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The Sun Video Focus Questions
The Sun Video Focus Questions

... Answers: 1. The sun is the largest body in our solar system, and it makes up about 99% of the solar system (more than all the other planets, comets, and asteroids combined.) 2. It takes the Earth 365 days to orbit the sun. 3. Copernicus and Galileo changed the way we view the universe today by provi ...
Matter is everything around you.
Matter is everything around you.

... for the most part, described the longitude and latitude lines of the earth. He was a believer that the earth was the centre of the universe and worked to advance this theory. The Ptolemaic system is explained why some planets seemed to move backwards for periods of time in their orbit around earth. ...
Astronomical Imaging: Overview
Astronomical Imaging: Overview

... to keep the object in the field of view: – camera/telescope moves from East to West – axis of rotation points at celestial pole (at Polaris in northern hemisphere) ...
Group 1 Notes for Week 8 - UGA Physics and Astronomy
Group 1 Notes for Week 8 - UGA Physics and Astronomy

... qualitatively. So, an explanation for the origin of the solar system must take into account these differences. There is also a gap in between these planets, physically – the asteroid belt, between 2-4 AU from the Sun. The planets beyond that are fairly well spaced out. So, the raw materials are diff ...
Study of the movement of the sun through the analysis of a shade.
Study of the movement of the sun through the analysis of a shade.

... The aim of this scientific project is to explore the sun shade along the academic year. The sun is a constant presence in our lifes, but we normally don’t pay attention to its movement neither to the changes in its positions in the different seasons. This research projects will allow the students to ...
HW: PSI Gravity Problems Worksheet With Answers
HW: PSI Gravity Problems Worksheet With Answers

... A) is cut to one fourth. B) is cut in half. C) doubles. D) quadruples 2. Two objects, with masses m1 and m2, are originally a distance r apart. The magnitude of the gravitational force between them is F. The masses are changed to 2m1 and 2m2, and the distance is changed to 4r. What is the magnitude ...
PSI AP Physics 1 Gravitation
PSI AP Physics 1 Gravitation

... A) is cut to one fourth. B) is cut in half. C) doubles. D) quadruples 2. Two objects, with masses m1 and m2, are originally a distance r apart. The magnitude of the gravitational force between them is F. The masses are changed to 2m1 and 2m2, and the distance is changed to 4r. What is the magnitude ...
Mon Aug 5, 2013 QUASAR DISCOVERY Quasars were discovered
Mon Aug 5, 2013 QUASAR DISCOVERY Quasars were discovered

... What’s the most distant star you can see? In 1987, there was a supernova in the Large Magellanic Cloud. It appeared as a 2nd magnitude star, (about the brightness of one of the stars of the Big Dipper,) and could be seen easily with the unaided eye. That star was about 160,000 light years away – tha ...
Astronomy I – Vocabulary you need to know:
Astronomy I – Vocabulary you need to know:

... Hour angle – The angle measured westward along the celestial equator from the local meridian to the hour circle passing through an object. Meridian - An imaginary north-south line in the sky that passes through the observer's zenith. Precession – The small wobbling motion around the Earth's axis tha ...
Vampy Astronomy Syllabus
Vampy Astronomy Syllabus

... Describe three important features of a telescope and rank them in order of importance. Construct a basic telescope using mostly materials that can be easily purchased at a hardware store. Use spectroscopy to identify elements. State the nebular theory for the formation of stars and planets. Provide ...
Document
Document

... • Difficult to observe • Hundreds discovered (> 2000 so far) Circa 2013, Courtesy Kepler: Billions!! • Jupiter to Earth sizes • Surprise: Some stars with Jupiter mass planets within 1 AU (revised theory of planet formation ?) • Goldilocks Zone: Habitable Distance out to ...
NATS 1311-From the Cosmos to Earth
NATS 1311-From the Cosmos to Earth

... The idea that scientists should prefer the simpler of two models that agree equally well with observations - the second hallmark - after medieval scholar William of Occam (1285 - 1349). For instance, original model of Copernicus (Sun-centered) did not match the data noticeably better than Ptolemy's ...
For stars
For stars

... Earth. • When m = M, then the star is located exactly 10 pc away • When mM, then the star appears dimmer than it would if it were 10 pc away so it must be farther than 10 pc ...
Formation of Solar System
Formation of Solar System

... The basis of the models that are popular now is the idea that Sun and planets all formed from the same material. Differences in composition arise during the formation of the system. [Does not preclude a mixture of these ideas] ...
Key 3 - UNLV Physics
Key 3 - UNLV Physics

... (c) looking at the change in velocity of a star from its spectra (d) looking at locations near stars for planets 36. Which of the following describes the Transit Method of detecting planets? (a) looking for reduced light as a planet passes between us and the star. (b) looking for the change in posit ...
April 2016 - Newbury Astronomical Society
April 2016 - Newbury Astronomical Society

... solid black line marked as: ‘North Celestial Pole’ and ‘South Celestial Pole’ is the tilted axis of rotation of Earth. The angle between Solar System axis and the Celestial Axis (Earth’s axis of rotation) marked as: ‘Axial tilt or Obliquity’ is the 23.4° tilt as discussed on the previous pages. The ...
Teacher`s Guide The Solar Empire: A Star is Born
Teacher`s Guide The Solar Empire: A Star is Born

... In 1989, solar events caused a blackout in Quebec. Discuss this event and other ways that activities on the sun, such a magnetic storms and solar flares, affect our environment and activities on Earth. How might this influence change as the sun continues to evolve? ...
4. Survey Observations
4. Survey Observations

... • Astronomers choose longitude to 
 increase to the right (to the east; 
 counter-clockwise looking 
 down on the north pole) ...
6th Grade Great Barrier Reef
6th Grade Great Barrier Reef

... The Universe: Big and Getting Bigger!  Beyond the Milky Way, there are billions more stars in the galaxies that are our closest neighbors.  One of our close neighbors is the Andromeda galaxy, but don’t expect to travel there soon.  Even though Andromeda is closer to us than most other galaxies, i ...
Orbit by Tega Jessa Everything in the universe circles or “orbits
Orbit by Tega Jessa Everything in the universe circles or “orbits

... presented argument against the geocentric model was introduced. The opposing theory was proposed by Nicolaus Copernicus and gave mankind its first taste of heliocentric cosmology, the view that the Sun was the center about which other celestial bodies orbited. About half a century later, Johannes Ke ...
Fourth Grade Earth in the Universe - K
Fourth Grade Earth in the Universe - K

... • 1.E.1 Recognize the features and patterns of the earth/moon/sun system as observed from Earth. • 1.E.1.1 Recognize differences in the features of the day and night sky and apparent movement of objects across the sky as observed from Earth. • 1.E.1.2 Recognize patterns of observable changes in the ...
The Motion of the Moon and Planets
The Motion of the Moon and Planets

... Why don’t we have an eclipse at every new and full moon? – The Moon’s orbit is tilted 5° to ecliptic plane… – So we have about two eclipse seasons each year, with a lunar eclipse at new moon and solar eclipse at full moon. ...
the text the talk here
the text the talk here

... remained in Athens for twenty years. Aristotle founded his own school, the Lyceum, which was more scientific than the Academy. In order to understand the physical universe, Aristotle looked for causes, which back then was a novel idea. The book that Raphael’s Aristotle is holding is the Nicomachean ...
Document
Document

... little bit smaller than Fg (down) because the car starts to lift just a little bit off the track because it wants to continue in a straight line path as it goes over the top ii) If the car travels fast over the top FN is directed downwards because the car actually lifts a lot off the track but a sec ...
Across 2. a slightly cooler region on the surface of the sun, caused
Across 2. a slightly cooler region on the surface of the sun, caused

... when two stars appear to be next to each other but can actually be very far apart ...
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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.
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