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PHYS 1303 (Stars and Galaxies) - Exam 3 Review

Total questions: 49

Worksheet time: 25mins

Name
Class
Date
1.

What is the name of our galaxy?

a)

Andromeda

b)

The Milky Way

c)

Triangulum

d)

Whirlpool

2.

What does AGN stand for in astronomy?

a)

Astronomical Galactic Network

b)

Active Galactic Nuclei

c)

Advanced Galactic Nebula

d)

Ancient Galactic Notation

3.

Which concept explains the origin of the universe?

a)

Galactic Evolution

b)

The Big Bang

c)

Dark Matter

d)

Interstellar Matter

4.

What does CMB stand for in cosmology?

a)

Cosmic Microwave Background

b)

Cosmic Magnetic Belt

c)

Central Milky Barrier

d)

Celestial Matter Base

5.

What type of galaxy is the Milky Way most likely classified as?

a)

Elliptical Galaxy

b)

Barred Spiral Galaxy

c)

Irregular Galaxy

d)

Lenticular Galaxy

6.

Approximately how many light years across is the Milky Way?

a)

10,000 Lt Yrs

b)

50,000 Lt Yrs

c)

100,000 Lt Yrs

d)

200,000 Lt Yrs

7.

What is found at the center of the Milky Way's nucleus?

a)

A large star cluster

b)

A supermassive black hole

c)

A nebula

d)

A planetary system

8.

Which type of stars are found in the Milky Way's nuclear bulge?

a)

Young O & B stars

b)

Population I stars

c)

Population II stars

d)

Red giant stars

9.

What is a characteristic of the Milky Way's halo?

a)

Contains interstellar dust

b)

Contains only hot interstellar gas

c)

Contains young stars

d)

Contains a supermassive black hole

10.

What is the primary function of dust in dark nebulae?

a)

Reflects light from nearby stars

b)

Blocks starlight from more distant stars

c)

Emits red light due to hydrogen

d)

Scatters stellar spectra

11.

What color is typically associated with reflection nebulae due to the scattering of light from hot young stars?

a)

Red

b)

Green

c)

Blue

d)

Yellow

12.

What causes the emission spectrum in emission nebulae?

a)

Reflection of light from nearby stars

b)

Absorption of light from distant galaxies

c)

Absorbed light from nearby bright stars causing fluorescence

d)

Scattering of light from the sun

13.

Why is the emission spectrum in emission nebulae typically red in color?

a)

Due to the presence of oxygen

b)

Due to the presence of nitrogen

c)

Due to the presence of hydrogen

d)

Due to the presence of helium

14.

What is a characteristic of barred spiral galaxies?

a)

Spiral arms attached to the ends of the "bar"

b)

Symmetric shape with no arms

c)

No current star formation

d)

Irregular shapes due to collisions

15.

What is a feature of elliptical galaxies?

a)

Presence of a barred central structure

b)

Symmetric shape with little to no interstellar dust

c)

Spiral arms coming from the central bulge

d)

Irregular shapes due to recent formation

16.

Which type of galaxy is more likely to have an Active Galactic Nucleus (AGN)?

a)

Barred spiral galaxies

b)

Elliptical galaxies

c)

Irregular galaxies

d)

Regular spiral galaxies

17.

What is a common trait of irregular galaxies?

a)

Symmetric shape with no arms

b)

No regular shapes, possibly due to collisions

c)

Presence of a barred central structure

d)

Spiral arms attached to the ends of the "bar"

18.

What is thought to be at the center of Active Galactic Nuclei (AGNs)?

a)

Super-Massive Black Holes

b)

Neutron Stars

c)

White Dwarfs

d)

Pulsars

19.

What are Quasars characteristic of?

a)

Earlier universe

b)

Future universe

c)

Present universe

d)

Parallel universe

20.

What does the term "Blasars" refer to?

a)

Looking down the barrel of a Quasar Jet

b)

A type of galaxy

c)

A type of star

d)

A type of nebula

21.

What are Seyfert Galaxies known for?

a)

Emission lines of highly ionized atoms

b)

Absorption lines of neutral atoms

c)

Reflection of light from stars

d)

Absorption of cosmic rays

22.

What are Liners associated with?

a)

Emission lines from neutral or slightly ionized atoms

b)

Absorption lines from highly ionized atoms

c)

Reflection of light from interstellar dust

d)

Absorption of gamma rays

23.

What do Radio-Loud-Lobes interact with?

a)

Intergalactic matter

b)

Cosmic microwave background

c)

Solar wind

d)

Earth's atmosphere

24.

What is less certain than stellar evolution scenarios according to the text?

a)

Galactic evolution

b)

Planetary formation

c)

Star formation

d)

Black hole creation

25.

What formed from smaller pre-galactic "blobs" according to the text?

a)

Larger galaxy-sized objects

b)

Black holes

c)

Nebulae

d)

Star clusters

26.

What type of galaxies formed with all older stars today?

a)

Smaller Elliptical Galaxies

b)

Spiral Galaxies

c)

Irregular Galaxies

d)

Dwarf Galaxies

27.

What type of collisions led to the formation of spirals?

a)

High angular momentum collisions

b)

Low energy collisions

c)

Random collisions

d)

Gravitational collisions

28.

What likely formed from collisions of large spirals?

a)

Giant Ellipticals

b)

Dwarf Galaxies

c)

Star Clusters

d)

Nebulae

29.

Why does galactic rotation not seem to become Keplerian?

a)

Because galaxies are too small

b)

Because of the presence of dark matter

c)

Because of the absence of gravitational forces

d)

Because of the presence of visible matter

30.

What does gravitational lensing by intermediate galactic clusters indicate?

a)

The presence of 2-3 times more mass than visible

b)

The presence of 5-6 times more mass than visible

c)

The presence of equal mass as visible

d)

The absence of any additional mass

31.

Why are intergalactic gas clouds too hot to be held together?

a)

Due to their own visible mass

b)

Due to the absence of dark matter

c)

Due to the presence of dark matter

d)

Due to gravitational forces

32.

What is dark matter not likely to be?

a)

Baryonic

b)

Non-baryonic

c)

Visible

d)

Invisible

33.

What does the clumping of clusters and superclusters of galaxies appear to be like?

a)

Foam-like or froth-like

b)

Solid-like or liquid-like

c)

Gas-like or plasma-like

d)

Crystal-like or glass-like

34.

What are the large regions found in the universe according to the text?

a)

Voids

b)

Stars

c)

Planets

d)

Black holes

35.

What type of structures are apparent in the universe?

a)

Wall-like structures

b)

Spiral-like structures

c)

Dome-like structures

d)

Cube-like structures

36.

When is it thought that the universe's structure was imprinted?

a)

During the Big Bang

b)

During the formation of the solar system

c)

During the creation of the Milky Way

d)

During the first supernova

37.

What indicates that the expansion of the universe is accelerating?

a)

The Supernova project using Type 1A Supernovae

b)

The movement of planets

c)

The rotation of galaxies

d)

The formation of new stars

38.

At what time does our understanding of the evolution of the Universe begin according to the Laws of Physics?

a)

Planck Time ~10^-43 s

b)

Quark Era ~10^-6 s

c)

Grand Unified Theories ~10^-35 s

d)

400,000 years after the Big Bang

39.

What significant event occurred during the Grand Unified Theories (GUT) period?

a)

Formation of atoms

b)

Rapid inflation of the Universe

c)

Separation of the Strong Force

d)

Nucleosynthesis of He and ²H

40.

During which era did the quarks and gluons precipitate into hadrons?

a)

Planck Era

b)

Quark Era

c)

GUT Era

d)

Nucleosynthesis Era

41.

What did the fluctuations in the Quark Era imprint?

a)

Primordial abundances of He and ²H

b)

Large Scale Structure

c)

Formation of atoms

d)

Dark Energy dominance

42.

When did atoms form in the Universe?

a)

During the Planck Time

b)

During the Quark Era

c)

About 400,000 years after the Big Bang

d)

At the end of the first second

43.

What is the Cosmic Microwave Background (CMB) evidence for?

a)

The Universe is expanding at an accelerating rate.

b)

The Universe is Flat and explains the contributions of Visible and Dark Matter and Dark Energy.

c)

The Universe is contracting.

d)

The Universe is static and unchanging.

44.

At what point in time was the light of the Cosmic Microwave Background released?

a)

~1 million years

b)

~400,000 years

c)

~10,000 years

d)

~100,000 years

45.

What does the Cosmic Microwave Background show about the early Universe?

a)

It shows the uniformity in densities.

b)

It shows the variation in densities.

c)

It shows the absence of any density variations.

d)

It shows the increase in densities over time.

46.

What are some of the factors included in the Drake Equation?

a)

Number of stars in the galaxy, fraction in habitable zone, probability of life evolving

b)

Distance from Earth, size of the galaxy, speed of light

c)

Number of black holes, fraction of dark matter, speed of sound

d)

Distance from the Sun, size of planets, number of moons

47.

Which of the following is a Rare Earth Factor?

a)

Need for Jupiter

b)

Distance from the Sun

c)

Number of black holes

d)

Speed of light

48.

What does SETI stand for?

a)

Search for Extra-Terrestrial Intelligence

b)

Space Exploration and Technology Institute

c)

Solar Energy Transmission Initiative

d)

Scientific Exploration of Terrestrial Inhabitants

49.

According to the document, what is the likelihood of primitive life in the universe?

a)

Very likely prolific and common

b)

Extremely rare and unlikely

c)

Only found on Earth

d)

Non-existent