Title: Weekly Review Session
1Weekly Review Session
- Monday or Wednesday after 430
2Geocentric Geostatic Models
3Platos model of the cosmos (400 - 300 BCE)
- Stars revolve once a day on one axis
- Sun, moon and planets have same motion
- - but second circular motion which moves them
relative to stars - As stars revolve, sun, moon and planets will be
in different position
4Eudoxus model of the cosmos
- 27 spheres
- 3 for sun
- 3 for moon
- 4 for each of 5 planets
- 1 for fixed stars
5Hippòpedon
- additional spheres combined with suitable speeds
and choice of axes - Gives planetary deviation from ecliptic and
retrograde motion
6Aristotles Universe
55 spheres
real made of aether
- no space between them
Celestial bodies attached
Rotate at different velocities
7Dominance of Aristotelian world system
Why geocentric-geostatic model?
Earthly
- corruptible
- earth absolutely heavy
- reaches proper place and stops
Celestial
- Objects in Heavens unchanging
- Only motion in Heavens is circular motion
8Why cant the Earth be moving?
- Rotation
- Earth 24,000 miles in circumference at equator
- 1 rotation in 24 hours
- Speed at equator 1,000 miles per hour (1467 ft/s)
- If 1 sec for object to fall floor moves
almost 1500 ft
9Why cant the Earth be moving?
- Revolution
- Earths period (assume circular 2pr) miles
5.84 x 108 miles - Period 365 days x 24 hr/day 8760 hr
- Velocity 66,705 mi/hr
Parallax
10Parallax Effect
11Parallax Effect
Large Parallax Angle
Small Parallax Angle
12Problems
- observations - not possible with simple
circular models - apparent size / brightness of planets vary
- apparent speed of planets vary
- planets have different shapes of retrograde
motion
13Ancient Modelsgeocentric geostatic
- Eudoxus nested homocentric spheres
(non-physical, mathematical entities) - Aristotle solid crystalline spheres
Cant account for Retrograde Motion or Varying
brightness of planets
14Retrograde Motion
15Ancient Modelsgeocentric geostatic
- Apollonius
- - introduced the epicycle to explain
planetary and retrograde motion - Hippararchus
- - database of around 850 stars
- - suns motion represented by a path around the
Earth that was an off-centered circle (eccentric) - Both reject idea of crystalline spheres
16Eccentric Circle Epicycle
17Epicycle on Deferent
18Explains retrograde motion varying brightness
19Dominance of Aristotelian Thought
- Objects in Heavens unchanging
? Only motion in Heavens is circular motion
20Ptolemy (85-165) Egyptian-born Greek astronomer
- synthesized Hipparchus' observations with his
own and extended to Apollonius' model of the
universe by introducing more epicycles
produced a model that was to become accepted as
the standard model until the 1600s
21Ptolemaic Model
- spherical, unmoving Earth in central region of
Universe ? its natural place - not strictly geocentric - model used eccentrics
10,000 Earth diameters from the center) but
geostatic - stars fixed on celestial sphere that rotated once
every 24 hours. - Sun and the five planets had their motions
explained by combinations of epicycles, deferents
and eccentrics. In total some seventy circles and
spheres were required
22Ptolemaic Model
- inspired by Plato - model should fit observations
despite appearances introduced equant into his
model - Each heavenly body had its own equant which did
not coincide with the center of a planet's
deferent - concept of equant broke with the concept that
motion of spheres should be uniform but effective
in accounting for the variations noted in the
retrograde motion of planets
23Ptolemys model complex but standard for 1,500
years
- It worked - could predict the position of a
planet to within 2 - It accounted for observed planetary motions,
retrograde motion and variations in brightness - It placed the Earth in its natural place at the
center of things, satisfying Aristotelian
philosophy - It matched with common sense. We do not feel the
Earth move and Ptolemy's model had a static Earth
24Strictly Uniform Circular Motion
the speed of the yellow object along the circle
is uniform
the circle shares a center with the Earth
the object sweeps out equal angles in equal times
25Basic Construction - Epicycle
26Epicycle on Deferent
Deferent produces eastward motion seen most of
the time
Epicycle produces retrograde motion
explains varying size brightness of planets
27Basic Construction - Eccentric
28Eccentric Circle
Green object sweeps out equal angles in equal
times, maintaining a constant speed in its
perfectly circular path
But from the Earth, the object appears to move
faster in the bottom half of its motion than in
the top half
The motion of the green object is perfectly
uniform - it will appear nonuniform to observer
on Earth because the Earth does not coincide with
the center of the motion
29Basic Construction - Equant
Basic Construction - Equant
30Equant Circle
Body on circular path that does not share a
center with Earth
Object's speed varies in its orbit around that
circle--moves faster in the bottom half, slower
on the top half
Motion is uniform in that red object sweeps out
equal angles in equal times from a point inside
the circle
This equant point, not at center of circle nor at
center of Earth
Speed of object is nonuniform from perspective of
equant point, center of equant circle, and center
of Earth
31Combinations of three constructions
32All together
Deferent only yellow
Deferent eccentric green
Deferent eccentric equant red
33Ptolemys Model
Centers of the inferior planet between Earth and
sun epicycles move on an imaginary line
connecting the Earth and the Sun
Lines connecting superior planets outside of
Earth-sun pair to the centers of their epicycles
parallel to the line connecting Earth and Sun
34Why would ancient astronomers believe in a
geocentric model?
1. All motion in the heavens is uniform circular
motion
2. Objects in the heavens are made from perfect
material and cannot change their properties
(e.g., brightness)
3. Earth is a the center of the Universe
35Medieval Aristotelian Astronomy
- Philosophy of Aristotle wedded to Medieval
theology
- Earth in center concern God had for mankind
36Ptolemaic Model
Successfully accounted for naked eye observations
made by the ancient Greeks
- Epicycles within the epicycles existed (as many
as 28 for some planets)
Sun-linked epicyles of the inferior planets
explain why they always remain close to the Sun
in the sky
The epicycles of the superior planets account for
their occasional bouts of retrograde motion
Displacement of Earth from center of deferants,
introduction of equant as center of uniform
rotation explain why the planets speed up
slightly when they are close to the Earth (and,
hence, appear brighter in the night sky), and
slow down when they are further away