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Chapter 4 Stars N'Galaxies,

Authored by Nicole Davis

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University

Chapter 4 Stars N'Galaxies,
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10 questions

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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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