mercredi 26 février 2014

SEAS AND OCEANS



seas and oceans

The seas and the oceans are  stretches of water salted, unlike wide and soft rivers such as the lakes, the rivers and the rivers.
The seas and the oceans cover  71 % with the surface of the Earth  and play an essential role in the climatic balance of the environment.
In the Northern hemisphere, the seas and the oceans represent 61 % of surface, against 81 % in the Southern hemisphere (also called "marine" hemisphere).

SEAS

The seas are smaller than the oceans. There are 3 types of seas: closed seas, inland seas and seas of the Mediterranean type.
The closed seas are the Caspian Sea and the sea of Aral (in Asia) and the Dead Sea (in the Middle East). These seas, which do not communicate with any other sea nor any ocean, are fed only by rivers. It is in fact of immense salted lakes; salt is there besides in quantity more significant than in the other seas and oceans.
The inland seas open on other seas. It is the case of the Black Sea or North Sea (which gives on the Baltic) (which communicates with the Mediterranean by the Bosphorus in Turkey). These seas are low depth.
Lastly, the seas of the Mediterranean type  are the largest seas and communicate with oceans, as the Mediterranean (which gives on the Atlantic Ocean), the sea of the Philippines (Pacific Ocean), the Caribbean Sea (Atlantic Ocean) or the sea of Arabia (Indian Ocean).

OCEANS

The oceans have for principal characteristics to be of a surface quite higher than that of the seas and to be delimited by several continents.
The Pacific Ocean is largest of all the oceans (165 million km² approximately, is 300 times the size of France) and deepest (more than 11 000 m to the pit of Mariannes). It is delimited in the east by the American continent and the west by Asia and Oceania.
Second by its surface (more than 80 million km²), the Atlantic Ocean  is delimited in the east by Europe and Africa and in the west by the American continent (North America, Central America and South America).
Lastly, the Indian Ocean  (more than 70 million km²) is almost entirely located in the Southern hemisphere. It is bordered in the east by Oceania and Indonesia, in north by India and the west by Africa.
To these three oceans are added the Arctic Ocean  (also called sea Arctic Glaciale because of its dimensions, "small" for an ocean) and the ocean Glacial the Antarctic  (or Antarctic Ocean).
The principal points of passage  between these oceans are:
the Bering Strait: located between Alaska (in the United States) and Russia, it connects the Pacific Ocean to the Arctic Ocean, in the Northern hemisphere;
the Magellan Strait,  Cape Horn  and  the Drake passage: located at the southern point and Chile, they connect the Pacific Ocean to the Atlantic Ocean, in the Southern hemisphere;
the strait of Bass: located at the south of Australia, it connects the Indian Ocean to the Pacific Ocean, in the Southern hemisphere;
the strait of Torres: located between New Guinea-News-Guinea and Australia, it connects the Indian Ocean to the Pacific Ocean, in the Southern hemisphere;
the course of the Needles: located at the southern point of South Africa, it marks the limit between the Indian Ocean and the Atlantic Ocean, in the Southern hemisphere.

MARINE WATER

The water of the seas and the oceans  is naturally salted. The average content salt (35 grams per liter) varies according to the fresh water arrival: the more there is fresh water, the less there is salt, and conversely.
The temperature of the water of the seas and the oceans varies according to  the depth of water,  the latitude  (position compared to the equator) and of the sun contribution , but also of the importance of  the marine currents. The sea waters of the Caribbean, for example, can reach a temperature of 30 °C, while in the Arctic Oceans and the Antarctic, the surface water is below 0 °C all the year.
The tides are a phenomenon which appears by  the rise  (flow) of water on the coasts then their  descent  (the backward flow). This movement is the consequence of the attraction of the Moon and the Sun  on the Earth. The tides function according to  a periodic rate/rhythm  (one or two tides per day). The amplitude  of the tides is more or less significant (the coefficient goes from 20 to 120) and depends on the seas (of 10 cm at sea the Mediterranean with nearly 20 m in the Atlantic Ocean).
The waves are undulatory movements on the surface of marine water, due to the winds. The waves are littoral when they arrive to the coast. If not, they are oceanic waves: one speaks then about  swell, left bearing of surface water on the open sea. More the spacing between two waves and their rate of travel are significant, more the swell is strong. The highest waves can measure up to 30 m (in the Pacific Ocean).
The marine currents are constant or periodic movements marine water: they are due to the winds or are produced by the descent and the rise of water (indeed, the difference of salinity, temperature and density of water causes this type of movements, in-depth). The importance of the currents is capital for the climatic balance of certain areas of the Earth.
The Gulf Stream, for example, is a current heat: it is born on the coasts from the Gulf of Mexico and goes up the North Atlantic at broad coasts of the North-American continent, under the blast pressure of south-west. Then, it deviates towards the east and joined Western Europe (France in particular) to which it brings soft and wet winters; without this marine current, this part of Europe would have the same climate as Canada.

LIFE AND RESOURCES OF THE SEAS AND THE OCEANS

The marine ecosystem particularly rich and is varied. Indeed, water of the seas and the oceans abounds in life, at the same time vegetable (the vegetable plankton and algae) and animal (the animal plankton, of many invertebrates, the fish, marine mammals). They have  considerable, but also energy resources  living  (the energy of the waves and tides for example, used to produce electricity) and  mineral  (oil and the gas).
For a long time, the man largely exploits these resources: they are for example the activities of  fishing  (become industrial to  the xx E century), of  intensive  trade or exploitation of  oil reservoirs  (at sea of North in particular), etc.
However, this exploitation is not without  dangers:  many fish species are threatened, are in process of extinction or disappeared from the seas and the oceans, and  the marine  water pollution became at certain places of planet a true plague.




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MESOPOTAMIE



Mésopotamie



Mésopotamie is  a historical area of the Middle East. It extends between two rivers,  the Tiger  and Euphrate  —it is besides from there that the area draws its name, which means "between two rivers" in Greek.
Mésopotamie corresponds overall to Iraq, and part of Syria and Iran current. Several significant civilizations of Antiquity lived there. 

CIVILIZATION SUMÉRIENNE

Sumériens live in  the south of Mésopotamie  to the IV E thousand-year-old before our era. Towards 3300 before J-C, they invent  the first written form: the wedge-shaped writing. This discovery is a revolutionist in the evolution of the man; it marks  the passage of prehistory to the history.
Civilization sumérienne is very technically advanced: invention and use of  the wheel, the irrigation,  the potter's wheel,  the plough  and  mathematics. It is as within civilization sumérienne as the first  cities appeared, with imposing architecture. Each city is controlled by a king who would hold his capacity of the gods. Most known are those of Kish, Lagash, Uruk and Ur. One of the most famous sovereigns of this period is legendary Gilgamesh, king d' Uruk to  the xxvii E century before J-C.
Each city seeking to dominate the others, Sumériens are made the war perpetually. Towards 2370 before J-C, a king manages to dominate the other cities and constitutes the first  kingdom of Sumer.

The KINGDOM OF SUMER AND AKKAD

At the same period, more in north in Mésopotamie, people live which adopted the written form of Sumériens. For a long time, the technical richnesses of Sumériens attract their covetousness. And towards 2325 before J-C, king  Sargon the Old one  seizes Sumer. After having founded its capital (Akkad), it  unifies Mésopotamie  and creates the kingdom of Sumer and Akkad. The kingdom declines however, after having fallen to the hands from wandering people.
Two centuries later, king d' Ur creates the prestigious  kingdom of Ur. It is at this period that the ziggourat  of  Ur is built (a pyramidal tower with several degrees). But towards 2004 before J-C, the kingdom of Ur breaks down in its turn under the blow of invasions of Élamites. To  the xx E century before our era, Mésopotamie becomes again a multitude of small rival States which are made the war perpetually.

the door of Ishtar in Babylon

Controlled by king Hammourabi, the city of Babylon benefits from these ceaseless wars. After having overcome the other kings, Hammourabi becomes the sovereign of  the kingdom of Babylon  into 1760 before J-C Babylon, the capital of Mésopotamie reunified, is more in north than the old cities sumériennes. Powerful monarch, Hammourabi makes thrive his kingdom; in particular, he is the author of  the first code of laws  of the history: the code of Hammourabi.
Under the successors of Hammourabi, the invasions begin again; this time, they are Kassites which penetrates in Mésopotamie. In the medium of  the xvi E century before our era, they seize Babylonia and restore the power with their profit of it. The dynasty kassite reign on Babylonia during 400 years. The kings of this civilization thrives are regarded as equal Pharaons of Egypt.

sumptuous court of Assyrie

To the xvi E century before J-C,  the north of Mésopotamie  is with the hands of Assyriens. The principal towns of Assyrie are Assur and Ninive. To  the xiii E century before J-C, under the pressure of migratory movements, Assyriens develop a genuine machine of war. The raids then then the conquest of the close territories, in particular Babylonia begin.
Two centuries later, a new dynasty controls the kingdom of Assyrie: one defines it as the dynasty néo-assyrienne.  Sargon II, whose reign extends from 721 to 705 before J-C, allows the Empire néo-assyrien its greater expansion. The empire is then very vast, in particular including Egypt, placed under protectorate. Sargon II controls from the city of Hard Sharrukin (today Khorsabad, in Iraq). Its successors, Sennachérib then  Assurbanipal, choose Ninive like capital.

THE SECOND KINGDOM OF BABYLON

To the vii E century before J-C, Babyloniens take again the top on Assyriens and supplant them. They melt a new kingdom in Mésopotamie, which one calls the kingdom néo-babylonien. The city of  Babylon, devastated at the time assyrienne, is rebuilt and equipped with an imposing architecture: hanging gardens of the palate of  Nabuchodonosor II  (one of the Seven wonders of the world), large ziggourat high of seven stages (probably at the origin of the myth of the tower of Babel), etc. The dynasty néo-babylonienne lasts approximately one century.
In 539 before J-C, the kingdom néo-babylonien is subjected by the king perse Cyrus the Large one. All Mésopotamie from now on is integrated into the Empire perse.








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vendredi 10 janvier 2014

ALBERT EINSTEIN



Albert Einstein


Albert Einstein (1879-1955) est un physicien américain d’origine allemande, inventeur de l’une des théories les plus importantes de la physique du xxe siècle : la théorie de la relativité.
Après des études médiocres, Einstein occupe un emploi d’ingénieur à Zurich (Suisse). En 1905, à l’âge de 26 ans, il obtient son doctorat de physique et révolutionne la physique avec la publication de ses découvertes sur l’effet photoélectrique (émission d’électrons par un métal sous l’action de radiations lumineuses), sur le mouvement brownien (description mathématique du mouvement de particules microscopiques dans un liquide ou un gaz), la relativité restreinte et l’équivalence matière-énergie (traduite par la célèbre équation mc2).
Sa théorie sur la relativité restreinte est fondée sur deux postulats :
– la relativité : toutes les lois de la physique sont similaires dans tous les repères inertiels ;
– l’invariance de la vitesse de la lumière dans le vide (environ 300 000 km/s) : cette vitesse, également appelée célérité et notée c, est une constante universelle.
La théorie de la relativité permet de donner une description logique et correcte des événements physiques dans des repères inertiels différents. Elle reste longtemps très controversée par la communauté scientifique.
En 1916, Einstein publie sa théorie de la relativité générale, qui englobe les lois de la relativité restreinte et les lois de la gravitation d’Isaac Newton. L’année suivante, il applique sa nouvelle théorie à la cosmologie (science de l’univers) et propose un modèle d’Univers statique (en équilibre, sans mouvement). Mais en 1929, Edwin Hubble démontre que l’Univers est en expansion (et donc non statique).
En 1921, Einstein reçoit le prix Nobel pour ses travaux sur l’effet photoélectrique. Son hypothèse que la lumière est constituée de « grains d’énergie » (qui sont par la suite appelés photons) possédant une énergie proportionnelle à la fréquence du rayonnement ne sera confirmée que 18 ans plus tard par le physicien américain Arthur Compton. Einstein apporte sa contribution à la physique quantique en étudiant le comportement des photons. Il fait publier en 1924 un article du physicien indien Satyendranath Bose sur ce sujet, et élabore ensuite avec lui la théorie statistique de Bose-Einstein.
Dès les années 1920, Einstein est un savant respecté, mais aussi un véritable héros populaire. Il n’hésite pas à utiliser son immense renommée pour défendre ses convictions politiques.
En 1933, Hitler prend le pouvoir, et Albert Einstein quitte l’Allemagne. Après un passage par Paris et la Belgique, il accepte un poste de professeur à l’université de Princeton (États-Unis).
En 1939, il écrit au président américain Franklin D. Roosevelt pour lui demander de lancer un programme de recherche sur l’énergie nucléaire, afin de ne pas laisser l’Allemagne nazie prendre de l’avance dans ce domaine (ce programme prendra le nom de projet Manhattan). Il ne fait cependant pas partie de l’équipe qui fabrique la première bombe atomique. En 1945, il réécrit au président américain pour tenter de le convaincre de ne pas utiliser cette arme. Lui qui est à l’origine de la physique nucléaire, il luttera jusqu’à sa mort contre la prolifération des armes atomiques.
Au-delà de la portée de ses travaux, qui sont à l’origine de la physique contemporaine, sa personnalité marginale et ses engagements politiques en ont fait un personnage mythique du xxe siècle.



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