miércoles, 5 de noviembre de 2008

Ingles 4º 2º

ciclo lectivo 2008

Profesora Stella goldensweig
Proyecto: Año Polar


TRABAJO 1
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Alumnos: pirulo pitulito popote

TP2

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martes, 4 de noviembre de 2008

ANTARTICA: Global Warming Effects 4*2*

Project Work

Antartica: Global Warming Effects


Students: Eduardo Rojas
Christian G. Palavecino

Teacher: Stella Maris Goldenzweig

Course. 4to 2da


Year: 2008



ANTARTICA: Global Warming Effects

Antarctica gives mixed signals on warming. Is the zone more sensitive to climatic change than other regions and scientists are looking to it to predict the future climate of the globe? No one can seem to agree about whether or not Antarctica is warming or cooling; various different studies claim one, the other, both, or that measuring melting as a sign of global temperature change is not applicable in Antarctica because cycles of melting and refreezing are part of normal glaciations. However, the majority of researchers seem to agree that the amount of ice that has been melting lately in Antarctica is cause for concern. Yet it seems a bit strange that they should preach about mankind's destruction of the environment when, in the name of research, Antarctica has been "conquered", colonized with an airport, roads, and power plants to house about 1200 people in the McMurdo station alone.

While the Arctic and the Antarctic experience similar greenhouse gas levels and solar radiation, each region responds in a dramatically different way, especially in temperature and loss of sea ice.
Scientists have concluded, based on new research since the 2007 Intergovernmental Panel on Climate Change Report, that a combination of factors is responsible for the recent dramatic sea ice loss in the Arctic as well as masking some of the effects in the Antarctic.

But there are inconsistent reports because the total surface area of Antarctica doubles in winter with the addition of sea ice. You can't expect an area three times the size of Australia to behave the same way throughout. This is a tricky region and is more likely to do its own thing as the rest of the planet warms.

Temperature
For most of the Antarctic, temperatures were not unusual, except on the Antarctic Peninsula, a finger of land and ice about 1,000 miles south of the tip of South America, which had the largest increase in temperatures of any location in the Southern Hemisphere.


Temperatures warmed by three degrees Fahrenheit. Warming temperatures and exposure to ocean waves were cited by the National Snow and Ice Data Center as the cause of the collapse of a 160-square-mile segment of the Wilkins Ice Shelf on the peninsula, which began collapsing in late February.

The Antarctic Peninsula is particularly sensitive to small rises in the annual average temperature, this has increased about 2.5C in the region in the last 50 years, and this is 2 or 3 times faster than the average in the rest of the world. This makes it an excellent study area.
The temperature of the rest of Antarctica - the other 96% - shows no current indications of rising.

If the whole of Antarctica were divided into grips about 60 to 70 percent of the squares would reveal a cooling trend, while warming would be seen in the other 30 to 40 percent of the overall area. So there's a slight net cooling for the entire continent.

Sea Ice
Story is clearer.
Gillett, a climate dynamics scientist, said, “In the Antarctic, the changes in winds and temperatures are consistent with how we would expect them to respond to increased greenhouse gases and depletion of stratospheric ozone.”
The depletion of ozone has strengthened the atmospheric circulation, called the Southern Annual Mode, or SAM. As the ozone hole recovers, the winds that currently whiz around Antarctica and block air masses from crossing into the continent’s interior would weaken, and Antarctica would no longer be so isolated from global warming patterns.

However, data on temperatures in Antarctica only really go back about 50 years, anything beyond that is surmised from ice cores or other sources and as a result we don't really know how the temperatures vary over even the medium term in Antarctica.


Biological Effects of Global Warming

Antarctica's only two flowering plant species that grow only on the Peninsula have spread considerably in the last few decades in both geographic distribution and also abundance in the areas where they are found. In some areas they are becoming the dominant species.



Penguins have also been suffering a steady decline in parts of the Antarctic
Peninsula region for the last 20 years. They are reducing in number and abandoning certain nesting sites

Studies have shown that stocks of krill in Antarctica have declined dramatically in recent years. The reason for this is likely to be a fall in the amount of sea ice in the winter months. There are commercial implications as well as scientific ones. The Southern Ocean is a valuable fisheries resource; many of the species caught feed on krill. Thousands of tourists are also attracted to Antarctica to enjoy the spectacular wildlife, most of which feed on krill. This decline in krill will also make it more difficult for the great baleen whales to return to pre-exploitation levels following their decimation in numbers.



The Future
The British Antarctic Survey, which has undertaken the majority of Britain's scientific research in the area, has the following positions: [6]
Ice makes polar climate sensitive by introducting a strong positive feedback loop.
Melting of continental Antarctic ice could contribute to global sea level rise.
Climate models predict more snowfall than ice melting during the next 50 years, but models are not good enough for them to be confident about the prediction.
Antarctica seems to be both warming around the edges and cooling at the center at the same time. Thus it is not possible to say whether it is warming or cooling overall.
There is no evidence for a decline in overall Antarctic sea ice extent.
The central and southern parts of the west coast of the Antarctic Peninsula have warmed by nearly 3°C. The cause is not known.
Changes have occurred in the upper atmosphere over Antarctica.

The area of strongest cooling appears at the South Pole, and the region of strongest warming lies along the Antarctic Peninsula. A possible explanation is that loss of UV-absorbing ozone may have cooled the stratosphere and strengthened the polar vortex, a pattern of spinning winds around the South Pole. The vortex acts like an atmospheric barrier, preventing warmer, coastal air from moving in to the continent's interior.
A stronger polar vortex might explain the cooling trend in the interior of Antarctica.
In their latest study (September 20, 2007) NASA researchers have confirmed that Antarctic snow is melting farther inland from the coast over time, melting at higher altitudes than ever and increasingly melting on Antarctica's largest ice shelf.
Scientists project that the ozone hole should fully recover by 2070.“As the ozone hole recovers, we expect that warming will appear on the central plateau of Antarctica and we will see a reduction in sea ice area,” said Turner.

Source: www.NOAA.com

Biologia: Dr. Hector Cuadrado

Quimica

Project Work: Carlos Landoni, Valentìn Delauro y Paola Fernandez

Antarctica

1) Climate; 2) Flora; 3) Fauna; 4) Territories Claims;
5) History; 6) Natural Resources; 7) The Antarctic Treaty
1) Climate
Antarctica is classified into three basic climate regions: the peninsula, coastal regions, and the interior.
Antarctic Peninsula Reaching farther north than any other part of the continent, the peninsula has the most moderate climate with its warmer temperatures and increased precipitation. Antarctica's wildlife is more dominant in this region. Here, millions of seabirds, and hundreds of thousands of marine mammals, come to breed and feed in the summer months. Although the peninsula has milder temperatures than the rest of the continent, it sustains the fiercest winds, with gusts recorded as high as 200 mph.
Coastal Regions The coastal regions are a balance between the Antarctic peninsula and the interior. The coasts are milder in temperature than the interior, and receive less precipitation that the peninsula. In the summer, warm ocean currents give this area a more moderate climate, but as winter approaches and the waters freeze, ice grows and the shoreline quickly cools. Coastal temperatures drop much lower than the peninsula. These regions rarely see rainfall, rather their precipitation usually occurs in the form of snow.
Antarctic Interior The coldest part of the continent is found in the interior. It is categorized primarily by its extreme cold and lack of precipitation. The coldest temperature ever recorded was at the Vostok research station, east of the South Pole; in July, 1983 the temperature reached -129 degrees Fahrenheit, creating a new world low. The sun stays below the horizon beginning in March and lasting through September. During these winter months the interior is almost in complete darkness with zero solar radiation to help heat the surface. Far away from the ocean, the interior receives no warming effects from the waters like the coastal regions and peninsula. Indirect sunrays and high elevation also add to the chilling temperatures of Antarctica's interior.
2) Flora
Lichens Of all the plants, lichens are best adapted to survive in the harsh polar climate. Some lichens have even been found only about 400 km from the South Pole. Lichens have proliferated in Antarctica mainly because there is little competition from mosses or flowering plants and because of their high tolerance of drought and cold. The peculiarity of lichens is that they are not one homogeneous organism but a symbiosis of two different partners, a fungus and an alga. The fungus part supplies the plant with water and nutritious salt, meanwhile the alga part organic substance, like carbohydrate produce. With this ideal "job-sharing", lichens can survive the hardest conditions. Far from the border of highly developed plants, lichens are the pioneers of the vegetation. Lichens aren’t only frugal and robust, they jug out because of their very low sensibility against frost. Some lichens, in an experiment, survived a bath in liquid nitrogen at minus 195 degrees. On icy rock, lichens have the same strategy as plants have developed in the sand of the Sahara: they form an "oasis". Like in the desert they miss water. They have only a chance to survive, if they settle in an area with a convenient, damp microclimate. Since what stops lichens to spread over the whole of Antarctica is not so much the big cold as the lack of water. For this reason they don’t settle in a place with the most sunshine, but in recesses and cracks between rocks. They like scanty soils, created by weathered rocks. They often quicken this process with secretion of acid. Snowflake are captured in the cracked rock and smelt on the dark lichens, they can absorb the vitally liquid. Especially unfavourable conditions are in the "dry valley" of East Antarctica, where big coldness and low snowfall meet. But even there scientists have found a dark cover on the north side of some rocks, which prove to be lichens. Under the microscope it was shown that the lichens penetrate the upper coat of the rock. With the dark colour the lichens absorb more light. This strategy enables the lichens to scrape a humble living in that quite high southern latitude.
Mosses Only a small number of moss species are found in Antarctica. Extensive fields occur in a few places on this continent and these are rarely more than 100 mm deep, even in the most favourable areas where there is shelter and plenty of water. Short moss turf and cushion moss is found most frequently in sandy and gravelly soils. No extensive peat formations are to be found. Mosses, like lichens, gather in colonies which make them possible to collect and retain more water. They also lose less by evaporation and show a marked ability to use water rapidly whenever it becomes available. Mosses have also become well adapted to the almost continuous light during the long days of a polar summer. One Antarctic moss, Bryum argenteum, produces more energy by photosynthesis in low light at 5°C than it does at 15°C, or higher. Photosynthesis can start within a few hours of thawing after a prolonged period of freezing, and almost immediately following short periods.
Algae More than 300 species of non-marine algae have been found in Antarctica. These very simple plants take many diverse forms and a few have become adapted to living in difficult polar environments. Blue-green and other algae are found growing in damp sand and gravel around lakes and tarns, along meltwater streams or in low-lying areas, where snowdrifts or seepage may collect. Some such as Prasiola crispa can tolerate high levels of nutrients and are found near bird colonies. Others – the snow algae - may form extensive and spectacular red, yellow or green patches in areas of permanent snow. Recent studies have shown that some blue-green algae live inside rocks in dry valleys. Commonly they are found under stones, particularly light-coloured quartz stones, where the microclimate is more favourable than in the surrounding sand or soil. Together with lichens, they are the only living things in a barren landscape.
3) Fauna
Antarctic Birds Millions of seabirds breed along the coast and offshore islands of Antarctica. To survive in the biting environment, Antarctic birds have waterproof plumage, and large compact bodies with a dense layer of fat under their skin. There are nineteen species of seabirds that breed along the continent. Due to the shortage of snow-free nesting regions, most seabirds tend to procreate in large, impressive concentrations making for ideal viewing conditions for the bird enthusiasts. The birds will migrate north as the summer months come to an end, spending the winter in more temperate climates.
Penguins One of Antarctica's most familiar wildlife, penguins are considered by many to be the continent's signature species. They spend over 75% of their lives as sea where they are most comfortable. Their bodies are designed for swimming. Powerful paddle muscles and a compact hydrodynamic body shape allow penguins to swim up to 25 mph. Impressive and elegant in the water, by contrast penguins awkwardly waddle and hop once ashore. While seventeen species of penguins can be found in the subantarctic regions - including coastal islands - only four types of the flightless birds breed on the continent itself: the Emperor, Adelie, Chinstrap, and Gentoo penguins.
Antarctic Seals Much of the early exploration of Antarctica and the Southern Ocean was do to the search for new seal communities. During the 19th and 20th century, many seals were hunted for their valuable skins and oils. Entire populations of species were driven to the brink of extinction. Thankfully, today, the seals are protected by a collection of agencies, and their numbers have continued to thrive. Because of the nutrient-rich feeding regions, and the lack of polar bears, the Antarctic has a much larger seal population than the Arctic. Most of their life is spent in water, but seals must return to land to breed. The best locations to view their breeding grounds are on the pack ice surrounding Antarctica, or along the coastal shores of the northern islands.

Whales Whales are divided into two main groups: toothed and baleen. The only toothed whales found in the Antarctic are the Orca and the Sperm whale, while a variety of baleen whales have been sited: Blue, Fin, Humpback, Minke, and Southern Right. Unlike the other wildlife of Antarctica, whales do not breed in the region. However, they do take advantage of the nutrient-filled waters in the austral summer, traveling great distances from their temperate breeding waters in the north. Like seals, several species of whales were hunted until near extinction in the mid-1900s. While regulations have been placed on whaling activities, these magnificent giants have not seen their populations recover as well as the seals. Today, the entire area surrounding Antarctica is recognized as a whale sanctuary.
4) Territories Claims



5) History
The idea of a large southern continent first appeared in the Greek writings of both Pythagoras and Aristotle. It was believed the earth would topple if a sizable landmass did not exist to balance out the northern continents. Today, we refer to that region as Antarctica. Although Captain James Cook was the first recorded explorer to cross the Antarctic Circle in 1773, he was not the first to see Antarctica's landmass. That acclaim would go to Russian Fabian van Bellinshausen fifty years later. Cook's accounts of the large seal and whale populations, however, helped influence further exploration of the Southern Ocean from sealers in search of the mammals' valued skins. In the 19th century over one thousand sealing ships traveled to the Antarctic regions and its shoreline. In the early 20th century, reaching the South Pole became a top priority for explorers. The first expeditions to actually declare the South Pole as their primary purpose were led by Robert F. Scott in 1902, and Irishman Ernest Shackleton in 1908. Neither would reach their desired destination, but Shackleton came frustratingly close, just 97 miles from the Pole before terminating his crusade. Shackleton had failed in his quest for the South Pole, but he returned to the continent in 1914 to claim a new prize: the first crossing on foot of the Antarctic continent. With a crew of 27, they set sail in early December. A month into the expedition, their ship, Endurance, was trapped and slowly crushed by pack ice. Salvaging what supplies they could, the crew was forced to abandon the ship, and struggle to stay alive in one of the most inhospitable environments in the world. The men would endure sub-zero temperatures and starvation for nearly 20 months, with no communication to the outside world. Incredibly, not a single man would be lost. Shackleton's journey of survival would become one of the most noted in Antarctica's history. Interest in Antarctica continued through the World Wars and into the Cold War. At that time, an American training facility was created to give US troops experience in polar conditions. In early spring of 1954, the first permanent scientific station was established by the Australian National Antarctic Research Expeditions. No single nation controls Antarctica, nor does the continent have any nations of its own. The Antarctic Treaty governs Antarctica. Originally signed in 1961 by 12 nations (Argentina, Australia, Belgium, Chile, French Republic, Japan, New Zealand, Norway, Union of South Africa, Union of Soviet Socialist Republics, United Kingdom of Great Britain and Northern Ireland, and United States of America) it now contains the signature of 44 countries. The treaty recognizes Antarctica's unique position on the planet as a shared environment to be used for peaceful purposes, and international cooperative scientific research. Together, Antarctica would be used in the interests of all human progress and to better humankind.
6) Natural Resources
IceOne of Antarctica's most important resources is ice. It is said that Antarctica's ice accounts for 90% of the worlds fresh water. As a resource it has potential as a fresh water supply. Some people have considered towing icebergs from Antarctica to parts of the world in need of fresh water. At present the delivery costs make these ventures unprofitable. Another possible use of the ice on Antarctica is as a long term deep freeze storage site for grain and other foods. Again the costs of shipping and handling are prohibitive. CoalThere are coal deposits found along the coast of Antarctica. It is also very wide spread throughout the Transantarctic Mountains. These deposits were formed between 35 million and 55 million years ago when Antarctica was covered by ancient swamps. Coal forms in swamps as plants die and are buried before they can be completely decomposed. They are then covered by other sediments such as sand and mud. This burial allows the hydrocarbons in the coal to be preserved for future generations to use. Coal is used as a source of direct heat and also to generate electricity incoal burning power plants. The main problem of developing coal in Antarctica is that the cost of mining and delivering the coal is so much higher than the cost of coal in the rest of the world market. It may bepossible for coal to be used in some small research stations for a source of heat. PetroleumPetroleum deposits are formed when plants and small animal remains are buried in a marine environment by sand and mud. These remains then build up as hydrocarbons and are trapped by a layer of rock that the hydrocarbons cannot pass through. These cap rocks then store the petroleum underground until it is pumped out by wells. At this time there has been no petroleum exploration attempted and there are no known petroleum resources in Antarctica. Most of the speculation about petroleum in Antarctica comes from finding petroleum on the other Southern continents which were at one time connected together. The petroleum deposits thought to be on the offshore regions of Antarctica would probably be most feasible to obtain although they would have to be exceptionally large to be considered for exploitation because of the following enormous exploration and development problems: Deeper water over the continental shelves;The presence of sea ice and icebergs;Short work season and hostile climate. Comparisons with other Gondwana continents suggest the existence of petroleum reserves in the interior of Antarctica. But these lie below the thick ice, ruling out development. This is due not only to the thickness of the ice but also the fact that it is sliding slowly towards the coast. Metallic MineralsMineral resources have not been found in great quantities so far due to the small amount of rock that is exposed. It is believed that since the other continents that were once attached to Antarctica to form Gondwana have metallic and nonmetallic minerals, that Antarctica probably has similar minerals. It is also known that rock layers such as those in Antarctica commonly contain large amounts of cobalt, chromium, nickel, vanadium, copper, iron and platinum group minerals. The search for sizable concentrations of metallic minerals below the ice will be a difficult prospecting venture which will require costly geophysical and geochemical surveying and core drilling. Geologists have found small deposits of minerals in Antarctica but these deposits are low in quality and occur in widely scattered places. The peninsula seems to have the highest probability of containing economic base-metal deposits. HydrothermalWhen fluids such as water are heated by the earth's interior, they can carry dissolved minerals in their fluid state such as quartz, gold, etc. When the solution of liquid and dissolved minerals cools in a new environment, the minerals are deposited as a solid. (The same way that candy forms crystals as it cools and hardens.) Magmatic SegregationAs liquid rock (magma) cools, the minerals in it separate. This is because the minerals have different densities and will separate with the denser minerals towards the bottom. (Think of how a bottle of Italian dressing separates into layers.) This separates the minerals into different layers resulting in concentrations of minerals in different places as the magma cools and hardens. SedimentationAs the earth is worn down and broken into pieces by wind, water, ice and other weathering processes, the pieces of the earth are carried by water into the oceans where they are deposited in layers. Since the pieces are different sizes and have different solubilities in water, they settle to the bottom and form different layers. This results in concentrations of the minerals separated into layers.
7) The Antarctic Treaty
The Antarctic Treaty was signed in 1959 by the 12 countries which had Antarctic stations during the International Geophysical Year (1957-58). These 'original signatories' were Argentina, Australia, Belgium, Chile, France, Japan, New Zealand, Norway, South Africa, United Kingdom, the United States and the USSR. The Treaty came into operation in 1961, and since then a further 14 countries have joined the original 12 as "Consultative Parties", i.e. 26 nations have full voting rights at meetings. Any Party to the Treaty which shows a genuine interest in Antarctica by conducting scientific research activities is entitled to become a Consultative Party. All decisions are made by consensus, i.e. all Consultative Parties must agree. The Treaty is open to any member of the United Nations and aims to further the principles of the UN Charter. It stipulates that the Antarctic should forever be used for peaceful purposes and prohibits military activity. Freedom of scientific research is guaranteed, and inspections can be carried out to ensure the Treaty is being observed. It applies to the area south of 60°South latitude. Seven nations claim territory, or 'sovereignty rights', in Antarctica: Argentina, Australia, Chile, France, New Zealand, Norway, and the United Kingdom, and two reserve the right to claim territory: the United States and Russia. These claims are not universally recognised and the Antarctic Treaty puts them legally on-hold to prevent disputes. Antarctic Treaty meetings are held every year, and deal with a range of scientific, environmental and operational issues related to cooperative activities in Antarctica.

IPY History: Leonardo

On three occasions over the past 125 years scientists from around the world banded together to organize concentrated scientific and exploring programs in the Polar Regions. In each major thrust, or “year,” scientific knowledge and geographical exploration were advanced, thereby extending understanding of many geophysical phenomena that influence nature’s global systems. Each polar year was a hallmark of international cooperation in science. The experience gained by scientists and governments in international cooperation set the stage for other international scientific collaboration. International scientific cooperation also paved the way for several political accords that gained their momentum from the polar years. IPY 2007-2008 will expand upon this legacy of scientific achievement and societal benefits.
First International Polar Year (1882-1883): The idea of International Polar Years was the inspiration of the Austrian explorer and naval officer Lt. Karl Weyprecht who was a scientist and co-commander of the Austro-Hungarian Polar Expedition of 1872-74.
From his experiences in the Polar Regions Weyprecht became aware that solutions to the fundamental problems of meteorology and geophysics were most likely to be found near the Earth’s poles. The key concept of the first IPY was that geophysical phenomena could not be surveyed by one nation alone; rather, an undertaking of this magnitude would require a coordinated international effort. 12 countries participated, and 15 expeditions to the poles were completed (13 to the Arctic, and 2 to the Antarctic). Beyond the advances to science and geographical exploration, a principal legacy of the First IPY was setting a precedent for international science cooperation. Unfortunately Weyprecht did not live to see his idea come to fruition.
Sites
Austria - Jan Mayen IslandAmerica 1 - Point Barrow, Alaska ( 71deg N )America 2 - Lady-Franklin-Bay at Discovery Harbor, Ellesmere Isl. ( 81deg 42'N) Denmark - Godthab, Western GreenlandEngland ( Canada ) - Fort Rae at the Great Slave LakeFrance - Orangebay at the southern tip of Tierra del Fuego (S. Hemisphere)Finland - Sodankyla & Kultala (at Ivalojoki River)Germany 1 - Kingua-Fjord at Cumberland Sound, Baffin IslandGermany 2 - Moltke-Hafen at Royal Bay, South Georgia (S Hemisphere)Holland - Dicksonhafen - the expedition vessel "Varna" sunk so the expedition made its observations in the Kara Sea near Waigach IslandNorway - Bossekop / Alten, AltenfjordRussia 1 - Karmakuly, Moller Bay, Nowaja SemljaRussia 2 - Sagasta at the Lena estuarySweden - Cap Thordsen in the Icefjord, Spitzbergen
Beyond the advances to science and geographical exploration, a principal legacy of the First IPY was setting a precedent for international science cooperation.

Second International Polar Year (1932-1933): The International Meteorological Organization proposed and promoted the Second IPY (1932–1933) as an effort to investigate the global implications of the newly discovered “Jet Stream.” 40 nations participated in the Second IPY, and it heralded advances in meteorology, magnetism, atmospheric science, and in the “mapping” of ionospheric phenomena that advanced radio science and technology. Forty permanent observation stations were established in the Arctic, creating a step-function expansion in ongoing scientific Arctic research. In Antarctica, the U.S. contribution was the second Byrd Antarctic expedition, which established a winter-long meteorological station approximately 125 miles south of Little America Station on the Ross Ice Shelf at the southern end of Roosevelt Island. This was the first research station inland from Antarctica’s coast.
The International Geophysical Year (1957-58): The International Geophysical Year (IGY), 1 July 1957 to 31 December 1958, celebrated the 75th and 25th anniversaries of the First and Second IPYs. The IGY was conceived by a number of post-WWII eminent physicists, including Sydney Chapman, James Van Allen, and Lloyd Berkner, at an informal gathering in Washington, DC in 1950. These individuals realized the potential of the technology developed during WWII (for example, rockets and radar), and they hoped to redirect the technology and scientific momentum towards advances in research, particularly in the upper atmosphere. The IGY’s research, discoveries, and vast array of synoptic observations revised or “rewrote” many notions about the Earth’s geophysics. One long disputed theory, continental drift, was confirmed. A U.S. satellite discovered the Van Allen Radiation Belt encircling the Earth. Geophysical traverses over the Antarctic icecap yielded the first informed estimates of the total size of Antarctica’s ice mass. For many disciplines, the IGY led to an increased level of research that continues to the present. The world’s first satellites were launched. A notable political result founded on the IGY was ratification of the Antarctic Treaty in 1961. The success of the IGY also fostered an additional year of research through the International Geophysical Cooperation. The Special Committee for the IGY became the model on which three post-IGY Scientific Committees developed, for Antarctic, Oceanic, and Space Research, and several focused research efforts including the International Year of the Quiet Sun. The scientific, institutional, and political legacies of the IGY endured for decades, many to the present day.


The Antarctic Treaty
The Antarctic Treaty was signed in Washington on 1 December 1959 by the twelve nations that had been active during the IGY (Argentina, Australia, Belgium, Chile, France, Japan, New Zealand, Norway, South Africa, United Kingdom, United States and USSR). The Treaty, which applies to the area south of 60° South latitude, is surprisingly short, but remarkably effective. Through this agreement, the countries active in Antarctica consult on the uses of a whole continent, with a commitment that it should not become the scene or object of international discord. In its fourteen articles the Treaty:
stipulates that Antarctica should be used exclusively for peaceful purposes, military activities, such as the establishment of military bases or weapons testing, are specifically prohibited;
guarantees continued freedom to conduct scientific research, as enjoyed during the IGY;
promotes international scientific cooperation including the exchange of research plans and personnel, and requires that results of research be made freely available;
sets aside the potential for sovereignty disputes between Treaty parties by providing that no activities will enhance or diminish previously asserted positions with respect to territorial claims, provides that no new or enlarged claims can be made, and makes rules relating to jurisdiction;
prohibits nuclear explosions and the disposal of radioactive waste;
provides for inspection by observers, designated by any party, of ships, stations and equipment in Antarctica to ensure the observance of, and compliance with, the Treaty;
requires parties to give advance notice of their expeditions;
provides for the parties to meet periodically to discuss measures to further the objectives of the Treaty; and
puts in place a dispute settlement procedure and a mechanism by which the Treaty can be modified.
The Treaty also provides that any member of the United Nations can accede to it. The Treaty now has 44 signatories, 27 are Consultative Parties on the basis of being original signatories or by conducting substantial research there. Membership continues to grow. A full list of the current parties to the Treaty appears at the end of this document.
Since entering into force on 23 June 1961, the Treaty has been recognized as one of the most successful international agreements. Problematic differences over territorial claims have been effectively set aside and as a disarmament regime it has been outstandingly successful. The Treaty parties remain firmly committed to a system that is still effective in protecting their essential Antarctic interests. Science is proceeding unhindered.
Since the first Antarctic Treaty Consultative Meeting (ATCM) in 1961, the parties have met frequently, now annually, to discuss issues as diverse as scientific cooperation, measures to protect the environment, and operational issues - and they are committed to taking decisions by consensus. This process has allowed the Antarctic Treaty to evolve into a system with a number of components that meet the special needs of managing activities in the Antarctic, while protecting national interests. This regime is now known by the broader title of the Antarctic Treaty System, which operates under the umbrella of the annual ATCM.
The Antarctic Treaty System
The Antarctic Treaty System comprises the Treaty itself and a number of related agreements. It also includes a range of organizations that contribute to the work of the decision-making forums.
In addition to the related agreements (described below), the Treaty System includes the recommendations, measures, decisions and resolutions of the Consultative Meetings relating to matters such as:
scientific cooperation;
protection of the Antarctic environment;
conservation of plants and animals;
preservation of historic sites;
designation and management of protected areas;
management of tourism;
information exchange;
collection of meteorological data;
hydrographic charting;
logistic cooperation; and
communications and safety.
The Treaty Parties have put in place rules relating to specific issues. The development of these agreements has allowed the implementation, with greater precision, of legally binding provisions for the regulation of activities in Antarctica.

Project Work: Carlos Landoni, Valentìn Delauro y Paola Fernandez

Project Work: Carlos Landoni, Valentìn Delauro y Paola Fernandez

Antarctica

1) Climate;
2) Flora;
3) Fauna;
4) Territories Claims;
5) History;
6) Natural Resources;
7) The Antarctic Treaty


1) Climate
Antarctica is classified into three basic climate regions: the peninsula, coastal regions, and the interior.
Antarctic Peninsula Reaching farther north than any other part of the continent, the peninsula has the most moderate climate with its warmer temperatures and increased precipitation. Antarctica's wildlife is more dominant in this region. Here, millions of seabirds, and hundreds of thousands of marine mammals, come to breed and feed in the summer months. Although the peninsula has milder temperatures than the rest of the continent, it sustains the fiercest winds, with gusts recorded as high as 200 mph.
Coastal Regions
The coastal regions are a balance between the Antarctic peninsula and the interior. The coasts are milder in temperature than the interior, and receive less precipitation that the peninsula. In the summer, warm ocean currents give this area a more moderate climate, but as winter approaches and the waters freeze, ice grows and the shoreline quickly cools. Coastal temperatures drop much lower than the peninsula. These regions rarely see rainfall, rather their precipitation usually occurs in the form of snow.

Antarctic Interior
The coldest part of the continent is found in the interior. It is categorized primarily by its extreme cold and lack of precipitation. The coldest temperature ever recorded was at the Vostok research station, east of the South Pole; in July, 1983 the temperature reached -129 degrees Fahrenheit, creating a new world low. The sun stays below the horizon beginning in March and lasting through September. During these winter months the interior is almost in complete darkness with zero solar radiation to help heat the surface. Far away from the ocean, the interior receives no warming effects from the waters like the coastal regions and peninsula. Indirect sunrays and high elevation also add to the chilling temperatures of Antarctica's interior.



2) Flora

Lichens
Of all the plants, lichens are best adapted to survive in the harsh polar climate. Some lichens have even been found only about 400 km from the South Pole. Lichens have proliferated in Antarctica mainly because there is little competition from mosses or flowering plants and because of their high tolerance of drought and cold. The peculiarity of lichens is that they are not one homogeneous organism but a symbiosis of two different partners, a fungus and an alga. The fungus part supplies the plant with water and nutritious salt, meanwhile the alga part organic substance, like carbohydrate produce. With this ideal "job-sharing", lichens can survive the hardest conditions. Far from the border of highly developed plants, lichens are the pioneers of the vegetation. Lichens aren’t only frugal and robust, they jug out because of their very low sensibility against frost. Some lichens, in an experiment, survived a bath in liquid nitrogen at minus 195 degrees. On icy rock, lichens have the same strategy as plants have developed in the sand of the Sahara: they form an "oasis". Like in the desert they miss water. They have only a chance to survive, if they settle in an area with a convenient, damp microclimate. Since what stops lichens to spread over the whole of Antarctica is not so much the big cold as the lack of water. For this reason they don’t settle in a place with the most sunshine, but in recesses and cracks between rocks. They like scanty soils, created by weathered rocks. They often quicken this process with secretion of acid. Snowflake are captured in the cracked rock and smelt on the dark lichens, they can absorb the vitally liquid. Especially unfavourable conditions are in the "dry valley" of East Antarctica, where big coldness and low snowfall meet. But even there scientists have found a dark cover on the north side of some rocks, which prove to be lichens. Under the microscope it was shown that the lichens penetrate the upper coat of the rock. With the dark colour the lichens absorb more light. This strategy enables the lichens to scrape a humble living in that quite high southern latitude.


Mosses Only a small number of moss species are found in Antarctica. Extensive fields occur in a few places on this continent and these are rarely more than 100 mm deep, even in the most favourable areas where there is shelter and plenty of water. Short moss turf and cushion moss is found most frequently in sandy and gravelly soils. No extensive peat formations are to be found. Mosses, like lichens, gather in colonies which make them possible to collect and retain more water. They also lose less by evaporation and show a marked ability to use water rapidly whenever it becomes available. Mosses have also become well adapted to the almost continuous light during the long days of a polar summer. One Antarctic moss, Bryum argenteum, produces more energy by photosynthesis in low light at 5°C than it does at 15°C, or higher. Photosynthesis can start within a few hours of thawing after a prolonged period of freezing, and almost immediately following short periods.
Algae More than 300 species of non-marine algae have been found in Antarctica. These very simple plants take many diverse forms and a few have become adapted to living in difficult polar environments. Blue-green and other algae are found growing in damp sand and gravel around lakes and tarns, along meltwater streams or in low-lying areas, where snowdrifts or seepage may collect. Some such as Prasiola crispa can tolerate high levels of nutrients and are found near bird colonies. Others – the snow algae - may form extensive and spectacular red, yellow or green patches in areas of permanent snow. Recent studies have shown that some blue-green algae live inside rocks in dry valleys. Commonly they are found under stones, particularly light-coloured quartz stones, where the microclimate is more favourable than in the surrounding sand or soil. Together with lichens, they are the only living things in a barren landscape.
3) Fauna
Antarctic Birds Millions of seabirds breed along the coast and offshore islands of Antarctica. To survive in the biting environment, Antarctic birds have waterproof plumage, and large compact bodies with a dense layer of fat under their skin. There are nineteen species of seabirds that breed along the continent. Due to the shortage of snow-free nesting regions, most seabirds tend to procreate in large, impressive concentrations making for ideal viewing conditions for the bird enthusiasts. The birds will migrate north as the summer months come to an end, spending the winter in more temperate climates.
Penguins One of Antarctica's most familiar wildlife, penguins are considered by many to be the continent's signature species. They spend over 75% of their lives as sea where they are most comfortable. Their bodies are designed for swimming. Powerful paddle muscles and a compact hydrodynamic body shape allow penguins to swim up to 25 mph. Impressive and elegant in the water, by contrast penguins awkwardly waddle and hop once ashore. While seventeen species of penguins can be found in the subantarctic regions - including coastal islands - only four types of the flightless birds breed on the continent itself: the Emperor, Adelie, Chinstrap, and Gentoo penguins.
Antarctic Seals Much of the early exploration of Antarctica and the Southern Ocean was do to the search for new seal communities. During the 19th and 20th century, many seals were hunted for their valuable skins and oils. Entire populations of species were driven to the brink of extinction. Thankfully, today, the seals are protected by a collection of agencies, and their numbers have continued to thrive. Because of the nutrient-rich feeding regions, and the lack of polar bears, the Antarctic has a much larger seal population than the Arctic. Most of their life is spent in water, but seals must return to land to breed. The best locations to view their breeding grounds are on the pack ice surrounding Antarctica, or along the coastal shores of the northern islands.

Whales Whales are divided into two main groups: toothed and baleen. The only toothed whales found in the Antarctic are the Orca and the Sperm whale, while a variety of baleen whales have been sited: Blue, Fin, Humpback, Minke, and Southern Right. Unlike the other wildlife of Antarctica, whales do not breed in the region. However, they do take advantage of the nutrient-filled waters in the austral summer, traveling great distances from their temperate breeding waters in the north. Like seals, several species of whales were hunted until near extinction in the mid-1900s. While regulations have been placed on whaling activities, these magnificent giants have not seen their populations recover as well as the seals. Today, the entire area surrounding Antarctica is recognized as a whale sanctuary.
4) Territories Claims
5) History
The idea of a large southern continent first appeared in the Greek writings of both Pythagoras and Aristotle. It was believed the earth would topple if a sizable landmass did not exist to balance out the northern continents. Today, we refer to that region as Antarctica. Although Captain James Cook was the first recorded explorer to cross the Antarctic Circle in 1773, he was not the first to see Antarctica's landmass. That acclaim would go to Russian Fabian van Bellinshausen fifty years later. Cook's accounts of the large seal and whale populations, however, helped influence further exploration of the Southern Ocean from sealers in search of the mammals' valued skins. In the 19th century over one thousand sealing ships traveled to the Antarctic regions and its shoreline. In the early 20th century, reaching the South Pole became a top priority for explorers. The first expeditions to actually declare the South Pole as their primary purpose were led by Robert F. Scott in 1902, and Irishman Ernest Shackleton in 1908. Neither would reach their desired destination, but Shackleton came frustratingly close, just 97 miles from the Pole before terminating his crusade. Shackleton had failed in his quest for the South Pole, but he returned to the continent in 1914 to claim a new prize: the first crossing on foot of the Antarctic continent. With a crew of 27, they set sail in early December. A month into the expedition, their ship, Endurance, was trapped and slowly crushed by pack ice. Salvaging what supplies they could, the crew was forced to abandon the ship, and struggle to stay alive in one of the most inhospitable environments in the world. The men would endure sub-zero temperatures and starvation for nearly 20 months, with no communication to the outside world. Incredibly, not a single man would be lost. Shackleton's journey of survival would become one of the most noted in Antarctica's history. Interest in Antarctica continued through the World Wars and into the Cold War. At that time, an American training facility was created to give US troops experience in polar conditions. In early spring of 1954, the first permanent scientific station was established by the Australian National Antarctic Research Expeditions. No single nation controls Antarctica, nor does the continent have any nations of its own. The Antarctic Treaty governs Antarctica. Originally signed in 1961 by 12 nations (Argentina, Australia, Belgium, Chile, French Republic, Japan, New Zealand, Norway, Union of South Africa, Union of Soviet Socialist Republics, United Kingdom of Great Britain and Northern Ireland, and United States of America) it now contains the signature of 44 countries. The treaty recognizes Antarctica's unique position on the planet as a shared environment to be used for peaceful purposes, and international cooperative scientific research. Together, Antarctica would be used in the interests of all human progress and to better humankind.
6) Natural Resources
IceOne of Antarctica's most important resources is ice. It is said that Antarctica's ice accounts for 90% of the worlds fresh water. As a resource it has potential as a fresh water supply. Some people have considered towing icebergs from Antarctica to parts of the world in need of fresh water. At present the delivery costs make these ventures unprofitable. Another possible use of the ice on Antarctica is as a long term deep freeze storage site for grain and other foods. Again the costs of shipping and handling are prohibitive. CoalThere are coal deposits found along the coast of Antarctica. It is also very wide spread throughout the Transantarctic Mountains. These deposits were formed between 35 million and 55 million years ago when Antarctica was covered by ancient swamps. Coal forms in swamps as plants die and are buried before they can be completely decomposed. They are then covered by other sediments such as sand and mud. This burial allows the hydrocarbons in the coal to be preserved for future generations to use. Coal is used as a source of direct heat and also to generate electricity incoal burning power plants. The main problem of developing coal in Antarctica is that the cost of mining and delivering the coal is so much higher than the cost of coal in the rest of the world market. It may bepossible for coal to be used in some small research stations for a source of heat. PetroleumPetroleum deposits are formed when plants and small animal remains are buried in a marine environment by sand and mud. These remains then build up as hydrocarbons and are trapped by a layer of rock that the hydrocarbons cannot pass through. These cap rocks then store the petroleum underground until it is pumped out by wells. At this time there has been no petroleum exploration attempted and there are no known petroleum resources in Antarctica. Most of the speculation about petroleum in Antarctica comes from finding petroleum on the other Southern continents which were at one time connected together. The petroleum deposits thought to be on the offshore regions of Antarctica would probably be most feasible to obtain although they would have to be exceptionally large to be considered for exploitation because of the following enormous exploration and development problems: Deeper water over the continental shelves;The presence of sea ice and icebergs;Short work season and hostile climate. Comparisons with other Gondwana continents suggest the existence of petroleum reserves in the interior of Antarctica. But these lie below the thick ice, ruling out development. This is due not only to the thickness of the ice but also the fact that it is sliding slowly towards the coast. Metallic MineralsMineral resources have not been found in great quantities so far due to the small amount of rock that is exposed. It is believed that since the other continents that were once attached to Antarctica to form Gondwana have metallic and nonmetallic minerals, that Antarctica probably has similar minerals. It is also known that rock layers such as those in Antarctica commonly contain large amounts of cobalt, chromium, nickel, vanadium, copper, iron and platinum group minerals. The search for sizable concentrations of metallic minerals below the ice will be a difficult prospecting venture which will require costly geophysical and geochemical surveying and core drilling. Geologists have found small deposits of minerals in Antarctica but these deposits are low in quality and occur in widely scattered places. The peninsula seems to have the highest probability of containing economic base-metal deposits. HydrothermalWhen fluids such as water are heated by the earth's interior, they can carry dissolved minerals in their fluid state such as quartz, gold, etc. When the solution of liquid and dissolved minerals cools in a new environment, the minerals are deposited as a solid. (The same way that candy forms crystals as it cools and hardens.) Magmatic SegregationAs liquid rock (magma) cools, the minerals in it separate. This is because the minerals have different densities and will separate with the denser minerals towards the bottom. (Think of how a bottle of Italian dressing separates into layers.) This separates the minerals into different layers resulting in concentrations of minerals in different places as the magma cools and hardens. SedimentationAs the earth is worn down and broken into pieces by wind, water, ice and other weathering processes, the pieces of the earth are carried by water into the oceans where they are deposited in layers. Since the pieces are different sizes and have different solubilities in water, they settle to the bottom and form different layers. This results in concentrations of the minerals separated into layers.
7) The Antarctic Treaty
The Antarctic Treaty was signed in 1959 by the 12 countries which had Antarctic stations during the International Geophysical Year (1957-58). These 'original signatories' were Argentina, Australia, Belgium, Chile, France, Japan, New Zealand, Norway, South Africa, United Kingdom, the United States and the USSR. The Treaty came into operation in 1961, and since then a further 14 countries have joined the original 12 as "Consultative Parties", i.e. 26 nations have full voting rights at meetings. Any Party to the Treaty which shows a genuine interest in Antarctica by conducting scientific research activities is entitled to become a Consultative Party. All decisions are made by consensus, i.e. all Consultative Parties must agree. The Treaty is open to any member of the United Nations and aims to further the principles of the UN Charter. It stipulates that the Antarctic should forever be used for peaceful purposes and prohibits military activity. Freedom of scientific research is guaranteed, and inspections can be carried out to ensure the Treaty is being observed. It applies to the area south of 60°South latitude. Seven nations claim territory, or 'sovereignty rights', in Antarctica: Argentina, Australia, Chile, France, New Zealand, Norway, and the United Kingdom, and two reserve the right to claim territory: the United States and Russia. These claims are not universally recognised and the Antarctic Treaty puts them legally on-hold to prevent disputes. Antarctic Treaty meetings are held every year, and deal with a range of scientific, environmental and operational issues related to cooperative activities in Antarctica.

Tema: Antarctica - Profesora: Stella Maris Goldenzweig

Students: Romina Sanchez
Sofìa Giuso

History
The history of Antarctica emerges from early Western theories of a vast continent, known as Terra Australis, believed to exist in the far south of the globe. The rounding of the Cape of Good Hope and Cape Horn in the 15th and 16th centuries proved that Terra Australis Incognita ("Unknown Southern Land"), if it existed, was a continent in its own right. In 1773 James Cook crossed the Antarctic Circle for the first time but although he discovered nearby islands, he did not catch sight of Antarctica itself.
In 1820, several expeditions claimed to have been the first to have sighted Antarctica. The first landing was probably just over a year later when American Captain John Davis, a sealer, set foot on the ice. Once the North Pole had been reached in 1909, several expeditions attempted to reach the South Pole. Many resulted in injury and death. The Norwegian Roald Amundsen finally claimed the prize following a dramatic race with the Briton Robert Falcon Scott in December 1911.
The search for Terra Australis Incognita
In the Western world, belief in a Terra Australis—a vast continent located in the far south of the globe to "balance" out the northern lands of Europe, Asia and North Africa—had existed for centuries. Aristotle had postulated a symmetry of the earth, which meant that there would be equally habitable lands south of the known world. The Greeks suggested that these two hemispheres, north and south, were divided by a 'belt of fire’
It was not until Prince Henry the Navigator began in 1418 to encourage the penetration of the torrid zone in the effort to reach India by circumnavigating Africa that the exploration of the southern hemisphere began. In 1473 Portuguese navigator Lopes Gonçalves proved that the equator could be crossed, and cartographers and sailors began to assume the existence of another, temperate continent to the south of the known world.
The doubling of the Cape of Good Hope in 1487 by Bartholomew Diaz first brought explorers within touch of the Antarctic cold, and proved that there was an ocean separating Africa from any Antarctic land that might exist. Ferdinand Magellan, who passed through the Straits of Magellan in 1520, assumed that the islands of Tierra del Fuego to the south were an extension of this unknown southern land, and it appeared as such on a map by Ortelius: Terra australis recenter inventa sed nondum plene cognita ("Southern land recently discovered but not yet known"). In 1513, the Ottoman Turkish admiral Piri Reis also drew a map that has been said to show part of the Antarctic continent.
The doubling of Cape Horn by Drake in 1578 proved that the Tierra del Fuego archipelago was of small extent and that any continent which lay to the south must be within the region of perpetual winter. European geographers connected the coast of Tierra del Fuego with the coast of New Guinea on their globes and allowing their imaginations to run riot in the vast unknown spaces of the south Atlantic, south Indian and Pacific oceans. They sketched the outlines of the Terra Australis Incognita ("Unknown Southern Land"), a vast continent stretching in parts into the tropics. The search for this great south land or Third World was a leading motive of explorers in the 16th and the early part of the 17th centuries.
Schouten and Le Maire rediscovered the southern extremity of Tierra del Fuego and named it Cape Horn in 1615. Quirós in 1606 took possession for the king of Spain all of the lands he had discovered in Australia del Espiritu Santo (the New Hebrides) and those he would discover "even to the Pole". Tasman in 1642 showed that New Holland (Australia) was separated by sea from any continuous southern continent.
Voyagers round the Horn frequently met with contrary winds and were driven southward into snowy skies and ice-encumbered seas; but so far as can be ascertained none of them before 1770 reached the Antarctic Circle, or knew it, if they did. The story of the discovery of land in 64° S. by Dirk Gerritz on board the Blijde Boodschap in 1599 was shown to be the result of a mistake of a commentator, Kasper Barlaeus, in 1622. A similar story of sighting "snow-covered mountains" beyond the 64° S in 1603 is told of the Spanish Gabriel de Castilla.
Better documented is the visit to South Georgia by Anthony de la Roché in 1675, the first ever discovery of land south of the Antarctic Convergence. Soon after the voyage cartographers started to depict on their maps ‘Roché Island’, honoring the discoverer. James Cook was aware of la Roché's discovery when surveying and mapping the island in 1775.
It may safely be said that all the navigators who fell in with the southern ice up to 1750 did so by being driven off their course by chance. An exception may perhaps be made in favor of Halley's voyage in HMS Paramour for magnetic investigations in the South Atlantic when he met the ice in 52° S. in January 1700; but that latitude was his farthest south. A determined effort on the part of the French naval officer Pierre Bouvet to discover the South Land described by a half legendary sieur de Gonneyville resulted only in the discovery of Bouvet Island in 54°10′ S., and in the navigation of 48° of longitude of ice-cumbered sea nearly in 55° S. in 1730.
In 1771, Yves Joseph Kerguelen sailed from France with instructions to proceed south from Mauritius in search of "a very large continent." He lighted upon a land in 50° S. which he called South France, and believed to be the central mass of the southern continent. He was sent out again to complete the exploration of the new land, and found it to be only an inhospitable island which he renamed in disgust the Isle of Desolation, but in which posterity has recognized his courageous efforts by naming it Kerguelen Land.
South of the Antarctic Circle
The obsession of the undiscovered continent culminated in the brain of Alexander Dalrymple, the brilliant and erratic hydrographer who was nominated by the Royal Society to command the Transit of Venus expedition to Tahiti in 1769. The command of the expedition was given by the admiralty to Captain James Cook. Sailing in 1772 with the Resolution, a vessel of 462 tons under his own command and the Adventure of 336 tons under Captain Tobias Furneaux, Cook first searched in vain for Bouvet Island, then sailed for 20 degrees of longitude to the westward in latitude 58° S, and then 30° eastward for the most part south of 60° S, a higher southern latitude than had ever been voluntarily entered before by any vessel. On January 17, 1773 the Antarctic Circle was crossed for the first time in history and the two ships reached 67° 15' S by 39° 35' E, where their course was stopped by ice.
Cook then turned northward to look for French Southern and Antarctic Lands, of the discovery of which he had received news at Cape Town, Cook reached the assigned latitude 10° too far east and did not see it. He turned south again and was stopped by ice in 61° 52′ S by 95° E and continued eastward nearly on the parallel of 60° S to 147° E. On March 16, the approaching winter drove him northward to rest in New Zealand and the tropical islands of the Pacific. In November 1773, Cook left New Zealand, having parted company with the Adventure, and reached 60° S by 177° W, whence he sailed eastward keeping as far south as the floating ice allowed. The Antarctic Circle was crossed on December 20 and Cook remained south of it for three days, being compelled after reaching 67° 31′ S to stand north again in 135° W.
A long detour to 47° 50′ S served to show that there was no land connection between New Zealand and Tierra del Fuego. Turning south again, Cook crossed the Antarctic Circle for the third time at 109° 30′ W before his progress was once again blocked by ice four days later at 71° 10′ S by 106° 54′ W. This point, reached on January 30, 1774, was the farthest south attained in the 18th century. With a great detour to the east, almost to the coast of South America, the expedition regained Tahiti for refreshment. In November 1774, Cook started from New Zealand and crossed the South Pacific without sighting land between 53° and 57° S to Tierra del Fuego; then, passing Cape Horn on December 29, he discovered the Isle of Georgia and Sandwich Land, the only ice-clad land he had seen, before crossing the South Atlantic to the Cape of Good Hope between 55° and 60°. He thereby laid open the way for future Antarctic exploration by exploding the myth of a habitable southern continent. Cook's most southerly discovery of land lay on the temperate side of the 60th parallel, and he convinced himself that if land lay farther south it was practically inaccessible and of no economic value.
First sighting of land
The first land south of the parallel 60° south latitude was discovered by the Englishman William Smith, who sighted Livingston Island on February 19, 1819. Few months later Smith returned to explore the other islands of the South Shetlands archipelago, landed on King George Island, and claimed the new territories for Britain.
In the meantime, the Spanish Navy ship San Telmo sank in September 1819 when trying to cross Cape Horn. Parts of her wreckage were found months later by sealers on the north coast of Livingston Island (South Shetlands). It is unknown if some survivor managed to be the first setting foot on these Antarctic islands.
The first confirmed sighting of Antarctica cannot be accurately attributed to one single person. It can, however, be narrowed down to three individuals. According to various sources, three men all sighted Antarctica within days or months of each other: Fabian von Bellingshausen, a captain in the Russian Imperial Navy; Edward Bransfield, a captain in the British navy; and Nathaniel Palmer, an American sealer out of Stonington, Connecticut. It is certain that on January 28, 1820 (New Style), the expedition led by Fabian von Bellingshausen and Mikhail Petrovich Lazarev on two ships reached a point within 20 miles (40 km) of the Antarctic mainland and saw ice-fields there. On January 30, 1820, Bransfield sighted Trinity Peninsula, the northernmost point of the Antarctic mainland, while Palmer sighted the mainland in the area south of Trinity Peninsula in November 1820. Bellingshausen's expedition also discovered Peter I Island and Alexander I Island, the first islands to be discovered south of the circle.
Exploration
Only slightly more than a year later, the first landing on the Antarctic mainland was arguably by the American Captain John Davis, a sealer, who claimed to have set foot there on February 7, 1821, though this is not accepted by all historians.
On December 1821, Nathaniel Palmer, an American sealer looking for seal breeding grounds, sighted what is now known as the Antarctic Peninsula, located in the continent's northwestern quadrant. In 1823, James Weddell, a British sealer, sailed into what is now known as the Weddell Sea.
The first person to realize that he had actually discovered a whole continent was Charles Wilkes, the commander of a United States Navy expedition. His 1840 voyage discovered what is now known as Wilkes Land, on the southeast quadrant of the continent.
After the North Magnetic Pole was located in 1831, explorers and scientists began looking for the South Magnetic Pole. One of the explorers, James Clark Ross, a British naval officer, identified its approximate location, but was unable to reach it on his trip in 1841. Commanding the British ships Erebus and Terror, he braved the pack ice and approached what is now known as the Ross Ice Shelf, a massive floating ice shelf over 100 feet (30 m) high. His expedition sailed eastward along the southern Antarctic coast discovering mountains which were since named after his ships: Mount Erebus, the most active volcano on Antarctica, and Mount Terror.
The first documented landing on the mainland of East Antarctica was at Victoria Land by the American sealer Mercator Cooper on January 26, 1853.
In 1897, an expedition led by Belgian Adrian de Gerlache left Antwerp, Belgium for Antarctica. The multi-national crew included a Romanian zoologist (Emil Racoviţă), a Polish geologist (Henryk Arctowski), a Belgian navigator/astronomer (George Lecointe), several Norwegians, including Roald Amundsen, and an American surgeon, Dr. Frederick Cook. In 1898, they became the first men to spend winter on Antarctica, when their ship Belgica became trapped in the ice. They became stuck on February 28, 1898, and only managed to get out of the ice on March 14, 1899. During their forced stay, several men lost their sanity, not only because of the Antarctic winter night and the endured hardship, but also because of the language problems between the different nationalities. A year later a British expedition commanded by Norwegian Carstens Borchgrevink became the first to intentionally spend winter on the continent itself.
British National Antarctic Expedition (Discovery)
The British National Antarctic Expedition (1901–1904), led by Robert Falcon Scott, came to within 857 km (463 nautical miles) of the South Pole from its base at McMurdo Sound.
Scottish National Antarctic Expedition
In 1903, the Scottish National Antarctic Expedition established Osmond House, a meteorological observatory on Laurie Island in the South Orkneys. A year later, ownership of the base was passed to Argentina and it was renamed Orcadas Base. It is the continent's oldest permanent base, and, until World War II, the only one present.
British Imperial Antarctic Expedition (Nimrod)
Ernest Shackleton, who had been a member of Scott's expedition, organized and led the British Imperial Antarctic Expedition (1907-09), again with the primary objective of reaching the South Pole. It came within 180 km (97 nautical miles) before having to turn back. during the expedition, Shackleton discovered the Beardmore Glacier and was the first to reach the polar plateau. Parties led by T. W. Edgeworth David also became the first to climb Mount Erebus and to reach the South Magnetic Pole.
Race to the Pole (Fram and Terra Nova)
On December 14, 1911, a party led by Norwegian polar explorer Roald Amundsen from the ship Fram became the first to reach the South Pole, using a route from the Bay of Whales (his camp Polheim and up the Axel Heiberg Glacier. Amundsen was followed by Robert Falcon Scott from the Terra Nova over a month later, using the route pioneered by Shackleton. Scott's party later died on the return journey after being delayed by a series of accidents, bad weather, and the declining physical condition of the men. The Amundsen-Scott South Pole Station was later named after these two men.
Imperial Trans-Antarctic Expedition (Endurance)
The Imperial Trans-Antarctic Expedition of 1914, led by Ernest Shackleton, set out to cross the continent via the pole, but their ship, the Endurance, was trapped and crushed by pack ice before they even landed. The expedition members survived after an epic journey on sledges over pack ice to Elephant Island. Then Shackleton and five others crossed the Southern Ocean, in an open boat called James Caird, and then trekked over South Georgia to raise the alarm at the whaling station Grytviken.
Exploration by air: 1930s to 1950s
US Navy Rear Admiral Richard Evelyn Byrd led five expeditions to Antarctica during the 1930s, 1940s, and 1950s. He overflew the South Pole with pilot Bernt Balchen on November 28 and 29, 1929, to match his overflight of the North Pole in 1926. Byrd's explorations had science as a major objective and pioneered the use of aircraft on the continent. Byrd is credited with doing more for Antarctic exploration than any other explorer. His expeditions set the scene for modern Antarctic exploration and research.
In 1946, Admiral Byrd and more than 4,700 military personnel returned to Antarctica in an expedition called Operation High Jump. Reported to the public as a scientific mission, the details were kept secret and it may have actually been training or testing mission for the military. The expedition was, in both military and scientific planning terms, put together very quickly. The group contained an unusually high amount of military equipment, including an aircraft carrier, submarines, military support ships, assault troops and military vehicles. The expedition was planned to last for eight months but was unexpectedly terminated after only two months. With the exception of some eccentric entries in Admiral Byrd's diaries, no real explanation for the early termination has ever been officially given.
It was not until October 31, 1956 that anyone reached the South Pole again; on that day US Navy Rear Admiral George J. Duffel and others successfully landed a R4D Skytrain (Douglas DC-3) aircraft.
During the International Geophysical Year of 1957, a large number of expeditions to the Antarctic were mounted.
Commonwealth Trans-Antarctic Expedition
In 1956, a United States Navy expedition set up the first permanent based at the South Pole, Amundsen-Scott South Pole Station, by airlift, to support the International Geophysical Year. In 1958, Edmund Hillary's party in the New Zealand party of the Commonwealth Trans-Antarctic Expedition became the third group in history to reach the South Pole by land, and the first group of motor vehicles to reach the pole. The British team led by Vivian Fuchs, met them at the pole shortly afterwards. The expedition completed the first overland crossing of the continent by land via the South Pole. New Zealand mountaineer Sir Edmund Hillary reached the Pole in early January 1958 using farm tractors equipped for polar travel, the first party since Scott's to reach the South Pole overland. Hillary was laying supply depots as part of the Commonwealth Trans-Antarctic Expedition and in typical Hillary style "detoured" to the pole because the trip had gone well. British explorer Sir Vivian Fuchs then arrived at the Pole from the opposite direction later in January, meeting Hillary. Fuchs continued on, making use of the provisions that Hillary had stored, and on March 2 succeeded in reaching Scott Base, completing the overland transpolar crossing that Shackleton had envisaged.

Climate
The blue ice covering Lake Fryxell, in the Transantarctic Mountains, comes from glacial melt water from the Canada Glacier and other smaller glaciers.
Antarctica is the coldest place on Earth. At the 3-kilometer (2 mi)-high Vostok Station in Antarctica, scientists recorded Earth's lowest temperature: −89 °C (−129 °F). As a comparison, this is 11 degrees colder than subliming dry ice. Antarctica is a frozen desert with little precipitation; the South Pole itself receives less than 10 centimeters (4 in) per year, on average. Temperatures reach a minimum of between −80 °C and −90 °C (−112 °F and −130 °F) in the interior in winter and reach a maximum of between 5 °C and 15 °C (41 °F and 59 °F) near the coast in summer. Sunburn is often a health issue as the snow surface reflects almost all of the ultraviolet light falling on it. Eastern Antarctica is colder than its western counterpart because of its higher elevation. Weather fronts rarely penetrate far into the continent, leaving the center cold and dry. Despite the lack of precipitation over the central portion of the continent, ice there lasts for extended time periods. Heavy snowfalls are not uncommon on the coastal portion of the continent, where snowfalls of up to 1.22 meters (48 in) in 48 hours have been recorded.
At the edge of the continent, strong katabatic winds off the polar plateau often blow at storm force. In the interior, however, wind speeds are typically moderate. During summer, more solar radiation reaches the surface during clear days at the South Pole than at the equator because of the 24 hours of sunlight each day at the Pole.
Antarctica is colder than the Arctic for two reasons. First, much of the continent is more than 3 kilometers (2 mi) above sea level, and temperature decreases with elevation. Second, the Arctic Ocean covers the north polar zone: the ocean's relative warmth is transferred through the icepack and prevents temperatures in the Arctic regions from reaching the extremes typical of the land surface of Antarctica.
Given the latitude, long periods of constant darkness or constant sunlight create climates unfamiliar to human beings in much of the rest of the world. The aurora australis, commonly known as the southern lights, is a glow observed in the night sky near the South Pole created by the plasma-full solar winds that pass by the Earth. Another unique spectacle is diamond dust, a ground-level cloud composed of tiny ice crystals. It generally forms under otherwise clear or nearly clear skies, so people sometimes also refer to it as clear-sky precipitation. A sun dog, a frequent atmospheric optical phenomenon, is a bright "spot" beside the true sun.
Source www.wikipedia.org

Lógica: Prof. Maria Del Carmen Ramos

INTRODUCCION

Hay muchos razonamientos cuya validez o invalidez no pueden decidirse con el análisis de la lógica proposicional, por consiguiente es necesario un análisis mas fino de la forma lógica de las proposiciones atómicas.
El siguiente razonamiento válido : Todos los gatos son mamíferos. Michi es un gato. Por lo tanto, Michi es mamífero. Este razonamiento resulta inválido para la lógica proposicional, ya que su condicional asociado tiene una forma no tautológica . Esto se debe a que la lógica proposicional analiza las proposiciones compuestas en proposiciones mas simples hasta llegar a las atómicas, deteniéndose allí.
Para estudiar razonamientos como el expresado es necesario un análisis más fino de la forma lógica de las proposiciones atómicas.
El objetivo del trabajo será analizar la lógica de predicados que constituye una ampliación de la lógica proposicional. Esta lógica establece una nítida distinción entre proposiciones singulares y generales y también diferencia a las universales de las existenciales. Estas distinciones no sólo tienen importancia en la teoría del razonamiento, sino implicaciones científicas y filosóficas.
La lógica de predicados supone la lógica proposicional; tiene una mayor riqueza para expresar proposiciones y para analizar razonamientos.
Pensar con claridad no es algo que se produzca natural o fácilmente sino algo que debe aprenderse y practicarse.

Trabajo Practico de Bonato, Brieva, Morales

Project Work
English

SUBJECT: The ozone hole in the South Pole

TEACHER: Stella Maris Goldenzweig

SUBMITTED DATE: 25-07-2008

COURSE: 5º 2º

MEMBERS: Bonato, María Agustina
Brieva, Melisa
Morales, Paula

Ozone depletion

Ozone depletion describes two distinct, but related observations: a slow, steady decline of about 4 percent per decade in the total amount of ozone in Earth's stratosphere since the late 1970s; and a much larger, but seasonal, decrease in stratospheric ozone over Earth's polar regions during the same period. The latter phenomenon is commonly referred to as the ozone hole. In addition to this well-known stratospheric ozone depletion, there are also tropospheric ozone depletion events, which occur near the surface in Polar Regions during spring.
The detailed mechanism by which the polar ozone holes are formed is different from that for the mid-latitude thinning, but the most important process in both trends is catalytic destruction of ozone by atomic chlorine and bromine.[1] The main source of these halogen atoms in the stratosphere is photodissociation of chlorofluorocarbon (CFC) compounds, commonly called freons, and of bromofluorocarbon compounds known as halons. These compounds are transported into the stratosphere after being emitted on the surface.
It is suspected that a variety of biological consequences such as increases in skin cancer, damage to plants, and reduction of plankton populations in the ocean's photic zone may result from the increased UV exposure due to ozone depletion.



The Montreal Protocol on Substances That Deplete the Ozone Layer

This protocol is an international treaty designed to protect the ozone layer by phasing out the production of a number of substances believed to be responsible for ozone depletion. The treaty was opened for signature on September 16, 1987 and entered into force on January 1, 1989 followed by a first meeting in Helsinki, May 1989. Since then, it has undergone seven revisions, in 1990 (London), 1991 (Nairobi), 1992 (Copenhagen), 1993 (Bangkok), 1995 (Vienna), 1997 (Montreal), and 1999 (Beijing). Due to its widespread adoption and implementation it has been hailed as an example of exceptional international co-operation with Kofi Annan quoted as saying it is “Perhaps the single most successful international agreement to date…”



Observations on ozone layer depletion

The most pronounced decrease in ozone has been in the lower stratosphere. However, the ozone hole is most usually measured not in terms of ozone concentrations at these levels (which are typically of a few parts per million) but by reduction in the total column ozone, above a point on the Earth's surface, which is normally expressed in Dobson units, abbreviated as "DU". Marked decreases in column ozone in the Antarctic spring and early summer compared to the early 1970s and before have been observed using instruments such as the Total Ozone Mapping Spectrometer (TOMS).
Reductions of up to 70% in the ozone column observed in the austral (southern hemispheric) spring over Antarctica and first reported in 1985 (Farman et al 1985) are continuing. Through the 1990s, total column ozone in September and October have continued to be 40–50% lower than pre-ozone-hole values. In the Arctic the amount lost is more variable year-to-year than in the Antarctic. The greatest declines, up to 30%, are in the winter and spring, when the stratosphere is colder.
Reactions that take place on polar stratospheric clouds (PSCs) play an important role in enhancing ozone depletion. PSCs form more readily in the extreme cold of Antarctic stratosphere. This is why ozone holes first formed are deeper, over Antarctica. Early models failed to take PSCs into account and predicted a gradual global depletion, which is why the sudden Antarctic ozone hole was such a surprise to many scientists.
In middle latitudes it is preferable to speak of ozone depletion rather than holes.
Ozone depletion also explains much of the observed reduction in stratospheric and upper tropospheric temperatures. The source of the warmth of the stratosphere is the absorption of UV radiation by ozone, hence reduced ozone leads to cooling. Some stratospheric cooling is also predicted from increases in greenhouse gases such as CO2; however the ozone-induced cooling appears to be dominant.



The ozone hole and its causes

The Antarctic ozone hole is an area of the Antarctic stratosphere in which the recent ozone levels have dropped to as low as 33% of their pre-1975 values. The ozone hole occurs during the Antarctic spring, from September to early December, as strong westerly winds start to circulate around the continent and create an atmospheric container. Within this polar vortex, over 50% of the lower stratospheric ozone is destroyed during the Antarctic spring.
The polar stratospheric clouds form during winter, in the extreme cold. Polar winters are dark, consisting of 3 months without solar radiation (sunlight). Not only lack of sunlight contributes to a decrease in temperature but also the polar vortex traps and chill air. Temperatures hover around or below -80 °C. These low temperatures form cloud particles and are composed of either nitric acid (Type I PSC) or ice (Type II PSC). Both types provide surfaces for chemical reactions that lead to ozone destruction.
The photochemical processes involved are complex but well understood. The key observation is that, ordinarily, most of the chlorine in the stratosphere resides in stable "reservoir" compounds, primarily hydrogen chloride (HCl) and chlorine nitrate (ClONO2). During the Antarctic winter and spring, however, reactions on the surface of the polar stratospheric cloud particles convert these "reservoir" compounds into reactive free radicals (Cl and ClO). The clouds can also remove NO2 from the atmosphere by converting it to nitric acid, which prevents the newly formed ClO from being converted back into ClONO2.
The role of sunlight in ozone depletion is the reason why the Antarctic ozone depletion is so important during spring. During winter, even though PSCs are at their most abundant, there is no light over the pole to drive the chemical reactions. During the spring, however, the sun comes out, providing energy to drive photochemical reactions, and melt the polar stratospheric clouds, releasing the trapped compounds.
Most of the ozone that is destroyed is in the lower stratosphere, in contrast to the much smaller ozone depletion through homogeneous gas phase reactions, which occurs primarily in the upper stratosphere.
Warming temperatures near the end of spring break up the vortex around mid-December. As warm, ozone-rich air flows in from lower latitudes, the PSCs are destroyed, the ozone depletion process shuts down, and the ozone hole heals.


An ozone hole was first observed in 1956

G.M.B. Dobson (Exploring the Atmosphere, 2nd Edition, Oxford, 1968) mentioned that when springtime ozone levels over Halley Bay were first measured, he was surprised to find that they were ~320 DU, about 150 DU below spring levels, ~450 DU, in the Arctic. These, however, were the pre-ozone hole normal climatological values. What Dobson describes is essentially the baseline from which the ozone hole is measured: actual ozone hole values are in the 150–100 DU range.
The discrepancy between the Arctic and Antarctic noted by Dobson was primarily a matter of timing: during the Arctic spring ozone levels rose smoothly, peaking in April, whereas in the Antarctic they stayed approximately constant during early spring, rising abruptly in November when the polar vortex broke down.
The behavior seen in the Antarctic ozone hole is completely different. Instead of staying constant, early springtime ozone levels suddenly drop from their already low winter values, by as much as 50%, and normal values are not reached again until December.



The most important consequence of ozone layer depletion

Since the ozone layer absorbs UVB ultraviolet light from the Sun, ozone layer depletion is expected to increase surface UVB levels, which could lead to damage, including increases in skin cancer. This was the reason for the Montreal Protocol. Although decreases in stratospheric ozone are well-tied to CFCs and there are good theoretical reasons to believe that decreases in ozone will lead to increases in surface UVB, there is no direct observational evidence linking ozone depletion to higher incidence of skin cancer in human beings. This is partly due to the fact that UVA, which has also been implicated in some forms of skin cancer, is not absorbed by ozone, and it is nearly impossible to control statistics for lifestyle changes in the populace.
Ozone, while a minority constituent in the earth's atmosphere, is responsible for most of the absorption of UVB radiation. The amount of UVB radiation that penetrates through the ozone layer decreases exponentially with the slant-path thickness/density of the layer. Correspondingly, a decrease in atmospheric ozone is expected to give rise to significantly increased levels of UVB near the surface.
Increases in surface UVB due to the ozone hole can be partially inferred by radioactive transfer model calculations, but cannot be calculated from direct measurements because of the lack of reliable historical (pre-ozone-hole) surface UV data, although more recent surface UV observation measurement programmes exist (e.g. at Lauder, New Zealand).
Because it is this same UV radiation that creates ozone in the ozone layer from O2 (regular oxygen) in the first place, a reduction in stratospheric ozone would actually tend to increase photochemical production of ozone at lower levels (in the troposphere), although the overall observed trends in total column ozone still show a decrease, largely because ozone produced lower down has a naturally shorter photochemical lifetime. This is destroyed before the concentrations could reach a level which would compensate for the ozone reduction higher up.


Source:
* http://en.wikipedia.org/wiki/Ozone_depletion
* http://www.theozonehole.com/
* http://ozonewatch.gsfc.nasa.gov/

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