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Captured 15 Jun 2021, 22:49 hrs ET, Springfield, VA, USA. Bortle 8 skies, Mallincam DS10C camera, Celestron 8 inch SCT f/10, exposure 20 sec, gain 20, bin 2, stack of 100 light frames, dark and flat frames subtracted, no filter.
Clouds: partly cloudy
Seeing: ok
Transparency: ok
Moon phase: 37%
FOV: 29 x 22 arcmin before crop
Resolution: 0.9 arcsec/pixel
Orientation: Up is South
Appearance: group of dim galaxies. NGC6166 is the nebulous object (small nebulosity with two light 'eyes') just right of center and NGC6158 is at 7:30 o'clock.
From NED: NGC 6166
Apparent magnitude: +11.8
Apparent size: 2 arcmin
Distance: 429 million light years
Redshift: z = 0.030
Type: cD
Age: 97% of the age of the Universe
From the Wikipedia:
Abell 2199 is a galaxy cluster in the Abell catalogue featuring a brightest cluster galaxy NGC 6166, a cD galaxy. Abell 2199 is the definition of a Bautz-Morgan type I cluster due to NGC 6166.
A brightest cluster galaxy (BCG) is defined as the brightest galaxy in a cluster of galaxies. BCGs include the most massive galaxies in the universe. They are generally elliptical galaxies which lie close to the geometric and kinematical center of their host galaxy cluster, hence at the bottom of the cluster potential well. They are also generally coincident with the peak of the cluster X-ray emission.
Formation scenarios for BCGs include:
Cooling flow—Star formation from the central cooling flow in high density cooling centers of X-ray cluster halos.
The study of accretion populations in BCGs has cast doubt over this theory and astronomers have seen no evidence of cooling flows in radiative cooling clusters. The two remaining theories exhibit healthier prospects.
Galactic cannibalism—Galaxies sink to the center of the cluster due to dynamical friction and tidal stripping.
Galactic merger—Rapid galactic mergers between several galaxies take place during cluster collapse.
It is possible to differentiate the cannibalism model from the merging model by considering the formation period of the BCGs. In the cannibalism model, there are numerous small galaxies present in the evolved cluster, whereas in the merging model, a hierarchical cosmological model is expected due to the collapse of clusters. It has been shown that the orbit decay of cluster galaxies is not effective enough to account for the growth of BCGs. The merging model is now generally accepted as the most likely one, but recent observations are at odds with some of its predictions. For example, it has been found that the stellar mass of BCGs was assembled much earlier than the merging model predicts.
BCGs are divided into various classes of galaxies: giant ellipticals (gE), D galaxies and cD galaxies. cD and D galaxies both exhibit an extended diffuse envelope surrounding an elliptical-like nucleus akin to regular elliptical galaxies. The light profiles of BCGs are often described by a Sersic surface brightness law, a double Sersic profile or a de Vaucouleurs law. The different parametrizations of the light profile of BCG's, as well as the faintness of the diffuse envelope lead to discrepancies in the reported values of the sizes of these objects.
The Bautz–Morgan classification was developed in 1970 by Laura P. Bautz and William Wilson Morgan to categorize galaxy clusters based on their morphology. It defines three main types: I, II, and III. Intermediate types (I-II, II-III) are also allowed. A type IV was initially proposed, but later redacted before the final paper was published.
A type I cluster is dominated by a bright, large, supermassive cD galaxy; for example Abell 2029 and Abell 2199. A type II cluster contains elliptical galaxies whose brightness relative to the cluster is intermediate to that of type I and type III. The Coma Cluster is an example of a type II. A type III cluster has no remarkable members, such as the Virgo Cluster. Type III has two subdivisions, type IIIE and type IIIS. Type IIIE clusters do not contain many giant spirals. Type IIIS clusters contain many giant spirals. The deprecated type IV was for clusters whose brightest members were predominantly spirals.
NGC 6166 is an elliptical galaxy in the Abell 2199 cluster. It lies 490 million light years away in the constellation Hercules. The primary galaxy in the cluster, it is one of the most luminous galaxies known in terms of X-ray emissions. NGC 6166 is a radio-loud quasar.
NGC 6166 is a supermassive, type cD galaxy, with several smaller galaxies within its envelope.
Suspected to have formed through a number of galaxy collisions, NGC 6166 has a large number of globular clusters (estimated as between 6,200 and 22,000 in 1996) orbiting the galaxy. A 2016 study, however, gave an even higher number (around 39,000) suggesting also that the halo of this galaxy blends smoothly with the intra-cluster medium. Because of that, the galaxy has richest globular cluster system known. The galaxy harbors a supermassive black hole at its center with a mass of nearly 30 billion M☉ based on dynamical modelling.
NGC 6166 is known to host an active nucleus, classified as an FR I source, which powers two symmetric parsec-scale radio jets and radio lobes and it is caused by the infall of gas into its center caused by a cooling flow that deposits 200 solar masses of gas every year there.
It has been proposed that a number of O-type stars may be present in the center of NGC 6166.
The Abell catalog of rich clusters of galaxies is an all-sky catalog of 4,073 rich galaxy clusters of nominal redshift z ≤ 0.2. This catalog supplements a revision of George O. Abell's original "Northern Survey" of 1958, which had only 2,712 clusters, with a further 1,361 clusters – the "Southern Survey" of 1989, published after Abell's death by co-authors Harold G. Corwin and Ronald P. Olowin from those parts of the south celestial hemisphere that had been omitted from the earlier survey.
The Abell catalog, and especially its clusters, are of interest to amateur astronomers as challenge objects to be viewed in dark locations on large aperture amateur telescopes.
A quasar (/ˈkweɪzɑːr/; also known as a quasi-stellar object, abbreviated QSO) is an extremely luminous active galactic nucleus (AGN), in which a supermassive black hole with mass ranging from millions to billions of times the mass of the Sun is surrounded by a gaseous accretion disk. As gas in the disk falls towards the black hole, energy is released in the form of electromagnetic radiation, which can be observed across the electromagnetic spectrum. The power radiated by quasars is enormous; the most powerful quasars have luminosities thousands of times greater than a galaxy such as the Milky Way. Usually, quasars are categorized as a subclass of the more general category of AGN. The redshifts of quasars are of cosmological origin.
The term quasar originated as a contraction of quasi-stellar [star-like] radio source – because quasars were first identified during the 1950s as sources of radio-wave emission of unknown physical origin – and when identified in photographic images at visible wavelengths, they resembled faint, star-like points of light. High-resolution images of quasars, particularly from the Hubble Space Telescope, have demonstrated that quasars occur in the centers of galaxies, and that some host galaxies are strongly interacting or merging galaxies. As with other categories of AGN, the observed properties of a quasar depend on many factors, including the mass of the black hole, the rate of gas accretion, the orientation of the accretion disk relative to the observer, the presence or absence of a jet, and the degree of obscuration by gas and dust within the host galaxy.
Quasars are found over a very broad range of distances, and quasar discovery surveys have demonstrated that quasar activity was more common in the distant past. The peak epoch of quasar activity was approximately 10 billion years ago.
More than a million quasars have been found. The nearest known quasar is about 600 million light-years away (Markarian 231).
The record for the most distant known quasar keeps changing. In 2017, the quasar ULAS J1342+0928 was detected at redshift z = 7.54. Light observed from this 800 million solar mass quasar was emitted when the universe was only 690 million years old. In 2020, the quasar Pōniuāʻena was detected from a time only 700 million years after the Big Bang, and with an estimated mass of 1.5 billion times the mass of our Sun. In early 2021, the quasar J0313-1806, with a 1.6 billion solar-mass black hole, was reported at z = 7.64, 670 million years after the Big Bang. In March 2021, PSO J172.3556+18.7734 was detected and has since been called the most distant known radio-loud quasar discovered.
The term "quasar" was first used in an article by astrophysicist Hong-Yee Chiu in May 1964, in Physics Today, to describe certain astronomically-puzzling objects:
So far, the clumsily long name "quasi-stellar radio sources" is used to describe these objects. Because the nature of these objects is entirely unknown, it is hard to prepare a short, appropriate nomenclature for them so that their essential properties are obvious from their name. For convenience, the abbreviated form "quasar" will be used throughout this paper.
Between 1917 and 1922, it became clear from work by Heber Curtis, Ernst Öpik and others, that some objects ("nebulae") seen by astronomers were in fact distant galaxies like our own. But when radio astronomy commenced in the 1950s, astronomers detected, among the galaxies, a small number of anomalous objects with properties that defied explanation.
The objects emitted large amounts of radiation of many frequencies, but no source could be located optically, or in some cases only a faint and point-like object somewhat like a distant star. The spectral lines of these objects, which identify the chemical elements of which the object is composed, were also extremely strange and defied explanation. Some of them changed their luminosity very rapidly in the optical range and even more rapidly in the X-ray range, suggesting an upper limit on their size, perhaps no larger than our own Solar System. This implies an extremely high power density. Considerable discussion took place over what these objects might be. They were described as "quasi-stellar [meaning: star-like] radio sources", or "quasi-stellar objects" (QSOs), a name which reflected their unknown nature, and this became shortened to "quasar".
The first quasars (3C 48 and 3C 273) were discovered in the late 1950s, as radio sources in all-sky radio surveys. They were first noted as radio sources with no corresponding visible object. Using small telescopes and the Lovell Telescope as an interferometer, they were shown to have a very small angular size. By 1960, hundreds of these objects had been recorded and published in the Third Cambridge Catalogue while astronomers scanned the skies for their optical counterparts. In 1963, a definite identification of the radio source 3C 48 with an optical object was published by Allan Sandage and Thomas A. Matthews. Astronomers had detected what appeared to be a faint blue star at the location of the radio source and obtained its spectrum, which contained many unknown broad emission lines. The anomalous spectrum defied interpretation.
British-Australian astronomer John Bolton made many early observations of quasars, including a breakthrough in 1962. Another radio source, 3C 273, was predicted to undergo five occultations by the Moon. Measurements taken by Cyril Hazard and John Bolton during one of the occultations using the Parkes Radio Telescope allowed Maarten Schmidt to find a visible counterpart to the radio source and obtain an optical spectrum using the 200-inch (5.1 m) Hale Telescope on Mount Palomar. This spectrum revealed the same strange emission lines. Schmidt was able to demonstrate that these were likely to be the ordinary spectral lines of hydrogen redshifted by 15.8%, at the time, a high redshift (with only a handful of much fainter galaxies known with higher redshift). If this was due to the physical motion of the "star", then 3C 273 was receding at an enormous velocity, around 47000 km/s, far beyond the speed of any known star and defying any obvious explanation. Nor would an extreme velocity help to explain 3C 273's huge radio emissions. If the redshift was cosmological (now known to be correct), the large distance implied that 3C 273 was far more luminous than any galaxy, but much more compact. Also, 3C 273 was bright enough to detect on archival photographs dating back to the 1900s; it was found to be variable on yearly timescales, implying that a substantial fraction of the light was emitted from a region less than 1 light-year in size, tiny compared to a galaxy.
Although it raised many questions, Schmidt's discovery quickly revolutionized quasar observation. The strange spectrum of 3C 48 was quickly identified by Schmidt, Greenstein and Oke as hydrogen and magnesium redshifted by 37%. Shortly afterwards, two more quasar spectra in 1964 and five more in 1965 were also confirmed as ordinary light that had been redshifted to an extreme degree. While the observations and redshifts themselves were not doubted, their correct interpretation was heavily debated, and Bolton's suggestion that the radiation detected from quasars were ordinary spectral lines from distant highly redshifted sources with extreme velocity was not widely accepted at the time.
An extreme redshift could imply great distance and velocity but could also be due to extreme mass or perhaps some other unknown laws of nature. Extreme velocity and distance would also imply immense power output, which lacked explanation. The small sizes were confirmed by interferometry and by observing the speed with which the quasar as a whole varied in output, and by their inability to be seen in even the most powerful visible-light telescopes as anything more than faint starlike points of light. But if they were small and far away in space, their power output would have to be immense and difficult to explain. Equally, if they were very small and much closer to our galaxy, it would be easy to explain their apparent power output, but less easy to explain their redshifts and lack of detectable movement against the background of the universe.
Schmidt noted that redshift is also associated with the expansion of the universe, as codified in Hubble's law. If the measured redshift was due to expansion, then this would support an interpretation of very distant objects with extraordinarily high luminosity and power output, far beyond any object seen to date. This extreme luminosity would also explain the large radio signal. Schmidt concluded that 3C 273 could either be an individual star around 10 km wide within (or near to) our galaxy, or a distant active galactic nucleus. He stated that a distant and extremely powerful object seemed more likely to be correct.
Schmidt's explanation for the high redshift was not widely accepted at the time. A major concern was the enormous amount of energy these objects would have to be radiating, if they were distant. In the 1960s no commonly accepted mechanism could account for this. The currently accepted explanation, that it is due to matter in an accretion disc falling into a supermassive black hole, was only suggested in 1964 by Edwin Salpeter and Yakov Zel'dovich, and even then it was rejected by many astronomers, because in the 1960s, the existence of black holes was still widely seen as theoretical and too exotic, and because it was not yet confirmed that many galaxies (including our own) have supermassive black holes at their center. The strange spectral lines in their radiation, and the speed of change seen in some quasars, also suggested to many astronomers and cosmologists that the objects were comparatively small and therefore perhaps bright, massive and not far away; accordingly that their redshifts were not due to distance or velocity, and must be due to some other reason or an unknown process, meaning that the quasars were not really powerful objects nor at extreme distances, as their redshifted light implied. A common alternative explanation was that the redshifts were caused by extreme mass (gravitational redshifting explained by general relativity) and not by extreme velocity (explained by special relativity).
Various explanations were proposed during the 1960s and 1970s, each with their own problems. It was suggested that quasars were nearby objects, and that their redshift was not due to the expansion of space (special relativity) but rather to light escaping a deep gravitational well (general relativity). This would require a massive object, which would also explain the high luminosities. However, a star of sufficient mass to produce the measured redshift would be unstable and in excess of the Hayashi limit. Quasars also show forbidden spectral emission lines, previously only seen in hot gaseous nebulae of low density, which would be too diffuse to both generate the observed power and fit within a deep gravitational well. There were also serious concerns regarding the idea of cosmologically distant quasars. One strong argument against them was that they implied energies that were far in excess of known energy conversion processes, including nuclear fusion. There were suggestions that quasars were made of some hitherto unknown form of stable antimatter regions and that this might account for their brightness. Others speculated that quasars were a white hole end of a wormhole, or a chain reaction of numerous supernovae.
Eventually, starting from about the 1970s, many lines of evidence (including the first X-ray space observatories, knowledge of black holes and modern models of cosmology) gradually demonstrated that the quasar redshifts are genuine and due to the expansion of space, that quasars are in fact as powerful and as distant as Schmidt and some other astronomers had suggested, and that their energy source is matter from an accretion disc falling onto a supermassive black hole. This included crucial evidence from optical and X-ray viewing of quasar host galaxies, finding of "intervening" absorption lines, which explained various spectral anomalies, observations from gravitational lensing, Peterson and Gunn's 1971 finding[citation needed] that galaxies containing quasars showed the same redshift as the quasars, and Kristian's 1973 finding that the "fuzzy" surrounding of many quasars was consistent with a less luminous host galaxy.
This model also fits well with other observations suggesting that many or even most galaxies have a massive central black hole. It would also explain why quasars are more common in the early universe: as a quasar draws matter from its accretion disc, there comes a point when there is less matter nearby, and energy production falls off or ceases, as the quasar becomes a more ordinary type of galaxy.
The accretion-disc energy-production mechanism was finally modeled in the 1970s, and black holes were also directly detected (including evidence showing that supermassive black holes could be found at the centers of our own and many other galaxies), which resolved the concern that quasars were too luminous to be a result of very distant objects or that a suitable mechanism could not be confirmed to exist in nature. By 1987 it was "well accepted" that this was the correct explanation for quasars, and the cosmological distance and energy output of quasars was accepted by almost all researchers.
Later it was found that not all quasars have strong radio emission; in fact only about 10% are "radio-loud". Hence the name "QSO" (quasi-stellar object) is used (in addition to "quasar") to refer to these objects, further categorised into the "radio-loud" and the "radio-quiet" classes. The discovery of the quasar had large implications for the field of astronomy in the 1960s, including drawing physics and astronomy closer together.
In 1979 the gravitational lens effect predicted by Albert Einstein's general theory of relativity was confirmed observationally for the first time with images of the double quasar 0957+561.
A study published in February, 2021, showed that there are more quasars in one direction (towards Hydra) than in the opposite direction, seemingly indicating that we are moving in that direction. But the direction of this dipole is about 28° away from the direction of our motion relative to the cosmic microwave background radiation.
In March, 2021, a collaboration of scientists, related to the Event Horizon Telescope, presented, for the first time, a polarized-based image of a black hole, particularly the black hole at the center of Messier 87, an elliptical galaxy approximately 55 million light-years away in the constellation Virgo, revealing the forces giving rise to quasars.
It is now known that quasars are distant but extremely luminous objects, so any light that reaches the Earth is redshifted due to the metric expansion of space.
Quasars inhabit the centers of active galaxies and are among the most luminous, powerful, and energetic objects known in the universe, emitting up to a thousand times the energy output of the Milky Way, which contains 200–400 billion stars. This radiation is emitted across the electromagnetic spectrum, almost uniformly, from X-rays to the far infrared with a peak in the ultraviolet optical bands, with some quasars also being strong sources of radio emission and of gamma-rays. With high-resolution imaging from ground-based telescopes and the Hubble Space Telescope, the "host galaxies" surrounding the quasars have been detected in some cases. These galaxies are normally too dim to be seen against the glare of the quasar, except with special techniques. Most quasars, with the exception of 3C 273, whose average apparent magnitude is 12.9, cannot be seen with small telescopes.
Quasars are believed—and in many cases confirmed—to be powered by accretion of material into supermassive black holes in the nuclei of distant galaxies, as suggested in 1964 by Edwin Salpeter and Yakov Zel'dovich. Light and other radiation cannot escape from within the event horizon of a black hole. The energy produced by a quasar is generated outside the black hole, by gravitational stresses and immense friction within the material nearest to the black hole, as it orbits and falls inward. The huge luminosity of quasars results from the accretion discs of central supermassive black holes, which can convert between 6% and 32% of the mass of an object into energy, compared to just 0.7% for the p–p chain nuclear fusion process that dominates the energy production in Sun-like stars. Central masses of 105 to 109 solar masses have been measured in quasars by using reverberation mapping. Several dozen nearby large galaxies, including our own Milky Way galaxy, that do not have an active center and do not show any activity similar to a quasar, are confirmed to contain a similar supermassive black hole in their nuclei (galactic center). Thus it is now thought that all large galaxies have a black hole of this kind, but only a small fraction have sufficient matter in the right kind of orbit at their center to become active and power radiation in such a way as to be seen as quasars.[43]
This also explains why quasars were more common in the early universe, as this energy production ends when the supermassive black hole consumes all of the gas and dust near it. This means that it is possible that most galaxies, including the Milky Way, have gone through an active stage, appearing as a quasar or some other class of active galaxy that depended on the black-hole mass and the accretion rate, and are now quiescent because they lack a supply of matter to feed into their central black holes to generate radiation.[43]
Quasars in interacting galaxies[44]
The matter accreting onto the black hole is unlikely to fall directly in, but will have some angular momentum around the black hole, which will cause the matter to collect into an accretion disc. Quasars may also be ignited or re-ignited when normal galaxies merge and the black hole is infused with a fresh source of matter. In fact, it has been suggested that a quasar could form when the Andromeda Galaxy collides with our own Milky Way galaxy in approximately 3–5 billion years.
In the 1980s, unified models were developed in which quasars were classified as a particular kind of active galaxy, and a consensus emerged that in many cases it is simply the viewing angle that distinguishes them from other active galaxies, such as blazars and radio galaxies.
The highest-redshift quasar known (as of December 2017) was ULAS J1342+0928, with a redshift of 7.54, which corresponds to a comoving distance of approximately 29.36 billion light-years from Earth (these distances are much larger than the distance light could travel in the universe's 13.8 billion year history because space itself has also been expanding).
More than 750000 quasars have been found (as of August 2020), most from the Sloan Digital Sky Survey. All observed quasar spectra have redshifts between 0.056 and 7.64 (as of 2021). Applying Hubble's law to these redshifts, it can be shown that they are between 600 million and 29.36 billion light-years away (in terms of comoving distance). Because of the great distances to the farthest quasars and the finite velocity of light, they and their surrounding space appear as they existed in the very early universe.
The power of quasars originates from supermassive black holes that are believed to exist at the core of most galaxies. The Doppler shifts of stars near the cores of galaxies indicate that they are revolving around tremendous masses with very steep gravity gradients, suggesting black holes.
Although quasars appear faint when viewed from Earth, they are visible from extreme distances, being the most luminous objects in the known universe. The brightest quasar in the sky is 3C 273 in the constellation of Virgo. It has an average apparent magnitude of 12.8 (bright enough to be seen through a medium-size amateur telescope), but it has an absolute magnitude of −26.7. From a distance of about 33 light-years, this object would shine in the sky about as brightly as our Sun. This quasar's luminosity is, therefore, about 4 trillion (4×1012) times that of the Sun, or about 100 times that of the total light of giant galaxies like the Milky Way. This assumes that the quasar is radiating energy in all directions, but the active galactic nucleus is believed to be radiating preferentially in the direction of its jet. In a universe containing hundreds of billions of galaxies, most of which had active nuclei billions of years ago but only seen today, it is statistically certain that thousands of energy jets should be pointed toward the Earth, some more directly than others. In many cases it is likely that the brighter the quasar, the more directly its jet is aimed at the Earth. Such quasars are called blazars.
The hyperluminous quasar APM 08279+5255 was, when discovered in 1998, given an absolute magnitude of −32.2. High-resolution imaging with the Hubble Space Telescope and the 10 m Keck Telescope revealed that this system is gravitationally lensed. A study of the gravitational lensing of this system suggests that the light emitted has been magnified by a factor of ~10. It is still substantially more luminous than nearby quasars such as 3C 273.
Quasars were much more common in the early universe than they are today. This discovery by Maarten Schmidt in 1967 was early strong evidence against steady-state cosmology and in favor of the Big Bang cosmology. Quasars show the locations where massive black holes are growing rapidly (by accretion). These black holes grow in step with the mass of stars in their host galaxy in a way not understood at present. One idea is that jets, radiation and winds created by the quasars shut down the formation of new stars in the host galaxy, a process called "feedback". The jets that produce strong radio emission in some quasars at the centers of clusters of galaxies are known to have enough power to prevent the hot gas in those clusters from cooling and falling on to the central galaxy.
Quasars' luminosities are variable, with time scales that range from months to hours. This means that quasars generate and emit their energy from a very small region, since each part of the quasar would have to be in contact with other parts on such a time scale as to allow the coordination of the luminosity variations. This would mean that a quasar varying on a time scale of a few weeks cannot be larger than a few light-weeks across. The emission of large amounts of power from a small region requires a power source far more efficient than the nuclear fusion that powers stars. The conversion of gravitational potential energy to radiation by infalling to a black hole converts between 6% and 32% of the mass to energy, compared to 0.7% for the conversion of mass to energy in a star like our Sun. It is the only process known that can produce such high power over a very long term. (Stellar explosions such as supernovas and gamma-ray bursts, and direct matter–antimatter annihilation, can also produce very high power output, but supernovae only last for days, and the universe does not appear to have had large amounts of antimatter at the relevant times.)
Since quasars exhibit all the properties common to other active galaxies such as Seyfert galaxies, the emission from quasars can be readily compared to those of smaller active galaxies powered by smaller supermassive black holes. To create a luminosity of 1040 watts (the typical brightness of a quasar), a super-massive black hole would have to consume the material equivalent of 10 stars per year. The brightest known quasars devour 1000 solar masses of material every year. The largest known is estimated to consume matter equivalent to 10 Earths per second. Quasar luminosities can vary considerably over time, depending on their surroundings. Since it is difficult to fuel quasars for many billions of years, after a quasar finishes accreting the surrounding gas and dust, it becomes an ordinary galaxy.
Radiation from quasars is partially "nonthermal" (i.e., not due to black-body radiation), and approximately 10% are observed to also have jets and lobes like those of radio galaxies that also carry significant (but poorly understood) amounts of energy in the form of particles moving at relativistic speeds. Extremely high energies might be explained by several mechanisms (see Fermi acceleration and Centrifugal mechanism of acceleration). Quasars can be detected over the entire observable electromagnetic spectrum, including radio, infrared, visible light, ultraviolet, X-ray and even gamma rays. Most quasars are brightest in their rest-frame ultraviolet wavelength of 121.6 nm Lyman-alpha emission line of hydrogen, but due to the tremendous redshifts of these sources, that peak luminosity has been observed as far to the red as 900.0 nm, in the near infrared. A minority of quasars show strong radio emission, which is generated by jets of matter moving close to the speed of light. When viewed downward, these appear as blazars and often have regions that seem to move away from the center faster than the speed of light (superluminal expansion). This is an optical illusion due to the properties of special relativity.
Quasar redshifts are measured from the strong spectral lines that dominate their visible and ultraviolet emission spectra. These lines are brighter than the continuous spectrum. They exhibit Doppler broadening corresponding to mean speed of several percent of the speed of light. Fast motions strongly indicate a large mass. Emission lines of hydrogen (mainly of the Lyman series and Balmer series), helium, carbon, magnesium, iron and oxygen are the brightest lines. The atoms emitting these lines range from neutral to highly ionized, leaving it highly charged. This wide range of ionization shows that the gas is highly irradiated by the quasar, not merely hot, and not by stars, which cannot produce such a wide range of ionization.
Like all (unobscured) active galaxies, quasars can be strong X-ray sources. Radio-loud quasars can also produce X-rays and gamma rays by inverse Compton scattering of lower-energy photons by the radio-emitting electrons in the jet.
Iron quasars show strong emission lines resulting from low-ionization iron (Fe II), such as IRAS 18508-7815.
Quasars also provide some clues as to the end of the Big Bang's reionization. The oldest known quasars (z = 6) display a Gunn–Peterson trough and have absorption regions in front of them indicating that the intergalactic medium at that time was neutral gas. More recent quasars show no absorption region, but rather their spectra contain a spiky area known as the Lyman-alpha forest; this indicates that the intergalactic medium has undergone reionization into plasma, and that neutral gas exists only in small clouds.
The intense production of ionizing ultraviolet radiation is also significant, as it would provide a mechanism for reionization to occur as galaxies form. Despite this, current theories suggest that quasars were not the primary source of reionization; the primary causes of reionization were probably the earliest generations of stars, known as Population III stars (possibly 70%), and dwarf galaxies (very early small high-energy galaxies) (possibly 30%).
Quasars show evidence of elements heavier than helium, indicating that galaxies underwent a massive phase of star formation, creating population III stars between the time of the Big Bang and the first observed quasars. Light from these stars may have been observed in 2005 using NASA's Spitzer Space Telescope, although this observation remains to be confirmed.
The taxonomy of quasars includes various subtypes representing subsets of the quasar population having distinct properties.
Radio-loud quasars are quasars with powerful jets that are strong sources of radio-wavelength emission. These make up about 10% of the overall quasar population. Radio-quiet quasars are those quasars lacking powerful jets, with relatively weaker radio emission than the radio-loud population. The majority of quasars (about 90%) are radio-quiet.
Broad absorption-line (BAL) quasars are quasars whose spectra exhibit broad absorption lines that are blueshifted relative to the quasar's rest frame, resulting from gas flowing outward from the active nucleus in the direction toward the observer. Broad absorption lines are found in about 10% of quasars, and BAL quasars are usually radio-quiet. In the rest-frame ultraviolet spectra of BAL quasars, broad absorption lines can be detected from ionized carbon, magnesium, silicon, nitrogen, and other elements.
Type 2 (or Type II) quasars are quasars in which the accretion disk and broad emission lines are highly obscured by dense gas and dust. They are higher-luminosity counterparts of Type 2 Seyfert galaxies.
Red quasars are quasars with optical colors that are redder than normal quasars, thought to be the result of moderate levels of dust extinction within the quasar host galaxy. Infrared surveys have demonstrated that red quasars make up a substantial fraction of the total quasar population.
Optically violent variable (OVV) quasars are radio-loud quasars in which the jet is directed toward the observer. Relativistic beaming of the jet emission results in strong and rapid variability of the quasar brightness. OVV quasars are also considered to be a type of blazar.
Weak emission line quasars are quasars having unusually faint emission lines in the ultraviolet/visible spectrum.
The energetic radiation of the quasar makes dark galaxies glow, helping astronomers to understand the obscure early stages of galaxy formation.
Because quasars are extremely distant, bright, and small in apparent size, they are useful reference points in establishing a measurement grid on the sky. The International Celestial Reference System (ICRS) is based on hundreds of extra-galactic radio sources, mostly quasars, distributed around the entire sky. Because they are so distant, they are apparently stationary to our current technology, yet their positions can be measured with the utmost accuracy by very-long-baseline interferometry (VLBI). The positions of most are known to 0.001 arcsecond or better, which is orders of magnitude more precise than the best optical measurements.
A grouping of two or more quasars on the sky can result from a chance alignment, where the quasars are not physically associated, from actual physical proximity, or from the effects of gravity bending the light of a single quasar into two or more images by gravitational lensing.
When two quasars appear to be very close to each other as seen from Earth (separated by a few arcseconds or less), they are commonly referred to as a "double quasar". When the two are also close together in space (i.e. observed to have similar redshifts), they are termed a "quasar pair", or as a "binary quasar" if they are close enough that their host galaxies are likely to be physically interacting.
As quasars are overall rare objects in the universe, the probability of three or more separate quasars being found near the same physical location is very low, and determining whether the system is closely separated physically requires significant observational effort. The first true triple quasar was found in 2007 by observations at the W. M. Keck Observatory Mauna Kea, Hawaii. LBQS 1429-008 (or QQQ J1432-0106) was first observed in 1989 and at the time was found to be a double quasar. When astronomers discovered the third member, they confirmed that the sources were separate and not the result of gravitational lensing. This triple quasar has a redshift of z = 2.076. The components are separated by an estimated 30–50 kiloparsecs (roughly 97,000-160,000 light years), which is typical for interacting galaxies. In 2013, the second true triplet of quasars, QQQ J1519+0627, was found with a redshift z = 1.51, the whole system fitting within a physical separation of 25 kpc (about 80,000 light years).
The first true quadruple quasar system was discovered in 2015 at a redshift z = 2.0412 and has an overall physical scale of about 200 kpc (roughly 650,000 light years).
A multiple-image quasar is a quasar whose light undergoes gravitational lensing, resulting in double, triple or quadruple images of the same quasar. The first such gravitational lens to be discovered was the double-imaged quasar Q0957+561 (or Twin Quasar) in 1979. An example of a triply lensed quasar is PG1115+08. Several quadruple-image quasars are known, including the Einstein Cross and the Cloverleaf Quasar, with the first such discoveries happening in the mid-1980s.
094253 Jack Reyes
Inspiration from banderitas and kites...kids to represent when creativity is at its peak
Milton Keynes, Midsummer Boulevard. The new hi-tech car park, adjacent to the grade 2 listed shopping mall, was designed by Leslie Jones Architecture and opened in 2019. Planned in the 1960s, and 'finished' in 1992, Milton Keynes is one of the last of the New Towns of the C20th. Planned with generally low rise buildings, it utilises a road layout according to street hierarchy principles, using a grid pattern of approximately 1 km (0.62 mi) intervals, rather than on the more conventional radial pattern. It has not however proved very sustainable, with major replacement work in the centre on buildings around just 3 decades old. Often referred to as a city, it has in fact been denied city status on a number of occasions, and remains Buckinghamshire's largest town.
Milton Keynes, Buckinghamshire, Home Counties, England - Midsummer Boulevard - Marlborough Gate car park
September 2021
danielsolisblog.blogspot.com/2012/04/hierarchy-of-interfa...
Hierarchy of Interface for Tabletop Games as observed by John Stavropoulos
TOOLS
The actual components of play, like character sheets, cheat sheets, boards and bits.
TEXT
The actual documented rules and how they are presented, including exact wording, procedures and game terms.
RULES
The parameters of play as best recalled by the players. Less formal than text, but more formal than the basic design intent.
INTENT
The assumptions of how a game would be played, often expressed directly by the designer with minimal formal documentation.
Source:
“This is why I feel game interfaces (character sheets, cheat sheets) are more important than rules text and rules text is more important than rules and rules are more important than design intent when it comes to actual play... we generally can’t assume players will read the rules, that GMs won’t remember more than 5-7 distinct pieces of information at a time without reference, and if we don’t provide teaching tools, that the game will be taught correctly.”
plus.google.com/u/0/111266966448135449970/posts/aqxmnLe61rg
DESIGN: Daniel Solis — danielsolis.com
“Dice,” “Pencil” symbol from The Noun Project collection.
“Paper” symbol by Tom Schott, from The Noun Project collection.
“Quote” symbol by Henry Ryder, from The Noun Project collection.
“Note” symbol by Brendan Lynch, from the Noune Project collection.
“Pawn” symbol by Kenneth Von Alt, from The Noun Project collection.
“Dialog” symbol by Dima Yagnyuk, from The Noun Project collection.
had these old mattresses sitting outside my house, to be thrown away, and I knew I had to do something eccentric! Its almost the reverse of this photo shot from the window I was posing in. Instead though, it was much darker and had a sense of 'a fall' the construction overalls innocence, I am also doing a photo every week of the construction site and going to put them together! I'm VERY behind on putting them together, so I will have to spend a day doing that XD
Pics from various XML code just made up out of copied parts. Made it up to 400 nodes. Some were pre-auto adjusting node size.
Pics from various XML code just made up out of copied parts. Made it up to 400 nodes. Some were pre-auto adjusting node size.
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SQUAT - SOUNDS
AUTONOMES KULTURZENTRUM HANAU
(Besetztes Haus / Metzgerstrasse-Squat in Hanau / Germany).
Photographs 1987-1994
- Please scroll down for english and german info) -
The Squat - Photos:
www.flickr.com/photos/sterneck/sets/72157627799174125
Squating the Parliament (1988):
www.flickr.com/photos/sterneck/sets/72157627923787960
Concert-Photos 1987-1988:
www.flickr.com/photos/sterneck/sets/72157627799191443
Concert-Photos 1989-1990:
www.flickr.com/photos/sterneck/sets/72157627923799072
Concert-Photos 1991-1992:
www.flickr.com/photos/sterneck/sets/72157627923811302
Concert-Photos 1993-1994:
www.flickr.com/photos/sterneck/sets/72157627923815978
- Concert-Photos 1989-1990:
Archbishop Kebab (Edinburgh, Scotland) - 1989
Citizen Fish (Warminster, England) - 1990
Die Trottel (Budapest, Hungary) - 1988
Do Or Die (Amsterdam, Netherlands) - 1990
Israelvis (Trondhrim, Norway) - 1989
Kina (Valle d'Aosta, Italy) - 1990
Life… But How To Live It? (Oslo, Norway) - 1989
Political Asylum (Edinburgh, Scotland) - 1989
Rikk Agnew (Fullerton, USA) - 1990
Robsie Richter (Hanau, Germany) - 1990
Sharon Tates Children (Stuttgart, Germany) - 1989
Sore Throat (Yorkshire, England) - 1990
Spongetunnel (Chicago, USA) - 1989
Ugly Food (Lübeck, Germany, Odense, Denmark) - 1989
Zygote (Bath, England) - 1990
..... and Friends and .....
.........
There were a lot more bands playing in the squat.
If you have photographs or recordings - please get in contact:
contact@sterneck.net
Thanx! *
- * -
THE SQUATED AUTONOMOUS CULTURE CENTER
METZGERSTRASSE / HANAU
In December 1986 some people in Hanau (Germany) decided to squat a house that had been empty for a long time, Metzgerstraße 8. They restored it and filled this free space with a new life.
Soon it became an ’Autonomous Culture-Center’ for the people and by the people, and also a focal point for a solidaric projects and for the resistance against ruling systems in all their repressive forms. The center has had a long history of attempts to establish a self-determined culture-center in Hanau, although it has always been repressed by the local city council.
The basic forum of the center is the ”squatter meeting,” which is open to everyone who has an interest in the squat as a counter-cultural free space. Decisions are made on the consent principle, which means that they try to find a decision that can be supported by everyone. Many activists in the squat, but not all, describe themselves as members of the autonomy movement, which connects anarchist, communist and feminist ideas.
At the moment there are a lot of projects, groups, and events that take place in the center. Everything is done on a do-it-yourself and nonprofit basis; no one receives money for her or his work. Solidarity, trust and self-determination are the basis for all work. Here are some examples:
- The ’Infoladen’ (Infoshop): The Infoshop is an opportunity to get information that can’t be found in the normal bourgeois media. There are a lot of autonomous, left radical and feminist leaflets, brochures and newspapers available. There is also a small media center and an archive that includes material on topics like anti-fascism, atomic politics, women’s liberation, internationalism, etc.
- The ’Volxküche’ (Peoples Kitchen): Frequently people from the community cook a vegetarian meal that is available for a small price. The idea behind this is to overcome isolation between people and the patriarchal roles typical in the kitchen, and, of course, to provide a good tasting meal for many people.
- The Concerts: Concerts in the center are organized, and absolutely dedicated to the principle of working in a self-determined way without a manager, an agency, or even a contract. The bands that play in the squat should have a mutual relation to the ideas of the center. There are no musical limits: Local punk bands have played there as well as jazz bands from North-America and Avantguarde projects from Eastern Europe. Some of the performances have been released on tapes and records.
In a way, the things that happen between the people in the center are more important than the events: changes in behavior, opportunities to live together without hierarchical structures, and new ways of relating. Although the squat is like an island in some ways, it’s far from a concrete utopia. Problems in interpersonal relations exist, as well as differences between ideals and real behaviour.
If people want to go alternative ways, the authorities try to stop them. In Hanau the local city council has said for a long time that none of the things the squatters do and organize represent culture. They decided in parliament that the center was to be closed and torn down without an alternative. In place of the squat, they planned to build five parking places. A decision that is very symbolic and characteristic. Certainly, the real aim was to destroy the ideas and the structures this center stands for.
The answer of the supporters of the Autonomous Culture-Center was the squatting of the parliament of the city. The politicians went out of the building and the squatters voted for the continuation of the center.
Up to now the authorities have not been able to realize their plans for various reasons. On the one hand there are many people who support the squat. There are also legal difficulties around closing it, and they are afraid of the resistance and activities that could take place after closing the squat.
But even if they evict the center, they can’t repress the ideas that the squat stands for. It’s about a self-determined culture and a self-determined life. It’s about dreams and ideals. It’s about consequence and change, here and now.
Wolfgang Sterneck, 2001.
Autonomes Kulturzentrum
Metzgerstrasse 8, D-63450 Hanau, Germany.
Autonomes Kulturzentrum Metzgerstraße:
- www.metzgerstrasse-hanau.org
- de-de.facebook.com/people/Metzgerstrasse-Acht-Hanau/10000...
- www.myspace.com/metzgerstrasse
Info on the Project of John Cage and Sterneck / KomistA in benefit of the squat:
- www.sterneck.net/john-cage/metzgerstrasse-e
- * -
SUBVERSIVE SOUNDS *
Konzerte im Autonomen Kulturzentrum Hanau.
Das besetzte Haus
Im Dezember 1986 kam es in Hanau zur Besetzung eines ehemaligen Nachtclubs in der Metzgerstraße 8. Das Gebäude, das zuvor über Jahre hinweg leer stand, wurde renoviert, neu gestaltet, umbenannt und wird seitdem als Autonomes Kulturzentrum genutzt. Das Ziel der Besetzung war es, einen Freiraum zu schaffen, in dem die Vorstellung einer autonomen Kultur wie auch die Wiederaneignung des entfremdeten Alltags konkret umsetzbar wird.
Vor diesem Hintergrund gelang es, ein Zentrum zu entwickeln, in dem solidarisches Handeln, kollektives Leben und politische Identität auf vielen Ebenen verschmelzen oder sich zumindest annähern. Die Metzgerstraße wurde dadurch zu einem wichtigen Bezugspunkt von dem auf verschiedenen Ebenen vielschichtige politische, soziale und kulturelle Impulse ausgingen.
Im Laufe der Jahre entstanden vielfältige Projekte wie die Volxküche (Essen zum Selbstkostenpreis), der Infoladen (Aktuelle politische Informationen und Archiv) und das Basta-Cafe (Treffpunkt und Sozialberatung). Die politischen Schwerpunkte der im Kulturzentrum aktiven Gruppen liegen unter anderen in den Bereichen 'Internationale Solidarität', Antifaschismus und 'Soziale Veränderung'.
Die Entscheidungen innerhalb des Kulturzentrums werden basisdemokratisch nach dem Konsensprinzip getroffen. Alle Aktivitäten basieren auf einer idealistischen Grundhaltung. Keine Person aus dem Zentrum erhält für ihre Tätigkeiten eine finanzielle Entlohnung.
Selbstbestimmte Kultur ohne Kommerz
Musik hatte von Anfang an in der Metzgerstraße eine besondere Bedeutung. Über das Musikhören hinaus machen viele AktivistInnen selbst Musik, veröffentlichen eigene Aufnahmen oder organisieren Konzerte. Im Sinne des DIY-Prinzipes ('Do it Yourself') werden die Auftritte im direkten Kontakt mit den MusikerInnen ohne Konzertagenturen und auch ohne Verträge auf völlig nichtkommerzieller Basis organisiert.
Eine Grundlage bildet ein solidarisches Verhältnis der MusikerInnen zur Metzgerstraße, was sich unter anderem auch in der Gage ausdrückt, die sich in der Regel auf die für die Band entstandenen Unkosten und die Verpflegung beschränkt. Der Eintrittspreis ist so ausgerichtet, dass er für alle interessierten Personen erschwinglich ist und die anfallenden Kosten deckt bzw. im Rahmen von Benefiz-Konzerten bestimmte Projekte unterstützt.
Freiräume statt Parkplätze
Während der ehemalige sozialdemokratische Kulturdezernat Hanaus davon sprach, dass in der Metzgerstraße keine Kultur stattfindet, bildete dass selbstorganisierte Zentrum durch die Auftritte von Bands aus Westeuropa und Nordamerika einen im Hanauer Kulturleben herausragenden internationalen Bezugspunkt. Die musikalische Bandbreite umfasst unter anderem Rockmusik in den verschiedensten Schattierungen, Punk, Hardcore, Folk und Jazz, sowie experimentelle und improvisierte Musik. Lokale Nachwuchsbands traten im Laufe der Jahre genauso auf wie renommierte Gruppen aus unterschiedlichsten Ländern. Einen Kultcharakter erlangten zudem die Nachtcafe-Sessions, an denen jeder und jede teilnehmen konnte.
Die Aufnahmen einiger Konzerte wurden später auf verschiedenen Tonträgern veröffentlicht. 1992 kam es daneben zur Veröffentlichung eines der Metzgerstraße gewidmeten Stücks des Avantgarde-Komponisten John Cage.
In den Anfangsjahren plante der Hanauer Magistrat das Haus nach einer Räumung abreißen zu lassen, um dort stattdessen fünf Parkplätze zu errichten. Die Kulturpolitik des Magistrates entlarvte sich dadurch in einer kaum zu übertreffenden symbolhaften Weise selbst. Das Vorhaben wurde jedoch nicht zuletzt in Folge einer Besetzung des Stadtparlamentes durch Unterstützerinnen des Kulturzentrums nicht weiter verfolgt.
Rund 25 Jahre nach der Besetzung wird das Haus weiterhin als Kulturzentrum genutzt. Im ansonsten auf Konsum und Kommerz ausgerichteten Stadtzentrum Hanaus ist es mit seinen vielfältigen Projekten kreativer wie auch subversiver Freiraum.
Wolfgang Sterneck, September 2011.
Autonomes Kulturzentrum Metzgerstraße:
- www.metzgerstrasse-hanau.org
- de-de.facebook.com/people/Metzgerstrasse-Acht-Hanau/10000...
- www.myspace.com/metzgerstrasse
Eine ausführliche Beschreibung der Geschichte des Kulturzentrums:
Freiräume entwickeln - Das besetzte autonome Kulturzentrum Metzgerstraße Hanau
- www.sterneck.net/squat/metzgerstrasse-d
English Info:
The squated Autonomous Culture Center Metzgerstrasse Hanau
- www.sterneck.net/squat/metzgerstrasse-e
Infos zum Benefiz-Projekt von John Cage und Sterneck / KomistA für das Kulturzentrum:
- * -
Foto: 1988 ? 1989
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I had to delete original and process scan again. It was just plain and gray.
My first BW film attempt after two years of digital.
Pics from various XML code just made up out of copied parts. Made it up to 400 nodes. Some were pre-auto adjusting node size.
091428
Monica Esquivel
I wanted to give the poster an artsy and organic feel, thus the many curves. The word "kalinangan" is related to culture, which I think Ateneo's is quite rich and diverse. I used black and gold to show this. The Ateneo art culture is also progressing, so, to show this growth, I used flowers.
092032
Jenny Lapus
I wanted to incorporate the banderitas used in the original poster, but in a different way. I stylized the text by adding drop shadows.
"The Cathedral Church of Christ, Blessed Mary the Virgin and St Cuthbert of Durham, commonly known as Durham Cathedral and home of the Shrine of St Cuthbert, is a cathedral in the city of Durham, England. It is the seat of the Bishop of Durham, the fourth-ranked bishop in the Church of England hierarchy. The present cathedral was begun in 1093, replacing the Saxon 'White Church', and is regarded as one of the finest examples of Norman architecture in Europe. In 1986 the cathedral and Durham Castle were designated a UNESCO World Heritage Site.
Durham Cathedral holds the relics of Saint Cuthbert, transported to Durham by Lindisfarne monks in the ninth century, the head of Saint Oswald of Northumbria, and the remains of the Venerable Bede. In addition, its library contains one of the most complete sets of early printed books in England, the pre-Dissolution monastic accounts, and three copies of Magna Carta.
From 1080 until 1836 the Bishop of Durham held the powers of an Earl Palatine, exercising military and civil leadership as well as religious leadership, in order to protect the English Border with Scotland. The cathedral walls formed part of Durham Castle, the chief seat of the Bishop of Durham.
There are daily Church of England services at the cathedral, with the Durham Cathedral Choir singing daily except Mondays and when the choir is on holiday. It is a major tourist attraction and received 694,429 visitors in 2018.
Durham (/ˈdʌrəm/, locally /ˈdɜrəm/) is a cathedral city and the county town of County Durham in North East England. The city lies on the River Wear, to the south-west of Sunderland, south of Newcastle upon Tyne and to the north of Darlington. Founded over the final resting place of St Cuthbert, its Norman cathedral became a centre of pilgrimage in medieval England. The cathedral and adjacent 11th-century castle were designated a World Heritage Site by UNESCO in 1986. The castle has been the home of Durham University since 1832. HM Prison Durham is also located close to the city centre. City of Durham is the name of the civil parish.
The name "Durham" comes from the Celtic element "dun", signifying a hill fort, and the Old Norse "holme", which translates to island. The Lord Bishop of Durham takes a Latin variation of the city's name in his official signature, which is signed "N. Dunelm". Some attribute the city's name to the legend of the Dun Cow and the milkmaid who in legend guided the monks of Lindisfarne carrying the body of Saint Cuthbert to the site of the present city in 995 AD. Dun Cow Lane is said to be one of the first streets in Durham, being directly to the east of Durham Cathedral and taking its name from a depiction of the city's founding etched in masonry on the south side of the cathedral. The city has been known by a number of names throughout history. The original Nordic Dun Holm was changed to Duresme by the Normans and was known in Latin as Dunelm. The modern form Durham came into use later in the city's history. The north-eastern historian Robert Surtees chronicled the name changes in his History and Antiquities of the County Palatine of Durham but states that it is an "impossibility" to tell when the city's modern name came into being.
Durham is likely to be Gaer Weir in Armes Prydein, derived from Brittonic cajr meaning "an enclosed, defensible site" (c.f. Carlisle; Welsh caer) and the river-name Wear." - info from Wikipedia.
Summer 2019 I did a solo cycling tour across Europe through 12 countries over the course of 3 months. I began my adventure in Edinburgh, Scotland and finished in Florence, Italy cycling 8,816 km. During my trip I took 47,000 photos.
Now on Instagram.
Become a patron to my photography on Patreon.
Kookie Santos
093328
We were asked to make a re-design of the poster of last year's Fine Arts Festival. This poster aims to inform its viewers easily through the use of hierarchy of elements. The information of all events is enclosed in the blue and yellow banderitas so that it may emphasize the information despite it's small size relative to the title of the main event (Kalinangan).
083131
RAMOS, Matthew Jacob F.
The logo basically reminded me of the boats and weavings in Mindanao, so I decided to go for that. This is the revision of my previous work on the subject. Hopefully, it looks practical.
Pics from various XML code just made up out of copied parts. Made it up to 400 nodes. Some were pre-auto adjusting node size.
Pics from various XML code just made up out of copied parts. Made it up to 400 nodes. Some were pre-auto adjusting node size.
Chittorgarh Fort (Hindi/Rajasthani: चित्तौड दुर्ग Chittorgarh Durg) is the largest fort in India and the grandest in the state of Rajasthan. It is a World Heritage Site. The fort, plainly known as Chittor, was the capital of Mewar and is today situated several kilometres south of Bhilwara. It was initially ruled by Guhilot and later by Sisodias, the Suryavanshi clans of Chattari Rajputs, from the 7th century, until it was finally abandoned in 1568 after the siege by Emperor Akbar in 1567. It sprawls majestically over a hill 180 m in height spread over an area of 280 ha above the plains of the valley drained by the Berach River. The fort precinct with an evocative history is studded with a series of historical palaces, gates, temples and two prominent commemoration towers. These monumental ruins have inspired the imagination of tourists and writers for centuries.
The fort was sacked three times between the 15th and 16th centuries; in 1303 Allauddin Khilji defeated Rana Ratan Singh, in 1535 Bahadur Shah, the Sultan of Gujarat defeated Bikramjeet Singh and in 1567 Emperor Akbar defeated Maharana Udai Singh II who left the fort and founded Udaipur. Each time the men fought bravely rushing out of the fort walls charging the enemy but lost every time. Following these defeats, Jauhar was committed thrice by more than 13,000 ladies and children of the Rajput heroes who laid their lives in battles at Chittorgarh Fort, first led by Rani Padmini wife of Rana Rattan Singh who was killed in the battle in 1303, and later by Rani Karnavati in 1537 AD.
Thus, the fort represents the quintessence of tribute to the nationalism, courage, medieval chivalry and sacrifice exhibited by the Mewar rulers of Sisodia and their kinsmen and women and children, between the 7th and 16th centuries. The rulers, their soldiers, the women folk of royalty and the commoners considered death as a better option than dishonor in the face of surrender to the foreign invading armies.
GEOGRAPHY
Chittorgarh, located in the southern part of the state of Rajasthan, 233 km from Ajmer, midway between Delhi and Mumbai on the National Highway 8 (India) in the road network of Golden Quadrilateral. Chittorgarh is situated where National Highways No. 76 & 79 intersect.
The fort rises abruptly above the surrounding plains and is spread over an area of 2.8 km2. The highest elevation at the fort is 1,075 m. It is situated on the left bank of the Berach river (a tributary of the Banas River) and is linked to the new town of Chittorgarh (known as the 'Lower Town') developed in the plains after 1568 AD when the fort was deserted in light of introduction of artillery in the 16th century, and therefore the capital was shifted to more secure Udaipur, located on the eastern flank of Aravalli hill range. Mughal Emperor Akbar attacked and sacked this fort which was but one of the 84 forts of Mewar,but the capital was shifted to Aravalli hills where heavy artillery & cavalry were not effective. A winding hill road of more than 1 km length from the new town leads to the west end main gate, called Ram Pol, of the fort. Within the fort, a circular road provides access to all the gates and monuments located within the fort walls.
The fort that once boasted of 84 water bodies has only 22 of them now. These water bodies are fed by natural catchment and rainfall, and have a combined storage of 4 billion litres that could meet the water needs of an army of 50,000. The supply could last for four years. These water bodies are in the form of ponds, wells and step wells.
HISTORY
Chittorgarh Fort is considered to be the largest fort of India in terms of area. It is stated that the fort was constructed by the Mauryans during the 7th century AD and hence derives its name after the Mauryan ruler, Chitrangada Mori, as inscribed on coins of the period. Historical records show Chittorgarh fort as the capital of Mewar for 834 years. It was established in 734 AD by Bappa Rawal, founder ruler in the hierarchy of the Sisodia rulers of Mewar. It is also said that the fort was gifted to Bappa Rawal as part of Solanki princess’s dowry in the 8th century. The fort was looted and destroyed at the hands of Emperor Akbar in 1568 AD and subsequently never resettled but only refurbished in 1905 AD. Three important battles were fought for control of the fort; in 1303, Ala-ud-din Khilji besieged the fort; in 1535, Sultan of Gujarat Bahadur Shah besieged the fort; and in 1568, Mughal Emperor Akbar attacked the fort. Not that there were only defeats at the fort. Excluding the periods of siege, the fort had always remained in possession of the Sisodias of the Guhilot (or Gehlot/Guhila) clan of Rajputs, who descended from Bappa Rawal. There were also success stories of establishment of the fort and its reconstruction after every siege, before it was finally abandoned in 1568, all of which are narrated.
Chittor is cited in the Mahabharat epic. It is said that Bhima, the second of the Pandava brothers of Epic Mahabaharata fame, known for his mighty strength gave a powerful hit with his fist to the ground that resulted in water springing up to form a large reservoir. It is called Bhimlat kund, an artificial tank named after Bhima. Folk legend also mentions that Bhima started building the fort.
BAPPA RAWAL
The earliest history linked to the Bappa Rawal's fort is that of the Huna Kingdom of Sialkot (of Mihir Kula 515-540 AD) that was destroyed by Yashodharman. This was subsequently seized by a new dynasty of kshatriyas called Tak or Taxaka. According to historians, the Taxak Mori were the lords of Chittor from a very early period. After a few generations, the Guhilots supplanted them. From 725 to 735 AD, there were numerous defenders who appear to have considered the cause of Chittor their own, the Tak from Asirgarh. This race appears to have retained possession of Asirgarh for at least two centuries after this event and one of its chieftain Bappa Rawal was the most conspicuous leader in the lineage of Prithvi Raj. In the poems of Chandar he is called the "Standard, bearer, Tak of Asir."
SIEGE OF 1303
Ala ud din Khilji, Sultan of Delhi, rallied his forces against Mewar, in 1303 AD. The Chittorgarh fort was till then considered impregnable and grand, atop a natural hill. But his immediate reason for invading the fort was his obsessive desire to capture Rani Padmini, the unrivalled beautiful queen of Rana Ratan Singh and take her into his harem. The Rana, out of politeness, allowed the Khilji to view Padmini through a set of mirrors. But this viewing of Padmini further fired Khilji’s desire to possess her. After the viewing, as a gesture of courtesy, when the Rana accompanied the Sultan to the outer gate, he was treacherously captured. Khilji conveyed to the queen that the Rana would be released only if she agreed to join his harem. But the queen had other plans. She agreed to go to his camp if permitted to go in a Royal style with an entourage, in strict secrecy. Instead of her going, she sent 700 well armed soldiers disguised in litters and they rescued the Rana and took him to the fort. But Khilji chased them to the fort where a fierce battle ensued at the outer gate of the fort in which the Rajput soldiers were overpowered and the Rana was killed. Khilji won the battle on August 26, 1303. Soon thereafter, instead of surrendering to the Sultan, the royal Rajput ladies led by Rani Padmini preferred to die through the Rajput’s ultimate tragic rite of Jauhar (self immolation on a pyre). In revenge, Khilji killed thirty thousand Hindus. He entrusted the fort to his son Khizr Khan to rule and renamed the fort as 'Khizrabad'. He also showered gifts on his son by way of
a red canopy, a robe embroidered with gold and two standards one green and the other black and threw upon him rubies and emeralds.
He returned to Delhi after the fierce battle at the fort.
RANA HAMMIR & SUCCESSORS
Khizr Khan’s rule at the fort lasted till 1311 AD and due to the pressure of Rajputs he was forced to entrust power to the Sonigra chief Maldeva who held the fort for 7 years. Hammir Singh, usurped control of the fort from Maldeva by “treachery and intrigue” and Chittor once again regained its past glory. Hammir, before his death in 1364 AD, had converted Mewar into a fairly large and prosperous kingdom. The dynasty (and clan) fathered by him came to be known by the name Sisodia after the village where he was born. His son Ketra Singh succeeded him and ruled with honour and power. Ketra Singh’s son Lakha who ascended the throne in 1382 AD also won several wars. His famous grandson Rana Kumbha came to the throne in 1433 AD and by that time the Muslim rulers of Malwa and Gujarat had acquired considerable clout and were keen to usurp the powerful Mewar state.
RANA KUMBHA & CLAN
There was resurgence during the reign of Rana Kumbha in the 15th century. Rana Kumbha, also known as Maharana Kumbhakarna, son of Rana Mokal, ruled Mewar between 1433 AD and 1468 AD. He is credited with building up the Mewar kingdom assiduously as a force to reckon with. He built 32 forts (84 fortresses formed the defense of Mewar) including one in his own name, called Kumbalgarh. But his end came in 1468 AD at the hands of his own son Rana Udaysimha (Uday Singh I) who assassinated him to gain the throne of Mewar. This patricide was not appreciated by the people of Mewar and consequently his brother Rana Raimal assumed the reins of power in 1473. After his death in May 1509, Sangram Singh (also known as Rana Sanga), his youngest son, became the ruler of Mewar, which brought in a new phase in the history of Mewar. Rana Sanga, with support from Medini Rai (a Rajput chief of Alwar), fought a valiant battle against Mughal emperor Babar at Khanwa in 1527. He ushered in a period of prestige to Chittor by defeating the rulers of Gujarat and also effectively interfered in the matters of Idar. He also won small areas of the Delhi territory. In the ensuing battle with Ibrahim Lodi, Rana won and acquired some districts of Malwa. He also defeated the combined might of Sultan Muzaffar of Gujarat and the Sultan of Malwa. By 1525 AD, Rana Sanga had developed Chittor and Mewar, by virtue of great intellect, valour and his sword, into a formidable military state. But in a decisive battle that was fought against Babar on March 16, 1527, the Rajput army of Rana Sanga suffered a terrible defeat and Sanga escaped to one of his fortresses. But soon thereafter in another attack on the Chanderi fort the valiant Rana Sanga died and with his death the Rajput confederacy collapsed.
SIEGE OF 1534
Bahadur Shah who came to the throne in 1526 AD as the Sultan of Gujarat besieged the Chittorgarh fort in 1534. The fort was sacked and, once again the medieval dictates of chivalry determined the outcome. Following the defeat of the Rana, it is said 13,000 Rajput women committed jauhar (self immolation on the funeral pyre) and 3,200 Rajput warriors rushed out of the fort to fight and die.
SIEGE OF 1567
The final Siege of Chittorgarh came 33 years later, in 1567, when the Mughal Emperor Akbar invaded the fort. Akbar wanted to conquer Mewar, which was being ably ruled by Rana Uday Singh II, a fine prince of Mewar. To establish himself as the supreme lord of Northern India, he wanted to capture the renowned fortress of Chittor, as a precursor to conquering the whole of India. Shakti Singh, son of the Rana who had quarreled with his father, had run away and approached Akbar when the later had camped at Dholpur preparing to attack Malwa. During one of these meetings, in August 1567, Shakti Singh came to know from a remark made in jest by emperor Akbar that he was intending to wage war against Chittor. Akbar had told Shakti Singh in jest that since his father had not submitted himself before him like other princes and chieftains of the region he would attack him. Startled by this revelation, Shakti Singh quietly rushed back to Chittor and informed his father of the impending invasion by Akbar. Akbar was furious with the departure of Shakti Singh and decided to attack Mewar to humble the arrogance of the Ranas. In September 1567, the emperor left for Chittor, and on October 20, 1567, camped in the vast plains outside the fort. In the meantime, Rana Udai Singh, on the advice of his council of advisors, decided to go away from Chittor to the hills of Udaipur. Jaimal and Patta, two brave army chieftains of Mewar, were left behind to defend the fort along with 8,000 Rajput warriors under their command. Akbar laid siege to the fortress. The Rajput army fought valiantly and Akbar himself had narrowly escaped death. In this grave situation, Akbar had prayed for divine help for achieving victory and vowed to visit the shrine of the sufi saint Khwaja at Ajmer. The battle continued till February 23, 1568. On that day Jaymal was seriously wounded but he continued to fight with support from Patta. Jayamal ordered jauhar to be performed when many beautiful princesses of Mewar and noble matrons committed self-immolation at the funeral pyre. Next day the gates of the fort were opened and Rajput soldiers rushed out bravely to fight the enemies. Jayamal and Patta who fought bravely were at last killed in action. One figure estimates that 30,000 soldiers were killed in action. Akbar immediately repaired himself to Ajmer to perform his religious vow.
RETURN OF THE FORT TO MEWAR
But in 1616, Jehangir returned Chittor fort to the Rajputs, when Maharana Amar Singh was the chief of Mewar. However, the fort was not resettled though it was refurbished several centuries later in 1905 during British Raj.
PRECINCTS
The fort which is roughly in the shape of a fish has a circumference of 13 km with a maximum width of 3 km and it covers an area of 700 acres. The fort is approached through a zig zag and difficult ascent of more than 1 km from the plains, after crossing over a bridge made in limestone. The bridge spans the Gambhiri River and is supported by ten arches (one has a curved shape while the balance have pointed arches). Apart from the two tall towers, which dominate the majestic fortifications, the sprawling fort has a plethora of palaces and temples (many of them in ruins) within its precincts.
The 305 hectares component site, with a buffer zone of 427 hectares, encompasses the fortified stronghold of Chittorgarh, a spacious fort located on an isolated rocky plateau of approximately 2 km length and 155m width.
It is surrounded by a perimeter wall 4.5 kilometres long, beyond which a 45° hill slope makes it almost inaccessible to enemies. The ascent to the fort passes through seven gateways built by the Mewar ruler Rana Kumbha (1433- 1468) of the Sisodia clan. These gates are called, from the base to the hill top, the Paidal Pol, Bhairon Pol, Hanuman Pol, Ganesh Pol, Jorla Pol, Laxman Pol, and Ram Pol, the final and main gate.
The fort complex comprises 65 historic built structures, among them 4 palace complexes, 19 main temples, 4 memorials and 20 functional water bodies. These can be divided into two major construction phases. The first hill fort with one main entrance was established in the 5th century and successively fortified until the 12th century. Its remains are mostly visible on the western edges of the plateau. The second, more significant defence structure was constructed in the 15th century during the reign of the Sisodia Rajputs, when the royal entrance was relocated and fortified with seven gates, and the medieval fortification wall was built on an earlier wall construction from the 13th century.
Besides the palace complex, located on the highest and most secure terrain in the west of the fort, many of the other significant structures, such as the Kumbha Shyam Temple, the Mira Bai Temple, the Adi Varah Temple, the Shringar Chauri Temple, and the Vijay Stambh memorial were constructed in this second phase. Compared to the later additions of Sisodian rulers during the 19th and 20th centuries, the predominant construction phase illustrates a comparatively pure Rajput style combined with minimal eclecticism, such as the vaulted substructures which were borrowed from Sultanate architecture. The 4.5 km walls with integrated circular enforcements are constructed from dressed stone masonry in lime mortar and rise 500m above the plain. With the help of the seven massive stone gates, partly flanked by hexagonal or octagonal towers, the access to the fort is restricted to a narrow pathway which climbs up the steep hill through successive, ever narrower defence passages. The seventh and final gate leads directly into the palace area, which integrates a variety of residential and official structures. Rana Kumbha Mahal, the palace of Rana Kumbha, is a large Rajput domestic structure and now incorporates the Kanwar Pade Ka Mahal (the palace of the heir) and the later palace of the poetess Mira Bai (1498-1546). The palace area was further expanded in later centuries, when additional structures, such as the Ratan Singh Palace (1528–31) or the Fateh Prakash, also named Badal Mahal (1885-1930), were added. Although the majority of temple structures represent the Hindu faith, most prominently the Kalikamata Temple (8th century), the Kshemankari Temple (825-850) the Kumbha Shyam Temple (1448) or the Adbuthnath Temple (15th- 16th century), the hill fort also contains Jain temples, such as Shringar Chauri (1448) and Sat Bis Devri (mid-15th century) Also the two tower memorials, Kirti Stambh (13th-14th century) and Vijay Stambha (1433-1468), are Jain monuments. They stand out with their respective heights of 24m and 37m, which ensure their visibility from most locations of the fort complex. Finally, the fort compound is home to a contemporary municipal ward of approximately 3,000 inhabitants, which is located near Ratan Singh Tank at the northern end of the property.
GATES
The fort has total seven gates (in local language, gate is called Pol), namely the Padan Pol, Bhairon Pol, Hanuman Pol, Ganesh Pol, Jodla Pol, Laxman Pol and the main gate named the Ram Pol (Lord Rama's Gate). All the gateways to the fort have been built as massive stone structures with secure fortifications for military defense. The doors of the gates with pointed arches are reinforced to fend off elephants and cannon shots. The top of the gates have notched parapets for archers to shoot at the enemy army. A circular road within the fort links all the gates and provides access to the numerous monuments (ruined palaces and 130 temples) in the fort.
During the second siege, Prince Bagh Singh died at the Padan Pol in 1535 AD. Prince Jaimal of Badnore and his clansman Kalla were killed by Akbar at a location between the Bhairon Pol and Hanuman Pol in the last siege of the fort in 1567 (Kalla carried the wounded Jaimal out to fight). Chhatris, with the roof supported by corbeled arches, have been built to commemorate the spots of their sacrifice. Their statues have also been erected, at the orders of Emperor Akbar, to commemorate their valiant deaths. At each gate, cenotaphs of Jaimal (in the form of a statue of a Rajput warrior on horseback) and Patta have also been constructed. At Ram Pol, the entrance gate to the fort, a Chaatri was built in memory of the 15 year old Patta of Kelwa, who had lost his father in battle, and saw the sword yielding mother and wife on the battle field who fought valiantly and died at this gate. He led the saffron robed Rajput warriors, who all died fighting for Mewar’s honour. Suraj Pol (Sun Gate) provides entry to the eastern wall of the fort. On the right of Suraj Pol is the Darikhana or Sabha (council chamber) behind which lie a Ganesha temple and the zenana (living quarters for women). A massive water reservoir is located towards the left of Suraj Pol. There is also a peculiar gate, called the Jorla Pol (Joined Gate), which consists of two gates joined together. The upper arch of Jorla Pol is connected to the base of Lakshman Pol. It is said that this feature has not been noticed anywhere else in India. The Lokota Bari is the gate at the fort’s northern tip, while a small opening that was used to hurl criminals into the abyss is seen at the southern end.
VIJAY STAMBHA
The Vijay Stambha (Tower of Victory) or Jaya Stambha, called the symbol of Chittor and a particularly bold expression of triumph, was erected by Rana Kumbha between 1458 and 1468 to commemorate his victory over Mahmud Shah I Khalji, the Sultan of Malwa, in 1440 AD. Built over a period of ten years, it raises 37.2 metres over a 4.4 m2 base in nine stories accessed through a narrow circular staircase of 157 steps (the interior is also carved) up to the 8th floor, from where there is good view of the plains and the new town of Chittor. The dome, which was a later addition, was damaged by lightning and repaired during the 19th century. The Stamba is now illuminated during the evenings and gives a beautiful view of Chittor from the top.
KIRTI STAMBHA
Kirti Stambha (Tower of Fame) is a 22 metres high tower built on a 9.1 m base with 4.6 m at the top, is adorned with Jain sculptures on the outside and is older (probably 12th century) and smaller than the Victory Tower. Built by a Bagherwal Jain merchant Jijaji Rathod, it is dedicated to Adinath, the first Jain tirthankar (revered Jain teacher). In the lowest floor of the tower, figures of the various tirthankars of the Jain pantheon are seen in special niches formed to house them. These are digambara monuments. A narrow stairway with 54 steps leads through the six storeys to the top. The top pavilion that was added in the 15th century has 12 columns.
RANA KUMBHA PALACE
At the entrance gate near the Vijaya Stamba, Rana Kumbha's palace (in ruins), the oldest monument, is located. The palace included elephant and horse stables and a temple to Lord Shiva. Maharana Udai Singh, the founder of Udaipur, was born here; the popular folk lore linked to his birth is that his maid Panna DaiPanna Dhai saved him by substituting her son in his place as a decoy, which resulted in her son getting killed by Banbir. The prince was spirited away in a fruit basket. The palace is built with plastered stone. The remarkable feature of the palace is its splendid series of canopied balconies. Entry to the palace is through Suraj Pol that leads into a courtyard. Rani Meera, the famous poetess saint, also lived in this palace. This is also the palace where Rani Padmini, consigned herself to the funeral pyre in one of the underground cellars, as an act of jauhar along with many other women. The Nau Lakha Bandar (literal meaning: nine lakh treasury) building, the royal treasury of Chittor was also located close by. Now, across from the palace is a museum and archeological office. The Singa Chowri temple is also nearby.
FATEH PRAKASH PALACE
Located near Rana Khumba palace, built by Rana Fateh Singh, the precincts have modern houses and a small museum. A school for local children (about 5,000 villagers live within the fort) is also nearby.
GAUMUKH RESERVOIR
A spring feeds the tank from a carved cow’s mouth in the cliff. This pool was the main source of water at the fort during the numerous sieges.
PADMINI´S PALACE
Padmini's Palace or Rani Padmini's Palace is a white building and a three storied structure (a 19th-century reconstruction of the original). It is located in the southern part of the fort. Chhatris (pavilions) crown the palace roofs and a water moat surrounds the palace. This style of palace became the forerunner of other palaces built in the state with the concept of Jal Mahal (palace surrounded by water). It is at this Palace where Alauddin was permitted to glimpse the mirror image of Rani Padmini, wife of Maharana Rattan Singh. It is widely believed that this glimpse of Padmini's beauty besotted him and convinced him to destroy Chittor in order to possess her. Maharana Rattan Singh was killed and Rani Padmini committed Jauhar. Rani Padmini's beauty has been compared to that of Cleopatra and her life story is an eternal legend in the history of Chittor. The bronze gates to this pavilion were removed and transported to Agra by Akbar.
OTHER SIGHTS
Close to Kirti Sthamba is the Meera Temple, or the Meerabai Temple. Rana Khumba built it in an ornate Indo–Aryan architectural style. It is associated with the mystic saint-poet Mirabai who was an ardent devotee of Lord Krishna and dedicated her entire life to His worship. She composed and sang lyrical bhajans called Meera Bhajans. The popular legend associated with her is that with blessings of Krishna, she survived after consuming poison sent to her by her evil brother-in-law. The larger temple in the same compound is the Kumbha Shyam Temple (Varaha Temple). The pinnacle of the temple is in pyramid shape. A picture of Meerabai praying before Krishna has now been installed in the temple.
Across from Padmini’s Palace is the Kalika Mata Temple. Originally, a Sun Temple dated to the 8th century dedicated to Surya (the Sun God) was destroyed in the 14th century. It was rebuilt as a Kali temple.
Another temple on the west side of the fort is the ancient Goddess Tulja Bhavani Temple built to worship Goddess Tulja Bhavani is considered sacred. The Tope Khana (cannon foundry) is located next to this temple in a courtyard, where a few old cannons are still seen.
JAUHAR MELA
The fort and the city of Chittorgarh host the biggest Rajput festival called the "Jauhar Mela". It takes place annually on the anniversary of one of the jauhars, but no specific name has been given to it. It is generally believed that it commemorates Padmini’s jauhar, which is most famous. This festival is held primarily to commemorate the bravery of Rajput ancestors and all three jauhars which happened at Chittorgarh Fort. A huge number of Rajputs, which include the descendants of most of the princely families, hold a procession to celebrate the Jauhar. It has also become a forum to air one's views on the current political situation in the country.
WIKIPEDIA
In these times of world economic crisis, we may find ourselves examining our more basic requirements as theorized by Abraham Maslow in his "hierarchy of needs".
Shivalaya | Badami | Karnataka | India | Dec | 2008
The capital of the Early Chalukyas, Badami is picturesquely situated at the mouth of a ravine between two rocky hills. Badami is famous for its four cave temples - all hewn out of sand stone on the precipice of a hill. The temples dates back to 6th-8th century.
This picturesque location has been used by Mani Ratnam in numerous scenes in his famous film "Guru"(2007)
Hierarchical Vigil by Metropolitan Hilarion and Bishop Nikolai of Manhattan in the presence of the Kursk-Root Icon The Vigil at St. John The Baptist Cathedral in Washington on September 10, 2021. Photo by Yuri Gripas
Pics from various XML code just made up out of copied parts. Made it up to 400 nodes. Some were pre-auto adjusting node size.
Die Trottel (Budapest, Hungary) - 1988
Live at
Autonomes Kulturzentrum Metzgerstrasse Hanau
.
SQUAT - SOUNDS
AUTONOMES KULTURZENTRUM HANAU
(Besetztes Haus / Metzgerstrasse-Squat in Hanau / Germany).
Photographs 1987-1994
- Please scroll down for english and german info) -
The Squat - Photos:
www.flickr.com/photos/sterneck/sets/72157627799174125
Squating the Parliament (1988):
www.flickr.com/photos/sterneck/sets/72157627923787960
Concert-Photos 1987-1988:
www.flickr.com/photos/sterneck/sets/72157627799191443
Concert-Photos 1989-1990:
www.flickr.com/photos/sterneck/sets/72157627923799072
Concert-Photos 1991-1992:
www.flickr.com/photos/sterneck/sets/72157627923811302
Concert-Photos 1993-1994:
www.flickr.com/photos/sterneck/sets/72157627923815978
- Concert-Photos 1989-1990:
Archbishop Kebab (Edinburgh, Scotland) - 1989
Citizen Fish (Warminster, England) - 1990
Die Trottel (Budapest, Hungary) - 1988
Do Or Die (Amsterdam, Netherlands) - 1990
Israelvis (Trondhrim, Norway) - 1989
Kina (Valle d'Aosta, Italy) - 1990
Life… But How To Live It? (Oslo, Norway) - 1989
Political Asylum (Edinburgh, Scotland) - 1989
Rikk Agnew (Fullerton, USA) - 1990
Robsie Richter (Hanau, Germany) - 1990
Sharon Tates Children (Stuttgart, Germany) - 1989
Sore Throat (Yorkshire, England) - 1990
Spongetunnel (Chicago, USA) - 1989
Ugly Food (Lübeck, Germany, Odense, Denmark) - 1989
Zygote (Bath, England) - 1990
..... and Friends and .....
.........
There were a lot more bands playing in the squat.
If you have photographs or recordings - please get in contact:
contact@sterneck.net
Thanx! *
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THE SQUATED AUTONOMOUS CULTURE CENTER
METZGERSTRASSE / HANAU
In December 1986 some people in Hanau (Germany) decided to squat a house that had been empty for a long time, Metzgerstraße 8. They restored it and filled this free space with a new life.
Soon it became an ’Autonomous Culture-Center’ for the people and by the people, and also a focal point for a solidaric projects and for the resistance against ruling systems in all their repressive forms. The center has had a long history of attempts to establish a self-determined culture-center in Hanau, although it has always been repressed by the local city council.
The basic forum of the center is the ”squatter meeting,” which is open to everyone who has an interest in the squat as a counter-cultural free space. Decisions are made on the consent principle, which means that they try to find a decision that can be supported by everyone. Many activists in the squat, but not all, describe themselves as members of the autonomy movement, which connects anarchist, communist and feminist ideas.
At the moment there are a lot of projects, groups, and events that take place in the center. Everything is done on a do-it-yourself and nonprofit basis; no one receives money for her or his work. Solidarity, trust and self-determination are the basis for all work. Here are some examples:
- The ’Infoladen’ (Infoshop): The Infoshop is an opportunity to get information that can’t be found in the normal bourgeois media. There are a lot of autonomous, left radical and feminist leaflets, brochures and newspapers available. There is also a small media center and an archive that includes material on topics like anti-fascism, atomic politics, women’s liberation, internationalism, etc.
- The ’Volxküche’ (Peoples Kitchen): Frequently people from the community cook a vegetarian meal that is available for a small price. The idea behind this is to overcome isolation between people and the patriarchal roles typical in the kitchen, and, of course, to provide a good tasting meal for many people.
- The Concerts: Concerts in the center are organized, and absolutely dedicated to the principle of working in a self-determined way without a manager, an agency, or even a contract. The bands that play in the squat should have a mutual relation to the ideas of the center. There are no musical limits: Local punk bands have played there as well as jazz bands from North-America and Avantguarde projects from Eastern Europe. Some of the performances have been released on tapes and records.
In a way, the things that happen between the people in the center are more important than the events: changes in behavior, opportunities to live together without hierarchical structures, and new ways of relating. Although the squat is like an island in some ways, it’s far from a concrete utopia. Problems in interpersonal relations exist, as well as differences between ideals and real behaviour.
If people want to go alternative ways, the authorities try to stop them. In Hanau the local city council has said for a long time that none of the things the squatters do and organize represent culture. They decided in parliament that the center was to be closed and torn down without an alternative. In place of the squat, they planned to build five parking places. A decision that is very symbolic and characteristic. Certainly, the real aim was to destroy the ideas and the structures this center stands for.
The answer of the supporters of the Autonomous Culture-Center was the squatting of the parliament of the city. The politicians went out of the building and the squatters voted for the continuation of the center.
Up to now the authorities have not been able to realize their plans for various reasons. On the one hand there are many people who support the squat. There are also legal difficulties around closing it, and they are afraid of the resistance and activities that could take place after closing the squat.
But even if they evict the center, they can’t repress the ideas that the squat stands for. It’s about a self-determined culture and a self-determined life. It’s about dreams and ideals. It’s about consequence and change, here and now.
Wolfgang Sterneck, 2001.
Autonomes Kulturzentrum
Metzgerstrasse 8, D-63450 Hanau, Germany.
Autonomes Kulturzentrum Metzgerstraße:
- www.metzgerstrasse-hanau.org
- de-de.facebook.com/people/Metzgerstrasse-Acht-Hanau/10000...
- www.myspace.com/metzgerstrasse
Info on the Project of John Cage and Sterneck / KomistA in benefit of the squat:
- www.sterneck.net/john-cage/metzgerstrasse-e
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SUBVERSIVE SOUNDS *
Konzerte im Autonomen Kulturzentrum Hanau.
Das besetzte Haus
Im Dezember 1986 kam es in Hanau zur Besetzung eines ehemaligen Nachtclubs in der Metzgerstraße 8. Das Gebäude, das zuvor über Jahre hinweg leer stand, wurde renoviert, neu gestaltet, umbenannt und wird seitdem als Autonomes Kulturzentrum genutzt. Das Ziel der Besetzung war es, einen Freiraum zu schaffen, in dem die Vorstellung einer autonomen Kultur wie auch die Wiederaneignung des entfremdeten Alltags konkret umsetzbar wird.
Vor diesem Hintergrund gelang es, ein Zentrum zu entwickeln, in dem solidarisches Handeln, kollektives Leben und politische Identität auf vielen Ebenen verschmelzen oder sich zumindest annähern. Die Metzgerstraße wurde dadurch zu einem wichtigen Bezugspunkt von dem auf verschiedenen Ebenen vielschichtige politische, soziale und kulturelle Impulse ausgingen.
Im Laufe der Jahre entstanden vielfältige Projekte wie die Volxküche (Essen zum Selbstkostenpreis), der Infoladen (Aktuelle politische Informationen und Archiv) und das Basta-Cafe (Treffpunkt und Sozialberatung). Die politischen Schwerpunkte der im Kulturzentrum aktiven Gruppen liegen unter anderen in den Bereichen 'Internationale Solidarität', Antifaschismus und 'Soziale Veränderung'.
Die Entscheidungen innerhalb des Kulturzentrums werden basisdemokratisch nach dem Konsensprinzip getroffen. Alle Aktivitäten basieren auf einer idealistischen Grundhaltung. Keine Person aus dem Zentrum erhält für ihre Tätigkeiten eine finanzielle Entlohnung.
Selbstbestimmte Kultur ohne Kommerz
Musik hatte von Anfang an in der Metzgerstraße eine besondere Bedeutung. Über das Musikhören hinaus machen viele AktivistInnen selbst Musik, veröffentlichen eigene Aufnahmen oder organisieren Konzerte. Im Sinne des DIY-Prinzipes ('Do it Yourself') werden die Auftritte im direkten Kontakt mit den MusikerInnen ohne Konzertagenturen und auch ohne Verträge auf völlig nichtkommerzieller Basis organisiert.
Eine Grundlage bildet ein solidarisches Verhältnis der MusikerInnen zur Metzgerstraße, was sich unter anderem auch in der Gage ausdrückt, die sich in der Regel auf die für die Band entstandenen Unkosten und die Verpflegung beschränkt. Der Eintrittspreis ist so ausgerichtet, dass er für alle interessierten Personen erschwinglich ist und die anfallenden Kosten deckt bzw. im Rahmen von Benefiz-Konzerten bestimmte Projekte unterstützt.
Freiräume statt Parkplätze
Während der ehemalige sozialdemokratische Kulturdezernat Hanaus davon sprach, dass in der Metzgerstraße keine Kultur stattfindet, bildete dass selbstorganisierte Zentrum durch die Auftritte von Bands aus Westeuropa und Nordamerika einen im Hanauer Kulturleben herausragenden internationalen Bezugspunkt. Die musikalische Bandbreite umfasst unter anderem Rockmusik in den verschiedensten Schattierungen, Punk, Hardcore, Folk und Jazz, sowie experimentelle und improvisierte Musik. Lokale Nachwuchsbands traten im Laufe der Jahre genauso auf wie renommierte Gruppen aus unterschiedlichsten Ländern. Einen Kultcharakter erlangten zudem die Nachtcafe-Sessions, an denen jeder und jede teilnehmen konnte.
Die Aufnahmen einiger Konzerte wurden später auf verschiedenen Tonträgern veröffentlicht. 1992 kam es daneben zur Veröffentlichung eines der Metzgerstraße gewidmeten Stücks des Avantgarde-Komponisten John Cage.
In den Anfangsjahren plante der Hanauer Magistrat das Haus nach einer Räumung abreißen zu lassen, um dort stattdessen fünf Parkplätze zu errichten. Die Kulturpolitik des Magistrates entlarvte sich dadurch in einer kaum zu übertreffenden symbolhaften Weise selbst. Das Vorhaben wurde jedoch nicht zuletzt in Folge einer Besetzung des Stadtparlamentes durch Unterstützerinnen des Kulturzentrums nicht weiter verfolgt.
Rund 25 Jahre nach der Besetzung wird das Haus weiterhin als Kulturzentrum genutzt. Im ansonsten auf Konsum und Kommerz ausgerichteten Stadtzentrum Hanaus ist es mit seinen vielfältigen Projekten kreativer wie auch subversiver Freiraum.
Wolfgang Sterneck, September 2011.
Autonomes Kulturzentrum Metzgerstraße:
- www.metzgerstrasse-hanau.org
- de-de.facebook.com/people/Metzgerstrasse-Acht-Hanau/10000...
- www.myspace.com/metzgerstrasse
Eine ausführliche Beschreibung der Geschichte des Kulturzentrums:
Freiräume entwickeln - Das besetzte autonome Kulturzentrum Metzgerstraße Hanau
- www.sterneck.net/squat/metzgerstrasse-d
English Info:
The squated Autonomous Culture Center Metzgerstrasse Hanau
- www.sterneck.net/squat/metzgerstrasse-e
Infos zum Benefiz-Projekt von John Cage und Sterneck / KomistA für das Kulturzentrum:
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