Astro 1500 Trivia October 25, 2024 - Lectures 15 and 16

Astro 1500 Trivia October 25, 2024 - Lectures 15 and 16

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15 Qs

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Astro 1500 Trivia October 25, 2024 - Lectures 15 and 16

Astro 1500 Trivia October 25, 2024 - Lectures 15 and 16

Assessment

Quiz

Physics

University

Hard

NGSS
HS-ESS1-3, HS-PS1-8, HS-ESS1-1

Standards-aligned

Created by

Amanda Weinstein

Used 16+ times

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15 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

45 sec • 1 pt

Media Image

Horizontal branch stars fuse helium, and helium fusion makes less energy than hydrogen fusion. So then, why does a horizontal branch star have a higher luminosity than a main sequence star?

Helium fusion happens faster

The helium fusing core is much larger than the hydrogen fusing core was

The star is fusing hydrogen and helium in the core

The star is fusing hydrogen in shells and helium in the core

Tags

NGSS.HS-ESS1-1

NGSS.HS-ESS1-3

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

A question to give you a sense of how much of a star's mass is in the core--what birth mass of a star corresponds to a core mass of 1.4 solar masses?

1.4 solar masses

2 solar masses

8 solar masses

16 solar masses

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

What keeps a white dwarf from collapsing?

Carbon's resistance to compression

Electrons that have the same properties as other electrons

Neutrons that have the same properties as other neutrons

Oxygen's resistance to compression

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

What happens if a white dwarf becomes more massive than 1.4 solar masses?

CRUNCH!

Dude, chill. It just gets more massive.

BOOM!

Tags

NGSS.HS-PS1-8

5.

MULTIPLE SELECT QUESTION

30 sec • 1 pt

Media Image

What happens when the core bounces before a supernova?

Trapped neutrinos escape

A shockwave blasts through the star

A black hole is formed

The star "gurgles" before exploding

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

Which is better at resisting collapse?

Neutron degeneracy pressure

Electron degeneracy pressure

They are equivalent, just present in different environments

7.

MULTIPLE CHOICE QUESTION

45 sec • 1 pt

Media Image

How do neutron stars become mostly neutrons?

The MS lifetime of the star made neutron-rich elements

Neutrons are captured from the supernova remnant

Extreme pressures merge electrons and protons

The protons are annihilated in the supernova

Tags

NGSS.HS-PS1-8

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