Proposed by Pythagoras and his pupils around 500 B.C.
Anaxagoras
Supported Pythagoras' proposal by observing the shadows that the Earth cast on the moon during a lunar eclipse (500 to 430 B.C.)
Aristotle
Listed several arguments for a spherical Earth around 340 B.C. (position of the North Star, shape of the Moon and the Sun, observation from ship traveling away)
Eratosthenes
Greek scientific writer, astronomer, and poet who made the first measurement of the size of Earth for which any details are known (born c. 276 BCE, died c. 194 BCE)
Eratosthenes' method
1. Measured the angle the Sun made with the vertical direction in Alexandria and Syene
2. Hypothesized that the light rays coming from the Sun were parallel and the Earth was curved
3. Computed the circumference of the Earth to be approximately 250,000 stadia (about 40,000 km)
Astronomical Phenomena
Events observable in the sky as studied by the scientific discipline of astronomy
Celestial Sphere
An imaginary sphere where all objects in heavens are projected, useful in pinpointing objects in space as well as defining Earth-based positions relative to the sky
Diurnal Motion
The apparent daily motion of celestial objects from eastto west in which celestial objects seem to riseand set
Annual Motion
The apparent yearly movement of the Earth across a background of stars, caused by Earth's revolution around the Sun
Phases of the Moon or Lunar Phases
New Moon
Waxing Crescent
First Quarter
Waxing Gibbous
Full Moon
Waning Gibbous
Third Quarter
Waning Crescent
New Moon
The side of the moon that is facing Earth is not illuminated by the sun
Waxing Crescent
The moon appears as a thin crescent shape in the sky, with only a small portion of its surface illuminated
First Quarter
The moon appears as a half-circle in the sky, with exactly half of its surface illuminated by the sun
Waxing Gibbous
The moon appears in a mostly illuminated crescent shape, with only a small part appearing dark
Full Moon
The entire face of the Moon that is visible from Earth is fully illuminated
Waning Gibbous
The Moon appears as a large and bright, but gradually shrinking, crescent shape in the sky
Third Quarter
The Moon appears as a half-moon shape, with half of its face illuminated by sunlight
Waning Crescent
The Moon appears as a thin crescent, with a small portion of its face illuminated by sunlight
Eclipse
The total or partial obscuring or another of one celestial body by another
Solar Eclipse
The Moon passes between the Sun and Earth, casting the Moon's shadow on Earth that either fully or partially blocks the Sun's light in some areas
Lunar Eclipse
The earth's shadow blocks out our view of the moon during the full moon
Geocentrism
The idea that the Earth is the center of the universe, popularized by Ptolemy in 150 BCE
Heliocentrism
The idea that the sun, not the Earth, is the center of the universe, argued by Copernicus in 1543
Tycho Brahe
Developed an early interest in astronomy, made significant astronomical observations, designed and built new instruments, calibrated them, and instituted nightly observations (1546-1601)
Tycho Brahe's model
The Earth is at the center of the universe, the Sun and Moon and the stars revolve around the Earth, and the other five planets revolve around the Sun
Johannes Kepler
Became Tycho Brahe's successor, was given access to Brahe's data on Mars, and formulated his three laws of planetary motion (1571-1630)
Kepler's Three Laws of Planetary Motion
Law of Ellipses: The path of the planets about the Sun is elliptical in shape, with the center of the Sun being located at one of the foci
Law of Equal Areas: An imaginary line drawn from the center of the Sun to the center of the planet will sweep out equal areas in equal intervals of time
Law of Harmonies: The square of the period of a planet orbiting around the sun and the cube of the long radius are proportional to each other