Module 13 Flashcards

1
Q

What are the three main types of galaxies classified by astronomers?

A
  • Spiral galaxies
  • Elliptical galaxies
  • Irregular galaxies

These classifications are based on their appearance and structural features.

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2
Q

What is the Hubble eXtreme Deep Field?

A

An image showing thousands of galaxies in a small patch of sky taken by the Hubble Space Telescope over 23 days.

This image helps estimate the total number of galaxies in the observable universe.

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3
Q

How many galaxies are estimated to be in the observable universe?

A

Well over 100 billion large galaxies and many more small ones.

This estimation is based on representative patches of the sky observed by telescopes.

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4
Q

What differentiates spiral galaxies from elliptical galaxies?

A

Spiral galaxies have a disk component and spiral arms, while elliptical galaxies lack a significant disk component and have only a halo.

Elliptical galaxies usually appear more rounded and redder due to older stars.

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5
Q

What are the two primary components of a spiral galaxy?

A
  • Disk component
  • Halo component

The disk contains stars and gas clouds, while the halo has older stars with random orbits.

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6
Q

What characterizes irregular galaxies?

A

They do not fit into the spiral or elliptical categories and often appear disorganized with young, massive stars.

Examples include the Magellanic Clouds.

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7
Q

What is the significance of galaxy color in relation to star formation?

A

Galaxies in the blue cloud have active star formation and young stars, while those in the red sequence contain older stars with little ongoing star formation.

This distinction helps in understanding a galaxy’s evolutionary path.

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8
Q

What does the tuning fork diagram created by Edwin Hubble represent?

A

A classification system for galaxies based on their shapes and components, with elliptical galaxies on the left and spiral galaxies on the right.

It shows the gradual change from elliptical to spiral characteristics.

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9
Q

Fill in the blank: Most galaxies in the red sequence are ______.

A

elliptical in shape.

They are typically redder due to the presence of older stars.

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10
Q

What type of galaxies are often found in loose collections of up to a few dozen?

A

Spiral galaxies with ongoing star formation.

Their environment influences their star formation activity.

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11
Q

How do astronomers infer the history of galaxies?

A

By observing different galaxies at various life stages and considering their distance and age.

This approach allows for understanding the evolution of galaxies over time.

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12
Q

What is the typical size range of dwarf galaxies?

A

Less than 1 million stars.

These are much smaller compared to giant galaxies with over 1 trillion stars.

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13
Q

True or False: The Milky Way Galaxy is classified as a spiral galaxy.

A

True.

It exhibits characteristics typical of spiral galaxies.

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14
Q

What does the presence of hot, young stars in a galaxy indicate?

A

Active star formation is occurring.

This is typically found in spiral and irregular galaxies.

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15
Q

What is a lenticular galaxy?

A

A type of galaxy that has a disk and halo but lacks spiral arms.

It is considered an intermediate class between spiral and elliptical galaxies.

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16
Q

What role does a galaxy’s environment play in its evolution?

A

It influences star formation rates and the transition between galaxy types.

Galaxies in denser environments may evolve differently compared to those in isolation.

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17
Q

What is the relationship between galaxy size and star formation cessation?

A

Larger galaxies tend to stop star formation sooner than smaller ones.

This is indicated by their position in the red sequence of galaxy color and luminosity diagrams.

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18
Q

What does the red sequence in galaxies suggest about star formation?

A

Star formation shuts down sooner in larger galaxies than in smaller ones

The red sequence refers to a group of galaxies that have ceased star formation and appear redder in color.

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19
Q

What are galaxy groups?

A

Loose collections of up to a few dozen galaxies

An example is our Local Group.

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20
Q

What distinguishes galaxy clusters from groups?

A

Galaxy clusters contain hundreds or thousands of galaxies and can be over 10 million light-years across

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21
Q

What percentage of large galaxies in the central regions of clusters are elliptical galaxies?

A

About 50%

Elliptical galaxies represent only about 15% of large galaxies found outside clusters.

22
Q

What role does a galaxy’s local environment play in its classification?

A

It helps determine whether a galaxy ends up as a spiral or elliptical galaxy

23
Q

What is parallax in astronomy?

A

The apparent shift in a star’s position as Earth orbits the Sun

24
Q

What is radar ranging?

A

A method where radio waves from Earth bounce off planets or objects to measure distance

25
What are standard candles?
Objects whose luminosity is known and can be used to calculate distance based on apparent brightness
26
What is the inverse square law for light?
A law that relates the brightness of an object to its distance from the observer
27
What are Cepheid variable stars?
A special class of luminous stars that pulsate in size, causing changes in brightness
28
What is Leavitt's law?
The relationship between a Cepheid's pulsation period and its luminosity
29
What is the significance of white dwarf supernovae in distance measurement?
They have nearly the same luminosity, making them valuable as standard candles for large distances
30
What was the Great Debate in astronomy?
A debate over the nature of spiral nebulae, whether they were part of the Milky Way or separate galaxies
31
Who were the main participants in the Great Debate?
Harlow Shapley and Heber Curtis
32
What was Shapley's argument in the Great Debate?
Spiral nebulae were gas clouds internal to the Milky Way
33
What was Curtis's position in the Great Debate?
Spiral nebulae were separate islands of stars
34
Fill in the blank: The distance to spiral nebulae was crucial for determining whether they were _______.
separate galaxies
35
What was the outcome of the Great Debate?
Neither Shapley nor Curtis scored a convincing victory
36
What was the rotation period claimed for the spiral nebula M101?
100,000 years ## Footnote This implied a relatively small and nearby structure, or else the rotation speed would exceed the speed of light.
37
What was the actual classification of the 1885 Andromeda 'nova' observed by Shapley?
Supernova ## Footnote This classification explained its surprising brightness.
38
Who was invited to join the staff at the Mount Wilson Observatory in 1917?
Edwin Hubble ## Footnote He delayed his acceptance to serve in World War I.
39
What significant discovery did Hubble make regarding Cepheids?
He discovered that some stars in the Andromeda spiral were Cepheids ## Footnote This allowed him to determine their luminosities using Leavitt's law.
40
What law did Hubble use to estimate the distance to the Andromeda Galaxy?
Leavitt's law ## Footnote It relates the period of Cepheid variables to their luminosity.
41
How did Hubble's measurements regarding the Andromeda Cepheids affect his conclusions?
He underestimated the true distance by about half ## Footnote This was due to not knowing about the two types of Cepheids.
42
What did Hubble's discovery about the Andromeda 'nebula' signify for the universe?
It proved that the Andromeda 'nebula' is a separate galaxy ## Footnote This changed the understanding of the universe from a single galaxy to many galaxies.
43
What did Hubble discover about the movement of galaxies in 1929?
The more distant a galaxy, the greater its redshift and the faster it moves away ## Footnote This led to the conclusion that the universe is expanding.
44
Who made the redshift measurements that Hubble initially used?
Vesto Slipher ## Footnote These measurements were made years earlier at the Lowell Observatory.
45
What is Hubble's law formula?
v = H₀ * d ## Footnote Where v is the recession speed, d is the distance, and H₀ is Hubble's constant.
46
What are the two practical difficulties encountered when using Hubble's law?
* Galaxies do not obey Hubble's law perfectly * Distances depend on the accurate measurement of Hubble's constant
47
What did the Hubble Space Telescope aim to measure regarding Hubble's constant?
An accurate value of Hubble's constant ## Footnote This was crucial for understanding distances to galaxies.
48
What chain of techniques is used to measure cosmic distances?
* Radar ranging * Parallax * Cepheid variables * Distant standards * Hubble's law
49
What implication does the expansion of the universe have on its history?
It suggests that the universe must have had a beginning ## Footnote This led to the concept of the Big Bang.
50
What does the Cosmological Principle imply about the universe's expansion?
The universe is not expanding into a void ## Footnote It suggests a more complex structure of cosmic expansion.
51
What is the significance of Hubble's discovery for our understanding of the universe?
It radically changed our view, revealing that the Milky Way is just one of many galaxies ## Footnote This opened up new avenues for astronomical research.
52
What did Hubble underestimate in his distance calculations?
The luminosities of Cepheids ## Footnote This was due to the fact that he observed the brighter type of Cepheid.