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1956 Fonteyn in 'Birthday Offering'.
Gala programme: www.flickr.com/photos/w77t/31616208571/in/photostream
Frederick Ashton created Birthday Offering to celebrate The Royal Ballet’s 25th anniversary - they were about to receive a royal charter and change their name from Sadler's Wells Ballet to The Royal Ballet.
The world première took place at the Royal Opera House, Covent Garden on 5th May 1956 and seven ballerinas take solo roles as well as being paired with solo male dancers - Margot Fonteyn was paired with Michael Somes.
That evening Birthday Offering was sandwiched between 'The Rake's Progress' and 'Façade' - both starring Robert Helpmann.
Born [Margaret Evelyn Hookham] on 18th May 1919 in Reigate, England and died on 21st Feb 1991 in Panama City, Panama.
Her debut was with the Vic-Wells Ballet in 1934 and initially danced under the name of Peggy Hookham then Margot Fontes, then Margot Fonteyn.
In the 1930s she and Robert Helpmann formed a very successful dance partnership and they dance together for 25 years.
Fonteyn was awarded a DBE in 1956.
Appointed prima ballerina assoluta of the Royal Ballet in 1979, as a gift for her 60th Birthday. The title was sanctioned by Queen Elizabeth II as patron of the company.
As a dancer she made her last appearance in Nureyev's 1979 summer season, and in Feb 1986 she appeared on stage for the last time as 'The Queen' in "The Sleeping Beauty".
The availability of oxygen is one of the most important indicators of the condition of a water body, because dissolved oxygen, or DO, (the amount of oxygen dissolved in water) is necessary for most aquatic organisms, including fish and invertebrates. Some species have very defined lower limits of DO that they can tolerate. Increases in DO can indicate improvements in water quality, such as has occurred in many parts of the world in the last 30 years. Over the two decades, rivers in Europe and Australasia have shown a significant statistical reduction in biological oxygen demand concentrations, (an indicator of the organic pollution of freshwater), suggesting positive trends. There was no change in the assessed results for North America, although there was a tighter data distribution, indicating the data available for 1991-2000 is less variable than for previous periods.
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Philippe Rekacewicz, February 2006
Drawing on research and statistical data since 2000, experts at the University of British Columbia in Vancouver have shown that catches reported by China are largely overestimated, concealing a substantial decline in world catches since the middle of the 1980s.
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Philippe Rekacewicz, February 2006
Global water type by percentage. Estimates of global water resources based on several different calculation methods have produced varied estimates. Shiklomanov in Gleick (1993) estimated that: - The total volume of water on earth is 1.4 billion km3. - The volume of freshwater resources is 35 million km3, or about 2.5% of the total volume. Of these, 24 million km3 or 68.9% is in the form of ice and permanent snow cover in mountainous regions, and in the Antarctic and Arctic regions. - Some 8 million km3 or 30.8% is stored underground in the form of groundwater (shallow and deep groundwater basins up to 2,000 metres, soil moisture, swamp water and permafrost). This constitutes about 97% of all the freshwater potentially available for human use. - Freshwater lakes and rivers contain an estimated 105,000 km3 or 0.3% of the world’s freshwater. - The total usable freshwater supply for ecosystems and humans is 200,000 km3 of water, which is less than 1% of all freshwater resources, and only 0.01% of all the water on earth (Gleick, 1993; Shiklomanov, 1999).
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Philippe Rekacewicz, February 2006
Welcome to the swinging sixties. Programme still sixpence cheaper than for the 1951 Lancs Grand National.
The programmes for Saturday 11th August 2001 commenced with a welcome from First Manchester and the Bolton Bus Group, and a reminder that Crook Street Depot (out of bounds) and Moor Lane and the surrounding streets were fully operational, Take Care and Be Aware at all times, paid credit to all who had moved mountains and molehills to make the day possible including GMPTE for allowing the event to take place and relaxing the vehicle age/type rules for certain tendered services, details of the day and a timetable of events, a brief history of the Atlantean, some cartoons, a personal reflection, and that some bespoke videos had been produced along with a raffle for a headboard.
Proceeds from the event were going to then named The Imperial Cancer Research Fund.
Swifts car park was closed for the day to allow a static display of visiting Atlanteans, thanks to all who attended.
I ran some 250 copies off, absolutely no idea how many we would need, on the depot printer. Some 2500 B/W and 250 front covers. I was just finishing packing up the sheets in the boxes they came in ready for a mass stapling session at home when I heard someone in the office say, "The printers out of ink, (They were huge!!) I only renewed the cartridges yesterday."
TIME TO DISAPPEAR!!
A ½-hourly shuttle between Moor Lane and the display at Crook Street was operated by Bolton 232.
But of course the star of the day was the last native fleet of GM Standard Atlanteans and they were near the end ......but we mustered 37 I think.
I arranged for all the Atlanteans to be rostered on local services where possible so each one visited Moor Lane Bus Station at least once an hour, sometimes twice.
The success of the day was summed up by a visitors comment in the press - There just seemed to be Atlanteans everywhere and its probably the last time we will ever witness such an event ....
I invited Dave Spencer for the day but he was unable to attend, otherwise engaged, and later told me he bitterly regretted not attending as he had heard that he'd missed a good day....
10 Years On was held on Sunday 21st August 2011 and a few similar programmes were produced. Being a Sunday the normal services were concentrated on the centre island platform on Moor Lane so thanks to TfGM, we were allowed to use the out of use bays for displaying the static visiting vehicles, (Crook Street having closed by this time), some privately owned and those from the Bolton Bus Preservation Group and those from The Selnec Preservation Society. Again thanks to all.
But this time there were no in service GM Standards and no CRUK participation.
A free hourly service Blackhorse Street to Bobs Smithy Pub on the peak of Chorley Old Road was run, so a much lower key day.
It all seems so long ago now, 21 years in the case of the native fleet......
It is estimated that water pollution denies close to 1.3 billion people (20% of the global population in 2000) access to clean water supplies. In 1986, WHO reported that there were 250 million new cases of waterborne diseases each year, causing the deaths of nearly 3.5 million people. An estimated 4.2 billion cases of waterborne diseases are reported each year, with diarrhoea accounting for 4 billion of the total (Cosgrove and Rijsberman, 2000; Revenga et al., 2000). Some 460 million people - more than 8% of the world’s population - live in countries using so much of their freshwater resources that they can be considered highly water stressed (UNCSD, 1999; WMO 1997). A further 25% of the population lives in countries approaching a position of serious water stress (WMO, 1997). An area is experiencing water stress when annual water supplies drop below 1,700 m3 per person. When annual water supplies drop below 1,000 m3 per person, the population faces water scarcity (UNPD, UNEP, World Bank, and WRI, 2000).
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Philippe Rekacewicz, February 2006
Alkalinity is commonly used to indicate a water body’s capacity to buffer against acidity; that is, the ability to resist, or dampen, changes in pH. Thus, alkaline compounds in water, such as bicarbonates, carbonates, and hydroxides, lower the acidity of the water and increase the pH. Alkalinity (as CaCO3) was analysed for all sampling stations available at the continental level. Concentrations remained reasonably steady between the two decades for Africa, Asia, South America and Australasia, but significant increases were noted for European and North American rivers, which may indicate a shift towards reduced acidic impacts at the continental scale. Overall, during the last 30 years , alkalinity has decreased in North America and Europe, but has significantly increased in Asia. Examination of the outflow stations in 82 monitored river basins indicate a decrease in bicarbonate concentrations between the two decades , in the northern latitudes, including North America, Europe and Asia. For the period 1976-1990, European rivers displayed the highest concentrations of calcium at a continental level, with concentrations varying between 2 mg and 50 mg per litre for major rivers. Comparing the two decades, observations of surface water showed an increase in calcium concentrations in the Laurentian shield region of North America, and in the rivers of the north central European region.
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Philippe Rekacewicz, February 2006
A 4 page Programme from 1945 for this war time Cup Final. Chelsea winning 2-0 in front of a gate of 90,000.
The International Space Station (ISS) is a space station (habitable artificial satellite) in low Earth orbit. The ISS programme is a joint project between five participating space agencies: NASA (United States), Roscosmos (Russia), JAXA (Japan), ESA (Europe), and CSA (Canada).[6][7] The ownership and use of the space station is established by intergovernmental treaties and agreements.[8]
The ISS serves as a microgravity and space environment research laboratory in which crew members conduct experiments in biology, human biology, physics, astronomy, meteorology, and other fields.[9][10][11] The station is suited for the testing of spacecraft systems and equipment required for missions to the Moon and Mars.[12] The ISS maintains an orbit with an average altitude of 400 kilometres (250 mi) by means of reboost manoeuvres using the engines of the Zvezda module or visiting spacecraft.[13] It circles the Earth in roughly 92 minutes and completes 15.5 orbits per day.[14]
The station is divided into two sections, the Russian Orbital Segment (ROS), which is operated by Russia, and the United States Orbital Segment (USOS), which is shared by many nations. Roscosmos has endorsed the continued operation of ISS through 2024,[15] but had previously proposed using elements of the Russian segment to construct a new Russian space station called OPSEK.[16]As of December 2018, the station is expected to operate until 2030.[17]
The first ISS component was launched in 1998, with the first long-term residents arriving on 2 November 2000.[18] Since then, the station has been continuously occupied for 18 years and 359 days.[19] This is the longest continuous human presence in low Earth orbit, having surpassed the previous record of 9 years and 357 days held by Mir. The latest major pressurised module was fitted in 2011, with an experimental inflatable space habitat added in 2016. Development and assembly of the station continues, with several major new Russian elements scheduled for launch starting in 2020. The ISS is the largest human-made body in low Earth orbit and can often be seen with the naked eye from Earth.[20][21] The ISS consists of pressurised habitation modules, structural trusses, solar arrays, radiators, docking ports, experiment bays and robotic arms. Major ISS modules have been launched by Russian Proton and Soyuz rockets and US Space Shuttles.[22]
The ISS is the ninth space station to be inhabited by crews, following the Soviet and later Russian Salyut, Almaz, and Mir stations as well as Skylab from the US. The station is serviced by a variety of visiting spacecraft: the Russian Soyuz and Progress, the US Dragon and Cygnus, the Japanese H-II Transfer Vehicle,[6] and the European Automated Transfer Vehicle. The Dragon spacecraft allows the return of pressurised cargo to Earth (downmass), which is used for example to repatriate scientific experiments for further analysis. The Soyuz return capsule has minimal downmass capability next to the astronauts.
The ISS has been visited by astronauts, cosmonauts and space tourists from 18 different nations. As of 14 March 2019, 236 people from 18 countries had visited the space station, many of them multiple times. The United States sent 149 people, Russia sent 47, nine were Japanese, eight were Canadian, five were Italian, four were French, three were German, and there were one each from Belgium, Brazil, Denmark, Kazakhstan, Malaysia, the Netherlands, South Africa, United Arab Emirates, South Korea, Spain, Sweden, and the United Kingdom.[23]
Contents
1 Purpose
2 Manufacturing
3 Assembly
4 Structure
5 Systems
6 Operations
7 Mission controls
8 Fleet operations
9 Life aboard
10 Crew health and safety
11 Orbital debris threats
12 End of mission
13 Cost
14 International co-operation
15 Sightings from Earth
16 See also
17 Notes
18 References
19 Further reading
20 External links
Purpose
The ISS was originally intended to be a laboratory, observatory, and factory while providing transportation, maintenance, and a low Earth orbit staging base for possible future missions to the Moon, Mars, and asteroids. However, not all of the uses envisioned in the initial Memorandum of Understanding between NASA and Roskosmos have come to fruition.[24] In the 2010 United States National Space Policy, the ISS was given additional roles of serving commercial, diplomatic[25] and educational purposes.[26]
Scientific research
Main article: Scientific research on the International Space Station
Comet Lovejoy photographed by Expedition 30 commander Dan Burbank
Expedition 8 Commander and Science Officer Michael Foale conducts an inspection of the Microgravity Science Glovebox
Fisheye view of several labs
CubeSats are deployed by the NanoRacks CubeSat Deployer
The ISS provides a platform to conduct scientific research, with power, data, cooling, and crew available to support experiments. Small uncrewed spacecraft can also provide platforms for experiments, especially those involving zero gravity and exposure to space, but space stations offer a long-term environment where studies can be performed potentially for decades, combined with ready access by human researchers.[27][28]
The ISS simplifies individual experiments by allowing groups of experiments to share the same launches and crew time. Research is conducted in a wide variety of fields, including astrobiology, astronomy, physical sciences, materials science, space weather, meteorology, and human research including space medicine and the life sciences.[9][10][11][29][30] Scientists on Earth have timely access to the data and can suggest experimental modifications to the crew. If follow-on experiments are necessary, the routinely scheduled launches of resupply craft allows new hardware to be launched with relative ease.[28] Crews fly expeditions of several months' duration, providing approximately 160 person-hours per week of labour with a crew of 6. However, a considerable amount of crew time is taken up by station maintenance.[9][31]
Perhaps the most notable ISS experiment is the Alpha Magnetic Spectrometer (AMS), which is intended to detect dark matter and answer other fundamental questions about our universe and is as important as the Hubble Space Telescope according to NASA. Currently docked on station, it could not have been easily accommodated on a free flying satellite platform because of its power and bandwidth needs.[32][33] On 3 April 2013, scientists reported that hints of dark matter may have been detected by the AMS.[34][35][36][37][38][39] According to the scientists, "The first results from the space-borne Alpha Magnetic Spectrometer confirm an unexplained excess of high-energy positrons in Earth-bound cosmic rays."
The space environment is hostile to life. Unprotected presence in space is characterised by an intense radiation field (consisting primarily of protons and other subatomic charged particles from the solar wind, in addition to cosmic rays), high vacuum, extreme temperatures, and microgravity.[40] Some simple forms of life called extremophiles,[41] as well as small invertebrates called tardigrades[42] can survive in this environment in an extremely dry state through desiccation.
Medical research improves knowledge about the effects of long-term space exposure on the human body, including muscle atrophy, bone loss, and fluid shift. This data will be used to determine whether high duration human spaceflight and space colonisation are feasible. As of 2006, data on bone loss and muscular atrophy suggest that there would be a significant risk of fractures and movement problems if astronauts landed on a planet after a lengthy interplanetary cruise, such as the six-month interval required to travel to Mars.[43][44]
Medical studies are conducted aboard the ISS on behalf of the National Space Biomedical Research Institute (NSBRI). Prominent among these is the Advanced Diagnostic Ultrasound in Microgravity study in which astronauts perform ultrasound scans under the guidance of remote experts. The study considers the diagnosis and treatment of medical conditions in space. Usually, there is no physician on board the ISS and diagnosis of medical conditions is a challenge. It is anticipated that remotely guided ultrasound scans will have application on Earth in emergency and rural care situations where access to a trained physician is difficult.[45][46][47]
Free fall
ISS crew member storing samples
A comparison between the combustion of a candle on Earth (left) and in a free fall environment, such as that found on the ISS (right)
Gravity at the altitude of the ISS is approximately 90% as strong as at Earth's surface, but objects in orbit are in a continuous state of freefall, resulting in an apparent state of weightlessness.[48] This perceived weightlessness is disturbed by five separate effects:[49]
Drag from the residual atmosphere.
Vibration from the movements of mechanical systems and the crew.
Actuation of the on-board attitude control moment gyroscopes.
Thruster firings for attitude or orbital changes.
Gravity-gradient effects, also known as tidal effects. Items at different locations within the ISS would, if not attached to the station, follow slightly different orbits. Being mechanically interconnected these items experience small forces that keep the station moving as a rigid body.
Researchers are investigating the effect of the station's near-weightless environment on the evolution, development, growth and internal processes of plants and animals. In response to some of this data, NASA wants to investigate microgravity's effects on the growth of three-dimensional, human-like tissues, and the unusual protein crystals that can be formed in space.[10]
Investigating the physics of fluids in microgravity will provide better models of the behaviour of fluids. Because fluids can be almost completely combined in microgravity, physicists investigate fluids that do not mix well on Earth. In addition, examining reactions that are slowed by low gravity and low temperatures will improve our understanding of superconductivity.[10]
The study of materials science is an important ISS research activity, with the objective of reaping economic benefits through the improvement of techniques used on the ground.[50] Other areas of interest include the effect of the low gravity environment on combustion, through the study of the efficiency of burning and control of emissions and pollutants. These findings may improve current knowledge about energy production, and lead to economic and environmental benefits. Future plans are for the researchers aboard the ISS to examine aerosols, ozone, water vapour, and oxides in Earth's atmosphere, as well as cosmic rays, cosmic dust, antimatter, and dark matter in the universe.[10]
Exploration
A 3D plan of the Russia-based MARS-500 complex, used for ground-based experiments which complement ISS-based preparations for a human mission to Mars
The ISS provides a location in the relative safety of Low Earth Orbit to test spacecraft systems that will be required for long-duration missions to the Moon and Mars. This provides experience in operations, maintenance as well as repair and replacement activities on-orbit, which will be essential skills in operating spacecraft farther from Earth, mission risks can be reduced and the capabilities of interplanetary spacecraft advanced.[12] Referring to the MARS-500 experiment, ESA states that "Whereas the ISS is essential for answering questions concerning the possible impact of weightlessness, radiation and other space-specific factors, aspects such as the effect of long-term isolation and confinement can be more appropriately addressed via ground-based simulations".[51] Sergey Krasnov, the head of human space flight programmes for Russia's space agency, Roscosmos, in 2011 suggested a "shorter version" of MARS-500 may be carried out on the ISS.[52]
In 2009, noting the value of the partnership framework itself, Sergey Krasnov wrote, "When compared with partners acting separately, partners developing complementary abilities and resources could give us much more assurance of the success and safety of space exploration. The ISS is helping further advance near-Earth space exploration and realisation of prospective programmes of research and exploration of the Solar system, including the Moon and Mars."[53] A crewed mission to Mars may be a multinational effort involving space agencies and countries outside the current ISS partnership. In 2010, ESA Director-General Jean-Jacques Dordain stated his agency was ready to propose to the other four partners that China, India and South Korea be invited to join the ISS partnership.[54] NASA chief Charlie Bolden stated in February 2011, "Any mission to Mars is likely to be a global effort".[55] Currently, US federal legislation prevents NASA co-operation with China on space projects.[56]
Education and cultural outreach
Original Jules Verne manuscripts displayed by crew inside Jules Verne ATV
The ISS crew provides opportunities for students on Earth by running student-developed experiments, making educational demonstrations, allowing for student participation in classroom versions of ISS experiments, and directly engaging students using radio, videolink and email.[6][57] ESA offers a wide range of free teaching materials that can be downloaded for use in classrooms.[58] In one lesson, students can navigate a 3-D model of the interior and exterior of the ISS, and face spontaneous challenges to solve in real time.[59]
JAXA aims to inspire children to "pursue craftsmanship" and to heighten their "awareness of the importance of life and their responsibilities in society."[60] Through a series of education guides, a deeper understanding of the past and near-term future of crewed space flight, as well as that of Earth and life, will be learned.[61][62] In the JAXA Seeds in Space experiments, the mutation effects of spaceflight on plant seeds aboard the ISS is explored. Students grow sunflower seeds which flew on the ISS for about nine months. In the first phase of Kibō utilisation from 2008 to mid-2010, researchers from more than a dozen Japanese universities conducted experiments in diverse fields.[63]
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ESA Astronaut Paolo Nespoli's spoken voice, recorded about the ISS in November 2017, for Wikipedia
Cultural activities are another major objective. Tetsuo Tanaka, director of JAXA's Space Environment and Utilization Center, says "There is something about space that touches even people who are not interested in science."[64]
Amateur Radio on the ISS (ARISS) is a volunteer programme which encourages students worldwide to pursue careers in science, technology, engineering and mathematics through amateur radio communications opportunities with the ISS crew. ARISS is an international working group, consisting of delegations from nine countries including several countries in Europe as well as Japan, Russia, Canada, and the United States. In areas where radio equipment cannot be used, speakerphones connect students to ground stations which then connect the calls to the station.[65]
First Orbit is a feature-length documentary film about Vostok 1, the first crewed space flight around the Earth. By matching the orbit of the International Space Station to that of Vostok 1 as closely as possible, in terms of ground path and time of day, documentary filmmaker Christopher Riley and ESA astronaut Paolo Nespoli were able to film the view that Yuri Gagarin saw on his pioneering orbital space flight. This new footage was cut together with the original Vostok 1 mission audio recordings sourced from the Russian State Archive. Nespoli, during Expedition 26/27, filmed the majority of the footage for this documentary film, and as a result is credited as its director of photography.[66] The film was streamed through the website firstorbit.org in a global YouTube premiere in 2011, under a free licence.[67]
In May 2013, commander Chris Hadfield shot a music video of David Bowie's "Space Oddity" on board the station; the film was released on YouTube.[68] It was the first music video ever to be filmed in space.[69]
In November 2017, while participating in Expedition 52/53 on the ISS, Paolo Nespoli made two recordings (one in English the other in his native Italian) of his spoken voice, for use on Wikipedia articles. These were the first content made specifically for Wikipedia, in space.[70][71]
Manufacturing
Main article: Manufacturing of the International Space Station
ISS module Node 2 manufacturing and processing in the SSPF
Since the International Space Station is a multi-national collaborative project, the components for in-orbit assembly were manufactured in various countries around the world. Beginning in the mid 1990s, the U.S. components Destiny, Unity, the Integrated Truss Structure, and the solar arrays were fabricated at the Marshall Space Flight Center and the Michoud Assembly Facility. These modules were delivered to the Operations and Checkout Building and the Space Station Processing Facility for final assembly and processing for launch.[72]
The Russian modules, including Zarya and Zvezda, were manufactured at the Khrunichev State Research and Production Space Center in Moscow. Zvezda was initially manufactured in 1985 as a component for Mir-2, but was never launched and instead became the ISS Service Module.[73]
The European Space Agency Columbus module was manufactured at the European Space Research and Technology Centre (ESTEC) in the Netherlands, along with many other contractors throughout Europe.[74] The other ESA-built modules - Harmony, Tranquility, the Leonardo MPLM, and the Cupola - were initially manufactured at the Thales Alenia Space factory located at the Cannes Mandelieu Space Center. The structural steel hulls of the modules were transported by aircraft to the Kennedy Space Center SSPF for launch processing.[75]
The Japanese Experiment Module Kibō, was fabricated in various technology manufacturing facilities in Japan, at the NASDA (now JAXA) Tanegashima Space Center, and the Institute of Space and Astronautical Science. The Kibo module was transported by ship and flown by aircraft to the KSC Space Station Processing Facility.[76]
The Mobile Servicing System, consisting of the Canadarm2 and the Dextre grapple fixture, was manufactured at various factories in Canada and the United States under contract by the Canadian Space Agency. The mobile base system, a connecting framework for Canadarm2 mounted on rails, was built by Northrop Grumman.
Assembly
Main articles: Assembly of the International Space Station and List of ISS spacewalks
The assembly of the International Space Station, a major endeavour in space architecture, began in November 1998.[3] Russian modules launched and docked robotically, with the exception of Rassvet. All other modules were delivered by the Space Shuttle, which required installation by ISS and shuttle crewmembers using the Canadarm2 (SSRMS) and extra-vehicular activities (EVAs); as of 5 June 2011, they had added 159 components during more than 1,000 hours of EVA (see List of ISS spacewalks). 127 of these spacewalks originated from the station, and the remaining 32 were launched from the airlocks of docked Space Shuttles.[77] The beta angle of the station had to be considered at all times during construction.[78]
The first module of the ISS, Zarya, was launched on 20 November 1998 on an autonomous Russian Proton rocket. It provided propulsion, attitude control, communications, electrical power, but lacked long-term life support functions. Two weeks later, a passive NASA module Unity was launched aboard Space Shuttle flight STS-88 and attached to Zarya by astronauts during EVAs. This module has two Pressurised Mating Adapter (PMAs), one connects permanently to Zarya, the other allowed the Space Shuttle to dock to the space station. At that time, the Russian station Mir was still inhabited, and the ISS remained uncrewed for two years. On 12 July 2000, Zvezda was launched into orbit. Preprogrammed commands on board deployed its solar arrays and communications antenna. It then became the passive target for a rendezvous with Zarya and Unity: it maintained a station-keeping orbit while the Zarya-Unity vehicle performed the rendezvous and docking via ground control and the Russian automated rendezvous and docking system. Zarya's computer transferred control of the station to Zvezda's computer soon after docking. Zvezda added sleeping quarters, a toilet, kitchen, CO2 scrubbers, dehumidifier, oxygen generators, exercise equipment, plus data, voice and television communications with mission control. This enabled permanent habitation of the station.[79][80]
The first resident crew, Expedition 1, arrived in November 2000 on Soyuz TM-31. At the end of the first day on the station, astronaut Bill Shepherd requested the use of the radio call sign "Alpha", which he and cosmonaut Krikalev preferred to the more cumbersome "International Space Station".[81] The name "Alpha" had previously been used for the station in the early 1990s,[82] and its use was authorised for the whole of Expedition 1.[83] Shepherd had been advocating the use of a new name to project managers for some time. Referencing a naval tradition in a pre-launch news conference he had said: "For thousands of years, humans have been going to sea in ships. People have designed and built these vessels, launched them with a good feeling that a name will bring good fortune to the crew and success to their voyage."[84] Yuri Semenov, the President of Russian Space Corporation Energia at the time, disapproved of the name "Alpha" as he felt that Mir was the first modular space station, so the names "Beta" or "Mir 2" for the ISS would have been more fitting.[83][85][86]
Expedition 1 arrived midway between the flights of STS-92 and STS-97. These two Space Shuttle flights each added segments of the station's Integrated Truss Structure, which provided the station with Ku-band communication for US television, additional attitude support needed for the additional mass of the USOS, and substantial solar arrays supplementing the station's existing 4 solar arrays.[87]
Over the next two year, the station continued to expand. A Soyuz-U rocket delivered the Pirs docking compartment. The Space Shuttles Discovery, Atlantis, and Endeavour delivered the Destiny laboratory and Quest airlock, in addition to the station's main robot arm, the Canadarm2, and several more segments of the Integrated Truss Structure.
The expansion schedule was interrupted by the Space Shuttle Columbia disaster in 2003 and a resulting hiatus in flights. The Space Shuttle was grounded until 2005 with STS-114 flown by Discovery.[88]
Assembly resumed in 2006 with the arrival of STS-115 with Atlantis, which delivered the station's second set of solar arrays. Several more truss segments and a third set of arrays were delivered on STS-116, STS-117, and STS-118. As a result of the major expansion of the station's power-generating capabilities, more pressurised modules could be accommodated, and the Harmony node and Columbus European laboratory were added. These were soon followed by the first two components of Kibō. In March 2009, STS-119 completed the Integrated Truss Structure with the installation of the fourth and final set of solar arrays. The final section of Kibō was delivered in July 2009 on STS-127, followed by the Russian Poisk module. The third node, Tranquility, was delivered in February 2010 during STS-130 by the Space Shuttle Endeavour, alongside the Cupola, followed in May 2010 by the penultimate Russian module, Rassvet. Rassvet was delivered by Space Shuttle Atlantis on STS-132 in exchange for the Russian Proton delivery of the US-funded Zarya module in 1998.[89] The last pressurised module of the USOS, Leonardo, was brought to the station in February 2011 on the final flight of Discovery, STS-133.[90] The Alpha Magnetic Spectrometer was delivered by Endeavour on STS-134 the same year.[91]
As of June 2011, the station consisted of 15 pressurised modules and the Integrated Truss Structure. Five modules are still to be launched, including the Nauka with the European Robotic Arm, the Prichal module, and two power modules called NEM-1 and NEM-2.[92] As of March 2019, Russia's future primary research module Nauka is set to launch in the summer of 2020, along with the European Robotic Arm which will be able to relocate itself to different parts of the Russian modules of the station.[93]
The gross mass of the station changes over time. The total launch mass of the modules on orbit is about 417,289 kg (919,965 lb) (as of 3 September 2011).[94] The mass of experiments, spare parts, personal effects, crew, foodstuff, clothing, propellants, water supplies, gas supplies, docked spacecraft, and other items add to the total mass of the station. Hydrogen gas is constantly vented overboard by the oxygen generators.
The ISS is a third generation[95] modular space station.[96] Modular stations can allow modules to be added to or removed from the existing structure, allowing greater flexibility.
Below is a diagram of major station components. The blue areas are pressurised sections accessible by the crew without using spacesuits. The station's unpressurised superstructure is indicated in red. Other unpressurised components are yellow. The Unity node joins directly to the Destiny laboratory. For clarity, they are shown apart.
Zarya
Zarya as seen by Space Shuttle Endeavour during STS-88
Zarya (Russian: Заря́, lit. 'Dawn'), also known as the Functional Cargo Block or FGB (from the Russian: "Функционально-грузовой блок", lit. 'Funktsionalno-gruzovoy blok' or ФГБ), is the first module of the ISS to be launched.[97] The FGB provided electrical power, storage, propulsion, and guidance to the ISS during the initial stage of assembly. With the launch and assembly in orbit of other modules with more specialized functionality, Zarya is now[when?] primarily used for storage, both inside the pressurized section and in the externally mounted fuel tanks. The Zarya is a descendant of the TKS spacecraft designed for the Russian Salyut program. The name Zarya, which means sunrise,[97] was given to the FGB because it signified the dawn of a new era of international cooperation in space. Although it was built by a Russian company, it is owned by the United States.[98]
Zarya was built from December 1994 to January 1998 at the Khrunichev State Research and Production Space Center (KhSC) in Moscow.[97]
Zarya was launched on 20 November 1998 on a Russian Proton rocket from Baikonur Cosmodrome Site 81 in Kazakhstan to a 400 km (250 mi) high orbit with a designed lifetime of at least 15 years. After Zarya reached orbit, STS-88 launched on 4 December 1998 to attach the Unity module.
Unity
Unity as seen by Space Shuttle Endeavour during STS-88
Main article: Unity (ISS module)
The Unity connecting module, also known as Node 1, is the first U.S.-built component of the ISS. It connects the Russian and United States segments of the station, and is where crew eat meals together.
The module is cylindrical in shape, with six berthing locations (forward, aft, port, starboard, zenith, and nadir) facilitating connections to other modules. Unity measures 4.57 metres (15.0 ft) in diameter, is 5.47 metres (17.9 ft) long, made of steel, and was built for NASA by Boeing in a manufacturing facility at the Marshall Space Flight Center in Huntsville, Alabama. Unity is the first of the three connecting modules; the other two are Harmony and Tranquility.
Unity was carried into orbit as the primary cargo of the Space Shuttle Endeavour on STS-88, the first Space Shuttle mission dedicated to assembly of the station. On 6 December 1998, the STS-88 crew mated the aft berthing port of Unity with the forward hatch of the already orbiting Zarya module. This was the first connection made between two station modules.
Zvezda
Zvezda as seen by Space Shuttle Endeavour during STS-97
Main article: Zvezda (ISS module)
Zvezda (Russian: Звезда́, meaning "star"), Salyut DOS-8, also known as the Zvezda Service Module, is a module of the ISS. It was the third module launched to the station, and provides all of the station's life support systems, some of which are supplemented in the USOS, as well as living quarters for two crew members. It is the structural and functional center of the Russian Orbital Segment, which is the Russian part of the ISS. Crew assemble here to deal with emergencies on the station.[99][100][101]
The basic structural frame of Zvezda, known as "DOS-8", was initially built in the mid-1980s to be the core of the Mir-2 space station. This means that Zvezda is similar in layout to the core module (DOS-7) of the Mir space station. It was in fact labeled as Mir-2 for quite some time in the factory. Its design lineage thus extends back to the original Salyut stations. The space frame was completed in February 1985 and major internal equipment was installed by October 1986.
The rocket used for launch to the ISS carried advertising; it was emblazoned with the logo of Pizza Hut restaurants,[102][103][104] for which they are reported to have paid more than US$1 million.[105] The money helped support Khrunichev State Research and Production Space Center and the Russian advertising agencies that orchestrated the event.[106]
On 26 July 2000, Zvezda became the third component of the ISS when it docked at the aft port of Zarya. (U.S. Unity module had already been attached to the Zarya.) Later in July, the computers aboard Zarya handed over ISS commanding functions to computers on Zvezda.[107]
Destiny
The Destiny module being installed on the ISS
Main article: Destiny (ISS module)
The Destiny module, also known as the U.S. Lab, is the primary operating facility for U.S. research payloads aboard the International Space Station (ISS).[108][109] It was berthed to the Unity module and activated over a period of five days in February, 2001.[110] Destiny is NASA's first permanent operating orbital research station since Skylab was vacated in February 1974.
The Boeing Company began construction of the 14.5-tonne (32,000 lb) research laboratory in 1995 at the Michoud Assembly Facility and then the Marshall Space Flight Center in Huntsville, Alabama.[108] Destiny was shipped to the Kennedy Space Center in Florida in 1998, and was turned over to NASA for pre-launch preparations in August 2000. It launched on 7 February 2001 aboard the Space Shuttle Atlantis on STS-98.[110]
Quest
Quest Joint Airlock Module
Main article: Quest Joint Airlock
The Quest Joint Airlock, previously known as the Joint Airlock Module, is the primary airlock for the ISS. Quest was designed to host spacewalks with both Extravehicular Mobility Unit (EMU) spacesuits and Orlan space suits. The airlock was launched on STS-104 on 14 July 2001. Before Quest was attached, Russian spacewalks using Orlan suits could only be done from the Zvezda service module, and American spacewalks using EMUs were only possible when a Space Shuttle was docked. The arrival of Pirs docking compartment on September 16, 2001 provided another airlock from which Orlan spacewalks can be conducted.[citation needed]
Pirs and Poisk
The Pirs module attached to the ISS.
Poisk after arriving at the ISS on 12 November 2009.
Main articles: Pirs (ISS module) and Poisk (ISS module)
Pirs (Russian: Пирс, lit. 'pier') and Poisk (Russian: По́иск, lit. 'search') are Russian airlock modules, each having 2 identical hatches. An outward-opening hatch on the Mir space station failed after it swung open too fast after unlatching, because of a small amount of air pressure remaining in the airlock.[111] All EVA hatches on the ISS open inwards and are pressure-sealing. Pirs was used to store, service, and refurbish Russian Orlan suits and provided contingency entry for crew using the slightly bulkier American suits. The outermost docking ports on both airlocks allow docking of Soyuz and Progress spacecraft, and the automatic transfer of propellants to and from storage on the ROS.[112]
Pirs was launched on 14 September 2001, as ISS Assembly Mission 4R, on a Russian Soyuz-U rocket, using a modified Progress spacecraft, Progress M-SO1, as an upper stage. Poisk was launched on 10 November 2009[113][114] attached to a modified Progress spacecraft, called Progress M-MIM2, on a Soyuz-U rocket from Launch Pad 1 at the Baikonur Cosmodrome in Kazakhstan.
Harmony
Harmony shown connected to Columbus, Kibo, and Destiny. PMA-2 faces. The nadir and zenith locations are open.
Main article: Harmony (ISS module)
Harmony, also known as Node 2, is the "utility hub" of the ISS. It connects the laboratory modules of the United States, Europe and Japan, as well as providing electrical power and electronic data. Sleeping cabins for four of the six crew are housed here.[115]
Harmony was successfully launched into space aboard Space Shuttle flight STS-120 on October 23, 2007.[116][117] After temporarily being attached to the port side of the Unity node,[118][119] it was moved to its permanent location on the forward end of the Destiny laboratory on November 14, 2007.[120] Harmony added 2,666 cubic feet (75.5 m3) to the station's living volume, an increase of almost 20 percent, from 15,000 cu ft (420 m3) to 17,666 cu ft (500.2 m3). Its successful installation meant that from NASA's perspective, the station was "U.S. Core Complete".
Tranquility
Tranquility in 2011
Main article: Tranquility (ISS module)
Tranquility, also known as Node 3, is a module of the ISS. It contains environmental control systems, life support systems, a toilet, exercise equipment, and an observation cupola.
ESA and the Italian Space Agency had Tranquility built by Thales Alenia Space. A ceremony on November 20, 2009 transferred ownership of the module to NASA.[121] On February 8, 2010, NASA launched the module on the Space Shuttle's STS-130 mission.
Columbus
The Columbus module on the ISS
Main article: Columbus (ISS module)
Columbus is a science laboratory that is part of the ISS and is the largest single contribution to the ISS made by the European Space Agency (ESA).
Like the Harmony and Tranquility modules, the Columbus laboratory was constructed in Turin, Italy by Thales Alenia Space. The functional equipment and software of the lab was designed by EADS in Bremen, Germany. It was also integrated in Bremen before being flown to the Kennedy Space Center (KSC) in Florida in an Airbus Beluga. It was launched aboard Space Shuttle Atlantis on 7 February 2008 on flight STS-122. It is designed for ten years of operation. The module is controlled by the Columbus Control Centre, located at the German Space Operations Centre, part of the German Aerospace Center in Oberpfaffenhofen near Munich, Germany.
The European Space Agency has spent €1.4 billion (about US$2 billion) on building Columbus, including the experiments that will fly in it and the ground control infrastructure necessary to operate them.[122]
Kibō
Kibō Exposed Facility on the right
Main article: Kibo (ISS module)
The Japanese Experiment Module (JEM), nicknamed Kibo (きぼう Kibō, Hope), is a Japanese science module for the ISS developed by JAXA. It is the largest single ISS module, and is attached to the Harmony module. The first two pieces of the module were launched on Space Shuttle missions STS-123 and STS-124. The third and final components were launched on STS-127.[123]
Pressurised Module
Experiment Logistics Module
Exposed Facility
Experiment Logistics Module
Remote Manipulator System
Cupola
The Cupola's windows with shutters open.
Main article: Cupola (ISS module)
The Cupola is an ESA-built observatory module of the ISS. Its name derives from the Italian word cupola, which means "dome". Its seven windows are used to conduct experiments, dockings and observations of Earth. It was launched aboard Space Shuttle mission STS-130 on 8 February 2010 and attached to the Tranquility (Node 3) module. With the Cupola attached, ISS assembly reached 85 percent completion. The Cupola's central window has a diameter of 80 cm (31 in).[124]
Rassvet
Rassvet as seen from the Cupola module during STS-132 with a Progress in the lower right
Main article: Rassvet (ISS module)
Rassvet (Russian: Рассве́т; lit. "dawn"), also known as the Mini-Research Module 1 (MRM-1) (Russian: Малый исследовательский модуль, МИМ 1) and formerly known as the Docking Cargo Module (DCM), is a component of the ISS. The module's design is similar to the Mir Docking Module launched on STS-74 in 1995. Rassvet is primarily used for cargo storage and as a docking port for visiting spacecraft. It was flown to the ISS aboard Space Shuttle Atlantis on the STS-132 mission on May 14, 2010,[125] and was connected to the ISS on May 18.[126] The hatch connecting Rassvet with the ISS was first opened on May 20.[127] On 28 June 2010, the Soyuz TMA-19 spacecraft performed the first docking with the module.[128]
Leonardo
Leonardo Permanent Multipurpose Module
Main article: Leonardo (ISS module)
The Leonardo Permanent Multipurpose Module (PMM) is a module of the ISS. It was flown into space aboard the Space Shuttle on STS-133 on 24 February 2011 and installed on 1 March. Leonardo is primarily used for storage of spares, supplies and waste on the ISS, which was until then stored in many different places within the space station. The Leonardo PMM was a Multi-Purpose Logistics Module (MPLM) before 2011, but was modified into its current configuration. It was formerly one of three MPLM used for bringing cargo to and from the ISS with the Space Shuttle. The module was named for Italian polymath Leonardo da Vinci.
Bigelow Expandable Activity Module
Progression of expansion of BEAM
Main article: Bigelow Expandable Activity Module
The Bigelow Expandable Activity Module (BEAM) is an experimental expandable space station module developed by Bigelow Aerospace, under contract to NASA, for testing as a temporary module on the ISS from 2016 to at least 2020. It arrived at the ISS on 10 April 2016,[129] was berthed to the station on 16 April, and was expanded and pressurized on 28 May 2016.
International Docking Adapter
IDA-1 upright
Main article: International Docking Adapter
The International Docking Adapter (IDA) is a spacecraft docking system adapter developed to convert APAS-95 to the NASA Docking System (NDS)/International Docking System Standard (IDSS). An IDA is placed on each of the ISS' two open Pressurized Mating Adapters (PMAs), both of which are connected to the Harmony module.
IDA-1 was lost during the launch failure of SpaceX CRS-7 on 28 June 2015.[130][131][132]
IDA-2 was launched on SpaceX CRS-9 on 18 July 2016.[133] It was attached and connected to PMA-2 during a spacewalk on 19 August 2016.[134] First docking was achieved with the arrival of Crew Dragon Demo-1 on 3 March 2019. [135]
IDA-3 was launched on the SpaceX CRS-18 mission in July 2019.[136] IDA-3 is constructed mostly from spare parts to speed construction.[137] It was attached and connected to PMA-3 during a spacewalk on 21 August 2019. [138]
Unpressurised elements
ISS Truss Components breakdown showing Trusses and all ORUs in situ
The ISS has a large number of external components that do not require pressurisation. The largest of these is the Integrated Truss Structure (ITS), to which the station's main solar arrays and thermal radiators are mounted.[139] The ITS consists of ten separate segments forming a structure 108.5 m (356 ft) long.[3]
The station was intended to have several smaller external components, such as six robotic arms, three External Stowage Platforms (ESPs) and four ExPRESS Logistics Carriers (ELCs).[140][141] While these platforms allow experiments (including MISSE, the STP-H3 and the Robotic Refueling Mission) to be deployed and conducted in the vacuum of space by providing electricity and processing experimental data locally, their primary function is to store spare Orbital Replacement Units (ORUs). ORUs are parts that can be replaced when they fail or pass their design life, including pumps, storage tanks, antennas, and battery units. Such units are replaced either by astronauts during EVA or by robotic arms.[142] Several shuttle missions were dedicated to the delivery of ORUs, including STS-129,[143] STS-133[144] and STS-134.[145] As of January 2011, only one other mode of transportation of ORUs had been utilised – the Japanese cargo vessel HTV-2 – which delivered an FHRC and CTC-2 via its Exposed Pallet (EP).[146][needs update]
Construction of the Integrated Truss Structure over New Zealand.
There are also smaller exposure facilities mounted directly to laboratory modules; the Kibō Exposed Facility serves as an external 'porch' for the Kibō complex,[147] and a facility on the European Columbus laboratory provides power and data connections for experiments such as the European Technology Exposure Facility[148][149] and the Atomic Clock Ensemble in Space.[150] A remote sensing instrument, SAGE III-ISS, was delivered to the station in February 2017 aboard CRS-10,[151] and the NICER experiment was delivered aboard CRS-11 in June 2017.[152] The largest scientific payload externally mounted to the ISS is the Alpha Magnetic Spectrometer (AMS), a particle physics experiment launched on STS-134 in May 2011, and mounted externally on the ITS. The AMS measures cosmic rays to look for evidence of dark matter and antimatter.[153][154]
The commercial Bartolomeo External Payload Hosting Platform, manufactured by Airbus, is due to launch in May 2019 aboard a commercial ISS resupply vehicle and be attached to the European Columbus module. It will provide a further 12 external payload slots, supplementing the eight on the ExPRESS Logistics Carriers, ten on Kibō, and four on Columbus. The system is designed to be robotically serviced and will require no astronaut intervention. It is named after Christopher Columbus's younger brother.[155][156][157]
Robotic arms and cargo cranes
Commander Volkov stands on Pirs with his back to the Soyuz whilst operating the manual Strela crane holding photographer Kononenko.
Dextre, like many of the station's experiments and robotic arms, can be operated from Earth and perform tasks while the crew sleeps.
The Integrated Truss Structure serves as a base for the station's primary remote manipulator system, called the Mobile Servicing System (MSS), which is composed of three main components. Canadarm2, the largest robotic arm on the ISS, has a mass of 1,800 kilograms (4,000 lb) and is used to dock and manipulate spacecraft and modules on the USOS, hold crew members and equipment in place during EVAs and move Dextre around to perform tasks.[158] Dextre is a 1,560 kg (3,440 lb) robotic manipulator with two arms, a rotating torso and has power tools, lights and video for replacing orbital replacement units (ORUs) and performing other tasks requiring fine control.[159] The Mobile Base System (MBS) is a platform which rides on rails along the length of the station's main truss. It serves as a mobile base for Canadarm2 and Dextre, allowing the robotic arms to reach all parts of the USOS.[160] To gain access to the Russian Segment a grapple fixture was added to Zarya on STS-134, so that Canadarm2 can inchworm itself onto the ROS.[161] Also installed during STS-134 was the 15 m (50 ft) Orbiter Boom Sensor System (OBSS), which had been used to inspect heat shield tiles on Space Shuttle missions and can be used on station to increase the reach of the MSS.[161] Staff on Earth or the station can operate the MSS components via remote control, performing work outside the station without space walks.
Japan's Remote Manipulator System, which services the Kibō Exposed Facility,[162] was launched on STS-124 and is attached to the Kibō Pressurised Module.[163] The arm is similar to the Space Shuttle arm as it is permanently attached at one end and has a latching end effector for standard grapple fixtures at the other.
The European Robotic Arm, which will service the Russian Orbital Segment, will be launched alongside the Multipurpose Laboratory Module in 2017.[164] The ROS does not require spacecraft or modules to be manipulated, as all spacecraft and modules dock automatically and may be discarded the same way. Crew use the two Strela (Russian: Стрела́; lit. Arrow) cargo cranes during EVAs for moving crew and equipment around the ROS. Each Strela crane has a mass of 45 kg (99 lb).
Planned componments
Nauka
Artist's rendering of the Nauka module docked to Zvezda.
Main article: Nauka (ISS module)
Nauka (Russian: Нау́ка; lit. Science), also known as the Multipurpose Laboratory Module (MLM), (Russian: Многофункциональный лабораторный модуль, or МЛМ), is a component of the ISS which has not yet been launched into space. The MLM is funded by the Roscosmos State Corporation. In the original ISS plans, Nauka was to use the location of the Docking and Stowage Module. Later, the DSM was replaced by the Rassvet module and it was moved to Zarya's nadir port. Planners anticipate Nauka will dock at Zvezda's nadir port, replacing Pirs.[165]
The launch of Nauka, initially planned for 2007, has been repeatedly delayed for various reasons. As of September 2019, the launch to the ISS is assigned to no earlier than December 2020.[166] After this date, the warranties of some of Nauka's systems will expire.
Prichal
Mockup of the Prichal module at the Yuri Gagarin Cosmonaut Training Center
Main article: Prichal (ISS module)
Prichal, also known as Uzlovoy Module or UM (Russian: Узловой Модуль "Причал", Nodal Module Berth),[167] is a 4-tonne (8,800 lb)[168] ball-shaped module that will allow docking of two scientific and power modules during the final stage of the station assembly, and provide the Russian segment additional docking ports to receive Soyuz MS and Progress MS spacecraft. UM is due to be launched in 2022.[169] It will be integrated with a special version of the Progress cargo ship and launched by a standard Soyuz rocket, docking to the nadir port of the Nauka module. One port is equipped with an active hybrid docking port, which enables docking with the MLM module. The remaining five ports are passive hybrids, enabling docking of Soyuz and Progress vehicles, as well as heavier modules and future spacecraft with modified docking systems. The node module was intended to serve as the only permanent element of the cancelled OPSEK.[170][171]
Science Power Modules 1 and 2
Science Power Module 1 (SPM-1, also known as NEM-1) Science Power Module 2 (SPM-2, also known as NEM-2) are modules planned to arrive at the ISS in 2022.[169][172][173] It is going to dock to the Prichal module, which is planned to be attached to the Nauka module.[173] If Nauka is cancelled, then the Prichal, SPM-1, and SPM-2 would dock at the zenith port of Zvezda. SPM-1 and SPM-2 would also be required components for the OPSEK space station.[174]
Bishop Airlock Module
Main article: Bishop Airlock Module
The NanoRacks Bishop Airlock Module is a commercially-funded airlock module intended to be launched to the ISS on SpaceX CRS-21 in August 2020.[175][176] The module is being built by NanoRacks, Thales Alenia Space, and Boeing.[177] It will be used to deploy CubeSats, small satellites, and other external payloads for NASA, CASIS, and other commercial and governmental customers.[178]
Cancelled componments
The cancelled Habitation module under construction at Michoud in 1997
Several modules planned for the station were cancelled over the course of the ISS programme. Reasons include budgetary constraints, the modules becoming unnecessary, and station redesigns after the 2003 Columbia disaster. The US Centrifuge Accommodations Module would have hosted science experiments in varying levels of artificial gravity.[179] The US Habitation Module would have served as the station's living quarters. Instead, the sleep stations are now spread throughout the station.[180] The US Interim Control Module and ISS Propulsion Module would have replaced the functions of Zvezda in case of a launch failure.[181] Two Russian Research Modules were planned for scientific research.[182] They would have docked to a Russian Universal Docking Module.[183] The Russian Science Power Platform would have supplied power to the Russian Orbital Segment independent of the ITS solar arrays.
Systems
Life support
Main articles: ISS ECLSS and Chemical oxygen generator
The critical systems are the atmosphere control system, the water supply system, the food supply facilities, the sanitation and hygiene equipment, and fire detection and suppression equipment. The Russian Orbital Segment's life support systems are contained in the Zvezda service module. Some of these systems are supplemented by equipment in the USOS. The MLM Nauka laboratory has a complete set of life support systems.
Atmospheric control systems
A flowchart diagram showing the components of the ISS life support system.
The interactions between the components of the ISS Environmental Control and Life Support System (ECLSS)
The atmosphere on board the ISS is similar to the Earth's.[184] Normal air pressure on the ISS is 101.3 kPa (14.69 psi);[185] the same as at sea level on Earth. An Earth-like atmosphere offers benefits for crew comfort, and is much safer than a pure oxygen atmosphere, because of the increased risk of a fire such as that responsible for the deaths of the Apollo 1 crew.[186] Earth-like atmospheric conditions have been maintained on all Russian and Soviet spacecraft.[187]
The Elektron system aboard Zvezda and a similar system in Destiny generate oxygen aboard the station.[188] The crew has a backup option in the form of bottled oxygen and Solid Fuel Oxygen Generation (SFOG) canisters, a chemical oxygen generator system.[189] Carbon dioxide is removed from the air by the Vozdukh system in Zvezda. Other by-products of human metabolism, such as methane from the intestines and ammonia from sweat, are removed by activated charcoal filters.[189]
Part of the ROS atmosphere control system is the oxygen supply. Triple-redundancy is provided by the Elektron unit, solid fuel generators, and stored oxygen. The primary supply of oxygen is the Elektron unit which produces O
2 and H
2 by electrolysis of water and vents H2 overboard. The 1 kW (1.3 hp) system uses approximately one litre of water per crew member per day. This water is either brought from Earth or recycled from other systems. Mir was the first spacecraft to use recycled water for oxygen production. The secondary oxygen supply is provided by burning O
2-producing Vika cartridges (see also ISS ECLSS). Each 'candle' takes 5–20 minutes to decompose at 450–500 °C (842–932 °F), producing 600 litres (130 imp gal; 160 US gal) of O
2. This unit is manually operated.[190]
The US Orbital Segment has redundant supplies of oxygen, from a pressurised storage tank on the Quest airlock module delivered in 2001, supplemented ten years later by ESA-built Advanced Closed-Loop System (ACLS) in the Tranquility module (Node 3), which produces O
2 by electrolysis.[191] Hydrogen produced is combined with carbon dioxide from the cabin atmosphere and converted to water and methane.
Power and thermal control
Main articles: Electrical system of the International Space Station and External Active Thermal Control System
Russian solar arrays, backlit by sunset
One of the eight truss mounted pairs of USOS solar arrays
Double-sided solar arrays provide electrical power to the ISS. These bifacial cells collect direct sunlight on one side and light reflected off from the Earth on the other, and are more efficient and operate at a lower temperature than single-sided cells commonly used on Earth.[192]
The Russian segment of the station, like most spacecraft, uses 28 volt low voltage DC from four rotating solar arrays mounted on Zarya and Zvezda. The USOS uses 130–180 V DC from the USOS PV array, power is stabilised and distributed at 160 V DC and converted to the user-required 124 V DC. The higher distribution voltage allows smaller, lighter conductors, at the expense of crew safety. The two station segments share power with converters.
The USOS solar arrays are arranged as four wing pairs, for a total production of 75 to 90 kilowatts.[193] These arrays normally track the sun to maximise power generation. Each array is about 375 m2 (4,036 sq ft) in area and 58 m (190 ft) long. In the complete configuration, the solar arrays track the sun by rotating the alpha gimbal once per orbit; the beta gimbal follows slower changes in the angle of the sun to the orbital plane. The Night Glider mode aligns the solar arrays parallel to the ground at night to reduce the significant aerodynamic drag at the station's relatively low orbital altitude.[194]
The station originally used rechargeable nickel–hydrogen batteries (NiH
2) for continuous power during the 35 minutes of every 90-minute orbit that it is eclipsed by the Earth. The batteries are recharged on the day side of the orbit. They had a 6.5-year lifetime (over 37,000 charge/discharge cycles) and were regularly replaced over the anticipated 20-year life of the station.[195] Starting in 2016, the nickel–hydrogen batteries were replaced by lithium-ion batteries, which are expected to last until the end of the ISS program.[196]
The station's large solar panels generate a high potential voltage difference between the station and the ionosphere. This could cause arcing through insulating surfaces and sputtering of conductive surfaces as ions are accelerated by the spacecraft plasma sheath. To mitigate this, plasma contactor units (PCU)s create current paths between the station and the ambient plasma field.[197]
ISS External Active Thermal Control System (EATCS) diagram
The station's systems and experiments consume a large amount of electrical power, almost all of which is converted to heat. To keep the internal temperature within workable limits, a passive thermal control system (PTCS) is made of external surface materials, insulation such as MLI, and heat pipes. If the PTCS cannot keep up with the heat load, an External Active Thermal Control System (EATCS) maintains the temperature. The EATCS consists of an internal, non-toxic, water coolant loop used to cool and dehumidify the atmosphere, which transfers collected heat into an external liquid ammonia loop. From the heat exchangers, ammonia is pumped into external radiators that emit heat as infrared radiation, then back to the station.[198] The EATCS provides cooling for all the US pressurised modules, including Kibō and Columbus, as well as the main power distribution electronics of the S0, S1 and P1 trusses. It can reject up to 70 kW. This is much more than the 14 kW of the Early External Active Thermal Control System (EEATCS) via the Early Ammonia Servicer (EAS), which was launched on STS-105 and installed onto the P6 Truss.[199]
Communications and computers
Main articles: Tracking and Data Relay Satellite and Luch (satellite)
See also: ThinkPad § Use in space
Diagram showing communications links between the ISS and other elements.
The communications systems used by the ISS
* Luch satellite and the Space Shuttle are not currently[when?] in use
Radio communications provide telemetry and scientific data links between the station and Mission Control Centres. Radio links are also used during rendezvous and docking procedures and for audio and video communication between crew members, flight controllers and family members. As a result, the ISS is equipped with internal and external communication systems used for different purposes.[200]
The Russian Orbital Segment communicates directly with the ground via the Lira antenna mounted to Zvezda.[6][201] The Lira antenna also has the capability to use the Luch data relay satellite system.[6] This system fell into disrepair during the 1990s, and so was not used during the early years of the ISS,[6][202][203] although two new Luch satellites—Luch-5A and Luch-5B—were launched in 2011 and 2012 respectively to restore the operational capability of the system.[204] Another Russian communications system is the Voskhod-M, which enables internal telephone communications between Zvezda, Zarya, Pirs, Poisk, and the USOS and provides a VHF radio link to ground control centres via antennas on Zvezda's exterior.[205]
The US Orbital Segment (USOS) makes use of two separate radio links mounted in the Z1 truss structure: the S band (audio) and Ku band (audio, video and data) systems. These transmissions are routed via the United States Tracking and Data Relay Satellite System (TDRSS) in geostationary orbit, allowing for almost continuous real-time communications with NASA's Mission Control Center (MCC-H) in Houston.[22][6][200] Data channels for the Canadarm2, European Columbus laboratory and Japanese Kibō modules were originally also routed via the S band and Ku band systems, with the European Data Relay System and a similar Japanese system intended to eventually complement the TDRSS in this role.[22][206] Communications between modules are carried on an internal wireless network.[207]
An array of laptops in the US lab
Laptop computers surround the Canadarm2 console
UHF radio is used by astronauts and cosmonauts conducting EVAs and other spacecraft that dock to or undock from the station.[6] Automated spacecraft are fitted with their own communications equipment; the ATV uses a laser attached to the spacecraft and the Proximity Communications Equipment attached to Zvezda to accurately dock with the station.[208][209]
The ISS is equipped with about 100 IBM/Lenovo ThinkPad and HP ZBook 15 laptop computers. The laptops have run Windows 95, Windows 2000, Windows XP, Windows 7, Windows 10 and Linux operating systems.[210] Each computer is a commercial off-the-shelf purchase which is then modified for safety and operation including updates to connectors, cooling and power to accommodate the station's 28V DC power system and weightless environment. Heat generated by the laptops does not rise but stagnates around the laptop, so additional forced ventilation is required. Laptops aboard the ISS are connected to the station's wireless LAN via Wi-Fi, which connects to the ground via Ku band. This provides speeds of 10 Mbit/s download and 3 Mbit/s upload from the station, comparable to home DSL connection speeds.[211][212] Laptop hard drives occasionally fail and must be replaced.[213] Other computer hardware failures include instances in 2001, 2007 and 2017; some of these failures have required EVAs to replace computer modules in externally mounted devices.[214][215][216][217]
The operating system used for key station functions is the Debian Linux distribution.[218] The migration from Microsoft Windows was made in May 2013 for reasons of reliability, stability and flexibility.[219]
In 2017, an SG100 Cloud Computer was launched to the ISS as part of OA-7 mission.[220] It was manufactured by NCSIST and designed in collaboration with Academia Sinica, and National Central University under contract for NASA.[221]
Operations
Expeditions and private flights
See also the list of International Space Station expeditions (professional crew), space tourism (private travellers), and the list of human spaceflights to the ISS (both).
Zarya and Unity were entered for the first time on 10 December 1998.
Soyuz TM-31 being prepared to bring the first resident crew to the station in October 2000
ISS was slowly assembled over a decade of spaceflights and crews
Each permanent crew is given an expedition number. Expeditions run up to six months, from launch until undocking, an 'increment' covers the same time period, but includes cargo ships and all activities. Expeditions 1 to 6 consisted of 3 person crews, Expeditions 7 to 12 were reduced to the safe minimum of two following the destruction of the NASA Shuttle Columbia. From Expedition 13 the crew gradually increased to 6 around 2010.[222][223] With the arrival of the US Commercial Crew vehicles in the late 2010s, expedition size may be increased to seven crew members, the number ISS is designed for.[224][225]
Gennady Padalka, member of Expeditions 9, 19/20, 31/32, and 43/44, and Commander of Expedition 11, has spent more time in space than anyone else, a total of 878 days, 11 hours, and 29 minutes.[226] Peggy Whitson has spent the most time in space of any American, totalling 665 days, 22 hours, and 22 minutes during her time on Expeditions 5, 16, and 50/51/52.[227]
Travellers who pay for their own passage into space are termed spaceflight participants by Roscosmos and NASA, and are sometimes referred to as space tourists, a term they generally dislike.[note 1] All seven were transported to the ISS on Russian Soyuz spacecraft. When professional crews change over in numbers not divisible by the three seats in a Soyuz, and a short-stay crewmember is not sent, the spare seat is sold by MirCorp through Space Adventures. When the space shuttle retired in 2011, and the station's crew size was reduced to 6, space tourism was halted, as the partners relied on Russian transport seats for access to the station. Soyuz flight schedules increase after 2013, allowing 5 Soyuz flights (15 seats) with only two expeditions (12 seats) required.[233] The remaining seats are sold for around US$40 million to members of the public who can pass a medical exam. ESA and NASA criticised private spaceflight at the beginning of the ISS, and NASA initially resisted training Dennis Tito, the first person to pay for his own passage to the ISS.[note 2]
Anousheh Ansari became the first Iranian in space and the first self-funded woman to fly to the station. Officials reported that her education and experience make her much more than a tourist, and her performance in training had been "excellent."[234] Ansari herself dismisses the idea that she is a tourist. She did Russian and European studies involving medicine and microbiology during her 10-day stay. The documentary Space Tourists follows her journey to the station, where she fulfilled "an age-old dream of man: to leave our planet as a "normal person" and travel into outer space."[235]
In 2008, spaceflight participant Richard Garriott placed a geocache aboard the ISS during his flight.[236] This is currently the only non-terrestrial geocache in existence.[237] At the same time, the Immortality Drive, an electronic record of eight digitised human DNA sequences, was placed aboard the ISS.[238]
Orbit
Graph showing the changing altitude of the ISS from November 1998 until November 2018
Animation of ISS orbit from 14 September 2018 to 14 November 2018. Earth is not shown.
The ISS is maintained in a nearly circular orbit with a minimum mean altitude of 330 km (205 mi) and a maximum of 410 km (255 mi), in the centre of the thermosphere, at an inclination of 51.6 degrees to Earth's equator. This orbit was selected because it is the lowest inclination that can be directly reached by Russian Soyuz and Progress spacecraft launched from Baikonur Cosmodrome at 46° N latitude without overflying China or dropping spent rocket stages in inhabited areas.[239][240] It travels at an average speed of 27,724 kilometres per hour (17,227 mph), and completes 15.54 orbits per day (93 minutes per orbit).[2][14] The station's altitude was allowed to fall around the time of each NASA shuttle flight to permit heavier loads to be transferred to the station. After the retirement of the shuttle, the nominal orbit of the space station was raised in altitude.[241][242] Other, more frequent supply ships do not require this adjustment as they are substantially higher performance vehicles.[28][243]
Orbital boosting can be performed by the station's two main engines on the Zvezda service module, or Russian or European spacecraft docked to Zvezda's aft port. The ATV is constructed with the possibility of adding a second docking port to its aft end, allowing other craft to dock and boost the station. It takes approximately two orbits (three hours) for the boost to a higher altitude to be completed.[243] Maintaining ISS altitude uses about 7.5 tonnes of chemical fuel per annum[244] at an annual cost of about $210 million.[245]
Orbits of the ISS, shown in April 2013
The Russian Orbital Segment contains the Data Management System, which handles Guidance, Navigation and Control (ROS GNC) for the entire station.[246] Initially, Zarya, the first module of the station, controlled the station until a short time after the Russian service module Zvezda docked and was transferred control. Zvezda contains the ESA built DMS-R Data Management System.[247] Using two fault-tolerant computers (FTC), Zvezda computes the station's position and orbital trajectory using redundant Earth horizon sensors, Solar
Mayara Magri in woman with water, performed as part of Beauty Mixed Programme.
www.roh.org.uk/tickets-and-events/beauty-mixed-programme-...
Biennalist
Biennalist is an Art Format commenting on active biennials and managed cultural events through artworks.Biennalist takes the thematics of the biennales and similar events like festivals and conferences seriously, questioning the established structures of the staged art events in order to contribute to the debate, which they wish to generate.
About artist Thierry Geoffroy/Colonel:
en.wikipedia.org/wiki/Thierry_Geoffroy
en.wikipedia.org/wiki/Emergency_Room_(art)
www.emergencyrooms.org/formats.html
Biennalist :
Biennalist is an Art Format commenting on active biennials and managed cultural events through artworks.Biennalist takes the thematics of the biennales and similar events like festivals and conferences seriously, questioning the established structures of the staged art events in order to contribute to the debate, which they wish to generate.
-------------------------------------------
links about Biennalist :
Thierry Geoffroy/Colonel:
en.wikipedia.org/wiki/Thierry_Geoffroy
en.wikipedia.org/wiki/Emergency_Room_(art)
www.emergencyrooms.org/formats.html
—--Biennale from wikipedia —--
The Venice International Film Festival is part of the Venice Biennale. The famous Golden Lion is awarded to the best film screening at the competition.
Biennale (Italian: [bi.enˈnaːle]), Italian for "biennial" or "every other year", is any event that happens every two years. It is most commonly used within the art world to describe large-scale international contemporary art exhibitions. As such the term was popularised by Venice Biennale, which was first held in 1895. Since the 1990s, the terms "biennale" and "biennial" have been interchangeably used in a more generic way - to signify a large-scale international survey show of contemporary art that recurs at regular intervals but not necessarily biannual (such as triennials, Documenta, Skulptur Projekte Münster).[1] The phrase has also been used for other artistic events, such as the "Biennale de Paris", "Kochi-Muziris Biennale", Berlinale (for the Berlin International Film Festival) and Viennale (for Vienna's international film festival).
Characteristics[edit]
According to author Federica Martini, what is at stake in contemporary biennales is the diplomatic/international relations potential as well as urban regeneration plans. Besides being mainly focused on the present (the “here and now” where the cultural event takes place and their effect of "spectacularisation of the everyday"), because of their site-specificity cultural events may refer back to,[who?] produce or frame the history of the site and communities' collective memory.[2]
The Great Exhibition in The Crystal Palace in Hyde Park, London, in 1851, the first attempt to condense the representation of the world within a unitary exhibition space.
A strong and influent symbol of biennales and of large-scale international exhibitions in general is the Crystal Palace, the gigantic and futuristic London architecture that hosted the Great Exhibition in 1851. According to philosopher Peter Sloterdijk,[3][page needed] the Crystal Palace is the first attempt to condense the representation of the world in a unitary exhibition space, where the main exhibit is society itself in an a-historical, spectacular condition. The Crystal Palace main motives were the affirmation of British economic and national leadership and the creation of moments of spectacle. In this respect, 19th century World fairs provided a visual crystallization of colonial culture and were, at the same time, forerunners of contemporary theme parks.
The Venice Biennale as an archetype[edit]
The structure of the Venice Biennale in 2005 with an international exhibition and the national pavilions.
The Venice Biennale, a periodical large-scale cultural event founded in 1895, served as an archetype of the biennales. Meant to become a World Fair focused on contemporary art, the Venice Biennale used as a pretext the wedding anniversary of the Italian king and followed up to several national exhibitions organised after Italy unification in 1861. The Biennale immediately put forth issues of city marketing, cultural tourism and urban regeneration, as it was meant to reposition Venice on the international cultural map after the crisis due to the end of the Grand Tour model and the weakening of the Venetian school of painting. Furthermore, the Gardens where the Biennale takes place were an abandoned city area that needed to be re-functionalised. In cultural terms, the Biennale was meant to provide on a biennial basis a platform for discussing contemporary art practices that were not represented in fine arts museums at the time. The early Biennale model already included some key points that are still constitutive of large-scale international art exhibitions today: a mix of city marketing, internationalism, gentrification issues and destination culture, and the spectacular, large scale of the event.
Biennials after the 1990s[edit]
The situation of biennials has changed in the contemporary context: while at its origin in 1895 Venice was a unique cultural event, but since the 1990s hundreds of biennials have been organized across the globe. Given the ephemeral and irregular nature of some biennials, there is little consensus on the exact number of biennials in existence at any given time.[citation needed] Furthermore, while Venice was a unique agent in the presentation of contemporary art, since the 1960s several museums devoted to contemporary art are exhibiting the contemporary scene on a regular basis. Another point of difference concerns 19th century internationalism in the arts, that was brought into question by post-colonial debates and criticism of the contemporary art “ethnic marketing”, and also challenged the Venetian and World Fair’s national representation system. As a consequence of this, Eurocentric tendency to implode the whole word in an exhibition space, which characterises both the Crystal Palace and the Venice Biennale, is affected by the expansion of the artistic geographical map to scenes traditionally considered as marginal. The birth of the Havana Biennial in 1984 is widely considered an important counterpoint to the Venetian model for its prioritization of artists working in the Global South and curatorial rejection of the national pavilion model.
International biennales[edit]
In the term's most commonly used context of major recurrent art exhibitions:
Adelaide Biennial of Australian Art, South Australia
Asian Art Biennale, in Taichung, Taiwan (National Taiwan Museum of Fine Arts)
Athens Biennale, in Athens, Greece
Bienal de Arte Paiz, in Guatemala City, Guatemala[4]
Arts in Marrakech (AiM) International Biennale (Arts in Marrakech Festival)
Bamako Encounters, a biennale of photography in Mali
Bat-Yam International Biennale of Landscape Urbanism
Beijing Biennale
Berlin Biennale (contemporary art biennale, to be distinguished from Berlinale, which is a film festival)
Bergen Assembly (triennial for contemporary art in Bergen, Norway)www.bergenassembly.no
Bi-City Biennale of Urbanism\Architecture, in Shenzhen and Hong Kong, China
Bienal de Arte de Ponce in Ponce, Puerto Rico
Biënnale van België, Biennial of Belgium, Belgium
BiennaleOnline Online biennial exhibition of contemporary art from the most promising emerging artists.
Biennial of Hawaii Artists
Biennale de la Biche, the smallest biennale in the world held at deserted island near Guadeloupe, French overseas region[5][6]
Biwako Biennale [ja], in Shiga, Japan
La Biennale de Montreal
Biennale of Luanda : Pan-African Forum for the Culture of Peace,[7] Angola
Boom Festival, international music and culture festival in Idanha-a-Nova, Portugal
Bucharest Biennale in Bucharest, Romania
Bushwick Biennial, in Bushwick, Brooklyn, New York
Canakkale Biennial, in Canakkale, Turkey
Cerveira International Art Biennial, Vila Nova de Cerveira, Portugal [8]
Changwon Sculpture Biennale in Changwon, South Korea
Dakar Biennale, also called Dak'Art, biennale in Dakar, Senegal
Documenta, contemporary art exhibition held every five years in Kassel, Germany
Estuaire (biennale), biennale in Nantes and Saint-Nazaire, France
EVA International, biennial in Limerick, Republic of Ireland
Göteborg International Biennial for Contemporary Art, in Gothenburg, Sweden[9]
Greater Taipei Contemporary Art Biennial, in Taipei, Taiwan
Gwangju Biennale, Asia's first and most prestigious contemporary art biennale
Havana biennial, in Havana, Cuba
Helsinki Biennial, in Helsinki, Finland
Herzliya Biennial For Contemporary Art, in Herzliya, Israel
Incheon Women Artists' Biennale, in Incheon, South Korea
Iowa Biennial, in Iowa, USA
Istanbul Biennial, in Istanbul, Turkey
International Roaming Biennial of Tehran, in Tehran and Istanbul
Jakarta Biennale, in Jakarta, Indonesia
Jerusalem Biennale, in Jerusalem, Israel
Jogja Biennale, in Yogyakarta, Indonesia
Karachi Biennale, in Karachi, Pakistan
Keelung Harbor Biennale, in Keelung, Taiwan
Kochi-Muziris Biennale, largest art exhibition in India, in Kochi, Kerala, India
Kortrijk Design Biennale Interieur, in Kortrijk, Belgium
Kobe Biennale, in Japan
Kuandu Biennale, in Taipei, Taiwan
Lagos Biennial, in Lagos, Nigeria[10]
Light Art Biennale Austria, in Austria
Liverpool Biennial, in Liverpool, UK
Lofoten International Art Festival [no] (LIAF), on the Lofoten archipelago, Norway[11]
Manifesta, European Biennale of contemporary art in different European cities
Mediations Biennale, in Poznań, Poland
Melbourne International Biennial 1999
Mediterranean Biennale in Sakhnin 2013
MOMENTA Biennale de l'image [fr] (formerly known as Le Mois de la Photo à Montréal), in Montreal, Canada
MOMENTUM [no], in Moss, Norway[12]
Moscow Biennale, in Moscow, Russia
Munich Biennale, new opera and music-theatre in even-numbered years
Mykonos Biennale
Nakanojo Biennale[13]
NGV Triennial, contemporary art exhibition held every three years at the National Gallery of Victoria, Melbourne, Australia
October Salon – Belgrade Biennale [sr], organised by the Cultural Center of Belgrade [sr], in Belgrade, Serbia[14]
OSTEN Biennial of Drawing Skopje, North Macedonia[15]
Biennale de Paris
Riga International Biennial of Contemporary Art (RIBOCA), in Riga, Latvia[16]
São Paulo Art Biennial, in São Paulo, Brazil
SCAPE Public Art Christchurch Biennial in Christchurch, New Zealand[17]
Prospect New Orleans
Seoul Biennale of Architecture and Urbanism
Sequences, in Reykjavík, Iceland[18]
Shanghai Biennale
Sharjah Biennale, in Sharjah, UAE
Singapore Biennale, held in various locations across the city-state island of Singapore
Screen City Biennial, in Stavanger, Norway
Biennale of Sydney
Taipei Biennale, in Taipei, Taiwan
Taiwan Arts Biennale, in Taichung, Taiwan (National Taiwan Museum of Fine Arts)
Taiwan Film Biennale, in Hammer Museum, Los Angeles, U.S.A.
Thessaloniki Biennale of Contemporary Art [el], in Thessaloniki, Greece[19]
Dream city, produced by ART Rue Association in Tunisia
Vancouver Biennale
Visayas Islands Visual Arts Exhibition and Conference (VIVA ExCon) in the Philippines [20]
Venice Biennale, in Venice, Italy, which includes:
Venice Biennale of Contemporary Art
Venice Biennale of Architecture
Venice Film Festival
Vladivostok biennale of Visual Arts, in Vladivostok, Russia
Whitney Biennial, hosted by the Whitney Museum of American Art, in New York City, NY, USA
Web Biennial, produced with teams from Athens, Berlin and Istanbul.
West Africa Architecture Biennale,[21] Virtual in Lagos, Nigeria.
WRO Biennale, in Wrocław, Poland[22]
Music Biennale Zagreb
[SHIFT:ibpcpa] The International Biennale of Performance, Collaborative and Participatory Arts, Nomadic, International, Scotland, UK.
—---Venice Biennale from wikipedia —
The Venice Biennale (/ˌbiːɛˈnɑːleɪ, -li/; Italian: La Biennale di Venezia) is an international cultural exhibition hosted annually in Venice, Italy by the Biennale Foundation.[2][3][4] The biennale has been organised every year since 1895, which makes it the oldest of its kind. The main exhibition held in Castello, in the halls of the Arsenale and Biennale Gardens, alternates between art and architecture (hence the name biennale; biennial).[5][6][7] The other events hosted by the Foundation—spanning theatre, music, and dance—are held annually in various parts of Venice, whereas the Venice Film Festival takes place at the Lido.[8]
Organization[edit]
Art Biennale
Art Biennale
International Art Exhibition
1895
Even-numbered years (since 2022)
Venice Biennale of Architecture
International Architecture Exhibition
1980
Odd-numbered years (since 2021)
Biennale Musica
International Festival of Contemporary Music
1930
Annually (Sep/Oct)
Biennale Teatro
International Theatre Festival
1934
Annually (Jul/Aug)
Venice Film Festival
Venice International Film Festival
1932
Annually (Aug/Sep)
Venice Dance Biennale
International Festival of Contemporary Dance
1999
Annually (June; biennially 2010–16)
International Kids' Carnival
2009
Annually (during Carnevale)
History
1895–1947
On April 19, 1893, the Venetian City Council passed a resolution to set up an biennial exhibition of Italian Art ("Esposizione biennale artistica nazionale") to celebrate the silver anniversary of King Umberto I and Margherita of Savoy.[11]
A year later, the council decreed "to adopt a 'by invitation' system; to reserve a section of the Exhibition for foreign artists too; to admit works by uninvited Italian artists, as selected by a jury."[12]
The first Biennale, "I Esposizione Internazionale d'Arte della Città di Venezia (1st International Art Exhibition of the City of Venice)" (although originally scheduled for April 22, 1894) was opened on April 30, 1895, by the Italian King and Queen, Umberto I and Margherita di Savoia. The first exhibition was seen by 224,000 visitors.
The event became increasingly international in the first decades of the 20th century: from 1907 on, several countries installed national pavilions at the exhibition, with the first being from Belgium. In 1910 the first internationally well-known artists were displayed: a room dedicated to Gustav Klimt, a one-man show for Renoir, a retrospective of Courbet. A work by Picasso "Family of Saltimbanques" was removed from the Spanish salon in the central Palazzo because it was feared that its novelty might shock the public. By 1914 seven pavilions had been established: Belgium (1907), Hungary (1909), Germany (1909), Great Britain (1909), France (1912), and Russia (1914).
During World War I, the 1916 and 1918 events were cancelled.[13] In 1920 the post of mayor of Venice and president of the Biennale was split. The new secretary general, Vittorio Pica brought about the first presence of avant-garde art, notably Impressionists and Post-Impressionists.
1922 saw an exhibition of sculpture by African artists. Between the two World Wars, many important modern artists had their work exhibited there. In 1928 the Istituto Storico d'Arte Contemporanea (Historical Institute of Contemporary Art) opened, which was the first nucleus of archival collections of the Biennale. In 1930 its name was changed into Historical Archive of Contemporary Art.
In 1930, the Biennale was transformed into an Ente Autonomo (Autonomous Board) by Royal Decree with law no. 33 of 13-1-1930. Subsequently, the control of the Biennale passed from the Venice city council to the national Fascist government under Benito Mussolini. This brought on a restructuring, an associated financial boost, as well as a new president, Count Giuseppe Volpi di Misurata. Three entirely new events were established, including the Biennale Musica in 1930, also referred to as International Festival of Contemporary Music; the Venice Film Festival in 1932, which they claim as the first film festival in history,[14] also referred to as Venice International Film Festival; and the Biennale Theatro in 1934, also referred to as International Theatre Festival.
In 1933 the Biennale organized an exhibition of Italian art abroad. From 1938, Grand Prizes were awarded in the art exhibition section.
During World War II, the activities of the Biennale were interrupted: 1942 saw the last edition of the events. The Film Festival restarted in 1946, the Music and Theatre festivals were resumed in 1947, and the Art Exhibition in 1948.[15]
1948–1973[edit]
The Art Biennale was resumed in 1948 with a major exhibition of a recapitulatory nature. The Secretary General, art historian Rodolfo Pallucchini, started with the Impressionists and many protagonists of contemporary art including Chagall, Klee, Braque, Delvaux, Ensor, and Magritte, as well as a retrospective of Picasso's work. Peggy Guggenheim was invited to exhibit her collection, later to be permanently housed at Ca' Venier dei Leoni.
1949 saw the beginning of renewed attention to avant-garde movements in European—and later worldwide—movements in contemporary art. Abstract expressionism was introduced in the 1950s, and the Biennale is credited with importing Pop Art into the canon of art history by awarding the top prize to Robert Rauschenberg in 1964.[16] From 1948 to 1972, Italian architect Carlo Scarpa did a series of remarkable interventions in the Biennale's exhibition spaces.
In 1954 the island San Giorgio Maggiore provided the venue for the first Japanese Noh theatre shows in Europe. 1956 saw the selection of films following an artistic selection and no longer based upon the designation of the participating country. The 1957 Golden Lion went to Satyajit Ray's Aparajito which introduced Indian cinema to the West.
1962 included Arte Informale at the Art Exhibition with Jean Fautrier, Hans Hartung, Emilio Vedova, and Pietro Consagra. The 1964 Art Exhibition introduced continental Europe to Pop Art (The Independent Group had been founded in Britain in 1952). The American Robert Rauschenberg was the first American artist to win the Gran Premio, and the youngest to date.
The student protests of 1968 also marked a crisis for the Biennale. Student protests hindered the opening of the Biennale. A resulting period of institutional changes opened and ending with a new Statute in 1973. In 1969, following the protests, the Grand Prizes were abandoned. These resumed in 1980 for the Mostra del Cinema and in 1986 for the Art Exhibition.[17]
In 1972, for the first time, a theme was adopted by the Biennale, called "Opera o comportamento" ("Work or Behaviour").
Starting from 1973 the Music Festival was no longer held annually. During the year in which the Mostra del Cinema was not held, there was a series of "Giornate del cinema italiano" (Days of Italian Cinema) promoted by sectorial bodies in campo Santa Margherita, in Venice.[18]
1974–1998[edit]
1974 saw the start of the four-year presidency of Carlo Ripa di Meana. The International Art Exhibition was not held (until it was resumed in 1976). Theatre and cinema events were held in October 1974 and 1975 under the title Libertà per il Cile (Freedom for Chile)—a major cultural protest against the dictatorship of Augusto Pinochet.
On 15 November 1977, the so-called Dissident Biennale (in reference to the dissident movement in the USSR) opened. Because of the ensuing controversies within the Italian left wing parties, president Ripa di Meana resigned at the end of the year.[19]
In 1979 the new presidency of Giuseppe Galasso (1979-1982) began. The principle was laid down whereby each of the artistic sectors was to have a permanent director to organise its activity.
In 1980, the Architecture section of the Biennale was set up. The director, Paolo Portoghesi, opened the Corderie dell'Arsenale to the public for the first time. At the Mostra del Cinema, the awards were brought back into being (between 1969 and 1979, the editions were non-competitive). In 1980, Achille Bonito Oliva and Harald Szeemann introduced "Aperto", a section of the exhibition designed to explore emerging art. Italian art historian Giovanni Carandente directed the 1988 and 1990 editions. A three-year gap was left afterwards to make sure that the 1995 edition would coincide with the 100th anniversary of the Biennale.[13]
The 1993 edition was directed by Achille Bonito Oliva. In 1995, Jean Clair was appointed to be the Biennale's first non-Italian director of visual arts[20] while Germano Celant served as director in 1997.
For the Centenary in 1995, the Biennale promoted events in every sector of its activity: the 34th Festival del Teatro, the 46th art exhibition, the 46th Festival di Musica, the 52nd Mostra del Cinema.[21]
1999–present[edit]
In 1999 and 2001, Harald Szeemann directed two editions in a row (48th & 49th) bringing in a larger representation of artists from Asia and Eastern Europe and more young artists than usual and expanded the show into several newly restored spaces of the Arsenale.
In 1999 a new sector was created for live shows: DMT (Dance Music Theatre).
The 50th edition, 2003, directed by Francesco Bonami, had a record number of seven co-curators involved, including Hans Ulrich Obrist, Catherine David, Igor Zabel, Hou Hanru and Massimiliano Gioni.
The 51st edition of the Biennale opened in June 2005, curated, for the first time by two women, Maria de Corral and Rosa Martinez. De Corral organized "The Experience of Art" which included 41 artists, from past masters to younger figures. Rosa Martinez took over the Arsenale with "Always a Little Further." Drawing on "the myth of the romantic traveler" her exhibition involved 49 artists, ranging from the elegant to the profane.
In 2007, Robert Storr became the first director from the United States to curate the Biennale (the 52nd), with a show entitled Think with the Senses – Feel with the Mind. Art in the Present Tense.
Swedish curator Daniel Birnbaum was artistic director of the 2009 edition entitled "Fare Mondi // Making Worlds".
The 2011 edition was curated by Swiss curator Bice Curiger entitled "ILLUMInazioni – ILLUMInations".
The Biennale in 2013 was curated by the Italian Massimiliano Gioni. His title and theme, Il Palazzo Enciclopedico / The Encyclopedic Palace, was adopted from an architectural model by the self-taught Italian-American artist Marino Auriti. Auriti's work, The Encyclopedic Palace of the World was lent by the American Folk Art Museum and exhibited in the first room of the Arsenale for the duration of the biennale. For Gioni, Auriti's work, "meant to house all worldly knowledge, bringing together the greatest discoveries of the human race, from the wheel to the satellite," provided an analogous figure for the "biennale model itself...based on the impossible desire to concentrate the infinite worlds of contemporary art in a single place: a task that now seems as dizzyingly absurd as Auriti's dream."[22]
Curator Okwui Enwezor was responsible for the 2015 edition.[23] He was the first African-born curator of the biennial. As a catalyst for imagining different ways of imagining multiple desires and futures Enwezor commissioned special projects and programs throughout the Biennale in the Giardini. This included a Creative Time Summit, e-flux journal's SUPERCOMMUNITY, Gulf Labor Coalition, The Invisible Borders Trans-African Project and Abounaddara.[24][25]
The 2017 Biennale, titled Viva Arte Viva, was directed by French curator Christine Macel who called it an "exhibition inspired by humanism".[26] German artist Franz Erhard Walter won the Golden Lion for best artist, while Carolee Schneemann was awarded a posthumous Golden Lion for Lifetime Achievement.[27]
The 2019 Biennale, titled May You Live In Interesting Times, was directed by American-born curator Ralph Rugoff.[28]
The 2022 edition was curated by Italian curator Cecilia Alemani entitled "The Milk of Dreams" after a book by British-born Mexican surrealist painter Leonora Carrington.[29]
The Biennale has an attendance today of over 500,000 visitors.[30][31][32]
Role in the art market[edit]
When the Venice Biennale was founded in 1895, one of its main goals was to establish a new market for contemporary art. Between 1942 and 1968 a sales office assisted artists in finding clients and selling their work,[33] a service for which it charged 10% commission. Sales remained an intrinsic part of the biennale until 1968, when a sales ban was enacted. An important practical reason why the focus on non-commodities has failed to decouple Venice from the market is that the biennale itself lacks the funds to produce, ship and install these large-scale works. Therefore, the financial involvement of dealers is widely regarded as indispensable;[16] as they regularly front the funding for production of ambitious projects.[34] Furthermore, every other year the Venice Biennale coincides with nearby Art Basel, the world's prime commercial fair for modern and contemporary art. Numerous galleries with artists on show in Venice usually bring work by the same artists to Basel.[35]
Central Pavilion and Arsenale[edit]
The formal Biennale is based at a park, the Giardini. The Giardini includes a large exhibition hall that houses a themed exhibition curated by the Biennale's director.
Initiated in 1980, the Aperto began as a fringe event for younger artists and artists of a national origin not represented by the permanent national pavilions. This is usually staged in the Arsenale and has become part of the formal biennale programme. In 1995 there was no Aperto so a number of participating countries hired venues to show exhibitions of emerging artists. From 1999, both the international exhibition and the Aperto were held as one exhibition, held both at the Central Pavilion and the Arsenale. Also in 1999, a $1 million renovation transformed the Arsenale area into a cluster of renovated shipyards, sheds and warehouses, more than doubling the Arsenale's exhibition space of previous years.[36]
A special edition of the 54th Biennale was held at Padiglione Italia of Torino Esposizioni – Sala Nervi (December 2011 – February 2012) for the 150th Anniversary of Italian Unification. The event was directed by Vittorio Sgarbi
On March 24, at a WFP warehouse in Goma, U.S. Ambassador James Swan (second left) handed a symbol of U.S. food assistance to WFP Country Representative Pablo Recalde. Vice Governor Feller Lutahichirwa accepted it on behalf of the people of North Kivu.
Photo by Kaukab Jhumra Smith/USAID
GOMA, NORTH KIVU -- On March 24, 2016, the United States Agency for International Development (USAID) announced an award of $42.75 million to the World Food Programme (WFP) in the Democratic Republic of the Congo (DRC), contributing to food assistance for more than 1.6 million vulnerable people in conflict-affected parts of the country.
Half this contribution is earmarked for local and regional food procurement, which will support local economies and stimulate regional agricultural markets. The other half will be used to procure food commodities in the U.S. or other international markets at favorable prices.
USAID’s contribution will allow WFP to continue its relief and recovery operations in the eastern and southern provinces of the DRC, including the most hard-to-reach areas affected by conflict and mass internal displacements.
USAID is the most important financial partner of WFP, a United Nations agency engaged in the fight against hunger in the DRC. Between 2011 and 2015, USAID provided approximately $221 million to WFP in the DRC, contributing to WFP’s emergency assistance to more than 14 million vulnerable people in that period.
Madrasa Teachers, Students and Indian Imams Training Programme was conducted in Pune in association with the MCES, Azam Campus in February 2010. Follow us on www.twitter.com/ukinindia.
Preparing young Queenslanders for life in the 1990s, we saw personal computers make their way into schools during the 80s with a strong focus on health, regional education and the arts by Queensland Education.
The photographic unit at the Premier’s Department, Office of State Affairs, captured a snapshot of various events, programmes and initiatives for school children throughout Queensland. This collection contains several arts, music and drama as well as students participating in computer usage.
In the early 1980s, several different computer manufacturers were vying for a foothold in the education market, Apple, Tandy, Atari, Sinclair, Amstrad, Microbee and many others. By 1985 Apple Macintosh was considered a standard system (alongside several others) for all states except Western Australia which adopted the BBC Model B and Microbee computer systems as a standard.
These photos are part are the photographic records held at Queensland State Archives, www.archivessearch.qld.gov.au/series/S189
1985
The discussion paper, Education 2000: Issues and options for the future of Education in Queensland was released.
The use of technology to enhance distance education, work in schools and educational administration was supported.
Approval was given for schools to alter the placement of the three pupil free days.
The Department of Education developed a policy on the education of gifted children.
The Special Education Resource Centres were formed as state-wide services, as part of the Division of Special Education.
Early special education officially commenced.
1986
The age of first attendance at primary school increased. Children had to turn five years by 31 January to be eligible for enrolment in Year 1.
There was an expansion of the curriculum in secondary schools and TAFE colleges evident in the further development of co-operative secondary-TAFE programs.
The Advisory Committee which reviewed submissions made in response to Education 2000 reported to the Minister.
The distance education trial began through the Mt Isa School of the Air.
A Preschool to Year 10 (P–10) Syllabus Framework was developed.
Endeavour Foundation schools transferred to Department of Education.
Policy Statement 15 Integration: Mainstreaming of Students with Special Needs introduced.
1987
Children had to turn 5 years by 31 December to be eligible for enrolment in Year 1 in the following year.
The Department of Education launched a series of documents entitled Meeting the Challenge which highlighted a corporate style of management.
The Department reshaped its central administration by strengthening the role of the Policy Committee, appointing a Chief Inspector and adopting comprehensive strategic planning processes.
In regions, initiatives were built on the commitment to decentralisation, while further devolution of responsibility occurred in the operational management of educational programs.
Two new education regions were formed (South Coast and Sunshine Coast regional offices).
The P–10 Curriculum Framework was developed and curriculum documents revised.
The Roma Middle School opened and catered for students in Years 4–10.
A post-compulsory college, the Alexandra Hills Senior College opened.
Two new centres of distance education opened at Longreach and Charters Towers.
1988
The Inspectorate was regionalised.
There was continued development of an integrated P–10 curriculum.
The senior secondary curriculum was broadened to cater for all learners.
Cooperative programs between secondary schools and TAFE colleges were conducted.
The use of computers and information technology in schools was given a high priority.
The Special Education Resource and Development Centres were formed as a consequence of the reorganisation of the Division of Special Education.
Individual education plans for students with disabilities were introduced as part of the new policy Policy Statement 16: Policy and Practice for Special Education Services.
The report National Overview of Educational Services for Isolated Severely Handicapped Children resulted from a Project of National Significance undertaken as a joint project of the Commonwealth Department of Employment Education and Training and the Department of Education Division of Special Services.
The Queensland School for the Deaf closes, as a consequence of decentralisation of services to students with hearing impairments during the 1980's. Programs for students with vision impairment were also decentralised during this period.
1989
A new Education Act 1989 was enacted.
The Department of Education's first strategic plan was adopted.
Decisions about school budgets were devolved to the school level.
There was an amalgamation of correspondence schools which became the School of Distance Education — Brisbane Centre P–12.
The first high school built to a new design opened at Bribie Island.
New prototype buildings for preschool, primary and special education units were assessed.
1989–1990
A comprehensive internal review of the Department of Education commenced through the consultation process, Education Have Your Say.
Professor Nancy Viviani reviewed Tertiary Entrance and produced the report, A Review of Tertiary Entrance in Queensland.
The Offices of Higher Education and Non-State Schooling were established.
The Department developed The Corporate Vision for Senior Schooling in Queensland to accommodate the diverse needs of students in Years 11 and 12.
The first entire primary school based on the new building model opened to students.
1990–1991
The report, Focus on Schools was released. A major restructure of the Department of Education followed.
The Public Sector Management Commission (PSMC) reviewed the Department of Education including its role, operations, responsibilities and management.
Greater responsibilities were devolved to 11 regions for resource, financial administration and human resource management.
A new English Language Arts Syllabus was introduced.
Priority was given to expanding languages other than English (LOTE).
The Viviani Report recommended the establishment of the Tertiary Entrance Procedures Authority (TEPA).
Consultants were engaged to assist in the development of an Equal Employment Opportunity (EEO) management plan.
The Equity Directorate (Workforce and Studies) was established. A social justice strategy was developed.
The PSMC developed guidelines for recruitment and selection based on merit and equity principles.
The inspectorate ended.
The report Focus on Schools recommended that a strategy for managing the integration policy in Queensland schools be developed as a matter of urgency, and that a state-wide support centre for students with low incidence disabilities be established. A restructure of the Department of Education followed.
Occupational therapists and physiotherapists were employed by the Department of Education to work in schools with students with disabilities. (These services were transferred from the Department of Families).
Policy Statement — Management of Support Teaching: Learning Difficulties (P–7) was introduced.
education.qld.gov.au/about-us/history/chronology-of-educa...
Increasing floods in between dry periods represent ideal conditions for spreading diseases such as cholera. In Nouakchott, the capital of Mauritania located in the desert, precipitations - when they occur - are always accompanied by a cholera epidemic, especially in poor areas where waste matter is not managed. Cholera had almost disappeared globally by the mid 1950s, but it reappeared and spread throughout the world during the last few decades. The World Health Organization (WHO) fears that a rapidly changing climate, combined with declining socio-economic conditions in the poorest part of the population, will contribute to an increasing spread of the disease.
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This photo has been graciously provided to be used in the GRID-Arendal resources library by: Philippe Rekacewicz, February 2006
Just in time for the Ashes 4th Test at Chester-le-Street are these kindly donated cricket programmes; New Zealand 1949 cricket tour handbook and souvenir programme, complete with filled out score card, and a South African 1951 tour fixture, facts and averages handbook.
Front cover from the theatre programme for a production of "The Dancing Years" at the Hippodrome Theatre, Keighley, staged by Keighley Amateur Operatic and Dramatic Society in November 1953.
Keighley Amateur Operatic and Dramatic Society's production of "The Dancing Years" played at the Hippodrome Theatre in Keighley for six nights (and a Saturday matinee) from Monday 9th November 1953. The musical was devised, written and composed by Ivor Novello. The audience were probably familiar with the musical as the film version had only come out in the UK in 1950. The KAODS production was produced and directed by Gene Anderton, with musical director R. Lewis Scargill.
The story is set in early twentieth century Vienna and is told in four episodes between 1911 and 1938. Young composer Rudi Kleber (played by Frederic W. Pye) sells his first composition to travelling prima donna Maria Zeigler (Olive Kitchen), who then persuades him to write more songs for her. Rudi falls for Maria who is already committed to benefactor Prince Charles Metterling (Arthur Day). As usual, misunderstandings abound, but for once, even over the 27 years, things are not resolved happily-ever-after, and the show ends with the shadow of the imminent World War II encroaching upon it.
The show also starred Alan Petty, Elsie Greenwell, Joan M. Corlas, Joyce Reed, Maureen F. Dacre, Sybil J. Calvert, Margaret Holmes, Joan Greenwood, Florence M. Bottomley, Dorothy Smith, Alice Chester, Frank Hopkinson, Richard Reed, Alice Hanson, Norman J. K. Langthorn, Betty M. Hird, Dennis Crocker, Reuben P. Drake, Norman Moulding and Glennis Copley. The part of Prince Charles Metterling was due to have been played by Dennis P. Smith, but veteran Amateurs performer Arthur Day had to step in with three days' notice when Smith fell ill. The dancing mistress was Irene Ogden.
The 44-page programme was printed by The Keighley Printers Ltd. of High Street, Keighley. It measures approximately 188 mm by 247 mm. The programme was part of an anonymous donation given in 2022.
Hong Kong (香港; "Fragrant Harbour"), officially Hong Kong Special Administrative Region of the People's Republic of China, is an autonomous territory on the southern coast of China at the Pearl River Estuary and the South China Sea. Hong Kong is known for its skyline and deep natural harbour. It has an area of 1104 km2 and shares its northern border with the Guangdong Province of Mainland China. With around 7.2 million Hongkongers of various nationalities, Hong Kong is one of the world's most densely populated metropolises.
After the First Opium War (1839–42), Hong Kong became a British colony with the perpetual cession of Hong Kong Island, followed by Kowloon Peninsula in 1860 and a 99-year lease of the New Territories from 1898. Hong Kong remained under British control for about a century until the Second World War, when Japan occupied the colony from December 1941 to August 1945. After the Surrender of Japan, the British resumed control. In the 1980s, negotiations between the United Kingdom and the People's Republic of China resulted in the 1984 Sino-British Joint Declaration, which provided for the transfer of sovereignty of Hong Kong on 30 June 1997. The territory became a special administrative region of China with a high degree of autonomy on 1 July 1997 under the principle of one country, two systems. Disputes over the perceived misapplication of this principle have contributed to popular protests, including the 2014 Umbrella Revolution.
In the late 1970s, Hong Kong became a major entrepôt in Asia-Pacific. The territory has developed into a major global trade hub and financial centre. The 44th-largest economy in the world, Hong Kong ranks top 10 in GDP (PPP) per capita, but also has the most severe income inequality among advanced economies. Hong Kong is one of the three most important financial centres alongside New York and London, and the world's number one tourist destination city. The territory has been named the freest market economy. The service economy, characterised by free trade and low taxation, has been regarded as one of the world's most laissez-faire economic policies, and the currency, the Hong Kong dollar, is the 13th most traded currency in the world.
The Hong Kong Basic Law empowers the region to develop relations and make agreements directly with foreign states and regions, as well as international organizations, in a broad range of appropriate fields. It is an independent member of APEC, the IMF, WTO, FIFA and International Olympic Committee among others.
Limited land created a dense infrastructure and the territory became a centre of modern architecture, and one of the world's most vertical cities. Hong Kong has a highly developed public transportation network covering 90 per cent of the population, the highest in the world, and relies on mass transit by road or rail. Air pollution remains a serious problem. Loose emissions standards have resulted in a high level of atmospheric particulates. Nevertheless, Hongkongers enjoy the world's longest or second longest life expectancies.
NAME
It is not known who was responsible for the Romanisation of the name "Hong Kong" but it is generally believed to be an early imprecise phonetic rendering of the pronunciation of the spoken Cantonese or Hakka name 香港, meaning "Fragrant Harbour". Before 1842, the name referred to a small inlet—now Aberdeen Harbour (香港仔, Sidney Lau: heung1gong2 jai2, Jyutping: hoeng1gong2 zai2, or Hiong1gong3 zai3 in a form of Hakka, literally means "Little Hong Kong")—between Aberdeen Island and the south side of Hong Kong Island, which was one of the first points of contact between British sailors and local fishermen. As those early contacts are likely to have been with Hong Kong's early inhabitants, the Tankas (水上人), it is equally probable that the early Romanisation was a faithful execution of their speech, i.e. hong1, not heung1. Detailed and accurate Romanisation systems for Cantonese were available and in use at the time.
The reference to fragrance may refer to the sweet taste of the harbour's fresh water estuarine influx of the Pearl River, or to the incense from factories, lining the coast to the north of Kowloon, which was stored near Aberdeen Harbour for export before the development of the Victoria Harbour.
In 1842, the Treaty of Nanking was signed and the name, Hong Kong, was first recorded on official documents to encompass the entirety of the island.
The name had often been written as the single word Hongkong until the government adopted the current form in 1926. Nevertheless, a number of century-old institutions still retain the single-word form, such as the Hongkong Post, Hongkong Electric and the Hongkong and Shanghai Banking Corporation.
The full official name, after 1997, is "Hong Kong Special Administrative Region of the People's Republic of China". This is the official title as mentioned in the Hong Kong Basic Law and the Hong Kong Government's website; however, "Hong Kong Special Administrative Region" and "Hong Kong" are widely accepted.
Hong Kong has carried many nicknames: the most famous among those is the "Pearl of the Orient", which reflected the impressive night-view of the city's light decorations on the skyscrapers along both sides of the Victoria Harbour. The territory is also known as "Asia's World City".
HISTORY
PRE-BRITISH
Archaeological studies support human presence in the Chek Lap Kok area (now Hong Kong International Airport) from 35,000 to 39,000 years ago and on Sai Kung Peninsula from 6,000 years ago.
Wong Tei Tung and Three Fathoms Cove are the earliest sites of human habitation in Hong Kong during the Paleolithic Period. It is believed that the Three Fathom Cove was a river-valley settlement and Wong Tei Tung was a lithic manufacturing site. Excavated Neolithic artefacts suggested cultural differences from the Longshan culture of northern China and settlement by the Che people, prior to the migration of the Baiyue (Viets) to Hong Kong. Eight petroglyphs, which dated to the Shang dynasty in China, were discovered on the surrounding islands.
ANCIENT CHINA
In 214 BC, Qin Shi Huang, the first emperor of China, conquered the Baiyue tribes in Jiaozhi (modern Liangguang region and Vietnam) and incorporated the territory into imperial China for the first time. Modern Hong Kong was assigned to the Nanhai commandery (modern Nanhai District), near the commandery's capital city Panyu. In Qin dynasty, the territory was ruled by Panyu County(番禺縣) up till Jin Dynasty.
The area of Hong Kong was consolidated under the kingdom of Nanyue (Southern Viet), founded by general Zhao Tuo in 204 BC after the collapse of the short-lived Qin dynasty. When the kingdom of Nanyue was conquered by the Han Dynasty in 111 BC, Hong Kong was assigned to the Jiaozhi commandery. Archaeological evidence indicates that the population increased and early salt production flourished in this time period. Lei Cheng Uk Han Tomb on the Kowloon Peninsula is believed to have been built during the Han dynasty.
IMPERIAL CHINA
Started from Jin dynasty to early period of Tang dynasty, the territory that now comprises Hong Kong was governed by Bao'an County (寶安縣). In Tang dynasty, the Guangdong region flourished as an international trading center. The Tuen Mun region in what is now Hong Kong's New Territories served as a port, naval base, salt production centre and later, base for the exploitation of pearls. Lantau Island was also a salt production centre, where the salt smugglers riots broke out against the government.
Under the Tang dynasty, the Guangdong (Canton) region flourished as a regional trading centre. In 736 AD, the first Emperor of Tang established a military stronghold in Tuen Mun in western Hong Kong to defend the coastal area of the region. The first village school, Li Ying College, was established around 1075 AD in the modern-day New Territories under the Northern Song dynasty. After their defeat by the Mongols, the Southern Song court briefly moved to modern-day Kowloon City (the Sung Wong Toi site), before its final defeat at the Battle of Yamen.
From the mid-Tang dynasty to early Ming dynasty, the territory that now comprises Hong Kong was governed by Dongguan County (東莞縣/ 東官縣). In Ming dynasty, the area was governed by Xin'an County (新安縣) before it was colonized by the British government. The indigenous inhabitants of what is now Hong Kong are identified with several ethnicities, including Punti, Hakka, Tanka) and Hoklo.
The earliest European visitor on record was Jorge Álvares, a Portuguese explorer who arrived in 1513. Having founded an establishment in Macau by 1557, Portuguese merchants began trading in southern China. However, subsequent military clashes between China and Portugal led to the expulsion of all Portuguese merchants from the rest of China.
In the mid-16th century, the Haijin order (closed-door, isolation policy) was enforced and it strictly forbade all maritime activities in order to prevent contact from foreigners by sea. From 1661 to 1669, Hong Kong was directly affected by the Great Clearance of the Kangxi Emperor, who required the evacuation of coastal areas of Guangdong. About 16,000 people from Hong Kong and Bao'an County were forced to emigrate inland; 1,648 of those who evacuated were said to have returned after the evacuation was rescinded in 1669.
BRITSH CROWN COLONY 1842–1941
In 1839, the refusal of Qing authorities to support opium imports caused the outbreak of the First Opium War between the British Empire and the Qing Empire. Qing's defeat resulted in the occupation of Hong Kong Island by British forces on 20 January 1841. It was initially ceded under the Convention of Chuenpee, as part of a ceasefire agreement between Captain Charles Elliot and Governor Qishan. While a dispute between high-ranking officials of both countries led to the failure of the treaty's ratification, on 29 August 1842, Hong Kong Island was formally ceded in perpetuity to the United Kingdom of Great Britain and Ireland under the Treaty of Nanking. The British officially established a Crown colony and founded the City of Victoria in the following year.
The population of Hong Kong Island was 7,450 when the Union Flag raised over Possession Point on 26 January 1841. It mostly consisted of Tanka fishermen and Hakka charcoal burners, whose settlements scattered along several coastal hamlets. In the 1850s, a large number of Chinese immigrants crossed the then-free border to escape from the Taiping Rebellion. Other natural disasters, such as flooding, typhoons and famine in mainland China would play a role in establishing Hong Kong as a place for safe shelter.
Further conflicts over the opium trade between Britain and Qing quickly escalated into the Second Opium War. Following the Anglo-French victory, the Crown Colony was expanded to include Kowloon Peninsula (south of Boundary Street) and Stonecutter's Island, both of which were ceded to the British in perpetuity under the Convention of Beijing in 1860.
In 1898, Britain obtained a 99-year lease from Qing under the Convention for the Extension of Hong Kong Territory, in which Hong Kong obtained a 99-year lease of the Lantau Island, the area north of Boundary Street in Kowloon up to Shenzhen River and over 200 other outlying islands.
Hong Kong soon became a major entrepôt thanks to its free port status, attracting new immigrants to settle from both China and Europe alike. The society, however, remained racially segregated and polarised under British colonial policies. Despite the rise of a British-educated Chinese upper-class by the late-19th century, race laws such as the Peak Reservation Ordinance prevented ethnic Chinese in Hong Kong from acquiring houses in reserved areas, such as the Victoria Peak. At this time, the majority of the Chinese population in Hong Kong had no political representation in the British colonial government. There were, however, a small number of Chinese elites whom the British governors relied on, such as Sir Kai Ho and Robert Hotung, who served as communicators and mediators between the government and local population.
Hong Kong continued to experience modest growth during the first half of the 20th century. The University of Hong Kong was established in 1911 as the territory's oldest higher education institute. While there was an exodus of 60,000 residents for fear of a German attack on the British colony during the First World War, Hong Kong remained peaceful. Its population increased from 530,000 in 1916 to 725,000 in 1925 and reached 1.6 million by 1941.
In 1925, Cecil Clementi became the 17th Governor of Hong Kong. Fluent in Cantonese and without a need for translator, Clementi introduced the first ethnic Chinese, Shouson Chow, into the Executive Council as an unofficial member. Under his tenure, Kai Tak Airport entered operation as RAF Kai Tak and several aviation clubs. In 1937, the Second Sino-Japanese War broke out when the Japanese Empire expanded its territories from northeastern China into the mainland proper. To safeguard Hong Kong as a freeport, Governor Geoffry Northcote declared the Crown Colony as a neutral zone.
JAPANESE OCCUPATION 1941–45
As part of its military campaign in Southeast Asia during Second World War, the Japanese army moved south from Guangzhou of mainland China and attacked Hong Kong on 8 December 1941. The Battle of Hong Kong ended with the British and Canadian defenders surrendering control of Hong Kong to Japan on 25 December 1941 in what was regarded by locals as Black Christmas.
During the Japanese occupation of Hong Kong, the Japanese army committed atrocities against civilians and POWs, such as the St. Stephen's College massacre. Local residents also suffered widespread food shortages, limited rationing and hyper-inflation arising from the forced exchange of currency from Hong Kong Dollars to Japanese military banknotes. The initial ratio of 2:1 was gradually devalued to 4:1 and ownership of Hong Kong Dollars was declared illegal and punishable by harsh torture. Due to starvation and forced deportation for slave labour to mainland China, the population of Hong Kong had dwindled from 1.6 million in 1941 to 600,000 in 1945, when Britain resumed control of the colony on 30 August 1945.
ECONOMY
As one of the world's leading international financial centres, Hong Kong has a major capitalist service economy characterised by low taxation and free trade. The currency, Hong Kong dollar, is the eighth most traded currency in the world as of 2010. Hong Kong was once described by Milton Friedman as the world's greatest experiment in laissez-faire capitalism, but has since instituted a regime of regulations including a minimum wage. It maintains a highly developed capitalist economy, ranked the freest in the world by the Index of Economic Freedom every year since 1995. It is an important centre for international finance and trade, with one of the greatest concentrations of corporate headquarters in the Asia-Pacific region, and is known as one of the Four Asian Tigers for its high growth rates and rapid development from the 1960s to the 1990s. Between 1961 and 1997 Hong Kong's gross domestic product grew 180 times while per-capita GDP increased 87 times over.
The Hong Kong Stock Exchange is the seventh largest in the world and has a market capitalisation of US$2.3 trillion as of December 2009. In that year, Hong Kong raised 22 percent of worldwide initial public offering (IPO) capital, making it the largest centre of IPOs in the world and the easiest place to raise capital. The Hong Kong dollar has been pegged to the US dollar since 1983.
The Hong Kong Government has traditionally played a mostly passive role in the economy, with little by way of industrial policy and almost no import or export controls. Market forces and the private sector were allowed to determine practical development. Under the official policy of "positive non-interventionism", Hong Kong is often cited as an example of laissez-faire capitalism. Following the Second World War, Hong Kong industrialised rapidly as a manufacturing centre driven by exports, and then underwent a rapid transition to a service-based economy in the 1980s. Since then, it has grown to become a leading centre for management, financial, IT, business consultation and professional services.
Hong Kong matured to become a financial centre in the 1990s, but was greatly affected by the Asian financial crisis in 1998, and again in 2003 by the SARS outbreak. A revival of external and domestic demand has led to a strong recovery, as cost decreases strengthened the competitiveness of Hong Kong exports and a long deflationary period ended. Government intervention, initiated by the later colonial governments and continued since 1997, has steadily increased, with the introduction of export credit guarantees, a compulsory pension scheme, a minimum wage, anti-discrimination laws, and a state mortgage backer.
The territory has little arable land and few natural resources, so it imports most of its food and raw materials. Imports account for more than 90% of Hong Kong's food supply, including nearly all of the meat and rice available there. Agricultural activity - relatively unimportant to Hong Kong's economy and contributing just 0.1% of its GDP - primarily consists of growing premium food and flower varieties. Hong Kong is the world's eleventh largest trading entity, with the total value of imports and exports exceeding its gross domestic product. It is the world's largest re-export centre. Much of Hong Kong's exports consist of re-exports, which are products made outside of the territory, especially in mainland China, and distributed via Hong Kong. Its physical location has allowed the city to establish a transportation and logistics infrastructure that includes the world's second busiest container port and the world's busiest airport for international cargo. Even before the transfer of sovereignty, Hong Kong had established extensive trade and investment ties with the mainland, which now enable it to serve as a point of entry for investment flowing into the mainland. At the end of 2007, there were 3.46 million people employed full-time, with the unemployment rate averaging 4.1% for the fourth straight year of decline. Hong Kong's economy is dominated by the service sector, which accounts for over 90% of its GDP, while industry constitutes 9%. Inflation was at 2.5% in 2007. Hong Kong's largest export markets are mainland China, the United States, and Japan.
As of 2010 Hong Kong is the eighth most expensive city for expatriates, falling from fifth position in the previous year. Hong Kong is ranked fourth in terms of the highest percentage of millionaire households, behind Switzerland, Qatar, and Singapore with 8.5 percent of all households owning at least one million US dollars. Hong Kong is also ranked second in the world by the most billionaires per capita (one per 132,075 people), behind Monaco. In 2011, Hong Kong was ranked second in the Ease of Doing Business Index, behind Singapore.
Hong Kong is ranked No. 1 in the world in the Crony Capitalism Index by the Economist.
In 2014, Hong Kong was the eleventh most popular destination for international tourists among countries and territories worldwide, with a total of 27.8 million visitors contributing a total of US$38,376 million in international tourism receipts. Hong Kong is also the most popular city for tourists, nearly two times of its nearest competitor Macau.
DEMOGRAPHICS
The territory's population in mid-2015 is 7.30 million, with an average annual growth rate of 0.8% over the previous 5 years. The current population of Hong Kong comprises 91% ethnic Chinese. A major part of Hong Kong's Cantonese-speaking majority originated from the neighbouring Guangdong province, from where many fled during the Second Sino-Japanese War, the Chinese Civil War, and the communist rule in China.
Residents of the Mainland do not automatically receive the Right of Abode, and many may not enter the territory freely. Like other non-natives, they may apply for the Right of Abode after seven years of continuous residency. Some of the rights may also be acquired by marriage (e.g., the right to work), but these do not include the right to vote or stand for office. However, the influx of immigrants from mainland China, approximating 45,000 per year, is a significant contributor to its population growth – a daily quota of 150 Mainland Chinese with family ties in Hong Kong are granted a "one way permit". Life expectancy in Hong Kong is 81.2 years for males and 86.9 years for females as of 2014, making it the highest life expectancy in the world.
About 91% of the people of Hong Kong are of Chinese descent, the majority of whom are Taishanese, Chiu Chow, other Cantonese people, and Hakka. Hong Kong's Han majority originate mainly from the Guangzhou and Taishan regions in Guangdong province. The remaining 6.9% of the population is composed of non-ethnic Chinese. There is a South Asian population of Indians, Pakistanis and Nepalese; some Vietnamese refugees have become permanent residents of Hong Kong. There are also Britons, Americans, Canadians, Japanese, and Koreans working in the city's commercial and financial sector. In 2011, 133,377 foreign domestic helpers from Indonesia and 132,935 from the Philippines were working in Hong Kong.
Hong Kong's de facto official language is Cantonese, a variety of Chinese originating from Guangdong province to the north of Hong Kong. English is also an official language, and according to a 1996 by-census is spoken by 3.1 percent of the population as an everyday language and by 34.9 percent of the population as a second language. Signs displaying both Chinese and English are common throughout the territory. Since the 1997 Handover, an increase in immigrants from communist China and greater interaction with the mainland's economy have brought an increasing number of Mandarin speakers to Hong Kong.
RELIGION
A majority of residents of Hong Kong have no religious affiliation, professing a form of agnosticism or atheism. According to the US Department of State 43 percent of the population practices some form of religion. Some figures put it higher, according to a Gallup poll, 64% of Hong Kong residents do not believe in any religion, and possibly 80% of Hong Kong claim no religion. In Hong Kong teaching evolution won out in curriculum dispute about whether to teach other explanations, and that creationism and intelligent design will form no part of the senior secondary biology curriculum.
Hong Kong enjoys a high degree of religious freedom, guaranteed by the Basic Law. Hong Kong's main religions are Buddhism, Taoism and Confucianism; a local religious scholar in contact with major denominations estimates there are approximately 1.5 million Buddhists and Taoists. A Christian community of around 833,000 forms about 11.7% of the total population; Protestants forms a larger number than Roman Catholics at a rate of 4:3, although smaller Christian communities exist, including the Latter-day Saints and Jehovah's Witnesses. The Anglican and Roman Catholic churches each freely appoint their own bishops, unlike in mainland China. There are also Sikh, Muslim, Jewish, Hindu and Bahá'í communities. The practice of Falun Gong is tolerated.
PERSONAL INCOME
Statistically Hong Kong's income gap is the greatest in Asia Pacific. According to a report by the United Nations Human Settlements Programme in 2008, Hong Kong's Gini coefficient, at 0.53, was the highest in Asia and "relatively high by international standards". However, the government has stressed that income disparity does not equate to worsening of the poverty situation, and that the Gini coefficient is not strictly comparable between regions. The government has named economic restructuring, changes in household sizes, and the increase of high-income jobs as factors that have skewed the Gini coefficient.
WIKIPEDIA
Deputy PM Nick Clegg meets students at Number 10 who are part of the government's Arrival Education programme and all of whom received their GCSE results this morning. 24 August 2010, Crown copyright
The Arts Council of Australia
Newcastle City Hall
April 1952
Souvenir Programme
Programme courtesy of Mrs R. Sharkey
Page 4
Reading a review of Let’s Make an Opera from the Newcastle Morning Herald and Miners Advocate 1952 provides a great insight into the performance. The cast consisted of five adults and hundreds of school children which was something of a challenge for the conductor Eric Starling who, ‘sometimes had to act as school teacher as well as conductor to enlist full co-operation from them’.
The play consisted of two parts, the preparation of the opera and its dress rehearsal followed by the actual opera. Audience involvement in the performance was also expected. ‘Owls, herons, turtle-doves and chaffinches will carol together when Newcastle audiences take their part in ‘Let’s Make an Opera”.
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