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A Short History of Astronomy

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Title: A Short History of Astronomy


1
A Short History of Astronomy
  • Ancient (before 500 BC)
  • Egyptians, Babylonians, Mayans, Incas, Chinese
  • Classical Antiquity (500 BC-500 AD)
  • Greeks, Romans Plato, Aristotle, Ptolemy
  • Middle Ages (500-1450 AD)
  • Arabic astronomers
  • Renaissance (1450-1550 AD)
  • Copernicus
  • Brahe, Kepler, Galilei, Newton

2
Ancient Astronomy
Newgrange, Ireland
Stonehenge, England
  • Pyramids,
  • Egypt

3
The Babylonians
  • Made systematic measurements as early as 2000 BC
  • By 800400 BC
  • State support for the calendar and astrology
  • Compiled the first star catalogs and began
    long-term records of planetary motions
  • Were able to predict lunar and solar eclipses
  • May also have invented astrology

4
The Greeks
  • Plato (428 BC)
  • Introduces the celestial sphere. The stars are
    fixed to a sphere that rotates around the Earth
  • introduces prejudice in favor of circles
  • values theory over observation

5
Alexander the Great(356-323 BC)
  • Much of the knowledge of the world came together
    as the rule of Alexander spread across Europe,
    Asia, and Northern Africa.
  • Founded the city of Alexandria
  • Library of Alexandria contained the written works
    and inventions of many great thinkers and
    scientists.

6
The Greeks
  • Aristotle (384322 BC)
  • Argued that the planets move on spheres around
    the Earth (geocentric model)
  • Argues that the earth is spherical based on the
    shape of its shadow on the moon during lunar
    eclipses
  • Aristarchus (310230 BC)
  • Attempts to measure relative distance and sizes
    of sun and moon
  • Proposes, nearly 2000 years before Copernicus,
    that all planets orbit the Sun, including the
    Earth (heliocentric model)

7
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8
Using the distance between the Earth and the Moon
as a baseline
9
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10
The Greeks
  • Eratosthenes (ca. 276 BC)
  • Measures the radius of the earth to about 20

11
Eratosthenes ( 200 B.C.)Calculation of the
Earths radius
Angular distance between Syene and Alexandria
70 Linear distance between Syene and Alexandria
5,000 stadia ? Earth Radius 40,000 stadia
(probably 14 too large) better than any
previous radius estimate.
12
The Greeks
  • Hipparchus (190 BC)
  • His star catalog a standard reference for sixteen
    centuries!
  • Introduces coordinates for the celestial sphere
  • Declination (dec)
  • Right Ascension (RA)
  • (analogous to latitude and longitude,
    respectively)

13
Ptolemy (140 AD)
  • Puts forth a complete geocentric model
  • dominates scientific thought during the Middle
    Ages
  • Longest lasting (wrong) theory ever 1000 yrs
  • Major Work Almagest

14
Retrograde Motion
15
Epicycles
  • Ptolemys explanation of retrograde motion
  • About 40(!) epicycles necessary to explain all
    observations ?complicated theory

16
Hypatia of Alexandria (355 or 370 - 415/416
A.D.) Exact dates are unknown. Many records
were destroyed.
  • Hypatia was, simply, the last great Alexandrian
    mathematician and philosopher.
  • Edited the work On the Conics of Apollonius

17
The Medieval Setting
  • Dominant Church
  • 1000 years of relative stagnation
  • Experimental research greatly reduced
  • To answer a question
  • Study the Bible or Aristotle!

18
The Renaissance Setting
  • Invention of the print (1450) by Gutenberg
  • ?Books widely available!
  • (Think Manuscripts vs Amazon.com)
  • End of Middle Age Church Domination
  • Back to the roots (renaissancerebirth)
  • Study of Arabic astronomers
  • Intellectual movement

19
Nicolas Copernicus (14731543)
  • Rediscovers the heliocentric model of Aristarchus
  • Planets on circles
  • needs 48(!!) epicycles to explain
  • different speeds of planets
  • Not more accurate than Ptolemy
  • Major Work De Revolutionibus Orbium
    Celestium
  • (published posthumously)

20
The heliocentric Explanation of retrograde
planetary motion
  • See also SkyGaze

21
The Scientific Method
  • Systematized by Francis Bacon, Descartes and
    Galileo in the 17th century
  • Not the only way of knowing, but a very
    successful one
  • A method to yield conclusions that are
    independent of the individual
  • Conclusions are based on observation

22
Tycho Brahe The Data Taker
  • Key question Where are
    things?
  • Catalogued positions of planets in Uraniborg and
    Prague
  • Working without telescope
  • Data ten times as accurate as before
  • Died at banquet binge drinking

Tycho Brahe (15461601)
23
Tycho Brahe
  • collects detailed and accurate (1-2 accuracy)
    observations of stellar and planetary positions
    over a period of 20 years
  • His research costed 5-10 of Danish GNP
  • shows that comets and novas are extralunar
    contrary to Aristotle
  • Shows that stars can change
  • (Supernova of 1572)

Tycho Brahe observing
24
Johannes KeplerThe Phenomenologist
  • Key question
  • How are things happening?
  • Major Works
  • Harmonices Mundi (1619)
  • Rudolphian Tables (1612)
  • Astronomia Nova
  • Dioptrice

Johannes Kepler (15711630)
25
Keplers Beginnings
  • Astrologer and Mystic
  • Tried to find music in the skies
  • Tried to explain distances of the
  • 5 known planets by
  • spheres resting on the
  • 5 mathematical bodies
  • ? pre-scientific

26
Johannes Kepler
  • Manuscript trying to disentangle
  • The mystery of Mars orbit ?

27
Keplers First Law
  • The orbits of the planets are ellipses, with the
    Sun at one focus

28
Ellipses
  • a semimajor axis e eccentricity

29
Conic Sections
  • From Halleys book (1710)

30
Keplers Second Law
An imaginary line connecting the Sun to any
planet sweeps out equal areas of the ellipse in
equal times
31
Keplers Third Law
  • The square of a planets orbital period is
    proportional to the cube of its orbital
    semi-major axis
  • P 2 ? a3
  • a
    P
  • Planet Orbital Semi-Major Axis Orbital Period
    Eccentricity P2/a3
  • Mercury 0.387 0.241 0.206 1.002
  • Venus 0.723 0.615 0.007 1.001
  • Earth 1.000 1.000 0.017 1.000
  • Mars 1.524 1.881 0.093 1.000
  • Jupiter 5.203 11.86 0.048 0.999
  • Saturn 9.539 29.46 0.056 1.000
  • Uranus 19.19 84.01 0.046 0.999
  • Neptune 30.06 164.8 0.010 1.000
  • Pluto 39.53 248.6 0.248 1.001
  • (A.U.) (Earth years)

32
Galileo Galilei The Experimentalist
  • Did experiments (falling bodies) rather
  • than studying Aristotle
  • Major Works
  • Siderius Nuntius (1610)
  • Dialogue concerning the Two Chief World Systems
    (1632)
  • The latter discusses Copernicus vs Ptolemy ?ban
    by Church (1633)
  • revoked by pope 1992
  • (15641642)

33
  • Siderius Nuntius (1610) Dialogo
    (1632)

34
Galileo Galilei (15641642)
  • Astronomical observations that contradict
    Aristotle
  • Observed mountains on the Moon, suggesting that
    the Earth is not unique
  • Sunspots suggests that celestial bodies are not
    perfect and can change
  • Observed four moons of Jupiter showed that not
    all bodies orbit Earth
  • Observed phases of Venus (and correlation of
    apparent size and phase) evidence that Venus
    orbits the Sun
  • Also observed
  • the rings of Saturn
  • that the Milky Way is made of stars

35
Phases of Venus
  • Heliocentric
  • (observed)

Geocentric (not observed)
36
Isaac Newton The Theorist
  • Key question
  • Why are things happening?
  • Invented calculus and physics while on vacation
    from college
  • His three Laws of Motion, together with the Law
    of Universal Gravitation, explain all of Keplers
    Laws (and more!)

Isaac Newton (16421727)
37
Isaac Newton (16421727)
  • Major Works
  • Principia (1687)
  • Full title Philosophiae naturalis principia
    mathematica
  • Opticks sic!(1704)
  • Major findings
  • Three axioms of motion
  • Universal gravity

38
Law of Universal Gravitation
  • Force G Mearth Mman / R2

39
Orbital Motion
40
Cannon Thought Experiment
  • http//www.phys.virginia.edu/classes/109N/more_stu
    ff/Applets/newt/newtmtn.html
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