
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'''Cosmology''', from the [[Greek language|Greek]]: | '''Cosmology''', from the [[Greek language|Greek]]: | ||
κοσμολογία (cosmologia, κόσμος ([[cosmos]]) order + λογος ([[logos]]) word, reason, plan) is the quantitative (usually [[mathematics|mathematical]]) study of the [[universe|Universe]] in its totality, and by extension, humanity's place in it. Though the word ''cosmology'' is recent (first used in 1730 in [[Christian Wolff (philosopher)|Christian Wolff]]'s ''Cosmologia Generalis''), study of the Universe has a long history involving [[science]], [[philosophy]], [[esotericism]], and [[religion]]. | κοσμολογία (cosmologia, κόσμος ([[cosmos]]) order + λογος ([[logos]]) word, reason, plan) is the quantitative (usually [[mathematics|mathematical]]) study of the [[universe|Universe]] in its totality, and by extension, humanity's place in it. Though the word ''cosmology'' is recent (first used in 1730 in [[Christian Wolff (philosopher)|Christian Wolff]]'s ''Cosmologia Generalis''), study of the Universe has a long history involving [[science]], [[philosophy]], [[esotericism]], and [[religion]]. | ||
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A more contemporary distinction between religion and philosophy, [[esoteric cosmology]] is distinguished from religion in its less tradition-bound construction and reliance on modern "intellectual understanding" rather than [[faith]], and from philosophy in its emphasis on [[spirituality]] as a formative concept. | A more contemporary distinction between religion and philosophy, [[esoteric cosmology]] is distinguished from religion in its less tradition-bound construction and reliance on modern "intellectual understanding" rather than [[faith]], and from philosophy in its emphasis on [[spirituality]] as a formative concept. | ||
| − | + | <center>For lessons on the [[topic]] of '''''Cosmology''''', follow [https://nordan.daynal.org/wiki/index.php?title=Category:Cosmology/TeaM this link].</center> | |
== Physical cosmology == | == Physical cosmology == | ||
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Modern scientific cosmology is usually considered to have begun in 1917 with [[Albert Einstein]]'s publication of his final modification of [[general relativity]] in the paper "Cosmological Considerations of the General Theory of Relativity," (although this paper was not widely available outside of Germany until the end of [[World War I]]). General relativity prompted [[cosmogony|cosmogonists]] such as [[Willem de Sitter]], [[Karl Schwarzschild]] and [[Arthur Eddington]] to explore the astronomical consequences of the theory, which enhanced the growing ability of [[astronomy|astronomers]] to study very distant objects. Prior to this (and for some time afterwards), physicists assumed that the Universe was static and unchanging. In parallel to this dynamic approach to cosmology, a debate was unfolding regarding the nature of the cosmos itself. On the one hand, Mount Wilson astronomer Harlow Shapley championed the model of a cosmos made up of the [[Milky Way]] star system only. [[Heber D. Curtis]], on the other hand, suggested spiral nebulae were star systems in their own right, island universes. This difference of ideas came to a climax with the organization of the [[Great Debate]] at the meeting of the (US) National Academy of Sciences in Washington on 26 April 1920. The resolution of the debate on the structure of the cosmos came with the detection of novae in the [[Andromeda galaxy]] by [[Edwin Hubble]] in 1923 and 1924. Their distance established spiral nebulae well beyond the edge of the Milky Way and as galaxies of their own. Subsequent modeling of the universe explored the possibility that the [[cosmological constant]] introduced by Einstein in his 1917 paper may result in an [[expanding universe]], depending on its value. Thus the [[big bang]] theory was proposed by the [[Belgium|Belgian]] priest [[Georges Lemaître]] in 1927 which was subsequently corroborated by [[Edwin Hubble]]'s discovery of the [[Redshift|red shift]] in 1929 and later by the discovery of the [[cosmic microwave background radiation]] by [[Arno Penzias]] and [[Robert Woodrow Wilson]] in 1964. These findings were a first step to rule out some of many [[Non-standard cosmology|alternative physical cosmologies]]. | Modern scientific cosmology is usually considered to have begun in 1917 with [[Albert Einstein]]'s publication of his final modification of [[general relativity]] in the paper "Cosmological Considerations of the General Theory of Relativity," (although this paper was not widely available outside of Germany until the end of [[World War I]]). General relativity prompted [[cosmogony|cosmogonists]] such as [[Willem de Sitter]], [[Karl Schwarzschild]] and [[Arthur Eddington]] to explore the astronomical consequences of the theory, which enhanced the growing ability of [[astronomy|astronomers]] to study very distant objects. Prior to this (and for some time afterwards), physicists assumed that the Universe was static and unchanging. In parallel to this dynamic approach to cosmology, a debate was unfolding regarding the nature of the cosmos itself. On the one hand, Mount Wilson astronomer Harlow Shapley championed the model of a cosmos made up of the [[Milky Way]] star system only. [[Heber D. Curtis]], on the other hand, suggested spiral nebulae were star systems in their own right, island universes. This difference of ideas came to a climax with the organization of the [[Great Debate]] at the meeting of the (US) National Academy of Sciences in Washington on 26 April 1920. The resolution of the debate on the structure of the cosmos came with the detection of novae in the [[Andromeda galaxy]] by [[Edwin Hubble]] in 1923 and 1924. Their distance established spiral nebulae well beyond the edge of the Milky Way and as galaxies of their own. Subsequent modeling of the universe explored the possibility that the [[cosmological constant]] introduced by Einstein in his 1917 paper may result in an [[expanding universe]], depending on its value. Thus the [[big bang]] theory was proposed by the [[Belgium|Belgian]] priest [[Georges Lemaître]] in 1927 which was subsequently corroborated by [[Edwin Hubble]]'s discovery of the [[Redshift|red shift]] in 1929 and later by the discovery of the [[cosmic microwave background radiation]] by [[Arno Penzias]] and [[Robert Woodrow Wilson]] in 1964. These findings were a first step to rule out some of many [[Non-standard cosmology|alternative physical cosmologies]]. | ||
| − | Recent observations made by the [[COBE]] and [[WMAP]] satellites observing this background radiation have effectively, in many scientists' eyes, transformed cosmology from a highly speculative science into a predictive science, as these observations matched predictions made by a theory called [[Cosmic inflation]], which is a modification of the standard [[big bang]] theory. This has led many to refer to modern times as the "Golden age of cosmology". [[Alan Guth]] is reported to have made this very claim in an [[Edge Foundation]] interview [ | + | Recent observations made by the [[COBE]] and [[WMAP]] satellites observing this background radiation have effectively, in many scientists' eyes, transformed cosmology from a highly speculative science into a predictive science, as these observations matched predictions made by a theory called [[Cosmic inflation]], which is a modification of the standard [[big bang]] theory. This has led many to refer to modern times as the "Golden age of cosmology". [[Alan Guth]] is reported to have made this very claim in an [[Edge Foundation]] interview [https://www.edge.org/documents/day/day_guth.html]. |
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| − | * [ | + | * [https://www.aip.org/history/cosmology/index.htm Cosmic Journey: A History of Scientific Cosmology] from the American Institute of Physics |
| − | * [ | + | * [https://www.strw.leidenuniv.nl/~icke/ps/CosmEquations.pdf Cosmology lecture notes] with a [[Wikipedia:List of GFDL content on the internet|GFDL license footer]] |
| − | + | * [https://www.asterdomus.com.br/Artigo_a_massa_do_Universo.htm The Mass of the Universe, in AsterDomus Planetarium site (portuguese)] | |
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[[Category: General Reference]] | [[Category: General Reference]] | ||
[[Category: Cosmology]] | [[Category: Cosmology]] | ||
Latest revision as of 23:43, 12 December 2020
Cosmology, from the Greek: κοσμολογία (cosmologia, κόσμος (cosmos) order + λογος (logos) word, reason, plan) is the quantitative (usually mathematical) study of the Universe in its totality, and by extension, humanity's place in it. Though the word cosmology is recent (first used in 1730 in Christian Wolff's Cosmologia Generalis), study of the Universe has a long history involving science, philosophy, esotericism, and religion.
Disciplines
In recent times, physics and astrophysics have come to play a central role in shaping what is now known as physical cosmology by bringing observations and mathematical tools to analyze the universe as a whole; in other words, in the understanding of the universe through scientific observation and experiment. This discipline, which focuses on the universe as it exists on the largest scale and at the earliest moments, is generally understood to begin with the big bang (possibly combined with cosmic inflation) - an expansion of space from which the Universe itself is thought to have emerged ~13.7 ± 0.2 billion (109) years ago. From its violent beginnings and until its various speculative ends, cosmologists propose that the history of the Universe has been governed entirely by physical laws.
Between the domains of religion and science, stands the philosophical perspective of metaphysical cosmology. This ancient field of study seeks to draw intuitive conclusions about the nature of the universe, man, god and/or their relationships based on the extension of some set of presumed facts borrowed from spiritual experience and/or observation.
Cosmology is often an important aspect of the origin beliefs of religions and mythologies that seek to explain the existence and nature of reality. In some cases, views about the creation (cosmogony) and destruction (eschatology) of the universe play a central role in shaping a framework of religious cosmology for understanding humanity's role in the universe.
A more contemporary distinction between religion and philosophy, esoteric cosmology is distinguished from religion in its less tradition-bound construction and reliance on modern "intellectual understanding" rather than faith, and from philosophy in its emphasis on spirituality as a formative concept.
Physical cosmology
Physical cosmology is the branch of physics and astrophysics that deals with the study of the physical origins of the Universe and the nature of the Universe on its very largest scales. In its earliest form it was what is now known as celestial mechanics, the study of the heavens. The Greek philosophers Aristarchus of Samos, Aristotle and Ptolemy proposed different cosmological theories. In particular, the geocentric Ptolemaic system was the accepted theory to explain the motion of the heavens until Nicolaus Copernicus, and subsequently Johannes Kepler and Galileo Galilei proposed a heliocentric system in the 16th century. This is known as one of the most famous examples of epistemological rupture in physical cosmology.
With Isaac Newton and the 1687 publication of Principia Mathematica, the problem of the motion of the heavens was finally solved. Newton provided a physical mechanism for Kepler's laws and his law of universal gravitation allowed the anomalies in previous systems, caused by gravitational interaction between the planets, to be resolved. A fundamental difference between Newton's cosmology and those preceding it was the Copernican principle that the bodies on earth obey the same physical laws as all the celestial bodies. This was a crucial philosophical advance in physical cosmology.
Modern scientific cosmology is usually considered to have begun in 1917 with Albert Einstein's publication of his final modification of general relativity in the paper "Cosmological Considerations of the General Theory of Relativity," (although this paper was not widely available outside of Germany until the end of World War I). General relativity prompted cosmogonists such as Willem de Sitter, Karl Schwarzschild and Arthur Eddington to explore the astronomical consequences of the theory, which enhanced the growing ability of astronomers to study very distant objects. Prior to this (and for some time afterwards), physicists assumed that the Universe was static and unchanging. In parallel to this dynamic approach to cosmology, a debate was unfolding regarding the nature of the cosmos itself. On the one hand, Mount Wilson astronomer Harlow Shapley championed the model of a cosmos made up of the Milky Way star system only. Heber D. Curtis, on the other hand, suggested spiral nebulae were star systems in their own right, island universes. This difference of ideas came to a climax with the organization of the Great Debate at the meeting of the (US) National Academy of Sciences in Washington on 26 April 1920. The resolution of the debate on the structure of the cosmos came with the detection of novae in the Andromeda galaxy by Edwin Hubble in 1923 and 1924. Their distance established spiral nebulae well beyond the edge of the Milky Way and as galaxies of their own. Subsequent modeling of the universe explored the possibility that the cosmological constant introduced by Einstein in his 1917 paper may result in an expanding universe, depending on its value. Thus the big bang theory was proposed by the Belgian priest Georges Lemaître in 1927 which was subsequently corroborated by Edwin Hubble's discovery of the red shift in 1929 and later by the discovery of the cosmic microwave background radiation by Arno Penzias and Robert Woodrow Wilson in 1964. These findings were a first step to rule out some of many alternative physical cosmologies.
Recent observations made by the COBE and WMAP satellites observing this background radiation have effectively, in many scientists' eyes, transformed cosmology from a highly speculative science into a predictive science, as these observations matched predictions made by a theory called Cosmic inflation, which is a modification of the standard big bang theory. This has led many to refer to modern times as the "Golden age of cosmology". Alan Guth is reported to have made this very claim in an Edge Foundation interview [1].
- Cosmic Journey: A History of Scientific Cosmology from the American Institute of Physics
- Cosmology lecture notes with a GFDL license footer
- The Mass of the Universe, in AsterDomus Planetarium site (portuguese)
