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Astro 1500 - Exam Review Pt 2

Total questions: 25

Worksheet time: 13mins

Name
Class
Date
1.

What will the sun become at the end of it's life?

a)

Brown Dwarf

b)

White Dwarf

c)

Neutron Star

d)

Black Hole

2.

What is the last element stars will fuse before they die?

a)

Helium

b)

Carbon

c)

Iron

d)

Uranium

3.

Alrighty then smart guy, then how is there gold in my phone right now?

a)

There isn't

b)

It was made in colliders on earth

c)

Created in other astronomical phenomena (supernovae, etc.)

d)

Results of chemical reactions on earth

4.

Rank these from strongest to weakest: Neutron Degeneracy Pressure , Fusion Pressure, Electron Degeneracy Pressure

a)

Fusion, Electron, Neutron

b)

Electron, Fusion, Neutron

c)

Neutron, Election, Fusion

d)

Electron, Electron, Electron

5.

What would happen to the earth if the moon were replaced by a black hole of mass equal to the moon?

a)

Tidal Forces would rip the earth apart

b)

Nothing much, tides would still be the same too

c)

It would slowly spiral inwards

d)

It would leave earth's orbit and begin orbiting the sun

6.

What does the solar system orbit?

a)

The black hole at the middle of the milky way

b)

The cumulative center of mass of everything in the milky way

c)

Proxima Centauri

d)

Nothing, the solar system only experiences random motion about the disk of the milky way

7.

If you triple the mass of a black hole, by how much does the escape velocity on the surface change?

a)

1/3

b)

3

c)

9

d)

It does not change

8.

What is our best evidence for dark matter?

a)

Rotation curves of stars in our galaxy

b)

Obscuration of light from far away stars

c)

Mysterious x-ray emissions from massive parts of galaxies

d)

All of the above

9.

Very roughly, how many stars formed in the milky way last year?

a)

6

b)

10 million

c)

1 billion

d)

100 billion

10.

How do we know what happens during galaxy mergers?

a)

Our galaxy merged with another in 1995, just ask an astronomy >30 yrs old

b)

Computer Simulations and observations of nearby galaxies

c)

CMBR perturbations

d)

The spin-flip line in hydrogen

11.

Where do elliptical galaxies generally form?

a)

In large voids of space

b)

In dense areas of galaxies

c)

13th and grand

d)

At least 5 Mpc from the nearest other elliptical galaxy (Pauli Exclusion Principle)

12.

We have direct, observational evidence for which kinds of black holes?

a)

Primordial

b)

Stellar Mass

c)

Intermediate mass

d)

Supermassive

13.

Where are we most likely to find population I stars in the milky way?

a)

The disk

b)

The center

c)

The Halo

d)

The image in the top left

14.

A neutron star will results from which of the below candidate stars?

a)

A star is 1.2X solar masses

b)

A star with 8X solar masses

c)

A star with 15X solar masses

d)

A star with 0.5X solar masses

15.

A short duration GRB is caused by ____, and a long duration GRB is caused by ____

a)

A Black Hole, Merging Black Holes

b)

Merging Neutron Stars, Hypernovas or Collapsars

c)

Hypernovas or Collapsars, Supernovas

d)

Pulsars, Merging Neutron Stars

16.

Is our galaxy moving towards or away from andromeda?

a)

Towards, the Universe is contracting and pulling everything together

b)

Towards, locally, gravity is strong enough to overpower the universe's expansion

c)

Away, locally, gravity is repulsive

d)

Away, the universe is expanding and pulling everything apart

17.

The mass of galaxies themselves are not enough to hold together huge filaments of material, what makes up the difference?

a)

Dark Energy

b)

Dark Matter

c)

The mass of the stars in the galaxies

d)

Nothing, these filaments are a momentary fluctuation of matter

18.

What disproved Einstein's notion that the universe is static and unchanging?

a)

Copernicus discovering the heliocentric orbit (meaning we move around the universe)

b)

Hubble's discovery the universe is expanding

c)

Supernovae

d)

The 1919 solar eclipse

19.

Of these options, which is the oldest?

a)

Globular Clusters

b)

Open Clusters

c)

Galaxy Clusters

d)

Black Holes

20.

What wavelength did the CMBR emit at 380,000 years post big bang?

a)

IR

b)

Visible

c)

Microwave

d)

Gamma Ray

21.

What is inflation in Astronomy?

a)

A period after the big bang where small scale density waves because large scale structures

b)

Everything gets more and more expensive which makes it harder for astronomers to get jobs

c)

A star quickly increases in size while not at the end of it's life

d)

Gas prices going up

22.

Gravity would resist expansion of the universe, what overpowers gravity to accelerate this expansion?

a)

Dark Matter

b)

Dark Energy

c)

Neutron Degeneracy Pressure

d)

Electron Degeneracy Pressure

23.

What percent of the universe is dark energy, by mass?

a)

5%

b)

27%

c)

68%

d)

95%

24.

Rank the boundaries of the universe from innermost to outermost.

a)

Surface of last scattering, Hubble sphere, Particle horizon

b)

Particle horizon, Surface of Last Scattering, Hubble Sphere

c)

Hubble sphere, Surface of last scattering, Particle Horizon

d)

The universe has no boundary

25.

What is the generally accepted value for H0?

a)

68 m/s/Mpc

b)

35 km/s/Mpc

c)

70 km/s/pc

d)

None of these options