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Stellar Explosions & Remnants

Total questions: 20

Worksheet time: 15mins

Name
Class
Date
1.

Term for "new star" that occurs in mass-transfer binary and/or white dwarf companion stars.

a)

supernova

b)

stella nova

c)

pulsar

d)

neutron star

2.

As material is added to the accretion disk, _____ may reach a temporary fusion point.

a)

pressures

b)

electron degeneracy

c)

temperatures

d)

matter

3.

Contact binaries may allow a white dwarf star to repeat

a)

electron degeneracy pressure.

b)

Roche lobe overload.

c)

flashes.

d)

explosions.

4.

A supernova occurs when a _____ star runs out of fuel (or overloads) and explodes.

a)

sun-like

b)

single

c)

massive

d)

double

5.

A ____ star with a mass of 1.4 suns may go supernova (I) if too much material accretes.

a)

white dwarf

b)

red dwarf

c)

red giant

d)

neutron

6.

Type II supernovae occur when a star with at least ____ times the mass of our sun explodes.

a)

1.4

b)

1.5

c)

3

d)

8

7.

Supernova 1987(a) occurred in this nearby galaxy 186,000 light years away.

a)

Andromeda

b)

Small Magellanic Cloud (SMC)

c)

Large Magellanic Cloud (LMC)

d)

M16

8.

Supernovae regularly occur in galaxies throughout the visible Universe.

a)

True

b)

False

9.

Type II supernovae explosions may leave behind a

a)

neutron star

b)

black hole

c)

pulsar

d)

white dwarf

10.

Neutron stars are formed when gravity squeezes electrons & _____ into neutrons in a supernova.

a)

protons

b)

isotopes

c)

quarks

d)

matter

11.

Neutron stars are between 1.4 - 3.2 solar masses and are compacted into an area

a)

the size of Earth.

b)

about the size of a large country.

c)

the size of the Sun.

d)

about the size of a city.

12.

One teaspoon of neutron star material can weigh more than

a)

Mt. Everest.

b)

a planet.

c)

a star.

d)

a black hole

13.

_____ are rapidly spinning neutron stars that are known as "lighthouses" in space.

a)

Quasars

b)

White dwarfs

c)

Pulsars

d)

Black holes

14.

Millisecond pulsars spin many times per second and have

a)

slowed down a lot over the years.

b)

very strong magnetic fields.

c)

sped up over the years.

d)

very weak magnetic fields.

15.

Pulsars were first detected in the 1960's by astronomers using radio telescopes.

a)

True

b)

False

16.

A black hole will form if the original star has at least _____ solar masses before collapse.

a)

four

b)

six

c)

eight

d)

ten

17.

The "cutoff mass" between a neutron star and a black hole is about ____ solar masses.

a)

1.4

b)

3.2

c)

4.4

d)

6.0

18.

The area or boundary in which nothing can return from a black hole is called

a)

the singularity.

b)

Interstellar.

c)

the path of no return.

d)

the event horizon.

19.

The ____ radius describes the size of the event horizon (which is black hole mass dependent).

a)

Hawking

b)

inner

c)

outer

d)

Schwarzschild

20.

There may be ____ of black holes in our galaxy alone - with Cygnus X-1 being the closest.

a)

billions

b)

millions

c)

hundreds

d)

thousands