View source for Draft:Original research/Regions

[[Image:Fifthinstarwingdisk.png|thumb|right|250px|The clear areas within the brown '''region''' correspond to the potential development of eyespot foci. Credit: [[commons:User:Mike Serfas|Mike Serfas]].]]
A '''region''' is a division or part of an area or volume having definable characteristics but not always fixed boundaries.

The origin of the word may be from ''regere'' which means 'to rule, direct'.
{{clear}}

==Theory of regions==

'''Def.''' "[a]ny [[wikt:considerable|considerable]] and [[wikt:connected|connected]] [[wikt:part|part]] of a [[wikt:space|space]] or [[wikt:surface|surface]]; specifically, a [[wikt:tract|tract]] of [[wikt:land|land]] or [[wikt:sea|sea]] of considerable but [[wikt:indefinite|indefinite]] [[wikt:extent|extent]]; a [[wikt:country|country]]; a [[wikt:district|district]]; in a broad sense, a place without special [[wikt:reference|reference]] to [[wikt:location|location]] or extent but viewed as an [[wikt:entity|entity]] for [[wikt:geographical|geographical]], [[wikt:social|social]] or [[wikt:cultural|cultural]] reasons"<ref name=RegionWikt>{{ cite book
|title=region
|publisher=Wikimedia Foundation, Inc
|location=San Francisco, California
|date=May 20, 2012
|url=http://en.wiktionary.org/wiki/region
|accessdate=2012-05-26 }}</ref> is called a '''region'''.

'''Region''' is most commonly found as a term used in terrestrial and astrophysics sciences also an area, notably among the different sub-disciplines of [[geography]], studied by [[w:Regional geography|regional geographers]]. Regions consist of [[w:subregions|subregions]] that contain clusters of like areas that are distinctive by their uniformity of description based on a range of statistical data, for example demographic, and locales.

==Regional astronomy==
{{main|Regions/Astronomy|Regional astronomy}}
[[Image:Center of the Milky Way Galaxy IV – Composite.jpg|thumb|right|250px|This is a composite image of the central region of our Milky Way galaxy. Credit: NASA/JPL-Caltech/ESA/CXC/STScI.]]
Any considerable and connected part of a space or surface studied in astronomy is an entity in regional astronomy.

"In celebration of the International Year of Astronomy 2009, NASA's Great Observatories -- the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory -- have produced a matched trio of images of the central region of our Milky Way galaxy. Each image shows the telescope's different wavelength view of the galactic center region, illustrating the unique science each observatory conducts."<ref name=Lavoie09>{{ cite book
|author=Sue Lavoie and Karen Boggs
|title=PIA12348: Great Observatories' Unique Views of the Milky Way
|publisher=NASA, JPL
|location=Pasadena, California USA
|date=November 10, 2009
|url=http://photojournal.jpl.nasa.gov/catalog/PIA12348
|accessdate=2013-03-14 }}</ref>

"In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon."<ref name=Lavoie09/>
{{clear}}

==Galactic-Center region==
{{main|Stars/Galaxies/Center regions|Galactic-center regions}}
At the top of this article is a composite image. "In celebration of the International Year of Astronomy 2009, NASA's Great Observatories -- the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory -- have produced a matched trio of images of the central region of our Milky Way galaxy. Each image shows the telescope's different wavelength view of the galactic center region, illustrating the unique science each observatory conducts."<ref name=Lavoie09>{{ cite book
|author=Sue Lavoie and Karen Boggs
|title=PIA12348: Great Observatories' Unique Views of the Milky Way
|publisher=NASA, JPL
|location=Pasadena, California USA
|date=November 10, 2009
|url=http://photojournal.jpl.nasa.gov/catalog/PIA12348
|accessdate=2013-03-14 }}</ref>

"In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon."<ref name=Lavoie09/>

===X-ray astronomy===
{{main|Radiation astronomy/X-rays|X-rays}}
[[Image:Center of the Milky Way Galaxy III – Chandra (X-ray).jpg|thumb|right|250px|This is a Chandra X-ray Observatory image of the Galactic Central region. Credit: NASA/CXC.]]
[[Image:Milky Way Galaxy center Chandra.jpg|thumb|right|250px|This is a 400 by 900 light-year mosaic of several Chandra X-ray Observatory images of the Galactic center region. Credit: NASA/UMass/D. Wang et al.]]
“From August 23 through September 24, 2003, the INTEGRAL Observatory conducted a deep survey of the Galactic-Center region with a record-breaking sensitivity at energies above 20 keV.”<ref name=Revnivtsev>{{ cite journal
|author=M. G. Revnivtsev, R. A. Sunyaev, D. A. Varshalovich, V. V. Zheleznyakov, A. M. Cherepashchuk, A. A. Lutovinov, E. M. Churazov, S. A. Grebenev and M. R. Gilfanov
|title=A hard X-ray survey of the Galactic-Center region with the IBIS telescope of the INTEGRAL observatory: A catalog of sources
|journal=Astronomy Letters
|date=June 2004
|volume=30
|issue=6
|pages=382-9
|url=http://www.springerlink.com/content/9513489828r8280j/
|arxiv=
|bibcode=
|doi=10.1134/1.1764884
|pmid=
|accessdate=2012-05-30 }}</ref>

At right is an image of the Galactic central region using the [[w:Chandra X-ray Observatory|Chandra X-ray Observatory]].

"X-rays detected by Chandra expose a wealth of exotic objects and high-energy features [Figure 3 (bottom frame of poster)]. In this image, pink represents lower energy X-rays and blue indicates higher energy. Hundreds of small dots show emission from material around black holes and other dense stellar objects. A supermassive black hole -- some four million times more massive than the Sun -- resides within the bright region in the lower right. The diffuse X-ray light comes from gas heated to millions of degrees by outflows from the supermassive black hole, winds from giant stars, and stellar explosions. This central region is the most energetic place in our galaxy."<ref name=Lavoie09/>

The second image at right is a "400 by 900 light-year mosaic of several Chandra images of the central region of our Milky Way galaxy ... [It] reveals hundreds of white dwarf stars, neutron stars, and black holes bathed in an incandescent fog of multimillion-degree gas. The supermassive black hole at the center of the galaxy is located inside the bright white patch in the center of the image. The colors indicate X-ray energy bands - red (low), green (medium), and blue (high)."<ref name=Watzke>{{ cite book
|author=Megan Watzke
|title=Chandra takes in bright lights, big city of Milky Way
|publisher=NASA Marshall Space Flight Center
|location=Huntsville, Alabama, USA
|date=January 9, 2002
|url=http://www.msfc.nasa.gov/news/news/photos/2002/photos02-004.html
|accessdate=2013-03-14 }}</ref>
{{clear}}

===Visual astronomy===
{{main|Radiation astronomy/Visuals|Visuals}}
[[Image:Center of the Milky Way Galaxy II – Hubble (Visible).jpg|thumb|right|250px|This is a visible image of the Galactic Central region from the Hubble Space Telescope. Credit: NASA/ESA/STScI.]]
"Although best known for its visible-light images, Hubble also observes over a limited range of infrared light [Figure 2 (middle frame of poster)]. The galactic center is marked by the bright patch in the lower right. Along the left side are large arcs of warm gas that have been heated by clusters of bright massive stars. In addition, Hubble uncovered many more massive stars across the region. Winds and radiation from these stars create the complex structures seen in the gas throughout the image.This sweeping panorama is one of the sharpest infrared pictures ever made of the galactic center region."<ref name=Lavoie09/>
{{clear}}

===Infrared astronomy===
{{main|Radiation astronomy/Infrareds|Infrareds}}
[[Image:Center of the Milky Way Galaxy I – Spitzer (Infrared).jpg|thumb|right|250px|This is an infrared image of the Galactic Central region using the Spitzer Space Telescope. Credit: NASA/JPL-Caltech.]]
"Spitzer's infrared-light observations provide a detailed and spectacular view of the galactic center region [Figure 1 (top frame of poster)]. The swirling core of our galaxy harbors hundreds of thousands of stars that cannot be seen in visible light. These stars heat the nearby gas and dust. These dusty clouds glow in infrared light and reveal their often dramatic shapes. Some of these clouds harbor stellar nurseries that are forming new generations of stars. Like the downtown of a large city, the center of our galaxy is a crowded, active, and vibrant place."<ref name=Lavoie09/>
{{clear}}

===Radio astronomy===
{{main|Radiation astronomy/Radios|Radio astronomy|Radios}}
[[Image:GCRT J1745-3009 2.jpg|thumb|right|250px|This is a radio image of the central region of the Milky Way galaxy. Credit: NRL/SBC Galactic Center Radio Group.]]
At right is a radio image of the central region of the Milky Way galaxy. The arrow indicates a supernova remnant which is the location of a newly-discovered transient, the bursting low-frequency radio source GCRT J1745-3009.
{{clear}}

==Dusty regions==
{{main|Rocks/Rocky objects/Dust|Dusty regions}}
[[Image:Hubble Interacting Galaxy Arp 220 (2008-04-24).jpg|thumb|right|250px|This is a Hubble Space Telescope image of Arp 220. Credit: NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University).]]
[[Image:RCW 120.jpg|thumb|right|250px|RCW 120 is a region of hot gas and glowing dust. Credit: NASA/JPL-Caltech/GLIMPSE-MIPSGAL Teams.]]
"Arp 220 [at right] appears to be a single, odd-looking galaxy, but is in fact a nearby example of the aftermath of a collision between two spiral galaxies. It is the brightest of the three galactic mergers closest to Earth, about 250 million light-years away in the constellation of Serpens, the Serpent. The collision, which began about 700 million years ago, has sparked a cracking burst of star formation, resulting in about 200 huge star clusters in a packed, '''dusty region''' about 5,000 light-years across (about 5 percent of the Milky Way's diameter). The amount of gas in this tiny region equals the amount of gas in the entire Milky Way Galaxy. The star clusters are the bluish-white bright knots visible in the Hubble image. Arp 220 glows brightest in infrared light and is an ultra-luminous infrared galaxy. Previous Hubble observations, taken in the infrared at a wavelength that looks through the dust, have uncovered the cores of the parent galaxies 1,200 light-years apart. Observations with NASA s Chandra X-ray Observatory have also revealed X-rays coming from both cores, indicating the presence of two supermassive black holes. Arp 220 is the 220th galaxy in Arp's Atlas of Peculiar Galaxies."<ref name=Evans>{{ cite book
|author=A. Evans
|title=Cosmic Collisions Galore!
|publisher=HubbleSite
|location=
|date=April 24, 2008
|url=http://hubblesite.org/newscenter/archive/releases/2008/16/image/aq/
|accessdate=2013-03-15 }}</ref> Bold added.

At lower right is a "glowing emerald nebula seen by NASA's Spitzer Space Telescope ... Named RCW 120, this region of hot gas and glowing dust can be found in the murky clouds encircled by the tail of the constellation Scorpius. The ring of dust is actually glowing in infrared colors that our eyes cannot see, but show up brightly when viewed by Spitzer's infrared detectors. At the center of this ring are a couple of giant stars whose intense ultraviolet light has carved out the bubble, though they blend in with other stars when viewed in infrared."<ref name=SpitzerSpaceTelescope>{{ cite book
|author=Spitzer Space Telescope
|title=In the Blackest Night, a Green Ring Nebula
|publisher=Jet Propulsion Laboratory, California Institute of Technology
|location=Pasadena, California USA
|date=June 14, 2011
|url=http://www.spitzer.caltech.edu/images/3647
|accessdate=2013-03-15 }}</ref>

"The green ring is where dust is being hit by winds and intense light from the massive stars. The green color represents infrared light coming from tiny dust grains called polycyclic aromatic hydrocarbons. These small grains have been destroyed inside the bubble. The red color inside the ring shows slightly larger, hotter dust grains, heated by the massive stars."<ref name=SpitzerSpaceTelescope/>

"This bubble is far from unique. ... Spitzer has found that such bubbles are common and can be found around O stars throughout our Milky Way galaxy. The small objects at the lower right area of the image may themselves be similar regions seen at much greater distances across the galaxy."<ref name=SpitzerSpaceTelescope/>

"RCW 120 can be found slightly above the flat plane of our galaxy, located toward the bottom of the picture. The green haze seen here is the diffuse glow of dust from the galactic plane."<ref name=SpitzerSpaceTelescope/>

"This is a three-color composite that shows infrared observations from two Spitzer instruments. Blue represents 3.6-micron light and green shows light of 8 microns, both captured by Spitzer's infrared array camera. Red is 24-micron light detected by Spitzer's multiband imaging photometer."<ref name=SpitzerSpaceTelescope/>
{{clear}}

==Astrophysics==
{{main|Astrophysics}}
[[Image:2MASS Image of the Tarantula Nebula.jpg|thumb|right|250px|The Tarantula Nebula is the dominant feature in our satellite galaxy the Large Magellanic Cloud (LMC). It is one of the largest known star formation regions anywhere. Credit: 2MASS/T. Jarrett, R. Hurt, NASA.]]
In astrophysics some regions have science-specific terms such as galactic clusters.
{{clear}}

==Geography==
{{main|Locations/Geography|Geography}}
In Geography, regions can be broadly divided by physical characteristics ([[w:physical geography|physical geography]]), human impact characteristics ([[w:human geography|human geography]]), and the interaction of Humanity and the environment ([[w:environmental geography|environmental geography]]). Geographic regions and subregions are mostly described by their imprecisely defined, and sometimes transitory boundaries, except in human geography where [[w:Jurisdiction (area)|jurisdiction]] areas such as national borders are clearly defined in law.

Apart from the [[Earth|global]] continental regions, there are also hydrospheric and atmospheric regions that cover the oceans, and discrete climates above the land and water masses of the planet. The land and water global regions are divided into subregions geographically bounded by large geological features that influence large-scale ecologies, such as plains and steppes, forested massifs, deserts, or mountainous regions. Subregions describe the areas within regions that are easily distinguished in both the geological and ecological observable features.

A region has its own nature that could not be moved. The first nature is its natural environment (landform, climate, etc.). The second nature is its physical elements complex that were built by people in the past. The third nature is its socio-cultural context that could not be replaced by new immigrants.

==Governments==
{{main|Incomes/Monopolies/Governments|Governments}}
With the origin of the word '''region''' being '''regere''' 'to rule' or 'ruling', a '''region''' is more than a '''part''' or a '''division'''. It is any entity, source, or object, for example, or a part of any of these where ruling is possible in some form.

That which may be said to be the '''ruling''' is the '''connection''' between two or more elements of the open set. Two or more elements that are connected are a '''group''', though not all groups need be composed of elements having a connection.

==Mathematics==
{{main|Mathematics}}
'''Def.''' a subset of <math>\R^n</math> that is [[w:open set|open]] (in the standard [[w:Euclidean topology|Euclidean topology]]), [[w:connected set|connected]] and [[w:empty set|non-empty]] is called a '''region''', or '''region of <math>\R^n</math>''', where <math>\R^n</math> is the n-dimensional real number system.

'''Theorem''' any connected, non-empty topology that maps to, or can be mapped to, a subset of <math>\R^n</math> is also a '''region''', or '''region of <math>\R^n</math>'''.

If the '''theorem''' is true, or at least sufficient portions of it are, then any field (not just a mathematical field) may have a region within it.

More generally, a region may be a division or part not necessarily of an area or volume having definable characteristics such as connectivity but not always fixed boundaries.

==Hypotheses==
{{main|Hypotheses}}
# Regions exist without [[dominant group]]s.
# '''Dominant groups''' may not exist without regions.
# In order for a '''dominant group''' to rule a subordinate group there must be a region within which the two groups co-exist.
# A group wanting to rule another group may create a region of overlap that results in the ruling of the second group.

==See also==
{{div col|colwidth=20em}}
* [[Draft:Archaeology|Archaeology]] (-12th Century) (70 kB) (10 September 2019)
* [[Draft:Original research/Balloons for astronomy]] (60 kB) (24 November 2019)
* [[Draft:Original research/Callisto]] (45 kB) (7 December 2019)
* [[Draft:Original research/Ceres]] (31 kB) (6 December 2019)
* [[Draft:Original research/Colonial India]] (10 kB) (22 October 2019)
* [[Draft:Original research/Dione]] (17 kB) (26 October 2019)
* [[Dominant group/Regions]] (21 kB) (13 January 2019)
* [[Draft:Electrospheres|Electrospheres]] (14 kB) (2 November 2019)
* [[Draft:Enceladus]] (39 kB) (4 October 2019)
* [[Draft:Fringe sciences|Fringe sciences]] (107 kB) (13 September 2019)
* [[Draft:Geomorphology]] (71 kB) (13 August 2019)
* [[Draft:Original research/Geoseismology]] (36 kB) (7 December 2019)
* [[Draft:Original research/Io]] (36 kB) (7 December 2019)
* [[Draft:Original research/Moon]] (105 kB) (24 October 2019)
* [[Draft:Reef geomorphology]] (19 kB) (2 September 2019)
* [[Regional Archaeology]] (5 kB) (9 July 2011)
* [[Regions/Astronomy|Regional astronomy]] (48 kB) (25 July 2019)
* [[Regional geography]] (0.9 kB) (25 April 2019)
* [[Draft:Regions]] (20 kB) (13 December 2019)
* [[Stars/Star-forming regions|Star-forming regions]] (97 kB) (19 October 2019‎)
* [[Stars/Active regions|Stellar active regions]] (102 kB) (18 November 2019)
* [[Draft:Original research/Titan]] (48 kB) (25 October 2019)
* [[Draft:Original research/Venus]] (87 kB) (25 October 2019)
* [[Draft:Original research/Vesta]] (35 kB) (6 December 2019)
{{Div col end}}

==References==
{{reflist|2}}

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* [http://nedwww.ipac.caltech.edu/ NASA/IPAC Extragalactic Database - NED]
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* [http://www.ncbi.nlm.nih.gov/sites/gquery NCBI All Databases Search]
* [http://www.ncbi.nlm.nih.gov/ncbisearch/ NCBI Site Search]
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* [http://psycnet.apa.org/ PsycNET]
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* [http://www.questia.com/ Questia - The Online Library of Books and Journals]
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