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Summary Of Astronomy

Published on Nov 18, 2015

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PRESENTATION OUTLINE

SUMMERY OF ASTRONOMY

By Keira Clyborne
Photo by fractalSpawn

ARISTOTLE

  • Greek philosopher
  • Thought the Earth was the center of all things
  • Realized when the Earth moves, the star's position would change
  • Used the Geocentric model
  • 384-322 BCE

ARISTARCHUS

  • 310-230 BCE
  • Greek astronomer and mathematician
  • Used the Heliocentric model
  • Attempted to measure distances to the sun and moon.
  • Ratio was too small

PTOLEMY

  • 100-170 CE
  • Lived in Alexandria, Egypt
  • Wrote the " Almagest"
  • Created. The Wheels on wheels system

NICOLAUS COPERNICUS

  • 1473-1543
  • Felt ptolemy's model was too complicated
  • Also used a wheels on wheels system
  • His Heliocentric model is seen as the first step of modern models

JOHANNES KEPLER

  • 1571-1630
  • German mathematician and astronomer
  • Did not believe planets to circle perfectly
  • Formed three principles (Kepler's Laws)

GALILEO GALILEI

  • 1564-1642
  • Used scientific methods
  • Added improvements to the telescope
  • Observed the moons, Io, Europa, Callisto and Ganymade. (Jupiter)
  • Observed that Earth was not the only thing orbited

ISAAC NEWTON

  • 1642-1727
  • First scientist to describe gravity scientifically
  • Formulated the "Law of universal gravitation"

EDWIN HUBBLE

  • 1889-1953
  • played a crucial role in establishing extragalactic astronomy
  • Proved "nebulae" were actually galaxies beyond the Milky Way.
  • Practiced armature boxing

GEOCENTRIC MODEL

  • Places the Earth at the center of the universe

HELIOCENTRIC MODEL

  • Places the Sun at the center of the universe

Kepler's first law:
Elliptical Orbits- planets orbit in a eclipse with the sun at one focus.

Kepler's second law:
Equal Areas, Equal Times: planets sweep out equal areas at equal times.
-at perihelion , the planets is moving faster
-at aphelion, planets is moving slower

Kepler's third law:
Length of Orbit/Distance from the Sun: the is a mathematical relationship to planets period of revolution and it's distance from the sun.

LAW OF UNIVERSAL GRAVITATION

  • The force of gravity:
  • Increases as the masses of the object increase
  • Decreases as the distance between the objects increases

Centripetal Force = planet's orbit

  • The sun's gravity is the force that keeps the planet in orbit