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Stars and Stellar Evolution Review

Total questions: 17

Worksheet time: 26mins

Name
Class
Date
1.

When a star is born, which quality determines how long that star will spend on the Main Sequence?

a)

Mass

b)

Color

c)

Spectral Class

d)

Equilibrium

2.

Which two qualities of a star are the MOST closely related? (ESRT - pg 4)

a)

Luminosity and Color

b)

Temperature and Color

c)

Mass and Color

d)

None of the Above

3.


Which star would burn hydrogen the fastest?

a)

a low-mass star

b)

a high-mass star

c)

an average star

d)

a black hole

4.

When is a star in equilibrium?

a)

During the Nebula stage

b)

When a black hole is beginning to form

c)

When the forces of gravity and fusion are the same

d)

During a Supernova

5.

What force helps push a cloud of gas and dust together to eventually make a star?

a)

Magnetism

b)

Pressure

c)

Gravity

d)

Centrifugal Force

6.

Which stars are the most likely to produce the heaviest elements?

a)

Low Mass stars

b)

Red Dwarfs

c)

High Mass stars

d)

All stars are capable

7.

This event occurs when high mass stars explode - sending heavy elements back into space

a)

A Black Hole

b)

A Supernova

c)

A Neutron Star

d)

A White Dwarf

8.

According to the HR Diagram (ESRT pg 4), as mass increases, _____________ also increases

a)

Luminosity

b)

Time spent on the Main sequence

c)

Nothing

9.

According to the Life Cycle of Stars (ESRT - Page 5), what factor best determines whether a star will become a black hole or a white dwarf

a)

Color

b)

Temperature

c)

Mass

10.

As an average sized star continues its life along the main sequence, which of the following is true?

a)

Hydrogen decreases as helium increases

b)

Iron decreases as helium increases

c)

Helium decreases as hydrogen increases

d)

Hydrogen and Helium remain equal

11.

What is the next stage in the life cycle of our Sun?

a)

White Dwarf

b)

Blue Supergiant

c)

Nebula

d)

Red Giant

12.

By comparing spectra observed from a star with the known emission lines (see ESRT pg 3), astronomers can determine the specific _______________present in a star.

a)

Gravity

b)

Elements

c)

Luminosity

d)

Solar Radius

13.

At the very end of its life cycle, what will our Sun become?

a)

A Black Hole

b)

A White Dwarf

c)

A Red Dwarf

d)

A Neutron Star

14.

You are an astronomer looking for planets that can support advanced life (like Earth). Which types of stars should you look near first?

a)

Massive, high energy stars

b)

Average sized, long living stars

c)

Stars that will supernova and send out heavy elements needed for survival

d)

Don't look near Stars.

15.

What is the approximate temperature of our Sun?

a)

22,000K

b)

9,500K

c)

3,200K

d)

5,800K

16.

Compared to our Sun, how much more luminous is the main sequence star Vega?

a)

10 times

b)

20 times

c)

100 times

d)

10,000 times

17.

Which spectral class contains the hottest stars?

a)

A

b)

O

c)

M

d)

G