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PHYSCI: How Did The Ancient Greeks Prove That The Earth Wasn't Flat?
PHYSCI: How Did The Ancient Greeks Prove That The Earth Wasn't Flat?
Ancient Greek
Around 500 B.C., most
Astronomy and Greeks believed
Cosmology that the Earth was round,
not flat. It
How did the was Pythagoras and his
Ancient Greeks pupils who
Around 500 B.C., most
Prove that the Greeks believed that
Earth Wasn't the Earth was round, not
flat. It was
Pythagoras and his
EXPLORE! pupils who were first to
Lesson 1.1 Around 500 B.C., most Greeks believed that the Earth was round,
not flat. It was Pythagoras and his pupils who were first to propose
Ancient Greek
a spherical Earth.
Astronomy and on the Moon during a lunar eclipse. He observed that during a
lunar eclipse, the Earth’s shadow was reflected on the Moon’s
surface. The shadow reflected was circular.
Cosmology Key Observations that led the Greeks to conclude that the Earth is
spherical:
How did the The Shadow that the Earth casts on the Moon during a
lunar eclipse is circular.
Ancient Greeks
Polaris - North Star was believed to be at a fixed position in
the sky. However, when the Greeks traveled to places nearer
the equator, like Egypt, they noticed that the North Star is
closer to the horizon.
Prove that the 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.
Earth Wasn't Disappearing Ships - If the Earth was flat, then a ship
traveling away from an observer should become smaller and
smaller until it disappeared. However, the Greeks observed
Lesson 1.1 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
Ancient Greek The Size of the Spherical Earth - Ancient scholars tried to
provide proof of a spherical Earth and its circumference
through calculations. It was Eratosthenes who gave the most
EUDOXUS’ MODEL
- The Sun, planets, and stars were then placed in giant
transparent spheres surrounding it.
HOMOCENTRIC MODEL
- Celestial spheres share one common center-earth
- 1st model of geocentric model
- Made up of 27 spheres
- 5 planets
PTOLEMY’S MODEL
- The Earth is at the center of the universe. The stars are fixed
on a sphere that revolves around the Earth, and the planets
(and the sun) revolve around the Earth at different distances.
Everything moves on perfect circles with constant speed.
- To account for Mars' retrograde motion two ingenious
geometrical devices were invented: the deferent (circular
path in which planets move) and the epicycle (a point close
to the orbit’s center).
- Planets move at a constant speed on the epicycle, and the
epicycle moves at a constant speed on the deferent around
the Earth. The combination of the two motions results in the
planet executing retrograde motion, with respect to the fixed
stars.
- Proposed the equant (a point close to the orbit’s center)
ARISTARCHUS’ MODEL
- Ancient Greek, Aristarchus was the first man who place the
sun at the center of the universe
- The sun and the stars are fixed
- The earth is revolving around the sun in a circular orbit
NICOLAUS COPERNICUS
- Copernicus realized that an object moving around you from
left to right looks the same as an object standing still while
you rotate from right to left.
- In his book, On the Revolution of Heavenly Spheres, he
wrote: "Every apparent change in respect to position is due to