If the Earth was flat then a ship traveling away from an observer should become smaller until it disappeared
The Greeks observed that the ship became smaller and then its hull disappeared first before the sail as if it was being enveloped by the water until it completely disappeared
The Greeks observed the disappearance of ships
This suggested the Earth was not flat
The Shape of the Sun and the Moon
Aristotle argued that if the Moon and the Sun were both spherical then perhaps, the Earth was also spherical
Aristotle proposed the Earth was spherical based on the shapes of the Sun and Moon
North Star
The North Star was believed to be at a fixed position in the sky
When the Greeks traveled to places nearer the equator, like Egypt, they noticed that the North Star is closer to the horizon
The North Star appearing closer to the horizon as you travel towards the equator
Suggests the Earth is not flat
Most Greeks believed the Earth was round, not flat
Around 500 BC
Pythagoras and his pupils
They were first to propose a spherical Earth
Anaxagoras further supported the proposal of a spherical Earth through his observations of the shadows that the Earth cast on the Moon during a lunar eclipse
500 to 430 BC
Celestial domain
Perfect, made up of the perfect substance "ether", can only move in perfect circular motion at constant speed
Diurnal/daily motion of the sky
1. Appearance that objects in the sky move relative to the Earth's local horizon (celestial objects: moon, Sun, stars, planets; there were only five known planets: Mercury, Venus, Mars, Jupiter, Saturn)
2. Observed for one whole day at the same location on Earth
Annual motion of the sky
1. Appearance that objects in the sky move relative to the background stars
2. Observed at the same time of the day and at the same location on Earth
Terrestrial domain
Imperfect, tendency of things to attain perfection is the cause of their motion
Things move towards the center of the Universe (center of the Earth) or away from it based on their composition of the elements (fire, air, water, earth)
The Greeks made major contributions in different fields, including philosophy, science and mathematics
Pythagoras
Believed the stars, planets, sun, and moon were attached to crystalline spheres which rotated around the Earth (Geocentric model)
The five known planets were Mercury, Venus, Mars, Jupiter, Saturn
Plato
Believed the attainment of perfection is the absence of change
Mathematical symmetries demonstrate perfect shapes (sphere and circle)
Celestial spheres being crystalline and containing the moon, the Sun and the stars
The daily and annual patterns of the sky must have a greater reality besides its appearance
Plato believed the entire cosmos was precisely formed with geometric shapes and that they were the key to understanding the mysteries of the universe
Eudoxus
Followed previous models of the universe but added auxiliary spheres to provide appropriate tilt to the planets' path
Aristotle
Believed the Earth is motionless at the center of the universe and all the stars and planets revolved around it
Stars and planets moved in circular paths (Geocentric model)
Retrograde motion of planets
1. Necessitates the addition of more mechanisms called "devices" to produce the visual motion of the planets
2. Combination of deferent and the epicycles is the most practically accurate device during that era
Aristarchus proposed that the earth rotates around the sun
Precession of Equinox
1. Position of the stars shifted in a systematic way from earlier Babylonian measures (Hipparchus)
2. Observable phenomena of the rotation of the heavens, a cycle which spans a period of approximately 25920 years
Shape of the Earth according to ancient Greeks
Flat disc
Possible shapes of the Earth according to ancient Greeks
Cylinder
Octagon
Flat disc
Sphere
Shape of the Earth as described by modern astronomy
Oblate spheroid
Possible shapes of the Earth as described by modern astronomy
Ellipsoid
Oblate spheroid
Hyperboloid
Oblate paraloid
Events where the circular shadow of the Earth can be observed
Solar eclipse
Lunar eclipse
Events where the circular shadow of the Earth can be observed
Solar eclipse
Summer solstice
Lunar eclipse
Winter solstice
Position of the North Star if you go nearer the equator
Farther away from the horizon
Possible positions of the North Star if you go nearer the equator
Closer to the horizon
The North Star is fixed wherever you are on the Earth
It disappears completely
Farther away from the horizon
What can be observed of a cruising ship if the Earth is a flat disc
It will become smaller and smaller until it disappears
Possible observations of a cruising ship if the Earth is a flat disc
It will shrink then only the sail will be visible until it completely disappears
It will become bigger and bigger
It will notchange its size
It will become smaller and smaller until it disappears
Evidences that the Earth is spherical according to Greeks
Rising and setting of the Sun in the east and the west, respectively
Point where the Sun rises and sets in the horizon varies in a year
Phases of the Moon
Lunar eclipse
Daily and annual motion of the stars
Planets Mercury, Venus, Mars, Jupiter, and Saturn
Motion
The ability of an object to change its position with respect to its surroundings in a given time
Motion is always observed and measured with a point of reference
All living things show motion whereas non-living things show motion only when force acts on it
Types of motion
Linear motion
Rectilinear
Curvilinear
Circular motion
Rotary motion
Oscillatory motion
Aristotle
An ancient Greek philosopher and polymath whose writings cover a broad range of subjects including physics, biology, zoology, metaphysics, logic, ethics, aesthetics, poetry, drama, music, rhetoric, psychology, linguistics, economics, politics, meteorology, geology, and government