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ПІДВЕДЕННЯ ПІДСУМКІВ КОНКУРСУ ТА НАГОРОДЖЕННЯ ПЕРЕМОЖЦІВ.
Додаток №5.
ЗАВДАННЯ ДО ОЛІМПІАДИ З ДИСЦИПЛІНИ «ІНОЗЕМНА МОВА»
АУДІЮВАННЯ
Інструкція.
Прослухайте уважно двічі текст.
ALBERT EINSTEIN
On March 29, 1919, there was an eclipse of the Sun. It was a particularly important eclipse. For years astronomers had eagerly awaited it, since it would enable them to check a revolutionary new theory in physics, proposed four years earlier by a scientist named Albert Einstein.
On the day of the eclipse one group of astronomers was stationed in Northern Brazil, another on an island of the western coast of Africa. Delicate cameras were set up and waiting. Pictures would be taken during the eclipse – not of the eclipsed Sun, but of the 8tars that appear in the suddenly darkened sky around the Sun.
Einstein had said that the position of the stars would be somewhat changed, since the rays of starlight passing near the Sun would be bent by the Sun's mass. To many scientists this sounded impossible. How could light, which was immaterial, they argued, be affected by gravity? If Einstein were correct, the picture of the Universe built up by the great Newton more than two hundred years earlier would have to be considerably revised.
The eclipse came. The pictures were taken and developed. The distances of the stars from the Sun and from one another were carefully measured. There could be no doubt about the results. Einstein was right. The light rays had been bent by the attraction of the Sun. One of the key points of Einstein's theory had been experimentally confirmed.
It was said that only twelve persons in the world really understood exactly at that time what Einstein meant in his theory of relativity. Yet throughout the civilized world everyone who read the newspapers knew that Einstein was a genius, that he had overthrown the foundations on which physics, chemistry and astronomy had rested for two hundred years, and upset all earlier concepts of the Universe. Later they learned that this revolution had made possible the development of the photoelectric cell, television, a whole series of electronic inventions, and, finally, the harnessing of atomic energy.
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