
Astronomy Study Questions
Flashcard
•
Science
•
7th Grade
•
Practice Problem
•
Easy
Sven Tice
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30 questions
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1.
FLASHCARD QUESTION
Front
Describe geocentric and heliocentric models of the solar system.
Back
Geocentric: Earth is in the middle
Heliocentric: The sun is in the middle of the solar system
2.
FLASHCARD QUESTION
Front
Describe the solar system models of Aristotle, Aristarchus, Ptolemy, Copernicus and Kepler.
Back
Aristotle: The Earth is motionless in the center of the universe, and all other celestial objects orbit it in perfect circles.
Aristarchus: The earth orbits the sun like all the other planets.
Ptolemy: Geocentric like Artistotle's model, only with epicycles (mini-orbits)
Copernicus: Geocentric, remarkably similar to Aristarchus' model, only with actual evidence
Kepler: Geocentric with elliptical orbits instead of perfect circles
3.
FLASHCARD QUESTION
Front
Describe the contributions of Galileo to our knowledge of the solar system.
Back
Discovered:
Moons of Jupiter
Phases of Venus and Mercury
Mountains on the moon
That the Milky Way is made of stars
4.
FLASHCARD QUESTION
Front
Why was the geocentric model widely accepted for well over 1000 years?
Back
Parallax was not observable without modern technology.
The Earth doesn't obviously appear to be moving
It looks like the sun is going around the Earth, not the other way around.
5.
FLASHCARD QUESTION
Front
How did the geocentric model of Ptolemy account for the retrograde motion of some of the planets?
Back
He added epicycles
6.
FLASHCARD QUESTION
Front
How is parallax used to estimate the distance to some of the stars?
Back
If you know the angle of the motion of a star in six months, you can use the tangent of an angle to calculate the length of the "missing side" of the triangle that is formed in the sky (with points at Earth, sun and the star).
7.
FLASHCARD QUESTION
Front
Describe how the solar system was formed. Include how the earth ended up with a large moon.
Back
When the sun was in its protostar phase, it spun off a disc of gas and dust, which eventually cooled, clumped together, and formed the planets and other objects in our solar system.
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