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Sir Isaac Newton and the scientific method
Isaac Newton's contribution to science
Isaac Newton's contribution to science
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Recommended: Sir Isaac Newton and the scientific method
After Isaac Newton algebraically found the speed of sound, he discovered that his answer varied from the answer found in the direct experiment done by William Derham. Newton was 15% off from the observed speed of sound. In an attempt to make fix his error, he took into account that air was composed of more than just oxygen and temperature fluctuated, but he was still off and his reasoning was confusing and illogical. Newton practically lied about his calculated speed of sound. Of the scientists that are taught in schools, Isaac Newton is one of them. Isaac Newton is one of the more well known scientists, while William Derham is not. Other well known scientists include: Albert Einstein and Leonardo Da Vinci, but what about the lesser known scientists. …show more content…
He determined that an invisible line that connected the planet to the sun were equal in area over the same amount of time (see figure 2), this was his second law, the Law of Areas.
Figure 2: A visual description of Kepler’s second law. Two shapes have been drawn by selecting four points a planet could be and then drawing a line to the center of the sun, the areas of the two shapes are equal.
Kepler’s third law, the Law of Periods, it states that the relationship between the period of two planets is connected to their distance from the sun. Kepler said that the square of the period was proportional to the cube of the radius of the planet (see figure 3). Figure 3: A visual description of Kepler’s third law, where T is the period of the planet, G is the gravitational constant (6.67 * 10 -11),
M is the mass of the planet, and a is semi-major axis.
Along with Kepler’s three laws of planetary motion, also determined that refraction drives vision in the eye and that using two eyes enables depth perception, with this knowledge, he made eyeglasses and explained how telescopes work. Kepler also claimed that gravity was caused by two bodies instead of one, that the sun rotates, and he created the word
1) A stationary body will stay stationary unless an external force is applied to it; 2) Force is equal to mass times acceleration, and a change in motion is proportional to the force applied; and 3) For every action, there is an equal and opposite reaction. (Bio.org, 2017) He invented the optics which he helped to inspire the build of the
So from that facts and his theory to solve the planet problem, he explained the retrograde motion. (Retrograde motion is actually an optical illusion because it appears to go backward as Earth passes).
Isaac Newton discovered gravity when an apple had fallen on his head. He then began to think about how the apple had fallen onto his head and thus Newton’s three laws of motion were created. Newton’s first law of motion is an object in motion tends to stay in motion; an object at rest tends to stay at rest, unless another force is acted upon it. Newton’s second law of motion is about the formula for force, which is force= mass*acceleration. Newton’s third law of motion is for every action there is an equal and opposite reaction. Furthermore, Isaac Newton created the three laws of motion.
Sir Isaac Newton made an enormous amount of contributions to the world of physics. He invented the reflecting telescope, proposed new theories of light and color, discovered calculus, developed the three laws of motion, and devised the law of universal gravitation. His greatest contribution to physics was the development of the three laws of motion. The first law was called the law of inertia; this law stated that, “Every object persists in its state of rest or uniform motion in a straight line unless it is compelled to change that state by forces impressed upon it.” The second law is called the law of acceleration; this law stated that, “Force is equal to the chan...
The first record of the movement of the planets was produced by Nicolaus Copernicus. He proposed that the earth was the center of everything, which the term is called geocentric. Kepler challenged the theory that the sun was the center of the earth and proposed that the sun was the center of everything; this term is referred to as heliocentric. Kepler’s heliocentric theory was accepted by most people and is accepted in today’s society. One of Kepler’s friends was a famous person named Galileo. Galileo is known for improving the design and the magnification of the telescope. With improvement of the telescope Galileo could describe the craters of the moon and the moons of Jupiter. Galileo also created the number for acceleration of all free falling objects as 9.8 meters per second. Galileo’s and Kepler’s theories were not approved by all people. Their theories contradicted verses in the bible, so the protestant church was extremely skeptical of both Galileo and Kepler’s
Johannes Kepler was a German astronomer and mathematician ho discovered that planetary motion is elliptical. Early in his life, Kepler wanted to prove that the universe obeyed Platonistic mathematical relationships, such as the planetary orbits were circular and at distances from the sun proportional to the Platonic solids (see paragraph below). However, when his friend the astronomer Tycho Brahe died, he gave Kepler his immense collection of astronomical observations. After years of studying these observations, Kepler realized that his previous thought about planetary motion were wrong, and he came up with his three laws of planetary motion. Unfortunately, he did not have a unifying theory for these laws. This had to until Newton formulated his laws of gravity and motion.
Isaac Newton’s story of how an apple falling from a tree that hit his head inspired him to formulate a theory of gravitation is one that all school children grow up hearing about. Newton is arguably one of the most influential scientific minds in human history. He has published books such as Arithmetica Universalis, The Chronology of Ancient Kingdoms, Methods of Fluxions, Opticks, the Queries, and most famously, Philosophiæ Naturalis Principia MathematicaHe formulated the three laws of gravitation, discovered the generalized binomial theorem, developed infinitesimal calculus (sharing credit with Gottfried Wilhelm Von Leibniz, who developed the theory independently), and worked extensively on optics and refraction of light. Newton changed the way that people look at the world they live in and how the universe works.
The three laws of motion are three rules that explain the motion of an object. The first law is the law of inertia. It states that every object remains at rest unless it is compelled by an external force. The second law is the law of acceleration. This law shows when there is a change in force, it causes a change in velocity. Finally, the third law states that every force in nature has an equal and opposite reaction. His discovery in calculus help confirms his second law of motion. Calculus also gave Isaac Newton powerful ways to solve mathematical problems. Lastly, for the color spectrum, he produced a beam of light from a tiny hole in a window shade. He placed a glass prism in front of the beam of light creating a color spectrum. In Newton’s undergraduate days, Newton was greatly influenced by the Hermetic tradition. After learning about the Hermetic tradition it influenced him to look at a different perspective into his discoveries and theories. One of the myths that followed the discovery is his discovery of universal gravitation. It is said that while Isaac Newton was thinking about the forces of nature, an apple fell on his head and he found the theory of gravity. There is no evidence that an apple fell on Newton’s head, but the evidence is shown that Newton got an idea of the theory of gravity when he saw an apple fall from a tree. During his life; however, Isaac Newton faced many obstacles. When he published some of his ideas in Philosophical Transaction of the Royal Society, some people challenged his ideas such as Robert Hooke and Christiaan Huygens to a point where Newton stopped publishing his work. During his life, he also suffered a nervous breakdown in a period of his life. He was convinced his friends were conspiring against him, and he couldn’t sleep at all for five
Copernicus was a scientist and philosopher whose theory proposed that the sun was stationary, and the heavens orbit around the sun. Galileo tried to convince the Church not to abolish the Copernican theory but was told that he was not to entertain such thoughts with others.... ... middle of paper ... ...(n.d.).
Later after Copernicus came Johannes Kepler and Galileo Galilei, who confirmed some of Copernicus’ observations. Kepler provided concise evidence of planetary motion regarding their path around the s...
Johannes Kepler was a German astronomer and mathematician who lived between 1671-1630. Kepler was a Copernican and initially believed that planets should follow perfectly circular orbits (“Johan Kepler” 1). During this time period, Ptolemy’s geocentric theory of the solar system was accepted. Ptolemy’s theory stated that Earth is at the center of the universe and stationary; closest to Earth is the Moon, and beyond it, expanding towards the outside, are Mercury, Venus, and the Sun in a straight line, followed by Mars, Jupiter, Saturn, and the “fixed stars”. The Ptolemaic system explained the numerous observed motions of the planets as having small spherical orbits called epicycles (“Astronomy” 2). Kepler is best known for introducing three effectual, applicable and valid laws of planetary motion by using the precise data he had developed from Tycho Brahe, a Danish astronomer, which helped Copernicus’s theory of the solar system gain universal reception (“Johan Kepler” 1). Nevertheless, he had made further effective contributions in the field of astronomy, which are valid to society and were used to change how the universe was perceived.
Johannes Kepler is now remembered for discovering the three laws of planetary motion, and writing about them in books that were published in 1609 and 1619. He also did important work in optics, discovered two new regular polyhedra, gave the first mathematical treatment of close packing of equal spheres, gave the first proof of how logarithms worked, and devised a method of finding the volumes of solids of revolution. This can be seen as contributing to the development of calculus. Not only did he help the development of calculus, but he calculated the most exact astronomical tables known today. This accuracy did much to establish the truth of heliocentric astronomy, which states that the sun, and not the earth, was the center of the planetary system.
Next, he saw four moons of Jupiter revolving around the Jupiter. Although, these discoveries did not prove the Copernicus’s theory, they gave framework for thinking universe in the new terms. He thought perhaps earth’s moon also revolves around the planet while the earth orbits around the sun. His another observation was that the Venus itself had phases like the moon had, even though the planet always appeared as a bright spot from the earth. (Strano 23-9). Moreover, in “Dialogue Concerning the Two Chief World Systems,” the astronomer Galileo Galilei did not prove that earth revolves around the sun or rotates in its axis, but he did prove Ptolemy was wrong about the arrangement of the planets (Gingerich 141). Thereafter, Galileo wanted to Earth was moving, not the sun, and he got his answer by observing ocean tides. “Galileo explains how the observed motion of the sea is a direct consequence of the two absolute motions of the earth in space: its axial rotation and its orbital motion about the sun” (Naylor 11-5). In short, he argues that the motion of earth cause tidal waves to move. The book was popular in its time before Roman Catholic church banned it. The church had an issue with Galileo supporting
Much to the dismay of the Church, two astronomers Galileo and Kepler had the audacity to challenge the authorities by suggesting that the sun-not the earth-was at the center of the universe. The church had a stronghold on the way the spiritual and physical world worked, so these discoveries only added to the Church’s resistance to their aims. Their discoveries came only after Kepler and Galileo began to question ancient theories about how the world functioned. These ancient truths were widely held but were inconsistent with the new observations that they had made. Kepler had discovered the laws of planetary motion which suggested that the planet would move in elliptical orbits, while Galileo followed with his discovery of the principle of inertia. Galileo concluded his finding b...
.... Throughout the book Ptolemy compared his own observations with those of Hipparchus, regarding the motion of the sun; Ptolemy found the lengths of the seasons and introduced a simple model for the sun which was a circular motion of uniform angular velocity however the earth would be displaced from the center referred to as eccentricity. He also used his own observations and those of Hipparchus to show that the fixed stars always maintain the same position relative to each other. Concerning his planetary theory, according to his model the path of a planet consisted of a circular motion on an epicycle while the center of the epicycle moving around a circle whose was offset from the earth. It is important to mention that the planetary theory introduces by Ptolemy was considered to be a noticeable achievement, since it predicted the motion of the planets fairly well.