• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
8th GRADE SCIENCE - Norwin School District
8th GRADE SCIENCE - Norwin School District

... The student will be able to… Calculate various work problems Compare and contrast natural and artificial satellites Compare and contrast rotation and revolution of Earth Explain how Earth’s revolution and tilt cause seasons Diagram the phases of the Moon Compare/contrast the conditions that lunar an ...
1 Intro to Astronomy
1 Intro to Astronomy

... – geocentrism: all the objects in the sky revolve about the earth and are fixed to a series of nested spheres, some of which are transparent, maybe made of crystal, which spin once per day; the stars may just be holes in the otherwise opaque sphere, letting sunlight through → If you don't have today ...
Solar System - HMXEarthScience
Solar System - HMXEarthScience

... C) They exert the same gravitational force on each other. D) They have elliptical orbits with the Sun at one focus. 37. The actual shape of the Earth's orbit around the Sun is best described as A) a very eccentric ellipse C) an oblate spheroid ...
gravity
gravity

... In the diagram , if we call gravitational force exerted on the apple action, what is the reaction force according to Newton’s 3rd law? a. It is the apple gravitationally pulling on the Earth. b. It is the apple pressing on the table. c. The apple exerts no reaction force. d. It is the table support ...
Astronomy Curriculum
Astronomy Curriculum

... elective, with elements of physics and mathematics, intended for those students who wish to further explore their interests in physical science. Students in astronomy will develop the skills to observe and record objects in the sky, aided by various elements of observational technology such as binoc ...
m02a01
m02a01

... You may have noticed that the dates corresponding to each zodiacal constellation are not the same as the dates commonly quoted for “star signs”. In the next Activity, we will investigate why this is so. Another question may have occurred to you: when the Sun is “in” Aquarius, for example, Aquarius ...
Ancient astronomy Part 8
Ancient astronomy Part 8

... medicine wheels demonstrated accurate observation, but calendars had little place ...
The Crust
The Crust

... Distance from Sun Width of asteroid belt (million km) ...
March 2013 - Joliet Junior College
March 2013 - Joliet Junior College

... The Vernal Equinox (start of spring) is on March 20th at 6:02 am. Since the first day of winter, the sun has been crossing the sky slightly higher every day. On the equinox the sun is directly above the Earth’s equator and will begin shining above the northern hemisphere until next September. On the ...
June - astra
June - astra

... Newsletter Editor – John Endreson, [email protected]; ...
Cycles: Earth, Sun, Moon by MTDavis
Cycles: Earth, Sun, Moon by MTDavis

... ONE ROTATION of the earth on it’s axis = ONE DAY ONE MOON CYCLE =about 29.5 DAYS, which should be ONE MONTH. 12 X 29.5 = 354 days, 11 days short of the real SOLAR CALENDAR, so Julius Caesar, with the help of Greek science, changed our months to 30 or 31 day months which no longer match the moon cyc ...
1 A future news release might report that a new planet has been
1 A future news release might report that a new planet has been

... 7) Mars cannot sustain liquid water on its surface because ___________its atmospheric pressure is too low________. Short Essay Questions (choose 1 of each pair of essay questions below): 1A) Define, describe and discuss the theory about the origins of our universe from the Big Bang. 1B) Define, desc ...
Study Guide #3 Answer Key
Study Guide #3 Answer Key

... light-years.[22] The distance from the Sun to the galactic center is now estimated at 26,000 ± 1400 light-years, while older estimates could put the Sun as far as 35,000 light-years from the central bulge. The galactic center harbors a compact object of very large mass as determined by the motion of ...
Earth-Moon-Sun System (seasons, moon phases
Earth-Moon-Sun System (seasons, moon phases

... During the northern hemisphere’s summer (when the axis points towards the Sun), it receives sunlight for a longer time (longer days, shorter nights) as well as more directly. (The Sun is higher in the sky, so it hits the surface more directly.) Moving from the equator to the poles, the length of th ...
$doc.title

... transits  every  4.4  days,  causing  the  starlight  to  dim  by  a  factor  of  1.7%  over  a  period  of  4.1  hr.   Kepler’s  third  law  gives  the  planet’s  semimajor  axis  as  a  =  0.056  AU.  From  this  information, ...
PHYSICS CHAPTER 8 : Universal Gravitation
PHYSICS CHAPTER 8 : Universal Gravitation

... Brahe was not known for his sunny disposition, so in 1597, out of favor with the new Danish king, Brahe moved to Prague. He became the astronomer to the court of Emperor Rudolph of Bohemia where, in 1600, a nineteenyear-old German Johannes Kepler (1571-1630) became one of his assistants. Although Br ...
Part 1
Part 1

... Universe (all space, all matter, all energy). Age of the Earth is ………………………………….. (see ESRT p. ...
Loops of Jupiter
Loops of Jupiter

... the map he gets surprised by the fact that there are no orbits of planets marked there. Finally he finds out that planets appear in the sky regularly and periodically but each time in a different place. Therefore, for each planet only a zone in the sky, in which the planet appears, could be marked o ...
Chapter 9
Chapter 9

... What type of galaxy is shown below? ...
Chapter 9
Chapter 9

... What type of galaxy is shown below? ...
this PDF file
this PDF file

... (iii) We all know/expect that many current and next-generation astronomical instruments are/will be equipped with polarimetric capabilities. But it is more surprising to learn that even smartphones may turn into spectropolarimeters that can be used by anyone to perform measurements of aerosols in th ...
Frostburg State Planetarium presents
Frostburg State Planetarium presents

... • East is about where sun rises each morning. • South is where sun is highest in sky (in mid day) • West is about where sun sets each afternoon. ...
etlife_exoplanets - University of Glasgow
etlife_exoplanets - University of Glasgow

... The distance from the Earth to the Sun is 150 million km. It takes sunlight more than eight minutes to travel this ...
Space Review Questions answers
Space Review Questions answers

... up of all the different colors of the rainbow. When light goes through a prism, it changes speed, and that speed change splits up the colors so they are not all mixed together. White light goes in, gets broken up, and the separate color components emerge. Like the prism, the gasoline is making it po ...
The Inner Planets
The Inner Planets

... Since Venus takes 7.5 Earth months to revolve around the sun and 8 months to rotate once on its axis, a day on Venus is longer than its year. Venus also rotate east to west, the only planet to do so. This retrograde rotation (backward) was probably caused by Venus being struck by a large object earl ...
< 1 ... 153 154 155 156 157 158 159 160 161 ... 311 >

Geocentric model



In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report