Lecture 28 Flashcards

1
Q

How does the Hubble Tuning Fork hypothesise galaxy evolution?

A

Hubble proposed that galaxies evolved from early type elliptical galaxies to late type spiral galaxies

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2
Q

What is the approximate number of galaxies in the universe?

A

Approximately 70 billion

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3
Q

What does the galaxy stellar mass function show?

A

It shows that small galaxies are 100-1000x more common than massive galaxies

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4
Q

What do galaxies form from?

A

Giant gas clouds

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5
Q

What are the steps of galaxy formation?

A
  1. Gravitational stability
  2. Disk formation
  3. Hierarchical growth
    4.
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6
Q

What is gravitational instability?

A

Gravity pulls mass together to form overdensities

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7
Q

What occurs during the disk formation step?

A

Angular momentum decides whether a galaxy will form a disk or spheroid shape

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8
Q

What occurs during hierarchical growth?

A
  • multiple gas clouds collide to form larger galaxies from smaller ones
  • old stars take random orbits in the halo
  • as the galaxy grows older, new stars continue to form
  • galactic cannibalism occurs: smaller galaxies and dust clouds are “eaten” by larger galaxies
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9
Q

What causes the arms within spiral galaxies?

A

The arms in spiral galaxies are spiral density waves. They are long lasting waves of molecular cloud and star collapse. They do not carry matter.

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10
Q

What causes the spiral structure within spiral galaxies?

A

Stars in galaxies move in elliptical orbits. The spiral arms are patterns within the galaxy, not physical structures. Stars move in and out of the arms.

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11
Q

What is the movement of gas and stars through the spiral arms?

A
  • gas and dust clouds approach the arm
  • gas clouds are compressed to form new stars
  • young, blue stars eventually run out of energy and move out of the arm
  • low mass stars are able to live long enough to move out of the arm
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12
Q

How can we observe the younger universe?

A

Since distance and time are intertwined, we can view very distant galaxies to view the early universe. This is as light travels at a finite speed.

(Imaging distant galaxies compresses information into 2D)

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13
Q

Why can the finite speed of light be used to view the distant past?

A
  • photons transport information
  • it takes time for the photons to reach us
  • once the photons finally reach us they give us a snapshot of the past
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14
Q

When was the highest rate of galaxy formation in the universe?

A

The highest rate of galaxy formation occurred at around 3 billion years

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15
Q

What do galaxy collisions do to stars and gas?

A

They separate stars from gas and trigger new star formation from compressed gas clouds

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16
Q

What can happen to stars when galaxies collide?

A

They can form long tidal tails

17
Q

How can elliptical galaxies form?

A

Through the collision of galaxies