Astro 150 S 2024 Final Review 1/2 - Apr 25, 2024 (1-14)
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Physics
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University
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Jake Simon
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20 questions
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1.
MULTIPLE CHOICE QUESTION
45 sec • 1 pt
What was the Copernican Revolution?
The shift from using a geocentric model to a heliocentric one
The shift from philosophy and intuition to empirical evidence to find truth
Copernicus's failed attempt to overthrow the Polish government
The shift to using the simplest explanation as the most likely one
Answer explanation
The shift from a geocentric to a heliocentric model was part of the Copernican revolution, but the Copernican revolution was more about how we found truth.
2.
MULTIPLE CHOICE QUESTION
45 sec • 1 pt
In ancient times, what was the major flaw of the Heliocentric model?
It could not explain retrograde loops
The Sun moved in the sky too much
It wasn't the simplest explanation
Parallax was not observed
Answer explanation
It wasn't until we developed advanced telescopes that we had instruments sensitive enough to detect stellar parallax.
3.
MULTIPLE CHOICE QUESTION
45 sec • 1 pt
What would the semimajor axis of a star with a 3 year period be?
9.14 AU
5.20 AU
3.02 AU
2.08 AU
Answer explanation
P is the period, so if we square the period of 3, we get 9. And then we take the cube root of 9 and that gets us 2.08 AU.
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Which force is responsible for light?
Strong nuclear force
Electromagnetic force
Weak nuclear force
5.
MULTIPLE CHOICE QUESTION
45 sec • 1 pt
Star 1
Star 2
They are the same
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
An blackbody with a blue peak wavelength should be ________ than one with a red peak wavelength?
Hotter
Cooler
Faster
Slower
Answer explanation
According to Wien's law, the peak wavelength of a blackbody is inversely proportional to its temperature. So, objects with a shorter (bluer) peak wavelength must be hotter.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What kind of spectrum do we see from the sun (and other stars)?
Emission spectrum
Absorption spectrum
Continuous spectrum
Blackbody spectrum
Answer explanation
This picture is the spectrum we see from the sun. It looks largely continuous, but there are some dark lines in there. Those are absorption lines, making this an absorption spectrum.
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