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GEOS 105 Final
Astronomy Final
Question | Answer |
---|---|
THALES | 600-700 BC // Calendar: length of a year // Ecliptic: path of sun across the sky |
PYTHAGORUS | 500 BC // Cosmos should be perfect (spherical) // Religious |
Anaxagorous | 420 BC // Phases of the moon // Moon goes around the Earth // Distance of Sun to the Earth // Light from the moon is reflected sunlight // Lousy estimate |
New Moon Rises/Sets | Sunrise // Sunset |
1st Quarter Rises/Sets | Noon // Midnight |
Full Moon Rises/Sets | Sunset // Sunrise |
3rd Quarter Rises/Sets | Midnight // Noon |
Aristotle | 300-350 BC // Round Earth |
Proofs of a round Earth | 1) Ship looks like it sinks 2) Polaris gets lower and lower 3) Lunar eclipse (shape of shadow of Earth) 4) Elephants (?) In different areas |
Aristarchus | 250 BC // Distance and size of the Sun, Moon, and Earth // Very wrong |
Eratosthenes | 200 BC // Size of Earth and diameter |
Hipparchus | 150 BC // Trigonometry // Magnitude Scale (Brightness) // Systematic observations // Distance Earth to Moon // Length of year // Star catalog // Luminosity (amt of energy given off) // Flux (as you move away, decreases) |
Ptolomy | Geocentricity // Retrograde Motion |
Copernicus | 1540 // Heliocentric // Moon 27 1/3 Days (Sidereal period) // Sidereal day = 23 hrs 54 min // Sydonic day = 24 hrs // 29 days (sydonic) to line up with Sun // Inferior planets (between Earth and Sun) // Superior (outside) |
Tycho Brahe | 1572 // Castel of Uranienborg // Created precise astronomical measurements of the solar system and more than 700 stars // Great observer |
Kepler | Credit for Brahe's work // Protege // How planets orbit |
3 Laws of orbit | 1) Planet's orbits are ellipses with the Sun at 1 FOCI 2) Planets sweep = areas in = time 3) Period of planet (to orbit the Sun) determines how long to go around (DISTANCE DETERMINES TIME) |
Galileo | 1607 // Moons orbiting Jupiter // Spots on Sun // Saturn has rings and moons // Disproved Ptolomy model // IMPERFECTION EXISTS |
Newton's Laws | 1) Object at rest tends to stay at rest and an object in motion tends to stay in motion unless acted on by an outside force 2) Force = Mass x Acceleration 3) Every action there is an equal and opposite reaction |
Continuous Spectrum | Hot, HIGH pressure gas or solid |
Absorbtion Spectrum | Continuous, low pressure gas |
Emission | Hot, LOW pressure gas |
Kelvin - Hemholtz | Potential/Gravitational -> Kinetic Energy (KE) -> Heat |
Hans Bethe | Ideal gas // Pressure is proportional to temperature (P ~ T) // Outward pressure force balances gravity // Forces cancel each other // Hydrostatic Equilibrium |
Temperature of the Sun | ~ 6000 Kelvin |
Main sequence stars have _______ core fusion! | Hydrogen |
As temperature increases, luminosity _________ ! | Increases |
Chandrasekhar | Astrophysicist // Electron degenerate objects CAN'T be bigger than 1.4 Solar Masses (mO) |