IB Physics Cosmology

IB Physics Cosmology

11th - 12th Grade

•

73 Qs

quiz-placeholder

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IB Physics Cosmology

IB Physics Cosmology

Assessment

Quiz

•

Physics

•

11th - 12th Grade

•

Practice Problem

•

Hard

•
NGSS
HS-ESS1-3, HS-ESS1-2, HS-ESS1-1

+5

Standards-aligned

Created by

Charles Martinez

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73 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following is the largest?

Planet

Galaxy

Satellite

Comet

Star

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following is the largest?

Parsec

Lightyear

Astronomical Unit

1 billion Kilometers

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

'Spectrum of frequencies emitted due to electron transitions from a higher energy level to a lower one' is the definition of which key term?

Continuous spectrum

Absorption spectrum

Transition spectrum

Emission spectrum

Tags

NGSS.HS-PS4-3

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

'Spectrum of frequencies emitted due to electron transitions from a higher energy level to a lower one' is the definition of which key term?

Continuous spectrum

Absorption spectrum

Transition spectrum

Emission spectrum

Tags

NGSS.HS-PS4-3

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which is the correct order for a star's life cycle?

Main sequence -> red dwarf -> white dwarf

Protostar -> main sequence -> neutron star -> Red giant

Main sequence -> red giant -> supernova -> neutron star

Red giant -> supernova -> white dwarf -> black dwarf

Tags

NGSS.HS-ESS1-1

NGSS.HS-ESS1-3

6.

MULTIPLE CHOICE QUESTION

20 sec • 1 pt

What is the reason a Main sequence star is so stable?

The number of atoms remain the same

The radiation pressure balances the pressure of weight

Magnetic forces within it hold it together

It has plenty of emotional support from it's friends

Tags

NGSS.HS-ESS1-1

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What do we call the point which determines whether a star will become a white dwarf, or a supernova?

Degeneracy limit

Hertzsprung-Russel constant

Supernova determination constant

Chandrasekhar limit

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