The apple and the Moon

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Name: ______________________________________________________________ The Apple and the Moon Instructions: Print the guiding questions and use them to write your answers as you read or watch the instructional media (reading, video, radio podcast, computer simulation, etc.). Type the number of the question and your answer (do not re-copy the original question) and send the completed report to Blackboard’s SafeAssign. For all questions, answer in your own words (paraphrase). Answers that are directly copied from any internet source, including the instructional media studied, will receive no credit. The Apple and the Moon 1. What scientist first proposed the law of Universal Gravitation? 2. What scientist single-handedly laid the foundation of modern astronomy? What is the name of his famous book and the publication year? 3. What are epicycles? How did Copernicus use them to explain how the heavenly bodies moved? 4. What evidence did Galileo find to support Copernicus’ ideas? 5. State in your own words Kepler’s first law. 6. State in your own words Kepler’s second law. 7. State in your own words Kepler’s third law. 8. According to Newton’s law of gravitation, the more massive two objects are, what happens to the gravitational force? The farther apart two objects are, what happens to the gravitational force? 9. What is “G”? (Not to be confused with “g”) 10. Compare the acceleration of a falling body on the Moon and on Earth. 11. What would happen if a cannonball is fired at a high enough horizontal speed? 12. What is weightlessness? 13. Explain the importance of measurement 1/20th of an inch. 14. Describe other life achievements of Isaac Newton.

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School: Purdue University

Please find attached the answers in doc and PDF format.Please let me know if you have any doubts or need any explanation/update.

1. Isaac Newton first proposed the law of Universal Gravitation.
2. Nicolaus Copernicus single-handedly laid the foundation of modern astronomy. His
famous book on astronomy is “On the Revolutions of the Heavenly Spheres”. It was
published in 1543, when he was on his death bed.
3. By definition, epicycle is some small circle, whose center moves along the circumference
of a larger circle. It can be understood by below diagram:





Here, green circle is an epicycle, whose center moves around the circumference of red
To explain the motion of heavenly bodies, Copernicus assumed Sun (yellow body at the
center is the Sun) to be at the center of red circle. Blue body is some planet, which is
revolving in green epicycle, which itself is moving on the circumference of red
circle(deferent) around Sun.
Galileo invented telescope. He was the first person to use telescope to study heavenly
bodies. With his telescope, he saw four moons orbiting Jupiter. This observation was
contrary to Ptolemaic model that all heavenly bodies orbit around Earth, but this
observation can be explained by Copernicus’ idea that Sun is the center of solar system
and all planets are orbiting around Sun. In his idea, as Earth’s moon is orbiting around
Earth, other planets’ moons are orbiting around them, which explains Galileo’s
Kepler's first law tells that planets don't orbit in an exactly circular orbit around Sun.
They orbit in an elliptical orbit with sun at one of the foci of ellipse, so their distance
from sun is not constant, it keeps on varying.
Kepler's second law tells that speed of a planet is not same all the time, while orbiting
around Sun. When planet is close to Sun, it moves faster.
Kepler's third law compares the time taken by different planets in orbiting around Sun. It
tells that time taken by a planet in orbiting around Sun depends on size of its orbit. The
bigger the orbit, the more will be the time taken in competing one cycle.
According to Newton's law of gr...

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