History of Astronomy – Guided Notes Part 1



Download 19.14 Kb.
Date conversion25.04.2016
Size19.14 Kb.
History of Astronomy – Guided Notes

Part 1 Astronomy: The oldest science?

    • As far back as the Stone and Bronze Ages, human cultures realized the cyclical nature of the ______________ in the sky

    • Monuments dating back to ~3000 BCE show alignments with astronomical significance that might have been used as _______________________ or ancient observatories




  • Mesopotamian Astronomy ~ 1200 BCE

    • Earliest Babylonian __________ catalogues recorded observations on clay tablets

    • Babylonian astronomy was the basis for much of what was done in _____________ astronomy later

Greco-Roman Astronomy


  • Major Greek Astronomers

    • Aristotle (384-322 B.C.E.) – major authority in ancient Greece, promoted the idea of a geocentric universe and _____________________________

    • Eratosthenes (276 - 194, B.C.E.) – calculated the circumference of Earth using shadows and trigonometry

    • Ptolemy (85--165 C.E.) -- Wanted to create a mathematical model of the universe and explain ___________________ (backward) motion of the planets

  • Astronomy in ancient Greece

    • Greek models were based on “first principles”, believed to be _______________________ and not questioned:

      • ______________________ Universe: Earth at the center of the Universe.

      • “Perfect Heavens”: Motions of all celestial bodies described by motions involving objects of “perfect” shape, i.e., _________________ or circles.

      • “Unchanging Heavens”: always was and always will be the same

  • Aristotle’s Model of the Universe

    • Earth was at the ________________ of the universe

    • The heavens were literally composed of 55 crystalline spheres to which the celestial objects were attached

    • Each sphere __________________ at a constant velocity (although some spheres rotated faster than others)




  • Motions of the “Wanderers”

    • The ancient Greeks tracked __________ objects that seemed to move against the background of fixed stars in the sky: the Sun, the Moon, Venus, Jupiter, _____________, Mercury, and Mars

    • They named them “planets” (the Greek word for wanderers), and Aristotle’s model could not explain the motion of these wanderers who sometimes even appeared to move backwards from one night to the next.

  • Ptolemaic Model of the Universe

    • Ptolemy created a model that more accurately explained the motions of the sky, including the retrograde (backwards) motion of the planets

    • Ptolemy’s model became the standard used by scholars for 1,500 years because:

      • It worked! It could predict the __________________ of a planet to within 2°.

      • It accounted for the observed planetary motions, including retrograde motion and variations in brightness.

      • It placed the _____________ in its “natural place” at the center of things

      • It matched with common sense. We do not feel the Earth move, and we can see the stars and planets move

    • Ptolemaic system of epicycles (still ________________________ ) was the “standard model” up until the Renaissance

Part 2 Astronomy in the Renaissance

  • Nicolaus Copernicus (1473 – 1543)

    • Polish lawyer, physician, and mathematician

    • Studied the planets and proposed a new model for the universe

    • His model caused controversy by “changing our place in the universe”, leading to what is known as the Copernican Revolution




  • Copernican Model of the Universe

    • The Heliocentric Universe

      • ______________ at the center

      • Earth was a planet, and the _____________ revolved around Earth while the earth revolved around the sun

      • Original model still accepted Aristotle’s ideas of uniform motion and circular orbits, so it _________ __________ perfectly predict the motion of the planets



  • Arrangement of the Planets

    • Copernicus made observations that allowed him to determine the ________________ of the 5 planets known at that time

      • Mercury and Venus can only be observed fairly __________ to the sun at dawn or dusk (their orbits must lie inside of Earth’s orbit, since they are always in the same direction as the sun)

      • Mars, Jupiter and Saturn can be observed at night when the sun is far below the horizon (only possible if _______________ is between the sun and these planets, so they must lie outside Earth’s orbit)

      • By measuring the ___________ it took planets to return to the ______________ position in the sky, he determined their distances from the sun

  • Copernican explanation of retrograde motion in a heliocentric universe

    • Retrograde (backward) motion of a planet occurs when the Earth “passes” the planet as they both orbit the sun

Kepler and Galileo: Refining Heliocentric Cosmology

  • Johannes Kepler (1571-1630)

    • Kepler used Tycho Brahe’s meticulous observations to deduce a __________________________ explanation for the motion of the planets

    • Determined that Copernicus made a ______________-- planets do not orbit the sun in perfect circles!

  • Kepler’s Laws of Planetary Motion

  1. The orbits of the planets are ellipses with the _________ at one focus

  2. A line from a planet to the sun sweeps over equal areas in equal intervals of time.

  3. A planet’s orbital period (P) squared is proportional to its average distance from the sun (a) cubed

http://science.sbcc.edu/physics/flash/Keplers%20Laws.html

  • Kepler’s First Law (orbital shapes)

    • Orbits of planets are _________________________ with the sun at one focus

      • Eccentricity = how _________________________________ an ellipse is

      • Planet’s orbits are very close to circular with __________ eccentricities



  • Kepler’s Second Law (changing speeds)

    • A line from a planet to the sun sweeps over ____________ areas in equal intervals of __________________

    • Planets move ________________ when closer to the sun

  • Kepler’s Third Law (length of years)

    • There is a mathematical relationship between the __________________ from the sun and the _______________ it takes the planet to complete its orbit.

    • P2 = a3

  • Galileo Galilei (1564- 1642)

    • Greatly improved upon the newly invented telescope and made discoveries in ________________ of the Heliocentric model of the solar system

    • Galileo discovered

      • Four _____________ of Jupiter

      • Surface structures on the moon (not a perfect _______________ )

      • Sun Spots

      • Phases of _______________, proving it orbits the Sun and not Earth

  • Conflict of Religion and Science

    • Galileo’s observations and evidence in support of the Copernican Theory created a ___________________ between a faith-based system and the scientific ways of thinking based on observation and evidence

    • His methods and conclusions are considered the birth of the __________ __________________________________


Part 3: A New Era of Science

  • Astronomy continued to evolve after the Renaissance

  • Mathematics as a tool for understanding the _________________ of the universe became the central focus

  • Isaac Newton (1643 - 1727)




    • Invented __________________ as a necessary tool to solve mathematical problems related to motion




    • Discovered the three laws of _______________




    • Discovered the universal law of mutual _____________________




  • Newton’s Laws of Motion

    • Newton’s 1st Law of Motion - A body at rest continues to rest, and a body in motion will continue in uniform motion in a straight line unless it is acted upon by some net force. (AKA- ____________________)

    • Newton’s 2nd Law of Motion - Acceleration (a) of a body is inversely proportional to its mass (m), directly proportional to the net force (F), and in the same direction as the net force. (F = m a)

    • Newton’s 3rd Law of Motion- to every action there is an equal and opposite ______________________

  • Newton’s Universal Law of Gravity

    • More Mass = ____________ gravitational force

    • More Distance = _____________ gravitational force

  • Mass vs. Weight

    • Your weight is a measure of the force of gravity acting on your body

    • Your mass is a measure of how much matter you contain.

      • Your mass will be __________________ on the moon

  • Newton’s Laws of Motion and Law of Universal Gravitation helped explain WHY the planets move the way that they do


The database is protected by copyright ©essaydocs.org 2016
send message

    Main page