the law of universal gravitation, an explanation of the nature of light, and methods of differential and integral calculus.
We can not help but say, perhaps, about the most famous Apple that fell next to the great scientist, prompting him to study the laws of falling. All his life, Newton was inspired by the great minds of the past – Descartes, Galileo and Kepler, and many of his works are based on their work. Conducting optical experiments, Newton built a mixed telescope-reflector, which in addition to its large size gave a 40-fold magnification. Rumors of the new instrument reached London, and after demonstrating his invention to the king, Newton became famous and in January 1672 was elected a fellow of the Royal society. Later, it was with an improved model of the Newtonian telescope that other galaxies, the planet Uranus, and redshifts were discovered. By 1687, Newton’s main work was published – “Mathematical principles of natural philosophy”, in which he summed up all his works, forming the law of universal gravitation, which described the gravitational interaction, and the three laws of motion.
The law of universal gravitation States that the force of gravitational attraction F between two immaterial points with masses m1 and m2 separated by a distance r acts along the line connecting them, is proportional to both masses and inversely proportional to the square of the distance.
Three laws of motion:
Newton’s first law: “Every body continues to be held in its state of rest or uniform and rectilinear motion, until and insofar as it is not forced by applied forces to change this state.”
Newton’s second law: “In an inertial frame of reference, the speed of change in the momentum of a material point is equal to the resultant of all external forces applied to it.”
Newton’s third law: “Action always has an equal and opposite reaction, otherwise – the interaction of two bodies on each other are equal and directed in opposite directions.”
These laws helped answer the question about the hypothetical acceleration of The earth’s satellite. Newton knew that the acceleration of the moon in orbit is 0.27 m/s2, and the degree of its orbit is 60 times the radius of the Earth. According to his calculations, the acceleration of a low satellite, that is, all objects on Earth, should exceed the acceleration of the moon by 602 = 3600 times. Using the law of gravity, Newton multiplied 0.27 by 3600 and obtained the famous acceleration of gravity g, equal to 9.8 m/s2.
In 1689 Newton was first elected to Parliament, and again in 1701. Isaac performed his parliamentary duties with the same conscientiousness with which he handled all matters. Written by Newton in 1704, the book “Optics”, in which he described the seven colors of the rainbow as the main colors of the spectrum, became the basis of this field of physics for the next hundred years. For his contribution to the development of science, the English Queen made Newton a knight. Isaac Newton was a very versatile man – in addition to physics, astronomy, and mathematics, he studied alchemy, theology, optical phenomena, and the theory of the ether (a hypothetical all-pervading medium). It was Newton who came up with the idea of making the edges of coins ribbed so that fraudsters could not cut off pieces of metal from them. Despite poor health in childhood, Isaac Newton lived for a full 84 years, dying in 1727, he was not married and left no descendants, but his students and followers made great discoveries in many areas of science.
PIERRE SIMON LAPLACE
For his many achievements in astronomy, physics, and mathematics, Laplace was nicknamed the French Newton. Pierre Simon Laplace was born in 1749 in the family of a farmer in Normandy. In 1765, Laplace entered the University of Caen. The first work of Laplace was associated with the theory of gambling. In the autumn of 1770, having given up his career as a priest and decided to devote himself to science, Laplace came to Paris. In 1773, he was admitted to the Paris Academy of Sciences, and in the same year his fundamental work was published – “On the principle of universal gravitation and on the age-old inequalities of the planets that depend on it”. Laplace was one of the first to openly declare that there should be no God in science, even if you believe in him. Because of the beginning of revolutionary unrest in France, Laplace was forced to flee Paris. In the small town of Melun near Paris, Pierre Simon wrote a book “Exposition of the system of the world”, in which he collected all the astronomical knowledge of the XVIII century, without using a single formula. But the main thing – in this book, Laplace presented his hypothesis of the origin of the Solar system. He suggested that the Solar system was born out of a hot gas nebula that surrounded the young Sun. As it cooled, the nebula began to shrink, and due to the rapid rotation, the centrifugal forces became comparable to gravity, and the nebula flattened, becoming a disk that began to break into rings. The matter in each ring began to thicken, becoming a protoplanet. This theory has existed for more than 100 years, but had a number of significant drawbacks. Also in his book, Pierre Simon came to the conclusion that there are bodies in the Universe with such a huge mass that even light can not leave them. Such bodies are now called black holes. Despite the armed coups in France, Laplace continued to work hard, becoming a member of most of the European academies, and in 1808, he became a member of the French Academy of Sciences. Napoleon, as Emperor, gave Laplace the title of count of the Empire. After the fall of Napoleon and the restoration of the Bourbon dynasty, Laplace received the title of Marquis, became a peer of France, and was awarded the highest order of the Legion of Honor. In 1827, Laplace fell ill and died at the age of 77. His last words were: “What we know is so insignificant compared to what we don’t know.”
WILLIAM HERSCHEL
In observational astronomy, William Herschel can be called Columbus, because he was the first with his telescope to go beyond our galaxy, expanding the Solar system and “moving” the Sun. William was born in 1738 in Germany in the family of a musician of the Hanoverian guard. From the age of 15, he played in the same orchestra on the violin, organ and oboe, the latter of which is the most complex instrument. In 1757, when the seven Years’ war began, the Anglo-Prussian army was defeated at the battle of Hastenbeck, and Herschel fled to England, for which he was accused of desertion. Herschel changed his name to English and quickly learned English. His musical interest led him to mathematics, which led him to optics, and optics to astronomy. From the age of 35 to the end of his life, he devoted himself entirely to astronomy. His observations of cosmic double stars and numerous works laid the Foundation for the modern theory of double stars. In 1781 William Herschel discovered a new planet in the Solar system – Uranus, for which he received the Copley medal, which is considered the oldest and most prestigious award of the Royal society of London, and in 1782 was awarded the Copley medal. He was given the title of astronomer by the king.
12-meter focal length telescope
Having assembled dozens of advanced telescopes, the largest of which is a 12-meter focal length telescope, Herschel studied deep space objects, discovering more than 2,400 such objects, known as nebulae. In addition to Uranus, Herschel discovered four other objects in the Solar system: in 1789, two moons of Saturn, Mimas and Enceladus, and in 1787, two moons of Uranus, Titania and Oberon. Herschel was the first to express the idea of the evolution of cosmic matter under the influence of gravitational forces. For almost 40 years, he observed sunspots and recorded their number, shape, and size. Herschel also hypothesized that the milky
