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Fall 2023 Astro 150 Final Review Part 1

Total questions: 17

Worksheet time: 15mins

Name
Class
Date
1.

If the Sun were the size of a basketball and placed on this desk, how far away would Alpha Centauri be?

a)

Howe Hall

b)

Ankeny

c)

Not even in this state

d)

Sioux City

2.

Which of these is NOT one of Kepler's laws of planetary motion?

a)

Planets orbit the sun in elliptical orbits

b)

An object at rest stays at rest unless perturbed by an outside force

c)

Planets move faster when closer to the sun

d)

P2 = a3

3.

What supports a star from collapsing under its own gravity?

a)

Outward radiation pressure.

b)

Pauli exclusion principle.

c)

Centrifugal force due to rotation.

d)

Support from magnetic field lines.

4.

Star 1 has a brightness of 4*1010 erg/s/cm2 . Star 2 is twice as far away with the same luminosity. What is its brightness, also in erg/s/cm2?

a)

1*1010

b)

4*105

c)

2*1010

d)

2*105

5.

You observe two stars. Star #1 has a temperature 10x that of Star #2, but Star #1 is 1/10th the size of Star #2. How does the luminosity of Star #1 compare to Star #2?

a)

L1/L2 = 102

b)

L1/L2 = 10-2

c)

L1/L2 = 104

d)

L1/L2 = 10-4

6.

What is the total amount of time our Sun will spend on the Main Sequence?

a)

~1 billion years

b)

~5 billion years

c)

~10 billion years

d)

~13.8 billion years

7.

What kind of object will our Sun eventually turn into?

a)

A brown dwarf

b)

A white dwarf

c)

A neutron star

d)

A black hole

8.

A white dwarf star has a surface temperature of ~12,000 K. A red giant star has a temperature of ~4,000 K. Which star (according to Wein's Law) has a shorter peak wavelength? ( λmaxT = const.\lambda_{\max}T\ =\ const. )

a)

White Dwarf

b)

Red Giant

c)

Neither

d)

Not enough information

9.

What is a radio interferometer?

a)

An irritating radio signal that distorts astronomical radio data

b)

Such a device does not exist

c)

A device radio astronomers use to filter out earth-based radio broadcasts

d)

Several radio telescopes working together to improve resolution

10.

What is NOT an advantage of a GROUND BASED telescope?

a)

You can see any wavelength

b)

They're cheaper to construct

c)

There's much fewer limitations on the size of the telescope

d)

If something goes wrong, it's easier to fix

11.

Why are spectral lines different for each material?

a)

The electron orbital energy levels are different for every material

b)

The nucleus absorbs different amounts of energy from incoming photons, depending on the material

c)

The gravity of the different kinds of atoms slow down photons differently

d)

They aren't--spectral lines are a fun demonstration but they don't have any real scientific use

12.

What happens to an electron within an atom when it absorbs a photon?

a)

It drops to the lowest energy level

b)

It rotates around the atom faster

c)

It drops to a lower energy level

d)

It rises to a higher energy level

13.

You measure the spectrum of a star and take note of its absorption lines. These lines appear at shorter wavelengths than their laboratory counterparts. What can you say about this star?

a)

It is red-shifted, moving towards us

b)

It is blue-shifted, moving towards us

c)

It is red-shifted, moving away from us

d)

It is blue-shifted, moving away from us

14.

If Earth was moved to 0.5 AU, by how much would the gravitational force increase or decrease?

a)

It would increase by a factor of 2

b)

It would increase by a factor of 4

c)

It would decrease by a factor of 2

d)

It would decrease by a factor of 4

15.

What is the correct order for the layers of the sun? (from the outside in?)

a)

Corona, Convective Zone, Photosphere, Core

b)

Core, Convective Zone, Photosphere, Corona

c)

Convective Zone, Photosphere, Corona, Core

d)

Corona, Photosphere, Convective Zone, Core

16.

How can we determine the age of a star cluster?

a)

Looking at where the stars lie on an HR diagram.

b)

By measuring the total luminosity of the star cluster.

c)

By using stellar parallax.

d)

By measuring its velocity dispersion.

17.

A closer star is more likely to have...

a)

A high proper motion and small parallax angle

b)

A high proper motion and a large parallax angle

c)

A small proper motion and a small parallax angle

d)

A small proper motion and a large parallax angle