• 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
eratoshenes_earth_measurement
eratoshenes_earth_measurement

... In the field of geodesy, however, Eratosthenes will always be remembered for his measurements of the Earth. A firm believer of a spherical Earth, he made a surprisingly accurate measurement of the circumference of the Earth. Details were given in his treatise On the measurement of the Earth which is ...
Lec 11 Galileo I Tel..
Lec 11 Galileo I Tel..

...  Avicenna (defending Aristotle…) had said if planets/stars received their light from the sun, phases would be visible, varying according to distance from the Sun  Albert of Saxony: (ad hoc defense of Aristotle…) replies that we don’t see phases because Venus and Mercury are transparent and absorb ...
Kiss of the goddess | The Economist
Kiss of the goddess | The Economist

... astronomers to map out much of the solar system, but everything was measured in terms of the distance from Earth to the sun, which was itself poorly known. In Kepler's day this distance, called the “astronomical unit”, was estimated to be about 8m kilometres. By Halley's time the consensus was 111m ...
Comets, Asteroids, and Meteors
Comets, Asteroids, and Meteors

... Mars and Jupiter. They named these objects Ceres, Pallas, Juno, and Vesta. Over the next 80 years, astronomers found over 300 more. These rocky objects, called asteroids, are too small and too numerous to be considered planets. Most asteroids revolve around the sun between the orbits of Mars and Jup ...
Chapter 9 Gravitation continued
Chapter 9 Gravitation continued

... Can you feel gravity? We previously determined that you can’t. 1) Hanging from a 100 m high diving board – your arms feel stretched by the upward force of bent board. 2) Standing on a bed – your legs feel compressed by the compressed springs in the mattress. The bent diving board or the compressed s ...
1 The Solar System - e
1 The Solar System - e

... Have you carefully observed the sun, moon and the other celestial bodies in the sky? There is evidence that man had shown an interest in knowing about them since ancient times. At present man can explore more than what is visible to the naked eye, as scientists have invented modern equipment to obs ...
Astronomy Club of Asheville June 2016 Sky Events
Astronomy Club of Asheville June 2016 Sky Events

... and Saturn will reign in the southeast.  Against the background of the constellation Leo, Jupiter is best viewed this month well before midnight, while it is still high in the sky.  Mars reached opposition (opposite the Sun from Earth) on May 22nd; so it’s nearest to Earth for the year, making thi ...
The celestial sphere, the coordinates system, seasons, phases of
The celestial sphere, the coordinates system, seasons, phases of

... precisely due east and sets precisely due west. ...
pompton lakes high school - Pompton Lakes School District
pompton lakes high school - Pompton Lakes School District

... movement of celestial bodies, nuclear forces within stars govern its evolution through the processes of stellar birth and death. These same processes governed the formation of our solar system 4.6 billion years ago. Essential Questions  What were the major discoveries that Galileo made concerning t ...
Space Notes - Holy Cross Collegiate
Space Notes - Holy Cross Collegiate

...  Objects in the sky have fascinated humans throughout time. The explanations of how these celestial objects came to be are even more fascinating.  Ancients developed their ideas of what was happening in the sky and explained it with their frame of reference.  The constellations were patterns that ...
pompton lakes high school - Pompton Lakes School District
pompton lakes high school - Pompton Lakes School District

... movement of celestial bodies, nuclear forces within stars govern its evolution through the processes of stellar birth and death. These same processes governed the formation of our solar system 4.6 billion years ago. Essential Questions  What were the major discoveries that Galileo made concerning t ...
Pre-Final Quiz Answers
Pre-Final Quiz Answers

... K (potassium-40) decays to 40Ar (argon-40) through nuclear capture of an electron and to 40Ca (calcium-40) through emission of a β particle. The decay half-life is approximately 1.26 billion years. The oldest rocks on Earth show ages of about 4 billion years. If a zircon crystal in these rocks forme ...
Revision sheet - Nour Al Maaref International School
Revision sheet - Nour Al Maaref International School

... A. Centripetal force is a force that makes a body follow a curved path. B. Centripetal force is a force that makes objects move in straight lines. C. Centripetal force is a force that is directed away from a center of rotation. D. Centripetal force is a force in which a smaller body acts on a larger ...
NATS1311_112008_bw
NATS1311_112008_bw

... - it increases the energy (heat) in lower atmosphere - it works like a blanket - it slows the escape of heat In the absence of the Greenhouse Effect, what would determine a planet’s surface temperature? - the planet's distance from the Sun - the planet’s overall reflectivity - the higher the albedo ...
Chapter 4: Making Sense of the Universe
Chapter 4: Making Sense of the Universe

... At any given time, how many high tides are there on Earth? A. One B. Two C. There may be none or one, depending on what time of day D. None, one, or two– depending on the time of day ...
Astronomical and Physical Sciences
Astronomical and Physical Sciences

... because comets contain too much heavy hydrogen, relatively rare in Earth’s oceans. Comets also contain too much argon. If comets were the source of only 1% of Earth’s water, then, using evolutionists’ assumptions, our atmosphere would contain 400 times more argon than it does. The few types of meteo ...
The Prague Astronomical Clock
The Prague Astronomical Clock

... 21 and September 23, respectively. On these days, the lengths of day and night are equal. The Ecliptic and the Zodiac As the Earth travels around the Sun, the Sun appears to be rising from a celestial background that changes over the course of the year. The apparent path of the Sun through the sky i ...
Chapter 1 Our Place in the Universe
Chapter 1 Our Place in the Universe

... • With Earth’s axis tilted by 23.5º (pointing to close to Polaris) It rotates in the same direction it orbits, counterclockwise as viewed from above the North Pole. The Earth orbital path defines a flat plane called the Ecliptic. The ecliptic is also the apparent path of the Sun in the celestial sph ...
Measuring Stellar Distances
Measuring Stellar Distances

... Measuring the parallactic ellipse (or parallactic angle) is difficult and the first credible measurement was not made until 1839. In general, atmospheric motions limit the angular resolution of a single ground-based image (photographic or digital) to an accuracy of 0.5 - 1.0 arc seconds which is not ...
2010 AP Gravitation Notes
2010 AP Gravitation Notes

... 14. Two artificial satellites, 1 and 2, orbit the Earth in circular orbits having radii R1 and R2, respectively, as shown above. If R2 = 2R1, the accelerations a2 and a1 of the two satellites are related by which of the following? (A) a2 = 4a1 (B) a2 = 2a1 (C) a2 = a1 (D) a2 = a1/2 (E) a2 = a1/4 ...
Explore the Planets
Explore the Planets

... the Sun in our Solar System. It is the planet we evolved on and the only planet in our Solar System that is known to support life. From a distance, our planet looks like a beautiful big blue marble. There are a number of things that make our planet unique in the solar system, not the least of which ...
Habitable Zone - Wando High School
Habitable Zone - Wando High School

... And at some point 4.1 bya, these conditions were met for the first time. But what was necessary for this to happen on Earth? There seem to be a few requirements of that a planet must meet in order to be habitable for life. First, the planet must fall inside the Habitable Zone. As you can see in the ...
Lec21_2D
Lec21_2D

... When a terrestrial planet enters its flooding stage, gases trapped inside the during formation (or created as a result of radioactive decay) will be outgassed. These gases include  H2, He, H2O, N2, CO2, and probably CH4 and NH3 As the planet cools, water vapor condenses out of the atmosphere and fa ...
Our Star: The Sun
Our Star: The Sun

... corona constantly and are unleashed into the solar system.  The matter in the corona is constantly ...
Extrasolar Planets = 403
Extrasolar Planets = 403

... Solar System Looks Like a Disk • As the planet’s distance from the sun increases; its period of revolution about the sun increases & velocity decreases • The planets revolve in orbits that are tilted less than 7° • Planets orbit in same direction ...
< 1 ... 98 99 100 101 102 103 104 105 106 ... 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