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Origin of Modern Astronomy Chapter 22
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22.1 Early Astronomy A.Ancient Greeks Aristotle- Earth is round because it casts a curved shadow on the Moon. (Luna eclipse)
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22.1 Early Astronomy A.Ancient Greeks Eratosthenes- measured the earth’s diameter.
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22.1 Early Astronomy A.Ancient Greeks Hipparchus (2 nd century B.C.) Star chart of 850 stars
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22.1 Early Astronomy A.Ancient Greeks Geocentric Model- earth centered and all objects “orbit” about the earth. Heliocentric Model- Sun centered
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22.1 Early Astronomy A.Ancient Greeks Ptolemaic System-Ptolemy Needed “epicycles” to make planets “retrograde”
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22.1 Early Astronomy B.Birth of Modern Astronomy Nicolaus Copernicus (1473-1543) Supported the Heliocentric Model in opposition of the Church.
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22.1 Early Astronomy B.Birth of Modern Astronomy Tycho Brahe (1546-1601) Very precise positions of Mars Johannes Kepler (1571-1630) Used Brahe’s information to discover 3 planetary laws.
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22.1 Early Astronomy B.Birth of Modern Astronomy Kepler’s Planetary Motion Laws 1.Move in ellipses. 2.Sweep out equal sectors in equal time. 3.Distance from Sun determines period of orbit.
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22.1 Early Astronomy B.Birth of Modern Astronomy Galileo Galilei (1564-1642) Pointed at telescope toward the stars….. 1.4 satellites about Jupiter 2.Planets were discs not pinpoints 3.Venus had “phases” 4.The Moon was not smooth 5.The Sun had “spots”
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22.1 Early Astronomy B.Birth of Modern Astronomy Sir Isaac Newton (1642-1727) Described laws of motion. First- inertia. Formulated and tested the Universal Law of Gravitation Gravity directly proportional to mass and inversely proportional to square of distance
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22.2 Earth-Moon-Sun System A. Motions of Earth Rotation-spin (1 day) Revolution-moves around Sun (1 yr.) Precession-swing about the axis (26 000 yr.)
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22.2 Earth-Moon-Sun System A. Motions of Earth Rotation Solar Day-time Sun returns to same position. About 24 hours Sidereal Day- turn 360 o, 23h 56m 4s
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22.2 Earth-Moon-Sun System A. Motions of Earth Revolution Perihelion- 150 million km Aphelion- 152 million km
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22.2 Earth-Moon-Sun System A. Motions of Earth Revolution Seasons because of axis tilt
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22.2 Earth-Moon-Sun System A. Motions of Earth Precession 26 000 years Change of tilt 21.5 o to 24.5 o 41 000 years
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22.2 Earth-Moon-Sun System A.Motions of Earth Solar System moving toward Vega at 20 km/s. Revolve about the Milky Way at 250 km/s 230 million year
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22.2 Earth-Moon-Sun System B. Earth-Moon System Perigee-closest Apogee-farthest
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22.2 Earth-Moon-Sun System B. Earth-Moon System Phases of the Moon
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22.2 Earth-Moon-Sun System B. Earth-Moon System Synodic month- 29 ½ days (Roman calendar) Sidereal month-27 1/3 days 2 more days to make a New Moon Revolves at 27 1/3 days. (same side)
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22.2 Earth-Moon-Sun System B.Earth-Moon System Eclipses Full Moon-Luna New Moon- Solar http://eclipse.gsfc.nasa.gov/eclipse.html
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22.3 Earth’s Moon Facts: 3475 km diameter 3.3x dense as water 1/6 G or 150 lbs man= 25 lbs on Moon A.Lunar Surface: dark lowlands bright highlands
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22.3 Earth’s Moon A.Lunar Surface: Craters- impacts by space debris
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22.3 Earth’s Moon A.Lunar Surface: Craters- Bright rays are created by recent impacts.
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22.3 Earth’s Moon A.Lunar Surface: Highlands: Some mountains are 8 km high.
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22.3 Earth’s Moon A.Lunar Surface: Maria: basaltic lava that “bleed out” Rilles- lava flows
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22.3 Earth’s Moon A.Lunar Surface: Regolith: ignous rock, beads and dust.
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22.3 Earth’s Moon A.Lunar History Most accepted model is Mars sized body collided with Earth.
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