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Stellar Evolution & Explosions

Stellar Evolution & Explosions

Assessment

Presentation

Science

9th - 12th Grade

Medium

NGSS
HS-ESS1-3, HS-ESS1-4, HS-ESS1-1

+2

Standards-aligned

Created by

Anne Schnabel

Used 24+ times

FREE Resource

28 Slides • 19 Questions

1

Stellar Evolution & Explosions

Unit 7 Part 2

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Evolution = end of a star's life

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Multiple Choice

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High-mass stars burn hotter & brighter because they have more _______ at their cores.

1

fusion

2

fuel

3

energy

4

pressure

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Multiple Choice

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When temperatures are high enough in the core of a high-mass star, this element starts to form.

1

helium

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carbon

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oxygen

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hydrogen

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Optional video link on Student Notes Pages

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Optional video link on Student Notes Pages

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Multiple Choice

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When an ______ core is reached in a high-mass star, gravity takes over.

1

iron

2

carbon

3

oxygen

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helium

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Multiple Choice

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When an iron core is reached gravity takes over and a(n) _________ occurs.

1

black hole

2

neutron star

3

quasar

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supernova

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Multiple Choice

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Supernovas are one of the largest _______ in the Universe.

1

events

2

stars

3

explosions

4

objects

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Multiple Choice

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All elements heavier than carbon were formed in supernova explosions.

1

True

2

False

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Multiple Choice

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_____ stars evolve and move off the main-sequence first; then intermediate stars & so on.

1

Low-mass

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Red giant

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High-mass

4

White dwarf

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Multiple Choice

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The dividing line between high & low-mass stellar evolution is called the

1

dividing line.

2

main sequence turn off.

3

zero-age main sequence.

4

HR Diagram.

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Multiple Select

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Close binary star systems that share stellar material can affect how each star _____.(check all that apply)

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lives

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evolves

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functions

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interacts

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Optional video link on Student Notes Pages

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Multiple Choice

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

1

supernova

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stella nova

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pulsar

4

neutron star

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Multiple Choice

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

1

pressures

2

electron degeneracy

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temperatures

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matter

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Multiple Choice

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Contact binaries may allow a white dwarf star to repeatedly

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electron degeneracy pressure.

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Roche lobe overload.

3

flash or explode.

4

implode.

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Multiple Select

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

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sun-like

2

single

3

massive

4

double

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Multiple Choice

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

1

white dwarf

2

red dwarf

3

red giant

4

neutron

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Multiple Choice

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

1

1.4

2

1.5

3

3

4

8

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Multiple Choice

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Supernovae regularly occur in galaxies throughout the visible Universe.

1

True

2

False

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Optional video link on Student Notes Pages

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We don't see what is in a black hole, rather we see the acretion disk around it of what is "falling in"

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Multiple Select

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Type II supernovae explosions may leave behind a (check all that apply)

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neutron star

2

black hole

3

pulsar

4

white dwarf

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Multiple Choice

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

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Quasars

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White dwarfs

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Pulsars

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Black holes

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Multiple Choice

We can see black holes because

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light can escape it

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energy can escape it

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I have x-ray vision

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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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