Because European Union was created.
Explanation:
- The Treaty on European Union, often referred to as the Maastricht Treaty, was signed on 7 February 1992 and entered into force on 1 November 1993.
- On the basis of this Treaty, the Member States established the European Union and thus marked a new stage in the integrating "the people of Europe into an ever firmer union, in which decisions are made as close as possible to the citizens."
- The Treaty establishes a European Union consisting of three pillars: the Community Pillar, a common foreign and security policy and cooperation in the field of justice and home affairs (today police and judicial cooperation in criminal matters), sets the goals of economic and monetary union, establishes EU citizenship, Community competence introduces social policy and integrates trans-European networks, industrial policy, consumer protection, education, youth and culture into common policies.
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Answer: the most reasonable one is B.
Explanation:
The correct answer is the Canadian Rebellion
It was an event in 1837 in which the Lower and Upper Canada had a series of rebellions against Britain because of the way they were treated as colonies. This brought them on the Brink of war with the United States for various reasons, mostly about Britain controlling areas on the New World and the fact that Canada didn't look the same as it does today.
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Copernican heliocentrism is the name given to the astronomical model developed by Nicolaus Copernicus and published in 1543. This model positioned the Sun at the center of the Universe, motionless, with Earth and the other planets orbiting around it in circular paths, modified by epicycles, and at uniform speeds. The Copernican model displaced the geocentric model of Ptolemy that had prevailed for centuries, which had placed Earth at the center of the Universe. Copernican heliocentrism is often regarded[by whom?] as the launching point to modern astronomy and the Scientific Revolution.
Heliocentric model from Nicolaus Copernicus' De revolutionibus orbium coelestium (On the Revolutions of the Heavenly Spheres)
Although he had circulated an outline of his own heliocentric theory to colleagues sometime before 1514, he did not decide to publish it until he was urged to do so late in his life by his pupil Rheticus. Copernicus's challenge was to present a practical alternative to the Ptolemaic model by more elegantly and accurately determining the length of a solar year while preserving the metaphysical implications of a mathematically ordered cosmos. Thus, his heliocentric model retained several of the Ptolemaic elements, causing inaccuracies such as the planets' circular orbits, epicycles, and uniform speeds,[1] while at the same time introducing such innovative ideas as:-
The Earth is one of several planets revolving around a stationary sun in a determined order.
The Earth has three motions: daily rotation, annual revolution, and annual tilting of its axis.
Retrograde motion of the planets is explained by the Earth's motion.
The distance from the Earth to the Sun is small compared to the distance from the Sun to the stars.
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