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Outline
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Chapter 3
  • The Science of Astronomy
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Everyday Science
  • Scientific Thinking is a fundamental part of human nature.


  • Scientists apply the scientific method to their inquiries about the universe.
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Ancient Observations
  • Central Africa: c. 6500 B.C. People use the observations of the moon to predict the weather.
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Graph depicts the annual rainfall pattern in central Nigeria, characterized by a wet season and a dry season.
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Modern measures of time still reflect their ancient astronomical roots.
  • 24 hour day – the time it takes the Sun to circle our sky.


  • Month – comes from the lunar cycle.


  • Calendar Year – Based on the cycle of the seasons.


  • Days of the week – named after the seven “naked-eye” objects that appear to move among the constellations. (Sun, Moon and five planets)


  • At night, the position and phase of the Moon give an indication of the time.


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The Seven Days of the Week and the Astronomical Objects They Honor
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Determining the time of day
  • In the daytime, ancient peoples could tell the time of day by observing the Sun’s path through the sky.


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The ancient Egyptians used huge obelisks as simple clocks/ (Sundials).
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Determining the Time of Year
  • Many cultures built structures to help them mark the seasons.


  • A good example of this is Stonehenge.
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The Sun Dagger– Chaco Canyon, New Mexico
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Lunar Cycles
  • Many ancient cultures used the lunar cycle as the basis of lunar calendars.


  • Metonic cycle:
    • The ancient Greek astronomer Meton (432 B.C.) observed that the dates of the lunar cycle repeat every 19 years.


  • Other cultures based their calendars on their ability to predict eclipses:
      • Babylonian Calendar
      • Mayan Calendar

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Observation of Planets and Stars
  • Many cultures made careful observations of the planets and the stars.


  • Mayan observatories of Central America had windows placed to allow for observations of Venus.
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"In the desert regions of..."
  • In the desert regions of Peru, many large figures of animals may have represented constellations to the Incas who lived there.
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From Observation to Science
  • Ancient Chinese Astronomers kept very detailed records of astronomical observations beginning 5,000 years ago.


  • They were the first to record an observation of a Supernova explosion, which we see today as the Crab Nebula.
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"In the Americas,"
  • In the Americas, the Mayans had developed a modern system of numbers and mathematics, which included the invention of the concept of zero.


  • It appears that virtually all cultures employed scientific thinking to varying degrees.
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The Modern Lineage
  • 3000 B.C. The establishment of civilization occurred in Egypt and Mesopotamia.


  • 2700-2100 B.C. Egyptians build the Great Pyramids.


  • 500 B.C. Greece rises as a military power.


  • 330 B.C. Alexander the Great expands the Greek empire throughout the middle east.


  • As a student of Aristotle, Alexander had a great interest in science and education.


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"300 B.C."
  • 300 B.C. The Library of Alexandria is established as the leading center of knowledge, housing more than half a million books.


  • ~ 415 A.D. The destruction of the library of Alexandria, along with the loss of most of the knowledge stored there.


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"One of the most important..."
  • One of the most important scientific contributions from ancient Greece was the idea of creating models to represent natural phenomena.


  • Models are still used today to help us in understanding natural phenomena.


  • Claudius Ptolemy (100-170)A.D. developed an Earth centered (geocentric) model of the universe that included the motions of the Sun, moon, and planets.


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Ptolemaic Model of the Universe
  • All heavenly motions proceed in perfect circles.


  • To explain retrograde motion, Ptolemy maintained that each planet moved along a small circle that, in turn, moved around a larger circle.


  •  This allowed for the observed westward (retrograde) motion that some planets exhibited.


  • The large circular orbit around the Earth was called the “Deferent”


  • The smaller circular motion along a “deferent” was called an epicycle.
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Ptolemy’s model of the Solar System/Universe
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The Copernican Revolution
  • 1543 Copernicus publishes De Revolutionibus Orbium Caelestium, “Concerning the Revolutions of the heavenly Spheres”.
  • Copernicus modifies the Ptolemaic model as noticeable discrepancies become more apparent with the improvements in observational astronomy.
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The Copernican Model of the Solar System
  • The Sun and not the Earth, is at the center of the solar system.


  • The earth does move, and like the other planets, orbits the sun.


  • The orbital paths follow perfect circles.
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Tycho Brahe (1546-1601)
  • Made detailed naked eye observations of the motions of the planets.


  • Coined the term NOVA for the observation of a supernova (Nova means “New Star”)


  • Showed that comets were distant objects rather than being phenomena of the Earth’s atmosphere, as argued by Aristotle.


  • In the course of 30 years, he had amassed the best astronomical data of the day It was accurate to within 1 arc-minute.
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Johannes Kepler (1571-1630)
  • A mathematician and a man of faith, who believed that understanding the geometry of the heavens would bring him closer to God.


  •  Inherited Tyco Brahe’s astronomical data.


  • With his mathematical skills, Kepler spent          20 years of his life trying to develop a consistent model to describe planetary motion.


  • His efforts culminated in what is known today as Kepler’s Three Laws of Planetary Motion.
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Kepler’s First law of planetary Motion
  • The orbit of each planet about the Sun is an ellipse with the Sun at one focus.
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Kepler’s Second Law of Planetary Motion
  • As a planet moves around its orbit, it sweeps out equal areas in equal times.
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Kepler’s Third Law of Planetary Motion
  • The square of a planet’s orbital period is proportional to the cube of its semi-major axis.
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"The Copernican view of the..."
  • The Copernican view of the solar system and Kepler’s three laws of planetary motion were very successful in explaining and predicting observations.


  • However, due to the degree to which the Ptolemaic model was ingrained in the current thinking of the day, major objections were put forth with regard to the new Copernican/Keplerian model.
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Main Objections to Copernican/Keplerian View
  • The Earth could not be moving because if it did, objects such as birds, falling stones, and clouds would be left behind as the Earth moved along its way.


  • The idea of noncircular orbits contradicted the ancient Greek belief that the heavens must be perfect and unchanging.


  • Stellar parallax should be detectable if the Earth orbits the Sun. (True, but difficult to detect)
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Galileo’s defuses all objections
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"Galileo performed careful experiments on..."
  • Galileo performed careful experiments on the motions of moving bodies and showed that a moving object remains in motion unless a force acts to stop it or change its direction.


  • Tycho’s observations of a comet and supernova showed that the heavens could change.


  •  The lack of noticeable stellar parallax was simply due to the fact that the stars were much farther away than anyone had previously thought.


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Galileo Invents the Telescope
  • Galileo observes four moons clearly orbiting Jupiter.


  • This shows that objects do orbit planets other than the Earth.



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Phases of Venus
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"Galileo observes that Venus goes..."
  • Galileo observes that Venus goes through phases much like the moon does. Only a Heliocentric model of the solar system can account for all observed phases.


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Galileo’s Other Telescopic Discoveries
  • Craters, mountains and cliffs on the Moon.
  • Sunspots