Method: by Ancient Greeks

Slides:



Advertisements
Similar presentations
Astronomy 1 – Winter 2011 Lecture 4; January
Advertisements

Observational Astronomy. Astronomy from space Hubble Space Telescope.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 5.
History of Astronomy The knowledge of the Ancients.
Models of the Solar System (C) Copyright all rights reserved
Ancient Astronomers Egyptians Egyptians Babylonians Babylonians Native Americans Native Americans Chinese Chinese Celts Celts Many Others Many Others.
Celestial Sphere Stars seem to be on the inner surface of a sphere surrounding the Earth.
Chapter 1: Origins of Modern Astronomy
From Aristotle to Newton The history of the Solar System (and the universe to some extent) from ancient Greek times through to the beginnings of modern.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
Greek Science II Fundamental Issues and Theories.
Historical Astronomy 10000BC-3000BC 10000BC –constellations, lunar cycle, discovery of planets? –calendar refinements for agriculture –counting schemes.
January 10, 2006Astronomy Chapter 1 Observing the Sky: The Birth of Astronomy What do we see when we look at the sky? Why did people look at the.
Astronomy Picture of the Day. Question The Moon has a(n) ________ orbit meaning ________. A. synchronous, its orbital period is equal to its rotation.
The Science of Astronomy Astronomy – understanding what happens in the sky Astrophysics – understanding what happens in space.
Solar Eclipse Size of Sun, Earth, etc. Lecture 6.
Question 1 Constellations appear to move across the sky at night because 1) the Earth orbits the Sun. 2) the Moon orbits the Earth. 3) stars are in constant.
Greek Astronomy. Ancient View of the Cosmos  Universe is 2-D  All celestial objects attached to a sphere.  Celestial Sphere is close  Climb a high.
Motions of the Earth and Sky Part II. Depending on the relative sizes and distances of the Sun and a moon, you might see an eclipse like this: Sun planet.
The Earth-Moon-Sun System
Motion of the Moon.
NATS From the Cosmos to Earth Our first exam will be Tuesday, September 23 at the regular class time. We will have a review today at 1:00 PM in.
A survey of the solar system Michael Balogh The solar system (PHYS 275)
AST 112 Motion of Objects in the Sky. The Celestial Sphere Imagine you’re where Earth is, but there’s no Earth. What do you see? Keep in mind: – Nearest.
Origin of Modern Astronomy
Sponge: List the five Moon phases. What are waxing and waning?
Ancient Cosmology Monday, September 29. geocentric For 2000 years, geocentric model for the universe was widely assumed. Spherical Earth at center of.
Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2013.
Problem Solving. Reminder: Quantitative Reasoning Amazingly powerful tool to understand the world around us Fundamentals: –Ratios –Graphs –Area &Volume.
Alta High Astronomy Intro: Astronomy A stellar course to be in!
History of Astronomy. Our Universe Earth is one of nine planets that orbit the sun The sun is one star in 100 billion stars that make up our galaxy- The.
Homework 1 Unit 2. Problems 13, 16, 18, Unit 3. Problems 9. 18, 19, 20 For Honors: special assignment (talk with me after the lecture if you have not done.
When the Moon enters the Earth’s shadow it causes a LUNAR eclipse – at time of full moon only. Can see lunar eclipse from anywhere on earth. Moon’s shadow.
Historical Astronomy History Aristotle – Aristarchus - Ptolemy.
SPACE SCIENCE UNIT 2 LESSON 1 Historical Modes of the Solar System.
1 Models of the Solar System Centered on the earth: geocentric Centered on the sun: heliocentric.
1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.
Astronomy 2 Overview of the Universe Winter Lectures on Greek Astronomy Joe Miller.
PHYS Create a MODEL (metaphor) Geometry Physics Aesthetics Compare observations with predictions of model Revise to improve match with observations.
LECTURE # 1 RELATIVITY I ARISTOTLE-NEWTON-GALILEO-EINSTEIN PHYS 420-SPRING 2006 Dennis Papadopoulos Acknowledge contributions from Chris Reynolds
Major Changes in Astronomy Within last 400 years: -- Earth is not the center -- Universe is immense Within last 200 years: -- Appreciate the age of the.
Phases of the Moon What Can You See
Space, Earth and Celestial Objects © Lisa Michalek.
Ancient Greek Thinking on Astronomy Aristotle’s geocentric model of the universe. 1.
2.1 History of Astronomy. What is Astronomy?  The branch of science that deals with celestial objects, space, and the physical universe as a whole.
Earth Science 22.1 Origins of Astronomy Origins of Astronomy.
Early Astronomy Chapter 22, Section 1.
MEASURING THE SOLAR SYSTEM Eratosthenes, Aristarchus The century after Euclid.
Quiz #2 Review Giants of Science (Ch. 2), Gravity and Motion (Ch. 3) Light and Atoms (Ch. 4) Thursday 29 September 2011 Also study the Quiz 1 recap notes.
Announcements Reading Assignment posted for Lecture planetarium Please turn off all electronic devices Please sign attendance sheet.
INTRO TO ASTRO Lesson 4: The Revolution. CHALLENGE OF THE DAY Prove it activity! Movie Debrief David Christian tells us why stories change. Can you think.
Planetary Motions and Lessons in Science. Can One Prove that the Earth is Round? Shadow of the Earth during a lunar eclipse Height of Polaris above the.
1 Giants of Science Our understanding of the Universe developed slowly over centuries. Most of the breakthroughs came through careful study of the positions.
Lecture 3 Ancient astronomy Aristarchus, Ptolemy Modern astronomy Copernicus, Tycho, Galileo, Kepler, Newton Circular satellite motion and tide Light.
Some Basic Facts 12 Constellations of the Zodiac: groups of stars
From the Earth-centered to the Sun-centered Model Tuesday, January 8.
Ancient Greek Astronomy
Title your notes: Models of the Solar System
Unit 2 Lesson 1 Historical Models of the Solar System Copyright © Houghton Mifflin Harcourt Publishing Company.
THE OLD GUYS. Astronomers Click on astronomers to guide you through the PowerPoint. All red boxes are links. Use them to guide you!
What we know about the universe has taken us thousand of years.
Astronomy vs. Astrology Astronomy: Astronomy: The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion,
History of Astronomy Why did ancient cultures study astronomy? Several cultures kept very exact records of astronomical events (and could even predict.
The Discovery of the Universe BC Aristotle 85 – 165 AD Claudius Ptolemy 1473 – 1543 AD Nicolaus Copernicus AD Tycho Brahe
Study of objects outside of Earth & its atmosphere.
History of Astronomy.
Models of the Solar System
Models of the Solar System
Models of the Solar System
Chapter 22 Section 1.
Presentation transcript:

Method: by Ancient Greeks Distant of Moon Method: by Ancient Greeks Present: So Leo Leon Leong

Introduction I : UN-AIDED OBSERVERS Imagine a time before satellites, planes,telephones, telescopes… What would you conclude about the world using just your own senses? Earth is at rest (i.e., motionless) Earth is flat Sun, Moon, planets, stars move in the sky (from East to West) Occasional bizarre things happen (comets, meteors)

Historical Astronomy part1: Ancient (Greek) astronomical measurements of the size of the Earth, Moon, distance to Sun Aristarchus (c. 280BCE) Use shadow of Earth on Moon Earth round, Earth 3x size of Moon (actually 3.7x) Use 1st qtr Moon angle to estimate Sun is ~20x farther than the Moon (actually 400x) Eratosthenes (c. 200 BCE) Used shadow angle of pole to measure radius of Earth (6,900 km), actual 6,400km (8% error!)

Cosmology of Eudoxus and Aristotle Fundamental “principles”: Earth is motionless Sun, Moon, planets and stars go around the Earth: geocentric model Eudoxus (408-355 B.C.) & Aristotle (384-322 B.C.) Proposed that all heavenly bodies are embedded in giant, transparent spheres that revolve around the Earth. Eudoxus needed a complex set of 27 interlocking spheres to explain observed celestial motions E.G., need to have 24-hr period =day and 365-day period=year for the Sun

Geocentric-model

Aristarchus of Samos (310-230 B.C.) Using eclipse data and geometry:  Measured relative sizes of Earth, 􀀁Moon  Curvature of Earth’s shadow on Moon during lunar eclipse ⇒ REarth=4×Rmoon  Measured distance to Moon  (duration of eclipse)÷(1 month)= (2REarth)÷(circumf. of Moon’s orbit)  Attempted to measure distance to Sun  Need to measure (using time interval ratios) the angle of Sun when Moon is exactly at 1st or 3rd quarter  Then use trigonometry and known Earth-Moon distance to get Sun’s distance  Meaured angle was too small, but still concluded Sun was very distant from Earth (20×Moon’s distance) and larger than the Earth (5×Earth’s diameter)  Note: true distance & size 20×larger http://www.perseus.tufts.edu/GreekScienceduke.usask.ca/~akkerman/ gthought/

Heliocentric model of Aristarchus Observations implied Sun is much larger than Earth Therefore proposed the first heliocentric model Sun is the center of the Universe Everything goes around the Sun Never accepted by others of his time  inconsistent with apparent perception of stationary Earth  No apparent shift in stellar positions could be observed over course of seasons  Prevailing culture was uncomfortable with the idea that Earth was not central to the Cosmos

More Assumptions The Moon receives its light from the Sun; The earth is in center of the sphere that carries the Moon. At the time of a Half Moon, our eyes are in the plane of the great circle that divides the dark from the bright portion of the Moon. At the time of a Half Moon, the Moon's angle from the Sun is less than a quadrant (90°) by 1/30 of a quadrant [that is, the angle is 90° - 3° = 87°]. The breadth of the Earth's shadow when the Moon passes through the shadow during a lunar eclipse is two Moons. Both the Moon and the Sun subtend 1/15 of the sign of the zodiac [that is, with 12 signs of the zodiac spaced around the ecliptic, (360° / 12) x 1/15 = 2°]. The Earth is a sphere. The Sun is very far away. The Moon orbits the Earth in such a way that eclipses can occur.

General Method Moon moves (relative to stars) at 360 degrees/month ~ 0.5 degrees/hour.

General Method 2. From duration of lunar eclipse, can infer angular size of Earth as seen from Moon.

General Method Compare to angular size of Moon as seen from Earth.

General Method Aristarchus concluded: Earth diameter = 3 x Moon diameter (close to true value).

General Method Combine with Eratosthenes measurement of Earth diameter to get Moon diameter in stadia (or km). i.e. 6300 km

General Method 6. Knowing angular size of Moon (0.5 degrees) and physical size of Moon, find the distance to Moon by:

Q&A

Reference http://www.darkoogle.com http://astronomers.org http://hk.yahoo.com http://www.wikipedia.org http://www.cliffsnotes.com/ http://www.astro.washington.edu/ http://www-ssg.sr.unh.edu/ http://galileoandeinstein.physics.virginia.edu/ http://forum.hkgolden.com

The End