
Stellar Evolution & Explosions
Presentation
•
Science
•
9th - 12th Grade
•
Medium
+2
Standards-aligned
Anne Schnabel
Used 24+ times
FREE Resource
28 Slides • 19 Questions
1
Stellar Evolution & Explosions
Unit 7 Part 2
2
3
4
Evolution = end of a star's life
5
6
Multiple Choice
High-mass stars burn hotter & brighter because they have more _______ at their cores.
fusion
fuel
energy
pressure
7
Multiple Choice
When temperatures are high enough in the core of a high-mass star, this element starts to form.
helium
carbon
oxygen
hydrogen
8
9
Optional video link on Student Notes Pages
10
11
Optional video link on Student Notes Pages
12
Multiple Choice
When an ______ core is reached in a high-mass star, gravity takes over.
iron
carbon
oxygen
helium
13
Multiple Choice
When an iron core is reached gravity takes over and a(n) _________ occurs.
black hole
neutron star
quasar
supernova
14
Multiple Choice
Supernovas are one of the largest _______ in the Universe.
events
stars
explosions
objects
15
Multiple Choice
All elements heavier than carbon were formed in supernova explosions.
True
False
16
17
18
19
Multiple Choice
_____ stars evolve and move off the main-sequence first; then intermediate stars & so on.
Low-mass
Red giant
High-mass
White dwarf
20
Multiple Choice
The dividing line between high & low-mass stellar evolution is called the
dividing line.
main sequence turn off.
zero-age main sequence.
HR Diagram.
21
22
23
24
25
Multiple Select
Close binary star systems that share stellar material can affect how each star _____.(check all that apply)
lives
evolves
functions
interacts
26
Optional video link on Student Notes Pages
27
28
29
30
Multiple Choice
Term for "new star" that occurs in mass-transfer binary and/or white dwarf companion stars.
supernova
stella nova
pulsar
neutron star
31
Multiple Choice
As material is added to the accretion disk, _____ may reach a temporary fusion point.
pressures
electron degeneracy
temperatures
matter
32
Multiple Choice
Contact binaries may allow a white dwarf star to repeatedly
electron degeneracy pressure.
Roche lobe overload.
flash or explode.
implode.
33
34
35
36
Multiple Select
A supernova occurs when a _____ star runs out of fuel (or overloads) and explodes. (check all that apply)
sun-like
single
massive
double
37
Multiple Choice
A ____ star with a mass of 1.4 suns may go supernova (I) if too much material accretes.
white dwarf
red dwarf
red giant
neutron
38
Multiple Choice
Type II supernovae occur when a star with at least ____ times the mass of our sun explodes.
1.4
1.5
3
8
39
Multiple Choice
Supernovae regularly occur in galaxies throughout the visible Universe.
True
False
40
41
42
Optional video link on Student Notes Pages
43
44
We don't see what is in a black hole, rather we see the acretion disk around it of what is "falling in"
45
Multiple Select
Type II supernovae explosions may leave behind a (check all that apply)
neutron star
black hole
pulsar
white dwarf
46
Multiple Choice
_____ are rapidly spinning neutron stars that are known as "lighthouses" in space.
Quasars
White dwarfs
Pulsars
Black holes
47
Multiple Choice
We can see black holes because
light can escape it
energy can escape it
I have x-ray vision
we see the light of the stars at its event horizon, they reflect off of objects around the accretion disk
Stellar Evolution & Explosions
Unit 7 Part 2
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