Unit 34 Flashcards

1
Q

Elliptical galaxy

A

A galaxy with an elliptical shape and little dust or gas

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2
Q

Spiral galaxy

A

A galaxy flattened into a disk shape with a pattern of spiral arms wound about a central nucleus. Spiral galaxies usually include dust, gas, and active regions of star formation.

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3
Q

Dust lanes

A

The dark colored (brownish) squiggly line type structures visible in galaxies.

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4
Q

Irregular galaxy

A

A non-symmetrical galaxy that does not have a well defined shape like either the spiral or elliptical galaxies. Irregular galaxies include dust, gas, and active star-forming regions

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5
Q

Star cluster

A

A group of stars that formed from the same cloud of material and have been held together in a cluster by gravitational forces.

A small open cluster can consist of only a few dozen members while a large globular cluster can contain more than a million individual stars.

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6
Q

What plays the biggest role in determining which type of galaxy forms?

A

Angular momentum

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7
Q

Local group

A

A small group of about two dozen galaxies that is associated with our milky way (we’re in it)

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8
Q

Galaxy cluster

A

A group of galaxies that is gravitationally bound together into a cluster, which vary greatly in size. A small cluster may have just a few members, while a large cluster may have several thousand.

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9
Q

Supercluster

A

clusters of clusters of galaxies

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10
Q

Void

A

The space between galaxy superclusters

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11
Q

Cosmological red shift
(or just Red Shift)

A

The shifting of galaxy light to the red end of the spectrum caused by the expansion of the universe.
Doppler stuff. Think of the same affect of a police siren coming towards you, passing you, then moving away. The sound you hear at different points in this process will be different because of the wavelengths

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12
Q

What is the Hubble Law?

A

The proportionality between the observed recessional velocity of a galaxy and the distance to that galaxy.

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13
Q

Hubble constant

A

The constant of proportionality, H, in the Hubble Law. It gives the rate at which our Universe is expanding

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14
Q

Cosmic microwave background

A

A uniform radiant field with an apparent temperature of 2.725 K that is observable in every direction.

Microwaves from the big bang. The universe’ temperature.

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15
Q

What do the COBE and WMAP tell us?

A

That there are slight variations in the microwave temperature

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16
Q

Dark matter

A

Unseen matter in galaxies and galaxy clusters that exerts gravity within them

17
Q

Dark energy

A

An energy associated with space that is causing the universal expansion to accelerate faster with time

18
Q

Cosmological constant

A

A constant introduced into the equations of general relativity by Albert Einstein in an attempt to cancel the predictions of the expanding nature of our universe.

19
Q

Where are newer stars and forming stars found in spiral galaxies?

A

In the arms

20
Q
A