Precursor of Science - Started the Theories and formulation of Hypothesis
Anaximander (610-545 BC)
Earth is a Cylinder and its Surface is Curved
Earth (Cylindrical) and Hollow at the center
Primary Element is Fire
Introduced the sundial
Hollow center
Earth is at the center
Pythagoras (570-490)
He was the first one to originate a spherical earth
North and South Constellations; Sinking Ships; and Lunar Eclipse
North and South Celestial Pole
North Star is believed to be at a fixed position
But when they travelled near the equator the North star appears to be closer
Sinking Ships
If the Earth was flat, then a ship traveling away from an observer should become smaller and smaller
But when the ship became smaller, its hull disappeared first which means that the Earth is curved
Partial Lunar Eclipse
Curved Shadow from a curved object
Pythagorean Model
Geocentric Model
Earth is round
Heavenly Bodies move in circle
Earth is at Rest and at the Center, and everything rotates on it
"The Music of Spheres" - motion of planets were mathematically related to musicalsounds and numbers
Plato(428-348 BC)
Earth is form of a globe having its extremes in every direction equidistant from the center
He believed that the universe is perfect or ethereal and unchanging
He further described the stars embedded in the outer space as ETERNAL AND DIVINE
Eudoxus of Cnidus (390-337 BCE)
Homocentric Model
1st model of the Geocentric Model
Celestial spheres share one common center (Earth)
27 interconnected spheres
Aristotle (384-322 BCE)
Earth is fixed as the center of the solar system that everything revolves around it
Proved that the earth is spherical
has 56 spheres around it (he added 3 sphere to jupiter and mars and added 4 to Sun, Moon, Venus and Mercury)
Primemovers - drives the motion of the planets
Erastosthenes
gave most accurate sizes during their time
40030 km - circumference of Earth
Using a stick
ClaudiusPtolemy (90-168 CE)
Earth Spherical Object
Planets moves with their independent motion which is Deferent and Epicycle
Deferent - Circular path in which planets moves
Epicycle - Circle where planets move in their own axis
Proposed the Equant - a point close to the orbit's center
Geocentric Astronomers
Pythagoras
Plato
Eudoxus
Aristotle
Eratosthenes
Ptolemy
Aristarchus' Model
Heliocentrism
1st to place the sun at the center of the universe
Sun and stars are fixed
Earth is revolving around the sun in a circular orbit
Nicolaus Copernicus (1473-1543)
proposed that the Earth revolved around the Sun.
corrected the geocentric theory and proposed the geocentric theory and proposed the Heliocentrictheory
Retrograde motion - in general, orbital, or rotational motion of an object in the direction opposite the rotation of its primary, that is the central object
direction from West to East
Copernicus' Model
Celestial motions are uniforms, infinite and circular
Planets revolved around the sun
Earth motion explains the retrograde motion os other planets
Earth spins on a tilted axis, which accounts for the seasons
Distance from the Earth to sun is smaller than earth to stars
TychoBrahe
modified the geocentric model
designed and built huge instruments used to make precise measurements of the positions of the planets
discovered supernova in the constellation Cassiopeia
observations of planetary motions that are important to the development of Kepler's Laws and other models of solar system
Tycho Brahe's Model
Geo-Heliocentric
the planets revolving around the earth, and the sun revolving around the earth
GalileoGalilei
telescope
discovered sunspots and rough surface of the moon
4 famous moons of Jupiter known as Galilean moons
Venus had phases like the moon
book "SidereusNuncius" (The StarryMessenger)
GalileoGalilei's Corrections
Lunar Craters
Phases of Venus
Moons of Jupiter
Sunspots
Supernova
Identical Size of the Stars
Johannes Kepler's 3 Laws of Planetary Motion
The Orbit Ellipses
Equal areas in equal time
Kepler's 1st Law
It states that the orbits of the planets are ellipses, with the sun at one focus
Perihelion - point nearest to the sun
Aphelion - point farthest to the sun
Kepler's 2nd Law
Planets travel faster during perihelion, travel slower during aphelion
Kepler's 3rdLaw
The cube of the radius of the orbit of a planet around the sun is proportional to the square of its period of revolution
The larger the planets orbit, the longer the revolution
The square of the revolution is directly proportional to the square of their averagedistances
1 Revolution of Planets
Mercury - 88 days
Venus - 225 days
Earth - 365 days
Mars - 687 days
Jupiter - 11.9 years
Saturn - 29.4 years
Halley's Comet - 76 years
Astronomical Unit
is the average distance between Earth and the Sun. which is about 93 million miles or 150 million kilometers