
Chapter 4 Stars N'Galaxies,
Authored by Nicole Davis
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1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the primary purpose of spectroscopy in astronomy?
To infer the nature of matter by the way it emits and absorbs radiation
To determine the size of galaxies
To measure the distance of stars
To calculate the age of the universe
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What causes the dark lines in the spectrum of the star Arcturus?
Absorption of light in the star's cooler atmosphere
Scattering of light by interstellar dust
Reflection of light from nearby planets
Emission of light from the star's core
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is a spectroscope primarily used for?
To magnify distant objects
To detect gravitational waves
To split light into its component colors
To measure the temperature of stars
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the main difference between a spectroscope and a spectrograph?
A spectroscope is used for sound waves, while a spectrograph is for light
A spectroscope is simpler and used for viewing, while a spectrograph records the spectrum
A spectroscope is used in laboratories, while a spectrograph is used in space
A spectroscope measures temperature, while a spectrograph measures pressure
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the photoelectric effect?
Scattering of light by atmospheric particles
Absorption of light by a black hole
Reflection of light from a surface
Emission of electrons from a surface when light is absorbed
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
According to the Bohr model, what happens when an electron moves to a higher energy state?
The atom loses its nucleus
The atom absorbs a photon
The atom emits a photon
The atom becomes a different element
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the Zeeman effect?
Absorption of spectral lines by interstellar dust
Shifting of spectral lines due to motion
Broadening of spectral lines due to temperature
Splitting of spectral lines due to magnetic fields
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