1 / 33

Chapter 2: The Rise of Astronomy

Chapter 2: The Rise of Astronomy. Ancient Roots: Early Homo-Sapiens. Ancient Roots: Egyptian. Ancient Roots: England. Ancient Roots: Mayan. Ancient Roots: Aztec. Ancient Roots: Incan. Ancient Roots: Cambodia. Ancient Roots: Anasazi. Early Ideas: Pythagoras.

hong
Download Presentation

Chapter 2: The Rise of Astronomy

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Chapter 2: The Rise of Astronomy

  2. Ancient Roots: Early Homo-Sapiens

  3. Ancient Roots: Egyptian

  4. Ancient Roots: England

  5. Ancient Roots: Mayan

  6. Ancient Roots: Aztec

  7. Ancient Roots: Incan

  8. Ancient Roots: Cambodia

  9. Ancient Roots: Anasazi

  10. Early Ideas: Pythagoras • Pythagoras in 500 B.C. taught that the Earth was round based on the belief that the sphere is the perfect shape used by the gods

  11. Early Ideas: Aristotle • By 300 B.C., Aristotle presented naked-eye observations for the Earth’s spherical shape: • Shape of Earth’s shadow on the Moon during an eclipse

  12. The Hot Debate! • A geo-centric cosmology is a theory that proposes Earth to be at the center of the universe. • versus • A helio-centric cosmology is a theory that proposes the Sun to be at the center of the universe.

  13. Aristotle’s model of a geo-centric solar system (384-322 BC) But model couldn’t account fully for retrograde motion of the planet!!!

  14. Retrograde motionis the apparent “backward” motion of a planet

  15. Ptolemy’s Geo-centric Solar System Tried to account for retrograde motion, but could not quite match observations

  16. Copernicus devised the first comprehensive helio-centric cosmology to successfully explain retrograde motion

  17. Tycho Brahe’s Golden Nose

  18. Mathematician Johannes Kepler created laws of planetary motion

  19. Kepler’s First Law: The orbit of a planet about the Sun is an ellipse with the Sun at one focus.

  20. Kepler’s Second Law: A line joining a planet and the Sun sweeps out equal areas in equal intervals of time. In other words, the closer a planet is in its orbit around the Sun, the faster its speed is.

  21. Kepler’s Third Law In other words, the planets that are closest to the Sun orbit the Sun at a faster speed than planets that are farther away.

  22. The orbit of a planet about the Sun is an ellipse with the Sun at one focus 1st Law 2nd Law The closer the planet is in its orbit around the Sun, the faster its speed is. The planets that are closest to the Sun orbit the Sun at a faster speed than planets that are farther away. 3rd Law Summary of Kepler’s Laws of Planetary Motion

  23. Italian scientist Galileo made discoveries that strongly supported a helio-centric cosmology “I do not feel obliged to believe that the samegod who has endowed us with sense, reason andintellect has intended us to forgo their use.” - Galileo

  24. Galileo’s telescope revealed that Jupiter had moons which orbited Jupiter instead of Earth.

  25. Galileo’s telescope revealed all phases of Venus which could only occur IF Venus orbits the Sun.

  26. Geo-centric or Helio-centric? Galileo Ptolemy Kepler Copernicus Aristotle

  27. Sir Isaac Newton What goes up, must come down!

  28. Newton’s Universal Law of Gravitation • Every body that has mass has gravity • The gravity between the two bodies increase with the mass • The gravity between the two bodies increase if they are closer together.

  29. Mass vs. Weight • Mass is a measure of the total amount of material in the object  remains the same everywhere • Weight is the force with which an object is pulled down while on the ground (due to gravity’s attraction)  changes depending on the body you are standing on

  30. Foucault proves that the Earth rotates!

More Related