Throughout history, scientific geniuses from Galileo to Newton have often believed in completely fantastical things from astrology to alchemy to straight-up magic. Do you think that you are a genius when it comes to astronomy? Test out how true your answer is by tackling this challenging astronomy quiz. Good luck!
The Sun
Venus
Mars
Jupiter
Saturn
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Daytime in Sydney, Australia.
Midnight in Sydney, Australia.
Midnight in Los Angeles.
Midday in Rio de Janeiro, Brazil.
Midnight everywhere.
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It's about 4 light-years from here to Alpha Centauri.
It will take me light-years to complete this homework assignment.
A light-year is about 10 trillion kilometers.
It will take the Voyager spacecraft about 20,000 years to travel just 1 light-year.
The Milky Way Galaxy is about 100,000 light-years in diameter.
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It contains between 100 billion and 1 trillion stars.
Our solar system is located very close to the center of the Milky Way Galaxy.
The galaxy is about 100,000 light-years in diameter.
One rotation of the galaxy takes about 200 million years.
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The Northern Hemisphere is closer to the Sun than the Southern Hemisphere.
The Northern Hemisphere is "on top" of Earth and therefore receives more sunlight.
The Northern Hemisphere is tilted toward the Sun and receives more direct sunlight.
The Northern Hemisphere is tilted away from the Sun and receives more indirect sunlight.
It isn't: both hemispheres have the same seasons at the same time.
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Size of a typical galaxy
Size of Pluto's orbit
Distance to the nearest star (other than our Sun)
1 light-year
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Tycho Brahe
Aristotle
Kepler
Galileo
Ptolemy
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30 degrees up, due West
On the northern horizon
Directly overhead
The answer depends on whether it's winter or summer.
The answer depends on what time of day (or night) it is.
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A model tries to represent all aspects of nature.
A model tries to represent only one aspect of nature.
A model can be used to explain and predict real phenomena.
All models that explain nature well are correct.
All current models are correct.
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Tycho Brahe
Copernicus
Kepler
Galileo
Ptolemy
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An explosion caused by putting together two volatile chemicals
The process of splitting nuclei to produce energy
The process of turning matter into pure energy
The process of combining lightweight nuclei to make heavier nuclei
A process that only occurs in bombs
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A spiral galaxy with a disk about 100,000 light-years in diameter and containing between 100 billion and 1 trillion stars
A spiral galaxy with a disk about a billion kilometers in diameter and containing between 100 million and 1 billion stars
A spiral galaxy with a disk about 100,000 light-years in diameter and containing about 100,000 stars
A spherically shaped collection of stars including our solar system and about a dozen other solar systems, stretching about 4 light-years in diameter
A spherically shaped collection of about 1 million stars that is about 100 light-years in diameter
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Central and South America
The Mediterranean and the Middle East
North America
China
Southern Asia
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To explain why more distant planets take longer to make a circuit through the constellations of the zodiac
To explain the fact that planets sometimes appear to move westward, rather than eastward, relative to the stars in our sky
To explain why the Greeks were unable to detect stellar parallax
To properly account for the varying distances of the planets from Earth
To explain why Venus goes through phases as seen from Earth
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Tycho Brahe
Copernicus
Kepler
Galileo
Ptolemy
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A planet travels faster when it is nearer to the Sun and slower when it is farther from the Sun.
A planet's period does not depend on the eccentricity of its orbit.
Planets that are farther from the Sun move at slower average speeds than nearer planets.
The period of a planet does not depend on its mass.
Planets have circular orbits.
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Tycho Brahe
Copernicus
Kepler
Galileo
Ptolemy
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A conundrum or unexplained set of facts
A radical change in scientific thought
A generally well established scientific theory or set of theories
A pseudoscientific idea
A historical theory that has been proved inaccurate
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It was produced in the Big Bang.
It was created by chemical reactions in interstellar space.
It was produced by nuclear fusion in stars.
It was made by our Sun.
It was made by nuclear fission of uranium and other radioactive materials.
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It is the brightest star in the sky.
It is the star straight overhead.
It appears very near the north celestial pole.
It is the star directly on your northern horizon.
It can be used to determine your longitude on Earth.
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Both the Northern and Southern hemispheres receive the same amount of sunlight on the equinoxes.
Both the Northern and Southern hemispheres receive the same amount of sunlight on the solstices.
The Northern Hemisphere receives the most direct sunlight on the summer solstice.
The Southern Hemisphere receives the most direct sunlight on the summer solstice.
Both A and C are true.
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Precession of Earth's axis
The tilt of Earth's axis
The combined effect of the rotation of Earth and its orbit about the Sun
Earth year being a non-integer number of Earth days
The non-circular orbit of Earth around the Sun
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Size of a typical planet
1 light-second
1 AU
Size of a typical star
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All raisins would be moving away from you at the same speed.
More distant raisins would be moving away from you faster.
More distant raisins would be moving away from you more slowly.
It depends: If you lived in a raisin near the left side of the cake, you'd see other raisins moving away from you, but they'd be coming toward you if you lived in a raisin near the right side of the cake.
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A theory cannot be taken seriously by scientists if it contradicts other theories developed by scientists over the past several hundred years.
A theory is a model designed to explain a number of observed facts.
If even a single new fact is discovered that contradicts what we expect according to a particular theory, then the theory must be revised or discarded.
A theory must make predictions that can be checked by observation or experiment.
A theory can never be proved beyond all doubt; we can only hope to collect more and more evidence that might support it.
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The size of a typical dorm room
The size of a typical campus building
The size of a typical campus
The size of a small city
The size of a western state (e.g.,Colorado)
60
360
3,600
100
10,000
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As Earth passes another planet, its gravitational pull slows down the other planet so that it appears to be traveling backward.
When planets are farther from the Sun, they move slower than when they are nearer the Sun; it is during this slower period that they appear to move backwards.
The other planets never really appear to move backward; the background stars shift due to Earth's revolution around the Sun.
As Earth passes another planet, the other planet appears to move backward with respect to the background stars, but the planet's motion does not really change.
Apparent retrograde motion is an illusion created by turbulence in Earth's atmosphere.
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Every day at noon.
At noon on the summer solstice.
At sunset on the spring equinox.
At noon on the day of full moon each month.
During the totality of a total solar eclipse.
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The retrograde motion of the planets.
The phases of the Moon.
Eclipses of the Sun.
Galileo's observation of stars in the Milky Way.
Galileo's observations of the moons of Jupiter.
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Earth is the size of a point about 1 meter away from the Sun.
Earth is the size of a golf ball about 1 meter away from the Sun.
Earth is the size of a point about 15 meters away from the Sun.
Earth is the size of a golf ball about 15 meters away from the Sun.
Earth is the size of a marble about 25 miles away from the Sun.
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About half the year
About a month about a month about a month
A few hours
A few seconds
Less than a millionth of a second
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10 thousand years
230 thousand years
1 million years
100 million years
230 million years
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There are only 88 official constellations.
Some constellations can be seen from both the Northern and Southern hemispheres.
Some constellations can be seen in both the winter and summer.
It is possible to see all the constellations from Earth's equator.
Most constellations will be unrecognizable hundreds of years from now.
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The planet rises in the west and sets in the east.
The planet appears to move eastward with respect to the stars over a period of many nights.
The planet moves backward through the sky.
The planet moves backward in its orbit around the Sun.
The planet moves through constellations that are not part of the zodiac.
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13,000 km/hr
1,300 km/hr
130 km/hr
13 km/hr
Not moving at all
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The Moon goes through a cycle of phases because it always has the same side facing Earth.
If you see a full Moon from North America, someone in South America would see a new moon.
The Moon's distance from Earth varies during its orbit.
The Moon is visible only at night.
The side of the Moon facing away from Earth is in perpetual darkness.
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29 1/2–day period of the lunar cycle.
12-month period of a lunar calendar.
19-year period over which the lunar phases occur on about the same dates.
18-year, 11-day period over which the pattern of eclipses repeats.
Period between successive Easters.
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Understand the origin of Earth.
Make a more accurate model of the universe.
Predict the passing of the seasons.
Predict human events.
Antagonize astronomers.
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About 5000 years ago
About 2000 years ago
About 1000 years ago
About 500 years ago
About 100 years ago
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We observe all stars to exhibit at least a slight amount of parallax.
Stellar parallax was first observed by ancient Greek astronomers.
The amount of parallax we see depends on how fast a star is moving relative to us.
It takes at least 10 years of observation to measure a star's parallax.
The closer a star is to us, the more parallax it exhibits.
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From A.D. 600 to A.D. 1800 in Greece
From A.D. 600 to A.D. 1800 in Egypt
From 300 B.C. to A.D. 400 in Rome
From 300 B.C. to A.D. 400 in Greece
From 300 B.C. to A.D. 400 in Egypt
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The phase of the Moon must be new, and the nodes of the Moon's orbit must be nearly aligned with Earth and the Sun.
The phase of the Moon must be full, and the nodes of the Moon's orbit must be nearly aligned with Earth and the Sun
The phase of the Moon can be new or full, and the nodes of the Moon's orbit must be nearly aligned with Earth and the Sun.
The phase of the Moon must be new, and the Moon's orbital plane must lie in the ecliptic.
The phase of the Moon must be full, and the Moon's orbital plane must lie in the ecliptic.
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The phase of the Moon must be new, and the nodes of the Moon's orbit must be nearly aligned with Earth and the Sun.
The phase of the Moon must be full, and the nodes of the Moon's orbit must be nearly 6 aligned with Earth and the Sun.
The phase of the Moon can be new or full, and the nodes of the Moon's orbit must be nearly aligned with Earth and the Sun.
The phase of the Moon must be new, and the Moon's orbital plane must lie in the ecliptic.
The phase of the Moon must be full, and the Moon's orbital plane must lie in the ecliptic.
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Tycho Brahe
Copernicus
Kepler
Galileo
Ptolemy
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Counting the number of stars.
Determining the amount of gas and dust.
Studying how stars are distributed in the Milky Way.
Studying the rotation of the galaxy.
Weighing various parts of the Milky Way.
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It lies along the band of light we call the Milky Way.
It represents an extension of Earth's equator onto the celestial sphere.
It cuts the dome of your local sky exactly in half.
It extends from your horizon due east, through your zenith, to your horizon due west.
It extends from your horizon due north, through your zenith, to your horizon due south.
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The length of a football field
2.5 miles
250 miles
2,500 miles
25,000 miles
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