Quasars and the Milky Way

Quasars and the Milky Way

Assessment

Interactive Video

Physics

9th - 10th Grade

Hard

Created by

Jackson Turner

FREE Resource

The video explores the universe's structure, focusing on quasars, the most powerful objects in existence. It details their discovery, characteristics, and the immense energy they generate through supermassive black holes. Quasars significantly impact galaxy formation and evolution by heating and expelling gas, affecting star formation. The video also speculates on the Milky Way's potential quasar history and future. Finally, it promotes learning with Brilliant.org to deepen understanding of scientific concepts.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary composition of the intergalactic medium?

Oxygen and Carbon

Hydrogen and Helium

Nitrogen and Argon

Iron and Nickel

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why were quasars initially thought to be stars?

They had similar temperatures to stars

They appeared as dots in radio waves

They were located within the Milky Way

They emitted visible light

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main source of energy for quasars?

Nuclear fusion

Magnetic fields

Chemical reactions

Supermassive black holes

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the role of accretion disks in quasars?

They provide fuel for black holes

They emit radio waves

They create magnetic fields

They stabilize galaxy rotation

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How do quasars influence the intergalactic medium?

By absorbing all nearby gas

By creating new galaxies

By emitting gravitational waves

By launching jets of matter

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How do quasars affect star formation in their host galaxies?

By reducing magnetic fields

By cooling the gas

By heating the gas

By increasing gravity

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a potential benefit of quasars reducing star formation?

Faster galaxy rotation

Increased galaxy size

Higher star density

More stable planetary environments

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