PowerPoint Presentation - Welcome to Modern Astronomy Fall 2003
... Welcome to Modern Astronomy Fall 2007 • Initial pleasantries, who I am, who you are • This should be the most interesting course you take in college • National Solar Observatory ...
... Welcome to Modern Astronomy Fall 2007 • Initial pleasantries, who I am, who you are • This should be the most interesting course you take in college • National Solar Observatory ...
Observing the Universe 1
... from the Earth, east to west, west to east, north to south or south to north. (a) Sun ...
... from the Earth, east to west, west to east, north to south or south to north. (a) Sun ...
Observing
... Declination -The coordinates do not move or vary with location on the Earth, they are fixed to the stars ...
... Declination -The coordinates do not move or vary with location on the Earth, they are fixed to the stars ...
Chapter 28 Notes
... • Copernicus’ heliocentric model – 1543, Polish scientist – Planets (including Earth) orbit the Sun in circular orbits – Supporting evidence collected by Tycho Brahe ...
... • Copernicus’ heliocentric model – 1543, Polish scientist – Planets (including Earth) orbit the Sun in circular orbits – Supporting evidence collected by Tycho Brahe ...
Washington State Standards Substantiated By STC Gems Kit: Space
... Unit 4: Why Do We Have Moon Phases and Eclipses? 4.1: Observing the Moon 4.2: Finding Patterns in Moon Observations 4.3; Understanding Moon Phases 4.4: Understanding Eclipses of the Moon and Sun 4.5: Impossible Missions ...
... Unit 4: Why Do We Have Moon Phases and Eclipses? 4.1: Observing the Moon 4.2: Finding Patterns in Moon Observations 4.3; Understanding Moon Phases 4.4: Understanding Eclipses of the Moon and Sun 4.5: Impossible Missions ...
un Facts About Venus F
... It’s named after the Roman goddess of love and beauty. It’s the only planet named after a female. It has no moons or rings Unlike most other planets, it rotates clockwise (retrograde rotation). Billions of years ago its climate may have been similar to Earth One day on Venus is longer than one year ...
... It’s named after the Roman goddess of love and beauty. It’s the only planet named after a female. It has no moons or rings Unlike most other planets, it rotates clockwise (retrograde rotation). Billions of years ago its climate may have been similar to Earth One day on Venus is longer than one year ...
Chapter 10
... Sun, Moon and stars Using a compass and an astrolabe, they were able to describe the position of any celestial body in relation to the direction North as well as in relation to the ...
... Sun, Moon and stars Using a compass and an astrolabe, they were able to describe the position of any celestial body in relation to the direction North as well as in relation to the ...
KS2 Earth and Space
... huge the distances involved are. Pupils will learn about how gravity keeps our solar system together. We then focus in to the Earth with pupils exploring the rotation of the Earth, day, night and shadows by getting hands-on with globes and torches. Pupils can see at first hand why it is that differe ...
... huge the distances involved are. Pupils will learn about how gravity keeps our solar system together. We then focus in to the Earth with pupils exploring the rotation of the Earth, day, night and shadows by getting hands-on with globes and torches. Pupils can see at first hand why it is that differe ...
Unit 2 Study Guide - Effingham County Schools
... 25. Why is gravity important to the solar system? It holds everything in their orbits. 26. This terrestrial planet (Venus) has the densest atmosphere and this terrestrial planet (Mercury) does not have any atmosphere. 27. Name the terrestrial planets. Mercury, Venus, Earth, and Mars 28. Venus’ atmo ...
... 25. Why is gravity important to the solar system? It holds everything in their orbits. 26. This terrestrial planet (Venus) has the densest atmosphere and this terrestrial planet (Mercury) does not have any atmosphere. 27. Name the terrestrial planets. Mercury, Venus, Earth, and Mars 28. Venus’ atmo ...
The Universe Starring Man? The Impact of Scientific
... Theory and Evidence: back to the Copernican Revolution • In fact all the evidence is compatible with both theories • Nonetheless 3 pieces of evidence in particular were – rightlytaken to indicate that the Ptolemaic theory was false. • Order of the planets • Planetary stations and retrogressions • B ...
... Theory and Evidence: back to the Copernican Revolution • In fact all the evidence is compatible with both theories • Nonetheless 3 pieces of evidence in particular were – rightlytaken to indicate that the Ptolemaic theory was false. • Order of the planets • Planetary stations and retrogressions • B ...
Astronomy Objective 1 1. An asteroid is a small, rocky object that
... 6. A comet is a small body of ice, rock, and cosmic dust that follows an elliptical orbit around the sun that gives off gases and dust in the form of a tail as it passes close to the sun. 7. A constellation is one of 88 regions into which the sky is divided in order to describe locations of celestia ...
... 6. A comet is a small body of ice, rock, and cosmic dust that follows an elliptical orbit around the sun that gives off gases and dust in the form of a tail as it passes close to the sun. 7. A constellation is one of 88 regions into which the sky is divided in order to describe locations of celestia ...
Lecture 4, PPT version
... upon it and noticing that same star placed close to the stars which antiquity attributed to Cassiopeia. When I had satisfied myself that no star of that kind had ever shone forth before, I was led into such perplexity by the unbelievability of the thing that I began to doubt the faith of my own eyes ...
... upon it and noticing that same star placed close to the stars which antiquity attributed to Cassiopeia. When I had satisfied myself that no star of that kind had ever shone forth before, I was led into such perplexity by the unbelievability of the thing that I began to doubt the faith of my own eyes ...
The Earth in Space
... • Voyager 1 = 14 light hours away; took 32 years (1977) to get there - .0017 ly away - 38,400 mph ...
... • Voyager 1 = 14 light hours away; took 32 years (1977) to get there - .0017 ly away - 38,400 mph ...
Lesson 2_GoingSolar
... million kilometers closer to the sun during January than in July. The change in Earth’s distance from the sun doesn’t affect ...
... million kilometers closer to the sun during January than in July. The change in Earth’s distance from the sun doesn’t affect ...
Today`s Powerpoint
... But if you support geocentric model, you must attribute retrograde motion to actual motions of planets, leading to loops called “epicycles”. ...
... But if you support geocentric model, you must attribute retrograde motion to actual motions of planets, leading to loops called “epicycles”. ...
Section 17.1 - CPO Science
... and all objects that are gravitationally bound to the sun. • The solar system is roughly divided into the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and ...
... and all objects that are gravitationally bound to the sun. • The solar system is roughly divided into the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and ...
Chapter 6 Study Guide
... 15. The times when day and night are of equal length are called ______________________. 16. The force that pulls the moon toward Earth is called ___________________________. 17. If you are in a car that stops suddenly, your body keeps moving because it has ...
... 15. The times when day and night are of equal length are called ______________________. 16. The force that pulls the moon toward Earth is called ___________________________. 17. If you are in a car that stops suddenly, your body keeps moving because it has ...
File
... arguing in favor of a heliocentric (Sun-centered) solar system, titled, “On the Revolutions of the Celestial Spheres.” Perhaps fearing reprisals, he didn’t have his book published until his death, in 1543, and he dedicated it to Pope Paul III. ...
... arguing in favor of a heliocentric (Sun-centered) solar system, titled, “On the Revolutions of the Celestial Spheres.” Perhaps fearing reprisals, he didn’t have his book published until his death, in 1543, and he dedicated it to Pope Paul III. ...
The Science of Life in the Universe (Chap 2
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
The Science of Life in the Universe (Chap 2
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
Discussion of Chapter 2 Material
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
The Science of Life in the Universe (Chap 2
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
Topic 3: Astronomy
... rotation: the turning of an object on its axis revolution: the movement of a body in orbit around an object Models of the Universe Geocentric (“Earth-centered”) models proposed by Aristotle, Ptolemy - the Earth is located at the center of the universe and does not move - the stars are fixed on a t ...
... rotation: the turning of an object on its axis revolution: the movement of a body in orbit around an object Models of the Universe Geocentric (“Earth-centered”) models proposed by Aristotle, Ptolemy - the Earth is located at the center of the universe and does not move - the stars are fixed on a t ...
The Science of Life in the Universe (Chap 2
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
Discussion of Chapter 2 Material
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
... Given that we discover a civilization around other stars, let’s examine the closest that such a civilization could be from the Earth. The nearest star is 4.3 light years distant from Earth. This means that a two-way ...
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.