Geocentric/Heliocentric

Slides:



Advertisements
Similar presentations
Motion through the universe
Advertisements

Topic IV: Motions of the Earth, Moon and Sun
Actual Earth Motions.
Section 2: Movements of the Earth
Unit III: The Earth in Space
Motions of the Earth, Moon and Sun
Topic 4 Motions of the Earth, Moon, and Sun
Apparent Motions of Celestial Objects
MOTIONS OF EARTH, MOON AND SUN
26.2 Movements of Earth.
Celestial Observations
Astronomy.
Aim: What are the apparent motions of the stars and planets?
Motions of Earth, Moon, and Sun. Apparent Motions of Celestial Objects An apparent motion is a motion that an object appears to make. Apparent motions.
The Earth in Space Ch 26.
Trivia Question of the Day. Astronomy Picture of the Day Astronomy Picture of the Day.
Concept 3: Longitude and earth’s rotation I. Rotation is the spinning of an object on its axis (imaginary.
Chapter 4 - Space Lesson 17: Earth Movements – Rotation and Revolution.
Space, Earth and Celestial Objects © Lisa Michalek.
Earth’s Motions in Space
Chapter 6: Earth’s Motions in Space Ms. Johnson Foundations.
Unit 4 Motions of Earth, Moon, and Sun. Apparent Motions of Celestial Objects Apparent Apparent motion is the motion an object appears to make. Can be.
SOLAR SYSTEM MODELS  EARTH CENTERED SYSTEM DEVELOPED BY PTOLEMY  WAS ACCEPTED UNTIL THE 1960’S  SUN CENTERED SYSTEM DEVELOPED BY COPERNICUS  MODERN.
Intro to Astronomy Ch 26. Value of Astronomy Astronomy: the scientific study of the universe Scientists who study the universe are called astronomers.
Aim: What are some celestial and terrestrial observations? A. Celestial Object Object – any object observed in the sky during the day or night (ex: stars,
Astronomy Final Review. Geocentric Model --Earth is in the center of the system and everything revolves around it.
TOPIC 4. How does the Earth rotate? The Earth spins on its axis which, is an imaginary line through the planet from the north to the south pole.
Celestial Objects and Motions
EARTH IN SPACE. A reminder about earth  The earth is almost a sphere  We locate points on the sphere with 3 coordinates – Longitude (180º W º.
Grade 8.  Parallax  Perihelion  Aphelion  Seasons  Summer Solstice  Tropic of Cancer  Winter Solstice  Tropic of Capricorn  Vernal Equinox 
Astronomy: Apparent Motions Making sense of celestial observations.
Geocentric Model Heliocentric Model Did you know???? (do not write)  It wasn’t until 1851 that experimental proof of the motion of Earth was found.
Earth and Space Science
Rotation and Revolution
Don’t Write What is in Green. Geocentric Model.
Movements of the Earth Chapter Rotation vs. Revolution  Rotation = The spinning of the Earth on its axis.  This is what gives us our days.  Revolution.
The Universe. A Celestial Object is any object in our universe above our atmosphere. A Celestial Object is any object in our universe above our atmosphere.
New observations lead to changes in scientific theory What’s wrong with the image on the right, which shows Ptolemy’s popular scientific theory 2000 years.
EARTH’S MOTIONS Week of March 28 th. BELLRINGER: MARCH 28 TH List some evidence you are aware of or that you experience that proves Earth is moving.
22 Chapter 22 Origin of Modern Astronomy Starter 1.Compare and contrast the geocentric and heliocentric models. 2.Describe Kepler’s three laws of planetary.
Think About It: For 1,700 years what did we believe about the Earth and the Sun and their motions? Why did we believe that? For 1,700 years what did we.
Geocentric Model Earth centered solar system Old model – disproven.
 .
Question of the Day What is the Shape of Earth’s Orbit?
Why do our seasons change?
How does the geocentric model differ from the heliocentric model?
Earths Motions Objectives:
Rotation and Revolution
Aim: What are the apparent motions of the stars and planets?
Rotation and Revolution
Astronomy Motions of the Earth and Sun
Astronomy
TOPIC 3 EARTH MOTIONS.
Earth Among the Stars Earth Rotates… Earth rotation causes…
I think: ______________
Why do our seasons change?
Assignment 3: Sun, Earth, and moon
For most of human history, people thought ALL celestial objects rose in the East, moved across the sky at 150 per hour and set in the west. But its really.
Geocentric vs. Heliocentric Models
Mr. Ahearn Earth Science 2010
Chapter 24.1 Planet Earth.
Earth Motions Astronomy Page 8 ©Mark Place,
Earth Motions ©Mark Place,
Why do our seasons change?
EARTH'S MOTION.
Rotation (Ro ‘Day’ tion)
Earth Motions Astronomy Page 8 ©Mark Place,
EARTH'S MOTION.
Earth Motions.
Aim: How is the Earth moving?
Presentation transcript:

Geocentric/Heliocentric

Models to Explain Motion Geocentric Model – Earth centered. Planets, stars, and other objects revolve around Earth. This model was able to explain the apparent motion of the stars, sun, and moon. Could not explain retrograde motion and foucault pendulum motion.

Retrograde Motion Retrograde motion is an apparent motion of planets (over weeks to months) when they appear to change position with respect to the background field of stars.

Retrograde Motion Cont… Retrograde motion is caused by Earth and other planets revolution around the Sun in different orbits at different speeds.

Retrograde Motion of the Planets Note: outer planets are slower http://www.flex.com/~jai/astrology/retrograde.html

Models to Explain Motion Heliocentric Model – Sun centered. Earth rotates on an imaginary axis and revolves around the Sun. The Moon revolves around Earth. Explained all of the observations made by the scientists including retrograde motion.

Actual Earth Motion Rotation – Earth spins on its axis from west to east at 15 degrees per hour. The Sun, Moon, stars appears to move across the sky at a rate of 15 degrees per hour. The Foucault pendulum and the Coriolis Effect confirm Earth’s rotation.

Foucault Pendulum A pendulum is a freely swinging weight. Over a day, the direction of motion of a pendulum will appear to change. Actually, Earth is rotating under the pendulum.

Coriolis Effect Coriolis Effect - the bending of winds and currents due to the rotation of Earth. Northern Hemisphere, they bend to the right. Southern Hemisphere, they bend to the left.

Evidence of revolution Different constellations throughout the year. Earth’s Revolution Earth revolves around the Sun once a year. It revolves approx. 1° per day. Earth is closest to the Sun on January 3rd. This is called the perihelion. Earth is farthest to the Sun on July 3rd. This is called the aphelion. Evidence of revolution Seasons Different constellations throughout the year.

http://www.onr.navy.mil/focus/spacesciences/observingsky/sun2.htm