Ancient Greeks: Early Astronomy Flashcards

1
Q

How old is the oldest record of astronomy (and what is it?)

A

Bone carving of the phases of the lunar cycle
Aurignacian culture of Europe
32000 BC

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2
Q

Late Stone Age Europe

A

Goseck Henge, oldest solstice observatory
4900 BC
(That rock thing)

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3
Q

Egypt

Also what other countries did stuff like this?

A

Pyramids and pole star
2600 BC
India, China, Mesoamerica, etc did stuff like this too

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4
Q

Babylonians

A

Eclipse observations
Periodicity
Mathematics (base 60)
1200 BC

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5
Q

Greeks (overview)

A

Realized sky is three-dimensional
Eudoxus’ concentric spheres model dominated cosmology for 2000y
400 BC

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6
Q

Antikythera mechanism

A
100 BC
Archimedes? Hipparchus? Who knows
Super super cool
All these super precise gears predicted all this stuff
"More valuable than Mona Lisa"
Like 2000 years ahead of its time
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7
Q

Greeks realizing sky is 3D

A
  • immediately explains phases of moon
  • explains eclipses
  • what is SHAPE of earth? (Pythagoras, Aristotle)
  • what is SIZE of earth compared to moon?
  • can use lunar eclipses to see shape
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8
Q

Aristarchus

A

310-230 BC
Calculated RELATIVE distances (ex earth to sun/earth to moon ratio)
Calculated RELATIVE sizes (ex diameter of sun/diameter of moon ratio)
Did this inspire his unprecedented belief that Earth orbits the Sun?

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9
Q

Eratosthenes

A

Calculated ABSOLUTE size of Earth
Given relative sizes (Aristarchus), can now compute absolute sizes
276-196 BC

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10
Q

Hipparchus

A

190-120 BC
Accurately catalogues 100s of star positions
Discovered precession of equinoxes
Determined length of year to within 6 min
Established stellar magnitude scale
Computed more accurate EM distance
Now more absolute distances can be found

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11
Q

Angular size of sun and moon

A

1/2 degree

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12
Q

Distance from syrene to Alexandria

A

5000 stades

1 stade maybe 185m?

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13
Q

What are the two theoretical streams in astronomy at this time?

A

Philolaus - heliocentric (declined after Aristarchus)

Plato - geocentric (widespread acceptance after Ptolemy)

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14
Q

Plato

A
428-348 BC
Asserted that all heavenly motions must be 
-in perfect circles
-at constant speed
(No evidence or physical explanation)
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15
Q

Eudoxus

A

400-347 BC

  • Student of Plato
  • First to attempt mathematical explanation of celestial motions (apparent circular motion of stars, apparent retrograde motion of Mars)
  • complexities with planetary motion: retrograde and changing brightness
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16
Q

Eudoxus’ model

A
Rotating sphere of stars
Rotating sphere of ecliptic inside
First sphere inside for synodic period
Second sphere inside for synodic period
Earth at centre
Nested spheres, inner sphere axis offset, planet in equator
Outer sphere CCW, inner sphere CW
17
Q

Problems with Eudoxus’ model

A

Does not explain changes in brightness of planets

18
Q

Apollonius

A
240-190BC
Introduced circle upon circle at constant speeds to explain varying speed and distance of moon and sun
Looks ~ pretty close to orbit
He was circle crazy
Hipparchus backed him up with math
19
Q

Ptolemy

A

100-170 AD
He did detailed calculations and refined Apollonius’ model
Approximately correct!
Had an equal angle law ~ Kepler area law

20
Q

Ptolemy’s model

A

Apollonius, but added
Eccentric (equivalent to a certain type of epicycle) (earth not centre of circle)
Equant (constant angular speed from Equant, varying physical speed along deferent) (sacrilege) (earth is off centre)

21
Q

Almagest

A

Ptolemy
Compiled all existing Astro knowledge + own innovations
Dominated astronomy for 1500 years
Eventually overthrown by Copernicus, Galileo, Kepler, Newton

22
Q

What destroyed the Ptolemaic model?

A

Galileo’s observation of the phases of Venus

23
Q

Problems with the Ptolemaic model

A

Angular data can’t determine orbital radio of planets, can only find ratio of radii

24
Q

Define synodic period

A

Time between stuff appearing in sky in same configuration