t

This scientist determined the nature of the forces that kept the planets in their orbits.

This scientist determined the nature of the forces that kept the planets in their orbits.

What term describes the apparent path of the sun upon the celestial sphere?

When I’m inspired to write something for the internet, I occasionally use a search engine to see if it’s already been done (and if it has, I won’t have to write it). In this case, my goal was to demonstrate the futility of using metaphysical theories to “fill in the gaps” in scientific knowledge. The following are some obvious examples:
Those ideas seemed to be too simple, at least to those who actually think about such things. On these thoughts, I found a plethora of commentary, parody, and satire, and one spoof “theory” already has a name: “Intelligent Falling Theory” (IFT). Now, I’d seen this theory mocked before, but I had no idea it had already swept the internet and turned into a “phenomenon” of various satirical parodies of the “intelligent design” concept. An article on Wikipedia called Intelligent Falling is a good place to start learning about IFT. Evangelical Scientists Refute Gravity With New ‘Intelligent Falling’ Theory from The Onion is the one I like best.

The belt of constellations through which all the planets move is called the ________.

The geocentric model (also known as geocentrism, and sometimes exemplified by the Ptolemaic system) is a superseded description of the Universe with Earth at its core in astronomy. The Sun, Moon, stars, and planets all orbited Earth in the geocentric model. 1st In several ancient cultures, such as Aristotle’s Classical Greece and Ptolemy’s Roman Egypt, the geocentric model was the prevailing explanation of the universe.
For over 1500 years, the astronomical predictions of Ptolemy’s geocentric model, established in the 2nd century CE, have been used to prepare astrological and astronomical charts. The geocentric model reigned supreme until the late 16th century, when it was eventually supplanted by Copernicus (1473-1543), Galileo (1564-1642), and Kepler’s heliocentric model (1571-1630). The transition between these two hypotheses was met with a lot of opposition. Some believed that a modern, unknown theory could not overthrow the geocentric consensus.

The apparent path of the sun upon the celestial sphere is called the

Johannes Kepler (/kplr/;[2]) was a German mathematician. [johans kpl, -ns -] in German (take a listen);[3] [number four] He was a German astronomer, mathematician, and astrologer who lived from December 27, 1571, to November 15, 1630. He is best known for his laws of planetary motion and his books Astronomia nova, Harmonices Mundi, and Epitome Astronomiae Copernicanae, which he wrote during the 17th century scientific revolution. These studies have laid the groundwork for Newton’s universal gravitational theory.
Kepler worked as a mathematics teacher at a seminary school in Graz, where he met Prince Hans Ulrich von Eggenberg and became friends with him. Later, he worked as an assistant to Tycho Brahe, an astronomer in Prague, and then as the imperial mathematician to Emperor Rudolf II and his two successors Matthias and Ferdinand II. He also served as an advisor to General Wallenstein and taught mathematics in Linz.
In addition, he made important contributions to optics, developed an improved version of the refracting (or Keplerian) telescope, and was listed in Galileo Galilei’s telescopic discoveries. He was a Rome’s Accademia dei Lincei corresponding member. (5)

The true shape of the planetary orbits was discovered by ________.

Johannes Kepler was a German mathematician and astronomer who discovered the Earth’s and planets’ elliptical orbits around the sun. He outlined three basic laws of planetary motion. He has made significant contributions to optics and geometry.
Johannes Kepler is best known for discovering the three Kepler laws of planetary motion, which were published in 1609 and 1619. He also did important work in optics (1604, 1611), discovered two new regular polyhedra (1619), gave the first mathematical treatment of close packing of equal spheres (leading to an explanation of the shape of the cells in a honeycomb, 1611), gave the first proof of how logarithms worked (1624), and devised a method of finding the volumes of solids of revolution that (with hindsight!) can be used as a method of finding the volumes of solids of revolution that (1615, 1616). Furthermore, he determined the most precise astronomical tables ever established, whose continued precision contributed significantly to the validation of heliocentric astronomy (Rudolphine Tables, Ulm, 1627).