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Space History • Ptolemy – 140 A.D. believed in geocentric system (planet revolve around Earth) • Planets and sun revolve (move) geo = Earth around Earth centric = Center • Planets revolve in smaller circles on a bigger circle at different rates and some have backward movements Space History • Copernicus – Early 1500’s believed in heliocentric system • helio Sun is= the Sun center and planets revolve around centric = Center • 6 planets: Mercury, Venus, Earth, Mars, Jupiter, and Saturn Space History • Galileo – 1500’s -1600’s believed in heliocentric system • 1st to use telescope to view objects in sky • 1st to see 4 moons revolving around Jupiter • Provided evidence that everything does not revolve around Earth - Venus goes through phases • Supported Copernicus’ theory – circular orbit Space History • Tycho Brache – late 1500’s observed planet positions of orbit for 20 years • Designed, built, and calibrated astronomy tools. • Johannes Kepler - 1600’s discovered via Tycho’s observations that planets move in elliptical orbits. Ellipse – An elongated circle, or oval shape Space History • Issac Newton – explained why the planets stay in orbit (inertia and gravity). • An object in motion stays in motion unless acted up on by an outside force – Inertia = The tendency of a Newton’s 1st Law of Motion (The Law moving object to continue moving of Inertia) or an object not moving to Gravity = The force that pulls remain stationary objects toward each other Gravity and Inertia • Inertia & Mass – Mass is the amount of matter in an object – The more MASS an object has, the more INERTIA the object has. – Bigger objects are harder to start & stop • Gravity – Depends on the masses of the objects and the distance between them Time line of Events • Ancient Greeks – 5 • • • • wandering star) points of light (planets = Ptolemy (140 A.D.) – geocentric system Copernicus (1514 - 43) – heliocentric system Brahe (1572-1598) – observed orbit of planets Galileo (1583-1633) – Provided evidence to support a heliocentric system (4 moons) • Kepler (1596-1619) – planets orbit move in elliptical • Newton (1664-) - explained force planets and motion of Systems Solar system = A large planetary •system Then – consisting 6 planets of smaller •planetary Now – 8 planets systems and objects. • Moon(s) revolve around some planets. • Each planet and its moon(s) = small system • Combinations of small systems = large systems Rotation vs. Revolution • Spinning on an axis • Causes night and day • Moving around another object • Causes seasons • About 24 hours = 1 turn • Takes about 1 yr for Earth to revolve around the sun The Sun • A star composed of H & He • Obtains energy via nuclear fusion The Sun http://videos.howstuffworks.com/hsw/6033-our-solar-system-the-structure-of-the-sun-video.htm • Core Nuclear fusion = combining of 2 • Photosphere atomic nuclei to produce a single • Chromosphere larger nucleus releasing energy. • Corona The Sun • Core – The central part of the sun, where nuclear fusion occurs Layer of the Sun • Photosphere – Inner layer – which makes light winds = A– stream of • Solar Chromosphere Middle layer photo = Light electrically charged particles – Visible during total solar eclipse chromo reddish= Color produced by the sun’s corona. – • causes Corona auroras - Outer layer forming a halo (crown) – visible only during total solar eclipse or special telescope Features on the Sun • The sun rotates on its axis every 30 days • Sunspots – vary in size – appear darker than rest of the photosphere b/c gives off less light and is cooler Sunspots dark, cooler – Occur = in A small groups or region pairs on the surface of the sun. Features on the Sun • Prominences - Reddish loop of gas protruding from the sun’s surface – links parts of sunspot regions. – About 10,000 degrees Celsius Features on the Sun • Solar flares – Explosion of H gas from the sun’s surface – occurs when loops in sunspot regions suddenly connect. – increase the solar wind from the corona – Cause magnetic storms auroras in Earth's night sky & disrupts radio transmission