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Johnlukes Astronomy Haiku Deck
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Published on Nov 20, 2015
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PRESENTATION OUTLINE
1.
ASTRONOMISTS
2.
ARISTOTLE
A greek philosopher
His model placed the moon,sun, planets,and stars on a series of circles that surround the earth.
He thought that if Earth went around the sun, then the relative position of stars would change as earth moves.
He lived from 384-322 BCE
3.
ARISTARCHUS
A greek astronomer and mathmetician
His model that he created was not widely known and liked.
He attempted to measure the relative distance from the moon and the sun.
His ratio of distance was to small but was important in the use of observation and gemoetry to solve a scientific problem.
Lived from 310-230 BCE
4.
PTOLEMY
An astronomef, geographer, and mathematician.
His book, that was named "Almagest" is one of the few books we have from this early in time.
The book was on the observation of planets going back as much as 800 years ago.
His theory was that planets moved on larger circles. " wheels on wheels"
Lived from 100-170 BCE
5.
COPERNICUS
He thought that Ptolemy's theory was to complicated.
He used "wheels on wheels" system, he thought that they should travel in perfect circles.
He also thought that earth circled the sun.
1473-1543
6.
KEPLER
He realized that requiring planetary motion to be exactly circular did not fit.
He took another path and found that ellipses fit best.
Lives from 1571-1630
7.
GALILEO
Scientific method
He helped improve the telescope.
Observed the moons Io, Europa, Callisto, and orbiting jupiter.
Lived from 1564-1642
8.
KEPLERS 1ST LAW
He carefully plotted the orbit of mars, and it showed a deformed circle.
After 8 years, he realized that this was an ellipse.
Kepler placed the sun at one of the foci of the ellipse.
9.
KEPLERS 2ND LAW
Using the shape of an ellipse, he looked deeper in to the data.
He found that when planets get closer to the sun, they get faster.
10.
KEPLERS 3RD LAW
He calculated the orbital period and the distance from the sun for the planets using tycho's data.
He discovered that the square of the orbital period was proportional to the cube of the planets distance from the sun.
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