1.
Paris
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Paris is the capital and most populous city of France. It has an area of 105 square kilometres and a population of 2,229,621 in 2013 within its administrative limits, the agglomeration has grown well beyond the citys administrative limits. By the 17th century, Paris was one of Europes major centres of finance, commerce, fashion, science, and the arts, and it retains that position still today. The aire urbaine de Paris, a measure of area, spans most of the Île-de-France region and has a population of 12,405,426. It is therefore the second largest metropolitan area in the European Union after London, the Metropole of Grand Paris was created in 2016, combining the commune and its nearest suburbs into a single area for economic and environmental co-operation. Grand Paris covers 814 square kilometres and has a population of 7 million persons, the Paris Region had a GDP of €624 billion in 2012, accounting for 30.0 percent of the GDP of France and ranking it as one of the wealthiest regions in Europe. The city is also a rail, highway, and air-transport hub served by two international airports, Paris-Charles de Gaulle and Paris-Orly. Opened in 1900, the subway system, the Paris Métro. It is the second busiest metro system in Europe after Moscow Metro, notably, Paris Gare du Nord is the busiest railway station in the world outside of Japan, with 262 millions passengers in 2015. In 2015, Paris received 22.2 million visitors, making it one of the top tourist destinations. The association football club Paris Saint-Germain and the rugby union club Stade Français are based in Paris, the 80, 000-seat Stade de France, built for the 1998 FIFA World Cup, is located just north of Paris in the neighbouring commune of Saint-Denis. Paris hosts the annual French Open Grand Slam tennis tournament on the red clay of Roland Garros, Paris hosted the 1900 and 1924 Summer Olympics and is bidding to host the 2024 Summer Olympics. The name Paris is derived from its inhabitants, the Celtic Parisii tribe. Thus, though written the same, the name is not related to the Paris of Greek mythology. In the 1860s, the boulevards and streets of Paris were illuminated by 56,000 gas lamps, since the late 19th century, Paris has also been known as Panam in French slang. Inhabitants are known in English as Parisians and in French as Parisiens and they are also pejoratively called Parigots. The Parisii, a sub-tribe of the Celtic Senones, inhabited the Paris area from around the middle of the 3rd century BC. One of the areas major north-south trade routes crossed the Seine on the île de la Cité, this place of land and water trade routes gradually became a town
2.
France
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France, officially the French Republic, is a country with territory in western Europe and several overseas regions and territories. The European, or metropolitan, area of France extends from the Mediterranean Sea to the English Channel and the North Sea, Overseas France include French Guiana on the South American continent and several island territories in the Atlantic, Pacific and Indian oceans. France spans 643,801 square kilometres and had a population of almost 67 million people as of January 2017. It is a unitary republic with the capital in Paris. Other major urban centres include Marseille, Lyon, Lille, Nice, Toulouse, during the Iron Age, what is now metropolitan France was inhabited by the Gauls, a Celtic people. The area was annexed in 51 BC by Rome, which held Gaul until 486, France emerged as a major European power in the Late Middle Ages, with its victory in the Hundred Years War strengthening state-building and political centralisation. During the Renaissance, French culture flourished and a colonial empire was established. The 16th century was dominated by civil wars between Catholics and Protestants. France became Europes dominant cultural, political, and military power under Louis XIV, in the 19th century Napoleon took power and established the First French Empire, whose subsequent Napoleonic Wars shaped the course of continental Europe. Following the collapse of the Empire, France endured a succession of governments culminating with the establishment of the French Third Republic in 1870. Following liberation in 1944, a Fourth Republic was established and later dissolved in the course of the Algerian War, the Fifth Republic, led by Charles de Gaulle, was formed in 1958 and remains to this day. Algeria and nearly all the colonies became independent in the 1960s with minimal controversy and typically retained close economic. France has long been a centre of art, science. It hosts Europes fourth-largest number of cultural UNESCO World Heritage Sites and receives around 83 million foreign tourists annually, France is a developed country with the worlds sixth-largest economy by nominal GDP and ninth-largest by purchasing power parity. In terms of household wealth, it ranks fourth in the world. France performs well in international rankings of education, health care, life expectancy, France remains a great power in the world, being one of the five permanent members of the United Nations Security Council with the power to veto and an official nuclear-weapon state. It is a member state of the European Union and the Eurozone. It is also a member of the Group of 7, North Atlantic Treaty Organization, Organisation for Economic Co-operation and Development, the World Trade Organization, originally applied to the whole Frankish Empire, the name France comes from the Latin Francia, or country of the Franks
3.
Silvia Torres-Peimbert
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Silvia Torres-Peimbert is a Mexican astronomer. She won the LOréal-UNESCO Awards for Women in Science in 2011 on behalf of Latin America for her work determining the composition of nebulae. Torres-Peimbert was born in Mexico City in 1940 and she studied Physics at the National Autonomous University of Mexico before going on to the University of California in Berkeley. She returned to Mexico to conduct research at her alma mater. She studies the creation of stars and the mass thrown out by mid-size stars and she has studied the distribution of helium left over from the first creation. In 1973 she became a professor at NAUM and from 1998 until 2002 she was a director of that institution, during this time she has worked closely with Manuel Peimbert. Torres-Peimbert and Peimbert had both been students of Guillermo Haro and she was the editor of the learned Journal of Astronomy and Astrophysics. She won the LOréal-UNESCO Awards for Women in Science in 2011 on behalf of Latin America, the award is given annually to leading women scientists with an award being given to five continents. She won the award for investigating the composition of nebulae which the organisers considered essential to our understanding of the beginning of the cosmos. She also won the Hans A. Bethe Prize in 2012 for her work in determining the quantities of helium, knowing about these elements allows cosmologists to understand the evolution of stars and galaxies
4.
French language
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French is a Romance language of the Indo-European family. It descended from the Vulgar Latin of the Roman Empire, as did all Romance languages, French has evolved from Gallo-Romance, the spoken Latin in Gaul, and more specifically in Northern Gaul. Its closest relatives are the other langues doïl—languages historically spoken in northern France and in southern Belgium, French was also influenced by native Celtic languages of Northern Roman Gaul like Gallia Belgica and by the Frankish language of the post-Roman Frankish invaders. Today, owing to Frances past overseas expansion, there are numerous French-based creole languages, a French-speaking person or nation may be referred to as Francophone in both English and French. French is a language in 29 countries, most of which are members of la francophonie. As of 2015, 40% of the population is in Europe, 35% in sub-Saharan Africa, 15% in North Africa and the Middle East, 8% in the Americas. French is the fourth-most widely spoken mother tongue in the European Union, 1/5 of Europeans who do not have French as a mother tongue speak French as a second language. As a result of French and Belgian colonialism from the 17th and 18th century onward, French was introduced to new territories in the Americas, Africa, most second-language speakers reside in Francophone Africa, in particular Gabon, Algeria, Mauritius, Senegal and Ivory Coast. In 2015, French was estimated to have 77 to 110 million native speakers, approximately 274 million people are able to speak the language. The Organisation internationale de la Francophonie estimates 700 million by 2050, in 2011, Bloomberg Businessweek ranked French the third most useful language for business, after English and Standard Mandarin Chinese. Under the Constitution of France, French has been the language of the Republic since 1992. France mandates the use of French in official government publications, public education except in specific cases, French is one of the four official languages of Switzerland and is spoken in the western part of Switzerland called Romandie, of which Geneva is the largest city. French is the language of about 23% of the Swiss population. French is also a language of Luxembourg, Monaco, and Aosta Valley, while French dialects remain spoken by minorities on the Channel Islands. A plurality of the worlds French-speaking population lives in Africa and this number does not include the people living in non-Francophone African countries who have learned French as a foreign language. Due to the rise of French in Africa, the total French-speaking population worldwide is expected to reach 700 million people in 2050, French is the fastest growing language on the continent. French is mostly a language in Africa, but it has become a first language in some urban areas, such as the region of Abidjan, Ivory Coast and in Libreville. There is not a single African French, but multiple forms that diverged through contact with various indigenous African languages, sub-Saharan Africa is the region where the French language is most likely to expand, because of the expansion of education and rapid population growth
5.
Astronomer
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An astronomer is a scientist in the field of astronomy who concentrates their studies on a specific question or field outside of the scope of Earth. They look at stars, planets, moons, comets and galaxies, as well as other celestial objects — either in observational astronomy. Examples of topics or fields astronomers work on include, planetary science, solar astronomy, there are also related but distinct subjects like physical cosmology which studies the Universe as a whole. Astronomers usually fit into two types, Observational astronomers make direct observations of planets, stars and galaxies, and analyze the data, theoretical astronomers create and investigate models of things that cannot be observed. They use this data to create models or simulations to theorize how different celestial bodies work, there are further subcategories inside these two main branches of astronomy such as planetary astronomy, galactic astronomy or physical cosmology. Today, that distinction has disappeared and the terms astronomer. Professional astronomers are highly educated individuals who typically have a Ph. D. in physics or astronomy and are employed by research institutions or universities. They spend the majority of their time working on research, although quite often have other duties such as teaching, building instruments. The number of astronomers in the United States is actually quite small. The American Astronomical Society, which is the organization of professional astronomers in North America, has approximately 7,000 members. This number includes scientists from other such as physics, geology. The International Astronomical Union comprises almost 10,145 members from 70 different countries who are involved in research at the Ph. D. level. Before CCDs, photographic plates were a method of observation. Modern astronomers spend relatively little time at telescopes usually just a few weeks per year, analysis of observed phenomena, along with making predictions as to the causes of what they observe, takes the majority of observational astronomers time. Astronomers who serve as faculty spend much of their time teaching undergraduate and graduate classes, most universities also have outreach programs including public telescope time and sometimes planetariums as a public service to encourage interest in the field. Those who become astronomers usually have a background in maths, sciences. Taking courses that teach how to research, write and present papers are also invaluable, in college/university most astronomers get a Ph. D. in astronomy or physics. Keeping in mind how few there are it is understood that graduate schools in this field are very competitive
6.
Astronomy
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Astronomy is a natural science that studies celestial objects and phenomena. It applies mathematics, physics, and chemistry, in an effort to explain the origin of those objects and phenomena and their evolution. Objects of interest include planets, moons, stars, galaxies, and comets, while the phenomena include supernovae explosions, gamma ray bursts, more generally, all astronomical phenomena that originate outside Earths atmosphere are within the purview of astronomy. A related but distinct subject, physical cosmology, is concerned with the study of the Universe as a whole, Astronomy is the oldest of the natural sciences. The early civilizations in recorded history, such as the Babylonians, Greeks, Indians, Egyptians, Nubians, Iranians, Chinese, during the 20th century, the field of professional astronomy split into observational and theoretical branches. Observational astronomy is focused on acquiring data from observations of astronomical objects, theoretical astronomy is oriented toward the development of computer or analytical models to describe astronomical objects and phenomena. The two fields complement each other, with theoretical astronomy seeking to explain the results and observations being used to confirm theoretical results. Astronomy is one of the few sciences where amateurs can play an active role, especially in the discovery. Amateur astronomers have made and contributed to many important astronomical discoveries, Astronomy means law of the stars. Astronomy should not be confused with astrology, the system which claims that human affairs are correlated with the positions of celestial objects. Although the two share a common origin, they are now entirely distinct. Generally, either the term astronomy or astrophysics may be used to refer to this subject, however, since most modern astronomical research deals with subjects related to physics, modern astronomy could actually be called astrophysics. Few fields, such as astrometry, are purely astronomy rather than also astrophysics, some titles of the leading scientific journals in this field includeThe Astronomical Journal, The Astrophysical Journal and Astronomy and Astrophysics. In early times, astronomy only comprised the observation and predictions of the motions of objects visible to the naked eye, in some locations, early cultures assembled massive artifacts that possibly had some astronomical purpose. Before tools such as the telescope were invented, early study of the stars was conducted using the naked eye, most of early astronomy actually consisted of mapping the positions of the stars and planets, a science now referred to as astrometry. From these observations, early ideas about the motions of the planets were formed, and the nature of the Sun, Moon, the Earth was believed to be the center of the Universe with the Sun, the Moon and the stars rotating around it. This is known as the model of the Universe, or the Ptolemaic system. The Babylonians discovered that lunar eclipses recurred in a cycle known as a saros
7.
Astronomical object
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An astronomical object or celestial object is a naturally occurring physical entity, association, or structure that current astronomy has demonstrated to exist in the observable universe. In astronomy, the object and body are often used interchangeably. Examples for astronomical objects include planetary systems, star clusters, nebulae and galaxies, while asteroids, moons, planets, and stars are astronomical bodies. A comet may be identified as both body and object, It is a body when referring to the nucleus of ice and dust. The universe can be viewed as having a hierarchical structure, at the largest scales, the fundamental component of assembly is the galaxy. Galaxies are organized groups and clusters, often within larger superclusters. Disc galaxies encompass lenticular and spiral galaxies with features, such as spiral arms, at the core, most galaxies have a supermassive black hole, which may result in an active galactic nucleus. Galaxies can also have satellites in the form of dwarf galaxies, the constituents of a galaxy are formed out of gaseous matter that assembles through gravitational self-attraction in a hierarchical manner. At this level, the fundamental components are the stars. The great variety of forms are determined almost entirely by the mass, composition. Stars may be found in systems that orbit about each other in a hierarchical organization. A planetary system and various objects such as asteroids, comets and debris. The various distinctive types of stars are shown by the Hertzsprung–Russell diagram —a plot of stellar luminosity versus surface temperature. Each star follows a track across this diagram. If this track takes the star through a region containing a variable type. An example of this is the instability strip, a region of the H-R diagram that includes Delta Scuti, RR Lyrae, the table below lists the general categories of bodies and objects by their location or structure. International Astronomical Naming Commission List of light sources List of Solar System objects Lists of astronomical objects SkyChart, Sky & Telescope Monthly skymaps for every location on Earth
8.
Star
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A star is a luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun, many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. However, most of the stars in the Universe, including all stars outside our galaxy, indeed, most are invisible from Earth even through the most powerful telescopes. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the stars lifetime, near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity, and many properties of a star by observing its motion through space, its luminosity. The total mass of a star is the factor that determines its evolution. Other characteristics of a star, including diameter and temperature, change over its life, while the environment affects its rotation. A plot of the temperature of stars against their luminosities produces a plot known as a Hertzsprung–Russell diagram. Plotting a particular star on that allows the age and evolutionary state of that star to be determined. A stars life begins with the collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, the remainder of the stars interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The stars internal pressure prevents it from collapsing further under its own gravity, a star with mass greater than 0.4 times the Suns will expand to become a red giant when the hydrogen fuel in its core is exhausted. In some cases, it will fuse heavier elements at the core or in shells around the core, as the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars. Meanwhile, the core becomes a remnant, a white dwarf. Binary and multi-star systems consist of two or more stars that are bound and generally move around each other in stable orbits. When two such stars have a close orbit, their gravitational interaction can have a significant impact on their evolution. Stars can form part of a much larger gravitationally bound structure, historically, stars have been important to civilizations throughout the world
9.
Planet
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The term planet is ancient, with ties to history, astrology, science, mythology, and religion. Several planets in the Solar System can be seen with the naked eye and these were regarded by many early cultures as divine, or as emissaries of deities. As scientific knowledge advanced, human perception of the planets changed, in 2006, the International Astronomical Union officially adopted a resolution defining planets within the Solar System. This definition is controversial because it excludes many objects of mass based on where or what they orbit. The planets were thought by Ptolemy to orbit Earth in deferent, at about the same time, by careful analysis of pre-telescopic observation data collected by Tycho Brahe, Johannes Kepler found the planets orbits were not circular but elliptical. As observational tools improved, astronomers saw that, like Earth, the planets rotated around tilted axes, and some shared such features as ice caps and seasons. Since the dawn of the Space Age, close observation by space probes has found that Earth and the planets share characteristics such as volcanism, hurricanes, tectonics. Planets are generally divided into two types, large low-density giant planets, and smaller rocky terrestrials. Under IAU definitions, there are eight planets in the Solar System, in order of increasing distance from the Sun, they are the four terrestrials, Mercury, Venus, Earth, and Mars, then the four giant planets, Jupiter, Saturn, Uranus, and Neptune. Six of the planets are orbited by one or more natural satellites, several thousands of planets around other stars have been discovered in the Milky Way. e. in the habitable zone. On December 20,2011, the Kepler Space Telescope team reported the discovery of the first Earth-sized extrasolar planets, Kepler-20e and Kepler-20f, orbiting a Sun-like star, Kepler-20. A2012 study, analyzing gravitational microlensing data, estimates an average of at least 1.6 bound planets for every star in the Milky Way, around one in five Sun-like stars is thought to have an Earth-sized planet in its habitable zone. The idea of planets has evolved over its history, from the lights of antiquity to the earthly objects of the scientific age. The concept has expanded to include not only in the Solar System. The ambiguities inherent in defining planets have led to much scientific controversy, the five classical planets, being visible to the naked eye, have been known since ancient times and have had a significant impact on mythology, religious cosmology, and ancient astronomy. In ancient times, astronomers noted how certain lights moved across the sky, as opposed to the fixed stars, ancient Greeks called these lights πλάνητες ἀστέρες or simply πλανῆται, from which todays word planet was derived. In ancient Greece, China, Babylon, and indeed all pre-modern civilizations, it was almost universally believed that Earth was the center of the Universe and that all the planets circled Earth. The first civilization known to have a theory of the planets were the Babylonians
10.
Asteroid
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Asteroids are minor planets, especially those of the inner Solar System. The larger ones have also been called planetoids and these terms have historically been applied to any astronomical object orbiting the Sun that did not show the disc of a planet and was not observed to have the characteristics of an active comet. As minor planets in the outer Solar System were discovered and found to have volatile-based surfaces that resemble those of comets, in this article, the term asteroid refers to the minor planets of the inner Solar System including those co-orbital with Jupiter. There are millions of asteroids, many thought to be the remnants of planetesimals. The large majority of known asteroids orbit in the belt between the orbits of Mars and Jupiter, or are co-orbital with Jupiter. However, other orbital families exist with significant populations, including the near-Earth objects, individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups, C-type, M-type, and S-type. These were named after and are identified with carbon-rich, metallic. The size of asteroids varies greatly, some reaching as much as 1000 km across, asteroids are differentiated from comets and meteoroids. In the case of comets, the difference is one of composition, while asteroids are composed of mineral and rock, comets are composed of dust. In addition, asteroids formed closer to the sun, preventing the development of the aforementioned cometary ice, the difference between asteroids and meteoroids is mainly one of size, meteoroids have a diameter of less than one meter, whereas asteroids have a diameter of greater than one meter. Finally, meteoroids can be composed of either cometary or asteroidal materials, only one asteroid,4 Vesta, which has a relatively reflective surface, is normally visible to the naked eye, and this only in very dark skies when it is favorably positioned. Rarely, small asteroids passing close to Earth may be visible to the eye for a short time. As of March 2016, the Minor Planet Center had data on more than 1.3 million objects in the inner and outer Solar System, the United Nations declared June 30 as International Asteroid Day to educate the public about asteroids. The date of International Asteroid Day commemorates the anniversary of the Tunguska asteroid impact over Siberia, the first asteroid to be discovered, Ceres, was found in 1801 by Giuseppe Piazzi, and was originally considered to be a new planet. In the early half of the nineteenth century, the terms asteroid. Asteroid discovery methods have improved over the past two centuries. This task required that hand-drawn sky charts be prepared for all stars in the band down to an agreed-upon limit of faintness. On subsequent nights, the sky would be charted again and any moving object would, hopefully, the expected motion of the missing planet was about 30 seconds of arc per hour, readily discernible by observers
11.
International Council for Science
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The International Council for Science is an international organization devoted to international cooperation in the advancement of science. Its members are national bodies and international scientific unions. As of 2012, it comprises 120 multi-disciplinary National Scientific Members, Associates and Observers representing 140 countries and 31 international, ICSU also has 22 Scientific Associates. ICSU’s mission is to international science for the benefit of society. To do this, ICSU mobilizes the knowledge and resources of the science community to, Identify and address major issues of importance to science. Facilitate interaction amongst scientists across all disciplines and from all countries, promote the participation of all scientists — regardless of race, citizenship, language, political stance, or gender — in the international scientific endeavour. Provide independent, authoritative advice to stimulate constructive dialogue between the community and governments, civil society, and the private sector. Activities focus on three areas, International Research Collaboration, Science for Policy, and Universality of Science, the universality of science in its broadest sense is about developing a truly global scientific community on the basis of equity and non-discrimination. It is also ensuring that science is trusted and valued by societies across the world. As such, it incorporates issues related to the conduct of science, capacity building, science education and literacy, access to data and information and the relationship between science and society. Underpinning this broader concept of universality is the Principle of the Universality of Science which is narrowly focused on the freedoms. Adherence to this Principle is a condition of ICSU membership, the Freedom and Responsibility Portal on the ICSUs website documents its activities in these areas. The ICSU Secretariat in Paris ensures the day-to-day planning and operations under the guidance of an elected Executive Board, ICSU has three Regional Offices − Africa, Asia and the Pacific as well as Latin America and the Caribbean. The principal source of ICSUs finances is the contributions it receives from its members, ISBN9780881350661 Crawford, Elisabeth Nationalism and Internationalism in Science, 1880-1939. Cambridge University Press ISBN9780521524742 Official website ICSU at University of Waterloo Scholarly Societies directory ICSU at United Nations
12.
Amateur astronomy
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Amateur astronomy is a hobby whose participants enjoy watching the sky, and the abundance of objects found in it with the unaided eye, binoculars, or telescopes. Many amateurs are beginners or hobbyists, while others have a degree of experience in astronomy and often assist. Amateur astronomers often look at the sky using nothing more than their eyes, people have studied the sky throughout history in an amateur framework, without any formal method of funding. It is only within about the past century, however, that amateur astronomy has become an activity clearly distinguished from professional astronomy, collectively, amateur astronomers observe a variety of celestial objects and phenomena. Common targets of amateur astronomers include the Moon, planets, stars, comets, meteor showers, and a variety of deep sky objects such as clusters, galaxies. Many amateurs like to specialise in observing particular objects, types of objects, one branch of amateur astronomy, amateur astrophotography, involves the taking of photos of the night sky. Most amateur astronomers work at visible wavelengths, but a small minority experiment with wavelengths outside the visible spectrum, non-visual amateur astronomy includes the use of infrared filters on conventional telescopes, and also the use of radio telescopes. Some amateur astronomers use home-made radio telescopes, while others use radio telescopes that were built for astronomy research but have since been made available for use by amateurs. The One-Mile Telescope is one such example, Amateur astronomers use a range of instruments to study the sky, depending on a combination of their interests and resources. Commercial telescopes are available, new and used, but it is common for amateur astronomers to build their own custom telescopes. Some people even focus on amateur telescope making as their primary interest within the hobby of amateur astronomy, although specialized and experienced amateur astronomers tend to acquire more specialized and more powerful equipment over time, relatively simple equipment is often preferred for certain tasks. Amateur astronomers also use star charts that, depending on experience and intentions, Amateur astronomers often like to keep records of their observations, which usually takes the form of an observing log. Observing logs typically record details about which objects were observed and when, sketching is sometimes used within logs, and photographic records of observations have also been used in recent times. The information gathered is used to help studies and interactions between amateur astronomers in yearly gatherings, although not professional information or credible, it is a way for the hobby lovers to share their new sightings and experiences. The Internet is a tool of amateur astronomers. The popularity of CCD imaging among amateurs has led to large numbers of web sites being written by individuals about their images, much of the social interaction of amateur astronomy occurs on mailing lists or discussion groups. Discussion group servers host numerous astronomy lists, a great deal of the commerce of amateur astronomy, the buying and selling of equipment, occurs online. Many amateurs use online tools to plan their observing sessions using tools such as the Clear Sky Chart
13.
14th arrondissement of Paris
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The 14th arrondissement of Paris is one of the 20 arrondissements of the capital city of France. Situated on the bank of the River Seine, it contains most of the Montparnasse district. It is today best known for its skyscraper, the Tour Montparnasse, and its railway terminus. The district has traditionally been home to artists as well as a Breton community. The 14th arrondissement also contains the Cité Internationale Universitaire de Paris, which is located near the Parc Montsouris, the land area of this arrondissement is 5.621 km². The 14th arrondissement attained its peak population in 1954 when it had 181,414 inhabitants and it continues to have a high density of both population and business activity with 132,844 inhabitants and 71,836 jobs as of the last census, in 1999. Aéroports de Paris has its office in the arrondissement. In addition Société dexploitation de lhebdomadaire Le Point, the company that operates Le Point, has its office in the arrondissement. SNCF, the French rail company, formerly had its office in Montparnasse. La Santé Prison, operated by the Ministry of Justice, is in the arrondissement, the head office of the Agency for French Education Abroad, the French international schooling network, is in the arrondissement. The International Astronomical Union head office is located on the floor of the Institut dAstrophysique de Paris
14.
Planetary nomenclature
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Since the invention of the telescope, astronomers have given names to the surface features they have discerned, especially on the Moon and Mars. To standardize planetary nomenclature, the International Astronomical Union was assigned in 1919 the task of selecting official names for features on solar system bodies. Later, as higher resolution images and maps available, additional features are named at the request of investigators mapping or describing specific surfaces, features. Anyone may suggest that a specific name be considered by a task group. If the members of the group agree that the name is appropriate. Names successfully reviewed by a group are submitted to the IAU Working Group for Planetary System Nomenclature. Upon successful review by the members of the WGPSN, names are considered provisionally approved and can be used on maps and in publications as long as the provisional status is clearly stated. Provisional names are presented for adoption to the IAUs General Assembly, which met triennially in the past. A name is not considered to be official — that is, Names adopted by the IAU must follow various rules and conventions established and amended through the years by the Union. These include, Nomenclature is a tool and the first consideration should be to make it simple, clear, the number of names chosen for each body should be kept to a minimum. Features should be named only when they have special scientific interest, duplication of the same surface feature name on two or more bodies, and of the same name for satellites and minor planets, is discouraged. Duplications may be allowed when names are especially appropriate and the chances for confusion are very small, individual names chosen for each body should be expressed in the language of origin. Transliteration for various alphabets should be given, but there will be no translation from one language to another, where possible, the themes established in early solar system nomenclature should be used and expanded on. Solar system nomenclature should be international in its choice of names, recommendations submitted to the IAU national committees will be considered, but final selection of the names is the responsibility of the International Astronomical Union. No names having political, military or religious significance may be used, persons being so honored must have been deceased for at least three years. When more than one spelling of a name is extant, the spelling preferred by the person, or used in an authoritative reference, diacritical marks are a necessary part of a name and will be used. Ring and ring-gap nomenclature and names for newly discovered satellites are developed in joint deliberation between WGPSN and IAU Commission 20, Names will not be assigned to satellites until their orbital elements are reasonably well known or definite features have been identified on them. Accessible and authoritative sources, including Internet sources, are required for adopted names, wikipedia is not sufficient as a source, but may be useful for identifying appropriate sources
15.
Benjamin Baillaud
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Édouard Benjamin Baillaud was a French astronomer. Born in Chalon-sur-Saône, Baillaud studied at the École Normale Supérieure and he worked as an assistant at the Paris Observatory beginning in 1872. Later he was director of the Toulouse Observatory from 1878 to 1907 and he greatly expanded the observatory and enthusiastically supported the Carte du Ciel project. He specialized in mechanics, in particular the motions of the satellites of Saturn. In 1903, the took over a facility on the Pic du Midi in the Pyrenees that had been founded by amateurs in the 1850s with the goal of putting a telescope there. However, the height of 2865 metres posed formidable logistical challenges, Baillaud organised a team of soldiers to erect a 0.5 metre reflecting telescope, and 0.25 metre refracting telescope on the summit. Though the French government agreed to fund the project, it was becoming clear that its objectives were hopelessly unrealistic. Baillaud was the President of the Société astronomique de France, the French astronomical society, Baillaud was active in time standardisation, becoming the founding president of the International Time Bureau and initiating the transmission of a time signal from the Eiffel Tower. Baillauds concern for the time standard led him to be an outspoken opponent of daylight saving time. Baillaud became founding president of the International Astronomical Union in 1919 and he retired as director of the Paris Observatory in 1926. He was an academician in the astronomy section of the Académie des Sciences. He won the Bruce Medal in 1923, the crater Baillaud on the Moon is named after him, and so are asteroids 11764 Benbaillaud and 1280 Baillauda. Distribution des prix du lycée de Saint-Quentin, impr. de J. Vidallet, -16 pages Thèses présentées à la Faculté des sciences de Paris pour obtenir le grade de docteur ès sciences mathématiques, par M. B. Exposition de la méthode de M. Gylden pour le développement des perturbations des cometes, Gauthier-Villars, -47 pages Theses de mathematiques, L. et J. -M. Douladoure -108 Pages Sur la méthode de Hansen pour la détermination des perturbations absolues des petites planètes,4 pages Sur une transformation trigonométrique employée par Hansen dans la théorie des perturbations,7 pages Détermination des éléments des orbites des cinq satellites intérieurs de Saturne. Gauthier-Villars Sur le calcul numérique des intégrales définies, Éd. Gauthier-Villar Recherches complémentaires sur le développement de la fonction pertubatrice. Cours dastronomie à lusage des étudiants des facultés des sciences, Éd, Gauthier-Villars,38 pages Étude du climat de Toulouse de 1863 à1900. -444 pages Comparaison des catalogues méridiens de Toulouse et de Leipzig, extrait des Comptes rendus de lAssociation française pour lavancement des sciences, congrès de Montauban,1902
16.
Alfred Fowler
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Alfred Fowler, CBE FRS was an English astronomer. Not to be confused with American astrophysicist William Alfred Fowler and he was born in Wilsden, Yorkshire and educated at Londons Normal School of Science, which was later absorbed into Imperial College, London. He was appointed Instructor of Astrophysics at Imperial College and worked there until his death and he was an expert in spectroscopy, being one of the first to determine that the temperature of sunspots was cooler than that of surrounding regions. He was elected a Fellow of the Royal Society in 1910, assistant Professor of Physics Imperial College and Technology, South Kensington. Associated in observations of eclipses of the sun with Sir Norman Lockyer in 1893,1896,1898,1900. He was awarded their Royal Medal in 1918 and delivered their Bakerian Lectures in 1914 and 1924, Fowler was president of the Royal Astronomical Society from 1919 to 1921 and died in Ealing, London in 1940. Bruce Medal page Awarding of Bruce medal, PASP4687 Awarding of RAS gold medal, MNRAS75355 ApJ941 MNRAS101132 Obs 63262 PASP52301
17.
William Wallace Campbell
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William Wallace Campbell was an American astronomer, and director of Lick Observatory from 1901 to 1930. He was born on a farm in Hancock County, Ohio, after a few years of local schooling he entered in 1882 the University of Michigan to study civil engineering, graduating Bachelor of Science in 1886. Whilst at university he developed his interest in astronomy when he read Simon Newcombs Popular Astronomy, after graduating he was appointed Professor of Mathematics at the University of Colorado but soon moved back to Michigan as an instructor in astronomy. In 1891 he was invited to work on spectroscopy at Lick Observatory in California, Campbell was a pioneer of astronomical spectroscopy and catalogued the radial velocities of stars. In 1893 he discovered the Wolf–Rayet star HD184738 and he was made a director of Lick Observatory from 1901 to 1930. His first 1919 observations were wrong, so he repeated them in 1922 and he thus led a team to Australia in 1922 where he photographed a solar eclipse. The data obtained provided further evidence supporting Albert Einsteins theory of relativity, in 1931 he accepted the role of president of the National Academy of Sciences in Washington. He served as 10th President of the University of California from 1923 to 1930 and he also served on the board of trustees for Science Service, now known as Society for Science & the Public, from 1923 to 1926. He served three terms as president of the Astronomical Society of the Pacific and he committed suicide in California at the age of 76 by leaping to his death from a fourth-story window in San Francisco. He was mostly blind and suffering bouts of aphasia. This was not only frustrating to him, but he felt that it left him a burden to his family in terms of care and expense. He married Elizabeth Ballard Thompson in 1892, they had three sons, Campbell led several of these expeditions
18.
Frank Watson Dyson
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Dyson was born in Measham, near Ashby-de-la-Zouch, Leicestershire, the son of the Rev Watson Dyson, a Baptist minister, and his wife, Frances Dodwell. They moved to Yorkshire in his youth, in 1894 he was given the post of Senior Assistant at Greenwich Observatory and worked on the Astrographic Catalogue, which was published in 1905. He was appointed Astronomer Royal for Scotland from 1905 to 1910 and he also, in 1924, introduced the distribution of the six pips via the BBC. He was for several years President of the British Horological Institute and was awarded their Gold Medal in 1928, Dyson was noted for his study of solar eclipses and was an authority on the spectrum of the corona and on the chromosphere. He is credited with organising expeditions to observe the 1919 solar eclipse at Brazil and Principe, Dyson died on board a ship while travelling from Australia to England in 1939 and was buried at sea. The crater Dyson on the Moon is named after him, as is the asteroid 1241 Dysona, in 1894 he married Caroline Bisset Best, the daughter of Palemon Best, with whom he had two sons and six daughters. Frank Dyson and theoretical physicist Freeman Dyson are not related, inspired, Dysons first attempt at writing was a 1931 piece of juvenilia entitled Sir Phillip Roberts Erolunar Collision – Sir Philip being a thinly disguised version of Sir Frank
19.
Georges Lecointe (explorer)
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Georges Lecointe was a Belgian naval officer and scientist. He was captain of the Belgica and second-in-command of the Belgian Antarctic Expedition, after his return to Belgium he was deeply involved in the foundation of the International Research Council and the International Astronomical Union. Georges Lecointe was born in Antwerp on 29 April 1869 and his father was a well-known mathematics teacher and he proved early on to be a gifted student. He entered the Royal Military Academy in 1886, the Belgian government detached him to the French Navy, where he was ultimately promoted to ship-of-the-line lieutenant in 1897. This detachment was exceptional and happened as a result of an audience with king Leopold II, it was granted to one other Belgian officer. Between 1894 and 1897 he trained on a number of ships in the Mediterranean, in his second book, La création dune marine nationale Belge, he pleaded for the re-creation of the Belgian Navy, which had been abolished in 1862. This, however, did not happen until the end of the World War I, Emile Danco, a mutual friend of Lecointe and expedition commander Adrien de Gerlache, proposed him in October 1896 to join the Belgian Antarctic Expedition. De Gerlache hired him in 1897 as captain of the Belgica and he was also responsible for the astronomical and hydrographical observations and, after Dancos death in 1898, measurements of the earths magnetism. The expedition set sail from Antwerp in August 1897 and started observations in the Antarctic region later that year, on 22 January 1898 sailor Carl Wiencke was washed overboard and drowned, despite a heroic rescue effort by Lecointe. They made their way to the Weddell Sea in early 1898, during astronomical observations on the pack ice, Lecointe was taken for a seal and narrowly escaped being shot. Both Lecointe and de Gerlache suffered heavily from scurvy, to the point where the command of the expedition had to be taken over by first mate Roald Amundsen. Despite de Gerlaches misgivings, they cajoled the sick expedition members into eating fresh seal and penguin meat, early in 1899 the crew finally managed to free the Belgica. On reaching South America Lecointe started exploring the Andes while de Gerlache sailed the Belgica back to Belgium, after his return, Lecointe published Au Pays des Manchots, chronicling the Belgica expedition. Lecointe was engaged to Charlotte Dumeiz before the departure of the Belgica, Charlotte Bay was named after her, and they married shortly after his return. The couple had three children, Henri, Charlotte and Louis-Georges, both sons studied at the Free University of Brussels. On his return he was promoted to captain-commandant, spent a time in the Belgian Legion during the Boxer war and was appointed as scientific director of the Royal Observatory in Uccle. In addition he oversaw a renovation of the observatory and was made responsible for the Belgian training ships. He served voluntarily during the First World War as a major and was involved in the defense of Antwerp
20.
Astronomische Gesellschaft Katalog
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The Astronomische Gesellschaft Katalog is an astrometric star catalogue. Compilation for the first version, AGK1, was started in 1861 by Friedrich Argelander, the second version, AGK2, was started in the 1920s, and published between 1951 and 1958 using photographic data obtained from the Bonn and Hamburg Observatories. The third version, AGK3, was started in 1956 and published in 1975 and it contains 183,145 stars north of declination –2° with mean positional errors of ±0.13 and mean proper motion errors of ±0. 009/year. Hoher List Observatory DavidDarling. info Astro. it AGK3 query form from VizieR
21.
Carte du Ciel
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Twenty observatories from around the world participated in exposing and measuring more than 22,000 photographic plates in an enormous observing programme extending over several decades. However, the appearance of the Hipparcos Catalogue in 1997 has led to an important development in the use of historical plate material. Different observatories around the world were charged with surveying specific declination zones, the Astrographic Catalogue plates, of typically 6 minutes exposure, were in due course photographed, measured, and published in their entirety. They yielded a catalogue of positions and magnitudes down to about 11.5 mag, for the second goal, a second set of plates, with longer exposures but minimal overlap, was to photograph all stars to 14 mag. A fascinating contemporary account of this vast international astronomical collaboration, published in 1912, is given by H. H. Turner, other aspects are covered in various papers in the Proceedings of IAU Symposium Number 133 held in 1988. For the Astrographic Catalogue,20 observatories from around the world participated in exposing and measuring more than 22,000 glass plates, around half of the observatories ordered telescopes from the Henry brothers in France, with others coming from the factory of Howard Grubb of Dublin. Each observatory was assigned a specific zone to photograph. The first such plate was taken in August 1891 at the Vatican Observatory, the participating observatories agreed to use a standardized telescope so that all plates had a similar scale of approximately 60 arcsec/mm. The measurable areas of the plates were 2. 1°×2. 1°, so the overlap pattern consisted of plates that were centred on every degree band in declination, many factors, such as reference catalogue, reduction technique and print formats were left up to the individual institutions. The positional accuracy goal was 0.5 arcsec per image, plate measurement was a protracted affair, with measuring done by eye and recorded by hand. The plates were turned over to a number of semi-skilled computers to determine the positions of the stars on each plate. The original goal of 11 mag for the magnitude was generally surpassed, however. In total, some 4.6 million stars were observed, the brightest stars were over-exposed on the plates, not measured, and therefore missing in the resulting catalogues. Publication of the measurements proceeded from 1902 to 1964, and resulted in 254 printed volumes of raw data, for decades the Astrographic Catalogue was largely ignored. The data were difficult to work with because they were neither in machine-readable form nor in equatorial coordinates. Decades of labour were expended internationally before the project was superseded by modern astronomical techniques, one problem was that the work took much longer than expected. As originally envisaged, the project was meant to have taken only 10 to 15 years, as a result, French astronomy in particular fell behind and lagged for decades. The still-more-ambitious Carte du Ciel component of the programme was undertaken by some of the participating observatories, the charts proved to be excessively expensive to photograph and reproduce, generally via engraved copper plates, and many zones were either not completed or properly published
22.
Mexico
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Mexico, officially the United Mexican States, is a federal republic in the southern half of North America. It is bordered to the north by the United States, to the south and west by the Pacific Ocean, to the southeast by Guatemala, Belize, and the Caribbean Sea, and to the east by the Gulf of Mexico. Covering almost two million square kilometers, Mexico is the sixth largest country in the Americas by total area, Mexico is a federation comprising 31 states and a federal district that is also its capital and most populous city. Other metropolises include Guadalajara, Monterrey, Puebla, Toluca, Tijuana, pre-Columbian Mexico was home to many advanced Mesoamerican civilizations, such as the Olmec, Toltec, Teotihuacan, Zapotec, Maya and Aztec before first contact with Europeans. In 1521, the Spanish Empire conquered and colonized the territory from its base in Mexico-Tenochtitlan, Three centuries later, this territory became Mexico following recognition in 1821 after the colonys Mexican War of Independence. The tumultuous post-independence period was characterized by instability and many political changes. The Mexican–American War led to the cession of the extensive northern borderlands, one-third of its territory. The Pastry War, the Franco-Mexican War, a civil war, the dictatorship was overthrown in the Mexican Revolution of 1910, which culminated with the promulgation of the 1917 Constitution and the emergence of the countrys current political system. Mexico has the fifteenth largest nominal GDP and the eleventh largest by purchasing power parity, the Mexican economy is strongly linked to those of its North American Free Trade Agreement partners, especially the United States. Mexico was the first Latin American member of the Organisation for Economic Co-operation and Development and it is classified as an upper-middle income country by the World Bank and a newly industrialized country by several analysts. By 2050, Mexico could become the fifth or seventh largest economy. The country is considered both a power and middle power, and is often identified as an emerging global power. Due to its culture and history, Mexico ranks first in the Americas. Mexico is a country, ranking fourth in the world by biodiversity. In 2015 it was the 9th most visited country in the world, Mexico is a member of the United Nations, the World Trade Organization, the G8+5, the G20, the Uniting for Consensus and the Pacific Alliance. Mēxihco is the Nahuatl term for the heartland of the Aztec Empire, namely, the Valley of Mexico, and its people, the Mexica and this became the future State of Mexico as a division of New Spain prior to independence. It is generally considered to be a toponym for the valley became the primary ethnonym for the Aztec Triple Alliance as a result. After New Spain won independence from Spain, representatives decided to name the new country after its capital and this was founded in 1524 on top of the ancient Mexica capital of Mexico-Tenochtitlan
23.
Australian Academy of Science
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The Australian Academy of Science was founded in 1954 by a group of distinguished Australians, including Australian Fellows of the Royal Society of London. The first president was Sir Mark Oliphant, the Academy is modelled after the Royal Society and operates under a Royal Charter, as such, it is an independent body, but it has government endorsement. The Academy Secretariat is in Canberra, at the Shine Dome, the objectives of the Academy are to promote science and science education through a range of activities. The Australian National Research Council was established in 1919 for the purpose of representing Australia on the International Research Council, the Council ceased to exist in 1954, replaced by the Australian Academy of Science. It was designed by architect Sir Roy Grounds, of Grounds, Romberg, when completed in 1959 its 45. 75-metre-diameter dome was the largest in Australia. On 1 December 1956, the Academys building design committee met in Adelaide to look over plans submitted by six architects, the plan accepted involved a 710-tonne reinforced concrete dome, which had to be supported by 16 thin supports. The concrete is approximately 60 cm thick at the base supports, the dome supports itself, with no internal wall holding it up. The building was named Becker House, for benefactor and Fellow of the Academy Sir Jack Ellerton Becker, in 2000, it was renamed in honour of Fellow John Shine, who donated one million dollars to renovate the dome. Science education is a commitment of Australian Academy of Science. Scientists judged by their peers to have made a contribution to knowledge in their field may be elected to Fellowship of the Academy. Twenty new Fellows may be elected every year, no more than two Fellows may be elected every three years on the basis of distinguished contributions to science by means other than personal research. A small number of distinguished foreign scientists with substantial connections to Australian science are elected as Corresponding Members, Fellows are denoted by the letters FAA after their name. Moran Medal to recognise outstanding research in one or more of the fields of applied probability, biometrics, mid career awards, Gustav Nossal Medal, to health researchers, Jacques Miller Medal, to experimental biomedicine researchers, Nancy Millis Medal for Women in Science. There are three other learned Academies in Australia, those of Humanities, Social Science and Technological Sciences, the four Academies cooperate through the Australian Council of Learned Academies, formed in 2010. List of Australian organisations with royal patronage Australian Academy of Science Australian Academy of Science Building
24.
French Academy of Sciences
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The French Academy of Sciences is a learned society, founded in 1666 by Louis XIV at the suggestion of Jean-Baptiste Colbert, to encourage and protect the spirit of French scientific research. It was at the forefront of developments in Europe in the 17th and 18th centuries. Currently headed by Sébastien Candel, it is one of the five Academies of the Institut de France, the Academy of Sciences makes its origin to Colberts plan to create a general academy. He chose a group of scholars who met on 22 December 1666 in the Kings library. The first 30 years of the Academys existence were relatively informal, in contrast to its British counterpart, the Academy was founded as an organ of government. The Academy was expected to remain apolitical, and to avoid discussion of religious, on 20 January 1699, Louis XIV gave the Company its first rules. The Academy received the name of Royal Academy of Sciences and was installed in the Louvre in Paris, following this reform, the Academy began publishing a volume each year with information on all the work done by its members and obituaries for members who had died. This reform also codified the method by which members of the Academy could receive pensions for their work, on 8 August 1793, the National Convention abolished all the academies. Almost all the old members of the previously abolished Académie were formally re-elected, among the exceptions was Dominique, comte de Cassini, who refused to take his seat. In 1816, the again renamed Royal Academy of Sciences became autonomous, while forming part of the Institute of France, in the Second Republic, the name returned to Académie des sciences. During this period, the Academy was funded by and accountable to the Ministry of Public Instruction, the Academy came to control French patent laws in the course of the eighteenth century, acting as the liaison of artisans knowledge to the public domain. As a result, academicians dominated technological activities in France, the Academy proceedings were published under the name Comptes rendus de lAcadémie des sciences. The Comptes rendus is now a series with seven titles. The publications can be found on site of the French National Library, in 1818 the French Academy of Sciences launched a competition to explain the properties of light. The civil engineer Augustin-Jean Fresnel entered this competition by submitting a new theory of light. Siméon Denis Poisson, one of the members of the judging committee, being a supporter of the particle-theory of light, he looked for a way to disprove it. The Poisson spot is not easily observed in every-day situations, so it was natural for Poisson to interpret it as an absurd result. However, the head of the committee, Dominique-François-Jean Arago, and he molded a 2-mm metallic disk to a glass plate with wax
25.
National Research Foundation of South Africa
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South Africa’s National Research Foundation is the intermediary agency between the policies and strategies of the Government of South Africa and South Africas research institutions. It was established on 1 April 1999 as a statutory body in accordance with the National Research Foundation Act. Dr Molapo Qhobela has been appointed the Chief Executive Officer of the National Research Foundation of South Africa with effect from 1 January 2016, the NRF Board is chaired by Professor Belinda Bozzolli. KZN Literary Tourism is a project which has received funding through the NRF, in 2004 the NRF founded seven Centres of Excellence, which aim to facilitate inter-disciplinary research with the aim of enhancing research and capacity building
26.
King Abdulaziz City for Science and Technology
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In 1977, the Saudi Arabian National Center for Science and Technology was established, with Prof. Rida M. S. This center was created as an independent scientific organization that is responsible for the promotion of science, however, the name was later changed into King Abdulaziz City for Science and Technology. In 1987, KACST has joined the International Council for Science as a National Member, in 1984, Abdul Rahman Al-Athel was named as the President of the city. In 2007, Mohammed Ibrahim Al-Suwaiyel, who used to be the KACST vice president for research, HH Dr. Turki AL Saud is the KACST vice president. This program was approved by the Council of Ministers in 2002 and this program has fifteen strategic technologies that will help the future development of Saudi Arabia. To achieve this goal, KACST started to work with the local and international organizations, for example, Nature Arabic Edition, KACST has collaborated with the Macmillan Publishers to translate Nature journal into Arabic. The print issues are available to qualified subscribers. Also, the contents of this journal will be online for free. Wiki Arabi, This is another project initiated by King Abdullahs Initiative for Arabic Content and this project aims to improve the content of the Arabic Wikipedia by translating the high-quality articles from other languages of Wikipedia. The first Wiki Arabi event was in 2010, where over 2000 articles were translated into Arabic, the second Wiki Arabi was in 2012. In 1988, KACST starts planning to develop technology in Saudi Arabia. Therefore, KACST decided to open the Atomic Energy Research Institute and this Institute will help Saudi Arabia to develop the nuclear power along with King Abdullah City for Atomic and Renewable Energy. Such as, SaudiComSat-1 and SaudiGeo-1 In 2006, KACST signed a agreement with CERN to participate in the construction of LINAC4 project. KACST engineers constructed a prototype of it. This prototype was then qualified at CERN, and now, KACST is working build up a high-energy physics community to participate in future CERN programs. In September 30,2008, KACST funded the team of Gravity Probe B. In 2012, KACST announced the first electrostatic accelerator in Saudi Arabia and this accelerator has been designed by the National Center of Mathematics and Physics. Information Technology requirements for research center and city staff is fulfilled by ITU section situated in building No.1, the King Abdulaziz City for Science and Technology operates the internet backbone in Saudi Arabia as well as the local registry address space
27.
Royal Astronomical Society
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The Royal Astronomical Society is a learned society that began as the Astronomical Society of London in 1820 to support astronomical research. It became the Royal Astronomical Society in 1831 on receiving its Royal Charter from William IV, a Supplemental Charter in 1915 opened up the fellowship to women. Meetings are held in Burlington House, in Piccadilly, London and they are involved in the production of astronomical journals and periodicals. The society has over 3000 members, around a third of whom live outside the UK, in addition, those members of the public who have an interest in astronomy and geophysics and wish to support the work of the society may become Friends of the RAS. One of the activities of the RAS is publishing refereed journals. It publishes two primary research journals, the Monthly Notices of the Royal Astronomical Society in astronomy and the Geophysical Journal International in geophysics and it also publishes the magazine A&G which includes reviews and other articles of wide scientific interest in a glossy format. Fellowship is open to anyone over the age of 18 who is considered acceptable to the society, as a result of the societys foundation in a time before there were many professional astronomers, no formal qualifications are required. However, around three quarters of fellows are professional astronomers or geophysicists, the society acts as the professional body for astronomers and geophysicists in the UK and fellows may apply for the Science Councils Chartered Scientist status through the society. The fellowship passed 3,000 in 2003, in 2009 an initiative was launched for those with an interest in astronomy and geophysics but without professional qualifications or specialist knowledge in the subject. Such people may join the Friends of the RAS, which offers popular talks, visits, ordinary meetings featuring lectures about research topics in astronomy and geophysics are normally held in Burlington House in London on the second Friday of every month from October through to May. Reports of the meetings appear in The Observatory magazine, scientific discussion meetings about particular research topics are held on the day of the ordinary meetings. These allow several speakers to present new research results and experts to present reviews of scientific fields, discussion meetings on two different topics within astronomy and geophysics frequently take place in parallel at different locations within Burlington House. The Society occasionally hosts meetings in other parts of the United Kingdom, the Society also sponsors the National Astronomy Meeting, a week-long general conference of professional astronomers, normally held each spring at a university campus in the United Kingdom. The Society holds occasional lunchtime public lectures in Central London aimed at a general, non-specialist, the Royal Astronomical Society has a more comprehensive collection of books and journals in astronomy and geophysics than the libraries of most universities and research institutions. The library receives some 300 current periodicals in astronomy and geophysics and its collection of astronomical rare books is second only to that of the Royal Observatory in Edinburgh in the UK. The RAS library is a resource not just for the society but also the wider community of astronomers, geophysicists. The society promotes astronomy to members of the public through their outreach pages for students, teachers. The RAS has a role in relation to UK public examinations, such as GCSEs
28.
Royal Swedish Academy of Sciences
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The Royal Swedish Academy of Sciences or Kungliga Vetenskapsakademien is one of the Royal Academies of Sweden. Every year the Academy awards the Nobel Prizes in Physics and Chemistry, the Sveriges Riksbank Prize in Economic Sciences in Memory of Alfred Nobel, the Crafoord Prize, the Academy has elected about 1.700 Swedish and 1.200 foreign members since it was founded in 1739. Hansson, appointed from 1 July 2015 The transactions of the Academy were published as its main series between 1739 and 1974, in parallel, other major series have appeared and gone, Öfversigt af Kungl. These lasted into the 1860s, when they were replaced by the single Bihang series, further restructuring of their topics occurred in 1949 and 1974. The purpose of the academy was to focus on practically useful knowledge, the academy was intended to be different from the Royal Society of Sciences in Uppsala, which had been founded in 1719 and published in Latin. The location close to the activities in Swedens capital was also intentional. The academy was modeled after the Royal Society of London and Academie Royale des Sciences in Paris, France, members of the Royal Swedish Academy of Sciences Official website Royal Swedish Academy of Sciences video site
29.
Russian Academy of Sciences
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Headquartered in Moscow, the Academy is considered a civil, self-governed, non-commercial organization chartered by the Government of Russia. It combines the members of RAS and scientists employed by institutions, the Academy currently includes around 650 institutions and 55,000 scientific researchers. There are three types of membership in the RAS, full members, corresponding members, and foreign members, Academicians and corresponding members must be citizens of the Russian Federation when elected. However, some academicians and corresponding members were elected before the collapse of the USSR and are now citizens of other countries, Members of RAS are elected based on their scientific contributions – election to membership is considered very prestigious. In the years 2005–2012, the academy had approximately 500 full and 700 corresponding members, but in 2013, after the Russian Academy of Agricultural Sciences and the Russian Academy of Medical Sciences became incorporated into the RAS, a number of the RAS members accordingly increased. As of November 2016, after the last elections, there were 944 full members and 1159 corresponding members in the renewed Russian Academy of Sciences, the RAS consists of 13 specialized scientific divisions, three territorial divisions, sometimes called branches, and 15 regional scientific centers. The Academy has numerous councils, committees, and commissions, all organized for different purposes, Siberian Division of the Russian Academy of Sciences The Siberian Division was established in 1957, with Mikhail Lavrentyev as founding chairman. Research centers are in Novosibirsk, Tomsk, Krasnoyarsk, Irkutsk, Yakutsk, Ulan-Ude, Kemerovo, Tyumen, as of 2005, the Division employed over 33,000 employees,58 of whom were members of the Academy. Ural Division of the Russian Academy of Sciences The Ural Division was established in 1932, research centers are in Yekaterinburg, Perm, Cheliabinsk, Izhevsk, Orenburg, Ufa and Syktyvkar. As of 2007, the Division employed 3,600 scientists,590 full professors,31 full members, started with just three members, The RSSI now has 3,100 members, including 57 from the largest research institutions. Russian universities and technical institutes are not under the supervision of the RAS, the Academy is also increasing its presence in the educational area. In 1990 the Higher Chemical College of the Russian Academy of Sciences was founded, the Academy gives out a number of different prizes, medals and awards among which, Lomonosov Gold Medal Lobachevsky Prize Demidov Prize Kurchatov Medal Pushkin Prize S. V. Expeditions to explore parts of the country had Academy scientists as their leaders or most active participants. A separate organization, called the Russian Academy, was created in 1783 to work on the study of the Russian language, presided over by Princess Yekaterina Dashkova, the Russian Academy was engaged in compiling the six-volume Academic Dictionary of the Russian Language. The Russian Academy was merged into the Imperial Saint Petersburg Academy of Sciences in 1841, in December 1917, Sergey Fedorovich Oldenburg, a leading ethnographer and political activist in the Kadet party, met with Vladimir Lenin to discuss the future of the Academy. They agreed that the expertise of the Academy would be applied to addressing questions of state construction, in 1925 the Soviet government recognized the Russian Academy of Sciences as the highest all-Union scientific institution and renamed it the Academy of Sciences of the USSR. The Soviet Sciences Academy would be affected like all universities by the rules imposed particularly those pertaining to censorship, the Soviet Science Academy ended up with a leader of the philosophy department who was placed there simply to keep the man out of trouble. The government decided to not execute or send the famous writer to the gulag because he had won the Stalin award, doing this would have discredited the Stalin award and thus Stalin the leader of the Communist party himself
30.
World War II
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World War II, also known as the Second World War, was a global war that lasted from 1939 to 1945, although related conflicts began earlier. It involved the vast majority of the worlds countries—including all of the great powers—eventually forming two opposing alliances, the Allies and the Axis. It was the most widespread war in history, and directly involved more than 100 million people from over 30 countries. Marked by mass deaths of civilians, including the Holocaust and the bombing of industrial and population centres. These made World War II the deadliest conflict in human history, from late 1939 to early 1941, in a series of campaigns and treaties, Germany conquered or controlled much of continental Europe, and formed the Axis alliance with Italy and Japan. Under the Molotov–Ribbentrop Pact of August 1939, Germany and the Soviet Union partitioned and annexed territories of their European neighbours, Poland, Finland, Romania and the Baltic states. In December 1941, Japan attacked the United States and European colonies in the Pacific Ocean, and quickly conquered much of the Western Pacific. The Axis advance halted in 1942 when Japan lost the critical Battle of Midway, near Hawaii, in 1944, the Western Allies invaded German-occupied France, while the Soviet Union regained all of its territorial losses and invaded Germany and its allies. During 1944 and 1945 the Japanese suffered major reverses in mainland Asia in South Central China and Burma, while the Allies crippled the Japanese Navy, thus ended the war in Asia, cementing the total victory of the Allies. World War II altered the political alignment and social structure of the world, the United Nations was established to foster international co-operation and prevent future conflicts. The victorious great powers—the United States, the Soviet Union, China, the United Kingdom, the Soviet Union and the United States emerged as rival superpowers, setting the stage for the Cold War, which lasted for the next 46 years. Meanwhile, the influence of European great powers waned, while the decolonisation of Asia, most countries whose industries had been damaged moved towards economic recovery. Political integration, especially in Europe, emerged as an effort to end pre-war enmities, the start of the war in Europe is generally held to be 1 September 1939, beginning with the German invasion of Poland, Britain and France declared war on Germany two days later. The dates for the beginning of war in the Pacific include the start of the Second Sino-Japanese War on 7 July 1937, or even the Japanese invasion of Manchuria on 19 September 1931. Others follow the British historian A. J. P. Taylor, who held that the Sino-Japanese War and war in Europe and its colonies occurred simultaneously and this article uses the conventional dating. Other starting dates sometimes used for World War II include the Italian invasion of Abyssinia on 3 October 1935. The British historian Antony Beevor views the beginning of World War II as the Battles of Khalkhin Gol fought between Japan and the forces of Mongolia and the Soviet Union from May to September 1939, the exact date of the wars end is also not universally agreed upon. It was generally accepted at the time that the war ended with the armistice of 14 August 1945, rather than the formal surrender of Japan
31.
Warsaw
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Warsaw is the capital and largest city of Poland. It stands on the Vistula River in east-central Poland, roughly 260 kilometres from the Baltic Sea and 300 kilometres from the Carpathian Mountains. Its population is estimated at 1.750 million residents within a metropolitan area of 3.101 million residents. The city limits cover 516.9 square kilometres, while the area covers 6,100.43 square kilometres. Once described as Paris of the East, Warsaw was believed to be one of the most beautiful cities in the world until World War II. On 9 November 1939, the city was awarded Polands highest military decoration for heroism, Warsaw is one of Europe’s most dynamic metropolitan cities. In 2012 the Economist Intelligence Unit ranked Warsaw as the 32nd most liveable city in the world, in 2017 the city came 4th in the “Business-friendly” category and 8th in the “Human capital and life style”. It was also ranked as one of the most liveable cities in Central, Warsaw is considered an Alpha– global city, a major international tourist destination and a significant cultural, political and economic hub. The city is a significant centre of research and development, BPO, ITO, the Warsaw Stock Exchange is the largest and most important in Central and Eastern Europe. Frontex, the European Union agency for external security, has its headquarters in Warsaw. Together with Frankfurt, London and Paris, Warsaw is also one of the cities with the highest number of skyscrapers in the European Union, the city is the seat of the Polish Academy of Sciences, Warsaw National Philharmonic Orchestra and the University of Warsaw. The historic city-centre of Warsaw with its picturesque Old Town in 1980 was listed as a UNESCO World Heritage Site, buildings represent examples of nearly every European architectural style and historical period. Warsaw provides many examples of architecture from the gothic, renaissance, baroque, neoclassical and modern periods, furthermore, the city is positioning itself as Europes chic cultural capital with thriving art and club scenes and renowned restaurants. Folk etymology attributes the city name to a fisherman, Wars, according to legend, Sawa was a mermaid living in the Vistula River with whom Wars fell in love. In actuality, Warsz was a 12th/13th-century nobleman who owned a village located at the site of Mariensztat neighbourhood. See also the Vršovci family which had escaped to Poland, the official city name in full is miasto stołeczne Warszawa. A native or resident of Warsaw is known as a Varsovian – in Polish warszawiak, warszawianin, warszawianka, warszawiacy, other names for Warsaw include Varsovia and Varsóvia, Varsovie, Varsavia, Warschau, װאַרשע /Varshe, Варшава /Varšava /Varshava, Varšuva, Varsó. The first fortified settlements on the site of todays Warsaw were located in Bródno, after Jazdów was raided by nearby clans and dukes, a new similar settlement was established on the site of a small fishing village called Warszowa
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Poland
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Poland, officially the Republic of Poland, is a country in Central Europe, situated between the Baltic Sea in the north and two mountain ranges in the south. Bordered by Germany to the west, the Czech Republic and Slovakia to the south, Ukraine and Belarus to the east, the total area of Poland is 312,679 square kilometres, making it the 69th largest country in the world and the 9th largest in Europe. With a population of over 38.5 million people, Poland is the 34th most populous country in the world, the 8th most populous country in Europe, Poland is a unitary state divided into 16 administrative subdivisions, and its capital and largest city is Warsaw. Other metropolises include Kraków, Wrocław, Poznań, Gdańsk and Szczecin, the establishment of a Polish state can be traced back to 966, when Mieszko I, ruler of a territory roughly coextensive with that of present-day Poland, converted to Christianity. The Kingdom of Poland was founded in 1025, and in 1569 it cemented a political association with the Grand Duchy of Lithuania by signing the Union of Lublin. This union formed the Polish–Lithuanian Commonwealth, one of the largest and most populous countries of 16th and 17th century Europe, Poland regained its independence in 1918 at the end of World War I, reconstituting much of its historical territory as the Second Polish Republic. In September 1939, World War II started with the invasion of Poland by Nazi Germany, followed thereafter by invasion by the Soviet Union. More than six million Polish citizens died in the war, after the war, Polands borders were shifted westwards under the terms of the Potsdam Conference. With the backing of the Soviet Union, a communist puppet government was formed, and after a referendum in 1946. During the Revolutions of 1989 Polands Communist government was overthrown and Poland adopted a new constitution establishing itself as a democracy, informally called the Third Polish Republic. Since the early 1990s, when the transition to a primarily market-based economy began, Poland has achieved a high ranking on the Human Development Index. Poland is a country, which was categorised by the World Bank as having a high-income economy. Furthermore, it is visited by approximately 16 million tourists every year, Poland is the eighth largest economy in the European Union and was the 6th fastest growing economy on the continent between 2010 and 2015. According to the Global Peace Index for 2014, Poland is ranked 19th in the list of the safest countries in the world to live in. The origin of the name Poland derives from a West Slavic tribe of Polans that inhabited the Warta River basin of the historic Greater Poland region in the 8th century, the origin of the name Polanie itself derives from the western Slavic word pole. In some foreign languages such as Hungarian, Lithuanian, Persian and Turkish the exonym for Poland is Lechites, historians have postulated that throughout Late Antiquity, many distinct ethnic groups populated the regions of what is now Poland. The most famous archaeological find from the prehistory and protohistory of Poland is the Biskupin fortified settlement, dating from the Lusatian culture of the early Iron Age, the Slavic groups who would form Poland migrated to these areas in the second half of the 5th century AD. With the Baptism of Poland the Polish rulers accepted Christianity and the authority of the Roman Church
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Nicolaus Copernicus
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Copernicus was born and died in Royal Prussia, a region that had been part of the Kingdom of Poland since 1466. A polyglot and polymath, he obtained a doctorate in law and was also a mathematician, astronomer, physician, classics scholar, translator, governor, diplomat. In 1517 he derived a quantity theory of money – a key concept in economics –, Nicolaus Copernicus was born on 19 February 1473 in the city of Toruń, in the province of Royal Prussia, in the Crown of the Kingdom of Poland. His father was a merchant from Kraków and his mother was the daughter of a wealthy Toruń merchant, Nicolaus was the youngest of four children. His brother Andreas became an Augustinian canon at Frombork and his sister Barbara, named after her mother, became a Benedictine nun and, in her final years, prioress of a convent in Chełmno, she died after 1517. His sister Katharina married the businessman and Toruń city councilor Barthel Gertner and left five children, Copernicus fathers family can be traced to a village in Silesia near Nysa. The villages name has been variously spelled Kopernik, Copernik, Copernic, Kopernic, Coprirnik, in the 14th century, members of the family began moving to various other Silesian cities, to the Polish capital, Kraków, and to Toruń. The father, Mikołaj the Elder, likely the son of Jan, Nicolaus was named after his father, who appears in records for the first time as a well-to-do merchant who dealt in copper, selling it mostly in Danzig. He moved from Kraków to Toruń around 1458, Nicolaus father was actively engaged in the politics of the day and supported Poland and the cities against the Teutonic Order. In 1454 he mediated negotiations between Polands Cardinal Zbigniew Oleśnicki and the Prussian cities for repayment of war loans, Copernicuss father married Barbara Watzenrode, the astronomers mother, between 1461 and 1464. The Modlibógs were a prominent Polish family who had been known in Polands history since 1271. The Watzenrode family, like the Kopernik family, had come from Silesia from near Świdnica and they soon became one of the wealthiest and most influential patrician families. Lucas Watzenrode the Elder, a merchant and in 1439–62 president of the judicial bench, was a decided opponent of the Teutonic Knights. In 1453 he was the delegate from Toruń at the Grudziądz conference that planned the uprising against them, Lucas Watzenrode the Younger, the astronomers maternal uncle and patron, was educated at the University of Kraków and at the universities of Cologne and Bologna. He was an opponent of the Teutonic Order, and its Grand Master once referred to him as the devil incarnate. In 1489 Watzenrode was elected Bishop of Warmia against the preference of King Casimir IV, as a result, Watzenrode quarreled with the king until Casimir IVs death three years later. Watzenrode was then able to close relations with three successive Polish monarchs, John I Albert, Alexander Jagiellon, and Sigismund I the Old. He was a friend and key advisor to each ruler, Watzenrode came to be considered the most powerful man in Warmia, and his wealth, connections and influence allowed him to secure Copernicus education and career as a canon at Frombork Cathedral
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Sydney
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Sydney /ˈsɪdni/ is the state capital of New South Wales and the most populous city in Australia and Oceania. Located on Australias east coast, the metropolis surrounds the worlds largest natural harbour, residents of Sydney are known as Sydneysiders. The Sydney area has been inhabited by indigenous Australians for at least 30,000 years, the first British settlers, led by Captain Arthur Phillip, arrived in 1788 to found Sydney as a penal colony, the first European settlement in Australia. Since convict transportation ended in the century, the city has transformed from a colonial outpost into a major global cultural. As at June 2016 Sydneys estimated population was 5,005,358, in the 2011 census,34 percent of the population reported having been born overseas, representing many different nationalities and making Sydney one of the most multicultural cities in the world. There are more than 250 different languages spoken in Sydney and about one-third of residents speak a language other than English at home and it is classified as an Alpha+ World City by the Globalization and World Cities Research Network, indicating its influence in the region and throughout the world. Ranked eleventh in the world for economic opportunity, Sydney has a market economy with strengths in finance, manufacturing. Its gross regional product was $337 billion in 2013, the largest in Australia, there is a significant concentration of foreign banks and multinational corporations in Sydney and the city is promoted as one of Asia Pacifics leading financial hubs. Its natural features include Sydney Harbour, the Royal National Park, man-made attractions such as the Sydney Opera House, Sydney Tower and the Sydney Harbour Bridge are also well known to international visitors. The first people to inhabit the now known as Sydney were indigenous Australians having migrated from northern Australia. Radiocarbon dating suggests human activity first started to occur in the Sydney area from around 30,735 years ago, the earliest British settlers called them Eora people. Eora is the term the indigenous used to explain their origins upon first contact with the British. Its literal meaning is from this place, prior to the arrival of the British there were 4,000 to 8,000 native people in Sydney from as many as 29 different clans. Sydney Cove from Port Jackson to Petersham was inhabited by the Cadigal clan, the principal language groups were Darug, Guringai, and Dharawal. The earliest Europeans to visit the area noted that the people were conducting activities such as camping and fishing, using trees for bark and food, collecting shells. Development has destroyed much of the citys history including that of the first inhabitants, there continues to be examples of rock art and engravings located in the protected Ku-ring-gai Chase National Park. The first meeting between the people and the British occurred on 29 April 1770 when Lieutenant James Cook landed at Botany Bay on the Kurnell Peninsula. He noted in his journal that they were confused and somewhat hostile towards the foreign visitors, Cook was on a mission of exploration and was not commissioned to start a settlement
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Australia
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Australia, officially the Commonwealth of Australia, is a country comprising the mainland of the Australian continent, the island of Tasmania and numerous smaller islands. It is the worlds sixth-largest country by total area, the neighbouring countries are Papua New Guinea, Indonesia and East Timor to the north, the Solomon Islands and Vanuatu to the north-east, and New Zealand to the south-east. Australias capital is Canberra, and its largest urban area is Sydney, for about 50,000 years before the first British settlement in the late 18th century, Australia was inhabited by indigenous Australians, who spoke languages classifiable into roughly 250 groups. The population grew steadily in subsequent decades, and by the 1850s most of the continent had been explored, on 1 January 1901, the six colonies federated, forming the Commonwealth of Australia. Australia has since maintained a liberal democratic political system that functions as a federal parliamentary constitutional monarchy comprising six states. The population of 24 million is highly urbanised and heavily concentrated on the eastern seaboard, Australia has the worlds 13th-largest economy and ninth-highest per capita income. With the second-highest human development index globally, the country highly in quality of life, health, education, economic freedom. The name Australia is derived from the Latin Terra Australis a name used for putative lands in the southern hemisphere since ancient times, the Dutch adjectival form Australische was used in a Dutch book in Batavia in 1638, to refer to the newly discovered lands to the south. On 12 December 1817, Macquarie recommended to the Colonial Office that it be formally adopted, in 1824, the Admiralty agreed that the continent should be known officially as Australia. The first official published use of the term Australia came with the 1830 publication of The Australia Directory and these first inhabitants may have been ancestors of modern Indigenous Australians. The Torres Strait Islanders, ethnically Melanesian, were originally horticulturists, the northern coasts and waters of Australia were visited sporadically by fishermen from Maritime Southeast Asia. The first recorded European sighting of the Australian mainland, and the first recorded European landfall on the Australian continent, are attributed to the Dutch. The first ship and crew to chart the Australian coast and meet with Aboriginal people was the Duyfken captained by Dutch navigator, Willem Janszoon. He sighted the coast of Cape York Peninsula in early 1606, the Dutch charted the whole of the western and northern coastlines and named the island continent New Holland during the 17th century, but made no attempt at settlement. William Dampier, an English explorer and privateer, landed on the north-west coast of New Holland in 1688, in 1770, James Cook sailed along and mapped the east coast, which he named New South Wales and claimed for Great Britain. The first settlement led to the foundation of Sydney, and the exploration, a British settlement was established in Van Diemens Land, now known as Tasmania, in 1803, and it became a separate colony in 1825. The United Kingdom formally claimed the part of Western Australia in 1828. Separate colonies were carved from parts of New South Wales, South Australia in 1836, Victoria in 1851, the Northern Territory was founded in 1911 when it was excised from South Australia
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Rome
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Rome is a special comune and the capital of Italy. Rome also serves as the capital of the Lazio region, with 2,873,598 residents in 1,285 km2, it is also the countrys largest and most populated comune and fourth-most populous city in the European Union by population within city limits. It is the center of the Metropolitan City of Rome, which has a population of 4.3 million residents, the city is located in the central-western portion of the Italian Peninsula, within Lazio, along the shores of the Tiber. Romes history spans more than 2,500 years, while Roman mythology dates the founding of Rome at only around 753 BC, the site has been inhabited for much longer, making it one of the oldest continuously occupied sites in Europe. The citys early population originated from a mix of Latins, Etruscans and it was first called The Eternal City by the Roman poet Tibullus in the 1st century BC, and the expression was also taken up by Ovid, Virgil, and Livy. Rome is also called the Caput Mundi, due to that, Rome became first one of the major centres of the Italian Renaissance, and then the birthplace of both the Baroque style and Neoclassicism. Famous artists, painters, sculptors and architects made Rome the centre of their activity, in 1871 Rome became the capital of the Kingdom of Italy, and in 1946 that of the Italian Republic. Rome has the status of a global city, Rome ranked in 2014 as the 14th-most-visited city in the world, 3rd most visited in the European Union, and the most popular tourist attraction in Italy. Its historic centre is listed by UNESCO as a World Heritage Site, monuments and museums such as the Vatican Museums and the Colosseum are among the worlds most visited tourist destinations with both locations receiving millions of tourists a year. Rome hosted the 1960 Summer Olympics and is the seat of United Nations Food, however, it is a possibility that the name Romulus was actually derived from Rome itself. As early as the 4th century, there have been alternate theories proposed on the origin of the name Roma. There is archaeological evidence of occupation of the Rome area from approximately 14,000 years ago. Evidence of stone tools, pottery and stone weapons attest to about 10,000 years of human presence, several excavations support the view that Rome grew from pastoral settlements on the Palatine Hill built above the area of the future Roman Forum. Between the end of the age and the beginning of the Iron age. However, none of them had yet an urban quality, nowadays, there is a wide consensus that the city was gradually born through the aggregation of several villages around the largest one, placed above the Palatine. All these happenings, which according to the excavations took place more or less around the mid of the 8th century BC. Despite recent excavations at the Palatine hill, the view that Rome has been indeed founded with an act of will as the legend suggests in the middle of the 8th century BC remains a fringe hypothesis. Traditional stories handed down by the ancient Romans themselves explain the earliest history of their city in terms of legend and myth
