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30,000 BCE
Earliest known recording of the skies
Bone carvings keep track of phases of Moon. Early people engraved patterns of lines on animal bones to keep track of the phases of the Moon. -
4000 BCE
First observatories
Mesopotamian ziggurats serve as observatories. Mesopotamian astronomers made careful observations from the tops of pyramid-like towers called ziggurats. -
2000 BCE
Temple of Amen-Ra at Karnak
The Temple of Amen-Ra at Karnak, Egypt was built so that its main axis points to the sunset at the summer solstice. -
2000 BCE
Lunar eclipse observed at Ur in Mesopotamia
The oldest known recording of a lunar eclipse took place at Ur more than 4000 years ago -
700 BCE
Babylonians predict lunar eclipses
The Babylonians used their long record of eclipses to see regular patterns of eclipses. They used these patterns to predict lunar eclipses. -
700 BCE
Hesiod describes practical uses for astronomy
Hesiod's poem The Works and Days contains practical astronomical advice for navigation and for agricultural activities. -
580 BCE
Anaximander describes model of Earth
Sun, Moon, stars. Anaximander's model was the forerunner of later Greek attempts to explain the heavens in non-mythological terms. -
550 BCE
Pythagoras and students develop model of solar system
The model of Pythagoras used circular paths for the celestial bodies and assumed most celestial bodies are spheres. -
450 BCE
Herodotus concludes Earth is at least thousands of years old
Herodotus reasoned that it would have taken millenia for the annual Nile flood to have produced the Nile delta. p.160. -
400 BCE
Eudoxus explains retrograde motion
Eudoxus explains retrograde motion. Eudoxus's explanation involved the rotation of spheres in opposite directions. This geocentric model had the Earth at its center -
350 BCE
Aristotle argues celestial bodies are spheres.
Aristotle used a number of proofs that the Earth is a sphere, including the observation that its shadow on the Moon during lunar eclipses is always a circle. -
280 BCE
Aristarchus finds relative dimensions of solar system
Aristarchus concluded that the Earth was much smaller than the distances to the celestial bodies. He also invented a heliocentric (Sun-centered) model for the solar system.