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Unraveling Ancient Astronomy: From Stone Monuments to Planetary Orbits

Explore the historical roots of astronomy from ancient cultures to Greek philosophers like Aristotle, unraveling celestial wonders and timekeeping methods. Learn about significant figures like Eratosthenes and their contributions to understanding Earth and the stars.

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Unraveling Ancient Astronomy: From Stone Monuments to Planetary Orbits

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  1. That’s the trouble with science. You’ve got a bunch of empiricists trying to describe things of unimaginable wonder.

  2. Gravity & Orbits Solar System Astronomy Chapter 3

  3. But first… history Solar System Astronomy

  4. Some History • Ancient cultures & astronomical knowledge • Already in the stone and bronze ages, human cultures realized the cyclic nature of motions in the sky. • Monuments dating back to ~ 3000 B.C. show alignments with astronomical significance. • Those monuments were probably used as calendars or even to predict eclipses

  5. Some History • Ancient cultures & astronomical knowledge • Nebra sky disk • ~1600 BC • bronze disk ~30cm diameter • sun or full moon, a lunar crescent, and stars (including Pleiades) • two golden arcs along the sides • marking angle between the solstices • arc at the bottom perhaps Milky Way or Rainbow

  6. Some History

  7. Some History • Ancient cultures & astronomical knowledge • Often timekeeping methods • Some objects ‘wandered’ • Greek πλανήτης, derivative of the word πλάνης "moving” • 7 in the sky • Sun • Moon • Mars • Mercury • Jupiter • Venus • Saturn

  8. Some History • Ancient cultures & astronomical knowledge • Often timekeeping methods • Some objects ‘wandered’ • Greek πλανήτης, derivative of the word πλάνης "moving” • 7 in the sky • Sun Dimanche • Moon Lundi • Mars Mardi • Mercury Mercredi • Jupiter Jeudi • Venus Vendredi • Saturn Samedi

  9. Some History • Ancient cultures & astronomical knowledge • Often timekeeping methods • Lunar cycles gave rise to months

  10. Some History • Ancient cultures & astronomical knowledge • Often timekeeping methods • When is Easter? • observed on the Sunday after the first full moon on or after the day of the vernal equinox • full moon involved is not an astronomical full moon, but an ecclesiastical moon – though it coincides more or less with the astronomical full moon • Easter falls on the first Sunday following the first ecclesiastical full moon that occurs on or after March 21 (the day of the ecclesiastical vernal equinox)

  11. Some History • Ancient cultures & astronomical knowledge • Often timekeeping methods • Sirius, the Dog Star • seiros σείριος, “scorcher” • Rising just before Sun marks the beginning of summer

  12. Some History • Ancient Greece • Astronomy was a branch of mathematics • Astronomers sought to create geometrical (mathematical) models that could imitate the appearances of celestial motions • tradition began with Pythagoreans, who placed astronomy among the four mathematical arts (along with arithmetic, geometry, and music) • Our conception of astronomy (and many sciences) inherited from Ancient Greek

  13. Some History • Ancient Greece • Eudoxus • Aristotle • Eratosthenes • Hipparchus • Ptolemy • All sought to describe motion of heavenly bodies • Mathematical behavior of motion

  14. Some History • Ancient Greece • Eudoxus (4009 – 356 BC) • assigned to each planet a set of 27 concentric spheres • first to attempt a mathematical description of the motions of the planets

  15. Some History • Ancient Greece • Aristotle (384 – 322 B.C.) • major authority of philosophy until late Middle Ages • divided universe into two parts • imperfect, changeable Earth • perfect heavens (described by spheres) • expanded Eudoxus’ model to 55 spheres • Aristotle taught the Earth is round • Why would he think that?

  16. Some History • Ancient Greece • Aristotle (384 – 322 B.C.) • perhaps the philosopher most respected by European thinkers during and after the Renaissance • erroneous positions taken as a given, which held back science • analysis of procreation presupposes: • active, ensouling masculine element bringing life to • inert, passive, female element • assertion that objects of different mass fall at different speeds under gravity • refuted by Philoponus

  17. Some History • Ancient Greece • Aristotle (384 – 322 B.C.) • held back science for 2000 years • refuted Democritus's claim Milky Way was multitude of stars • refuted stars of night sky were just like Sun • calculated they would have to be millions of times farther away than Sun • thus dismissed for hundreds of years • theory of the natural slave was used to justify European domination of Native Americans • On Animals…

  18. Some History • Ancient Greece • Eratosthenes (276 BC - 194 BC) • Greek mathematician, geographer and astronomer • contemporaries nicknamed him Beta (2nd letter of alphabet) –supposedly proved himself to be the second in the Mediterranean world in many fields • first known to have calculated the size of the Earth

  19. Some History • Ancient Greece • Eratosthenes (276 BC - 194 BC) • Angular distance between Syene and Alexandria is ~ 7° • Linear distance ~ 5,000 stadia • Earth Radius ~ 40,000 stadia • probably ~ 14 % too large

  20. Some History • Ancient Greece • Hipparchus (2nd century BC) • access to Babylonian observations & predictions • used to create better geometrical models, constructed accurate models for movement of Sun & Moon • moved Earth from center of spheres • compiled star catalogue • recorded the position and brightness of the stars • Considered among most important Greek astronomers (& greatest astronomer of antiquity by some) • introduced the concept of exact prediction into astronomy • last innovative astronomer before Ptolemy

  21. Some History • Ancient Greece • Ptolemy (c. 90 – c. 168) • compiled and extended the astronomical knowledge and theories of the ancient Greek & Babylonian world • star catalog in Almagest lists forty-eight constellations • ancestral to the modern system of constellations • geocentric model widely accepted until Copernicus

  22. Some History • Ancient Greece • Ptolemy (c. 90 – c. 168) • Retrograde motion…

  23. Some History • Ancient Greece • Ptolemy (c. 90 – c. 168) • Epicycles…

  24. Some History • Ancient Greece • Ptolemy (c. 90 – c. 168) • Epicycles • Ptolemaic system was considered the “standard model” of the Universe until the Copernican Revolution

  25. Some History • Copernican Revolution & beyond • 99 years that changed our view of the Universe • Nicolaus Copernicus • Galileo Galilei • Tycho Brahe • Johannes Kepler • Isaac Newton

  26. Some History • Copernican Revolution • Copernicus (1473-1543) • one of the great Renaissance polymaths • mathematician, astronomer, jurist, physician, classical scholar, governor, administrator, diplomat, economist, and soldier

  27. Some History • Copernican Revolution • Copernican Model • No center to universe • Center of Solar System near sun • heliocentric • Distance to Sun imperceptible vs distance to stars • Earth’s motion accounts for apparent motion: • rotation accounts for daily rotation of stars • annual cycle of Sun’s movements caused by Earth’s orbit • apparent retrograde motion of planets is caused by orbit

  28. Some History • Copernican Revolution • Copernican Model • arrived at correct order of the known planets • Explained precession of the equinoxes correctly • slow change in the position of the Earth's rotational axis • gave a clear account of the cause of the seasons • Earth's axis not perpendicular to plane of orbit • added motion to Earth, keeping axis pointed throughout the year at the same place in the heavens

  29. Some History • Copernican Revolution • Copernican Model • not experimentally better than Ptolemy’s • from 1543 publication until about 1700, few astronomers were convinced by the Copernican system, though the book was relatively widely circulated • influenced Galileo & Kepler, others • ironically, this was at the behest of the Catholic Church as part of the Catholic Reformation efforts for a means of creating a more accurate calendar for its activities

  30. Some History • Copernican Revolution • Galileo (1564 – 1642) • Italian • physicist • astronomer • astrologer • philosopher • closely associated with the Scientific Revolution

  31. Some History • Copernican Revolution • Galileo (1564 – 1642) • improved (but did not invent) telescope • invented first known microscope • observed Galilean moons • motion indicated orbits about Jupiter • observed rings of Saturn • observed full set of phases with Venus

  32. Some History • Copernican Revolution • Galileo (1564 – 1642) • improved (but did not invent) telescope • invented first known microscope • observed Galilean moons • motion indicated orbits about Jupiter • observed rings of Saturn • observed full set of phases with Venus

  33. Some History • Copernican Revolution • Galileo (1564 – 1642) • one of first Europeans to observe sunspots • Existence contradicted unchanging perfection of the heavens (Aristotle) • First to report lunar mountains & craters • Concluded “rough and uneven, and just like the surface of the Earth • Not Aristotle’s perfect sphere • Observed the Milky Way • Found to be multitude of distant stars

  34. Some History • Copernican Revolution • Galileo (1564 – 1642) • Demonstrated equal acceleration of unequal masses • Contrary to Aristotle • Determined rate objects fell • Demonstrated velocity constant (not zero) without outside force • Contrary to Aristotle • Basic principle of relativity

  35. Some History • Copernican Revolution • Galileo (1564 – 1642) • Early example of science conflicting with Church/authority • 1633 Heresy • required to recant heliocentric ideas • idea that Sun is stationary condemned as “formally heretical” • heliocentrism was never formally or officially condemned • ordered imprisoned • sentence later commuted to house arrest • Dialogue Concerning the Two Chief World Systems banned • and all past & future books

  36. Some History • Copernican Revolution • Tycho Brahe (1546 – 1602) • preeminent observational astronomer of pre-telescopic period • said to own 1% of Denmark’s entire wealth at one • observations of stellar/planetary positions unparalleled accuracy • observations of nova contradicted immutable heavens • Lost nose in duel 1566 • Fair amount of drinking involved • Replacement of silver & gold • Kept a jester (Jepp) beneath the table during dinner • Believed to be clairvoyant • Tame elk (or moose)…

  37. Some History • Copernican Revolution • Kepler (1571 – 1630) • German • Mathematician, astronomer, astrologer, sci-fi writer

  38. Some History • Copernican Revolution • Kepler (1571 – 1630) • Used the precise observational tables of Tycho Brahe to study planetary motion mathematically • Consistent description by abandoning both • Circular motion • Uniform motion • Planets move around the sun on elliptical paths, with non-uniform velocities

  39. Some History • Copernican Revolution • Kepler (1571 – 1630) • Kepler’s Laws • The orbits of the planets are ellipses with the sun at one focus • A line from a planet to the sun sweeps over equal areas in equal intervals of time • A planet’s orbital period (P) squared is proportional to its average distance from the sun (a) cubed

  40. Some History • Copernican Revolution • Kepler’s Law #1 & #2

  41. Some History • Copernican Revolution • Kepler’s Law #3

  42. Kepler’s Laws

  43. Some History • 99 years changed our universe

  44. Some History • Copernican Revolution Where do Kepler’s Laws come from? Why are they true? We don’t know… Until Newton.

  45. Some History • Copernican Revolution Where do Kepler’s Laws come from? Why are they true? We don’t know… Until Newton.

  46. Sir Isaac Newton, FRS

  47. Newton’s Laws • Newton discovered laws applying to all objects • Universal • Describe forces that act on all objects • Like gravity

  48. Newton’s Laws of Motion • Stationary objects stay stationary, moving objects stay in constant motion • Unless a force acts upon it • “constant” refers to speed AND direction • Forces change motion • No change in motion means no forces OR balanced forces #1

  49. Newton’s Laws of Motion • Force = mass × acceleration • F = ma a = F/m • More mass » less acceleration • Larger force » larger acceleration #2

  50. Newton’s Laws of Motion • Forces always come in pairs • Same size • Opposite direction • Applies to ALL forces, including gravity #3

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