1 / 50

The History of Astronomy

1 year. 1 month. retrograde motion. west. east. 5 planets. Mercury and Venus near Sun. west. east. Ptolemy's System. GeocentricPerfect CirclesEarthMoon Mercury VenusSunMarsJupiterSaturn Fixed Stars. Aristotle's Physics. 5 elementsNatural Motion. Ptolemy gets tricky. epicycle.

stewart
Télécharger la présentation

The History 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. The History of Astronomy

    3. Mercury and Venus near Sun

    4. Ptolemys System

    5. Aristotles Physics

    6. Ptolemy gets tricky

    10. Why Ptolemy needs Epicycles:

    11. Retrograde Motion & Brightness

    12. But why is the planet Always brighter at opposition?

    13. Mercury and Venus near Sun

    14. Ptolemy gets even trickier!!

    15. Arabic Astronomy

    16. Dante Alighieri (1265-1321)

    17. The Renaissance 1300s-1500s

    18. Nicolas Copernicus (1473-1543)

    19. A new Day

    20. Copernicuss issues with Ptolemy

    21. Lets put the Earth on an Epicycle

    22. Lets put the Earth on an Epicycle

    24. Retrograde Motion & Brightness

    27. Copernicus Invents New Time

    28. Copernicus Invents New Time

    29. Copernicus measures distances to Inner Planets

    30. Copernicus measures distances to Outer Planets

    31. Good & Bad

    32. Its still pretty tricky

    33. Stellar Parallax

    34. Tycho Brahe (1546-1601)

    36. Brahes Universe

    37. Galileo Galilei (1564-1642)

    38. Proof #1: the Moon

    39. Proof #2: Jupiters Moons

    40. Ptolemy

    41. Ptolemys Phases of Venus

    44. Johannes Kepler (1571-1630)

    47. #3: The square of the orbital period is proportional to the cube of the average orbital radius

    48. Rene Descartes (1596-1650)

    49. Isaac Newton (1642-1727)

More Related