U2 – Origins of the Universe – DE Astronomy

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20 Terms

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Stonehenge

believed to be a sort of 3D almanac/calendar to help identify important dates via specific celestial events

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Big Horn Medicine Wheel

native americans; similar with some alignments between spokes and the setting/rising sun and bright stars

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cosmology

study of the universe on the largest scales

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prograde motion

motion in eastward sense (west → east) (“regular”)

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retrograde motion

motion in westward sense (east → west) (“backwards”; those loops [Earth perspective] resulting from earth “overtaking” another planet)

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Ptolemaic Model

Ptolemy; geocentric model; fairly accurate to celestial sphere motions but very complex w/epicycles

<p>Ptolemy; geocentric model; fairly accurate to celestial sphere motions but very complex w/epicycles</p>
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Aristarchus of Samos

predicted heliocentric solar system

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Copernicus

credited with the (re)discovery of the heliocentric model; showed it provided natural explanation of observations

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Copernican Revolution

realization that Earth wasn’t at the center of the universe

(1) Earth not at center

(2) Moon orbits Earth

(3) planets revolve around Sun

(4) other stars much further away than Sun

(5) motion of stars due to rotation

(6) Sun’s “motion” due to Earth’s revolution/rotation

(7) retrograde an effect of Earth’s revolution

<p>realization that Earth wasn’t at the center of the universe</p><p>(1) Earth not at center</p><p>(2) Moon orbits Earth</p><p>(3) planets revolve around Sun</p><p>(4) other stars much further away than Sun</p><p>(5) motion of stars due to rotation</p><p>(6) Sun’s “motion” due to Earth’s revolution/rotation</p><p>(7) retrograde an effect of Earth’s revolution</p>
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Galileo Galilei

built his own telescope; discovered sunspots [Sun rotation], other planets’ moons [not geocentric], Venus phases [revolution around Sun], etc.

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aberration of light

(not the same as stellar parallax)

<p>(<strong>not</strong> the same as stellar parallax)</p>
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Tycho Brahe

observations of the night sky over many years at Uraniborg

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Johannes Kepler

developing laws of planetary motion; pure theorist primarily based on data via Tycho Brahe

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Kepler’s laws of planetary motion

(1) orbital paths are elliptical

(2) movement sweeps equal areas in same time

(3) P² proportional to a³ (in AU)

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Newtonian laws of motion

(1) object at rest will stay at rest until acted on by an outside force (inertia)

(2) F=ma

(3) every force has an equal and opposite reaction

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gravitational force equation

F = (GMm) / r²

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Newtonian alterations to Kepler’s laws

(1) planet + sun orbit their center of mass

(2)

(3) P² equals a³ (AU) / total mass of system (solar units)

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escape speed

v = sqrt(2GM/r)

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Caroline Herschel

discovered a bunch of planets and comets, very slay

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orbiting speed

v = 2πr/P