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Introduction to Astronomy Notes

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Page 1: Introduction to Astronomy Notes
Page 2: Introduction to Astronomy Notes

The scientific study of the universe

Astronomy:

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Originally suggested the universe had a large stationary Earth in the center, and the sun, moon, and the stars were arranged around the Earth in perfect spheres orbiting in perfect or constant speeds

Original Thoughts:

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As careful mathematical observations were made, they found the Sun, the Moon, and some of the “stars” did not follow paths as thoughts

Original Thoughts

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The “stars” that did not follow the predicted path, rather they “wandered” across the sky, and thus were called “planets”, the Greek word for “wander”

Original Thoughts

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Aristotle’s Theories:

• The Earth was in the center, and the Sun, the

Moon, the stars, and the planets orbited on

separate spheres that encased each other and

spun at different rates

• Motion caused by a supernatural being

• Earth was a sphere (could see shadow on moon

during eclipse) and non-moving (because we

could not feel it and falling objects would not

drop straight down)

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Earth centered, model of the Universe

Geocentric Universe:

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Retrograde Motion:

A problem with Aristotle’s theory

was that objects would travel one

direction across, the sky, stop,

and go backwards

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Ptolemy’s Theories:

• Geo-centric

• Each planet was fixed to a small

sphere that was fixed to a larger

sphere

• No changes made for a 1,000 years

until the inaccuracies in predictions

became to big to blame on primitive

equipment

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Copernicus’ Theories

• Proposed a sun-centered universe

with the Earth spinning on its axis

once a day

• Orbits were perfect circles

• Did not publish his findings until his

death because it contradicted the

Church’s beliefs

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Sun-centered universe

Heliocentric Universe:

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Tycho Brahe’s Contribution

Built a top of line observatory,

gathered and kept tremendous

amounts of data

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Johannes Kepler’s Theories

Laws of Planetary Motion:

• Each planet revolves around the Sun in an elliptical

orbit with the sun at one of the foci

• Planets do not move at a constant velocity (due to

gravity pulling)

• There is a mathematical relationship between the

time it takes a planet to revolve around the sun and

its average distance from the sun

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Galileo Galilei’s Contribution

Developed and refined the

telescope for view distant objects

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Explosion of matter that occurred 14 billion years ago, and thus the universe expanding since that point

Big Bang Theory:

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Universe:

The entirety of what we call outer space

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A collection of stars, dust, and gas bound together by gravity (ours is the Milky Way Galaxy)

Galaxy

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A collection of planets that revolve around a star (sun)

Solar System

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The average distance between the Earth and the sun; approximately 150 million kilometers

Astronomical Unit:

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The speed of light is 300,000 km/s

Light Speed

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The distance that light can travel in one year (9.46 km x 1012)

Light Year

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All the frequencies or wavelengths of electromagnetic waves (energy)

Electromagnetic Spectrum

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Notes on the Elec. Spec.

• What we see falls into the visible light spectrum

• Only stars emit visible light, everything else (planets & moons) are reflecting light

• Other instruments can detect the other electromagnetic waves

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An instrument that collects electromagnetic radiation from the sky and concentrates it for better observation

Telescopes

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Telescopes that only collect visible light

Optical Telescopes

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Refracting Telescope: Uses a set lenses to focus light

Reflecting Telescope: Uses a set of mirrors to focus light

Optical Telescopes

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Used to detect radio waves, gamma rays, and infrared rays

Invisible Electromagnetic Radiation Telescopes

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Telescopes that were launched into space to escape obstructive Earth’s atmosphere (Hubble Telescope)

Space Telescopes