Exploring the Universe: Black Holes and Quasars

Exploring the Universe: Black Holes and Quasars

Assessment

Interactive Video

Physics

11th - 12th Grade

Hard

Created by

Jennifer Brown

FREE Resource

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the significance of the 'smudge' or 'blob' in astronomy?

It is a new planet discovered in our solar system.

It represents a distant galaxy with a supermassive black hole.

It is a type of nebula.

It is a new type of star.

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does Abell 2744 help astronomers observe distant objects?

By absorbing cosmic radiation.

By emitting its own light.

By acting as a gravitational lens.

By reflecting light from nearby stars.

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is UHZ1 known for?

Being the largest galaxy in the universe.

Being a newly discovered planet.

Being the closest quasar to Earth.

Being the most distant quasar ever discovered.

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the Eddington limit?

The maximum speed a black hole can rotate.

The maximum distance a black hole can be observed.

The maximum rate at which a black hole can feed.

The minimum size a black hole can be.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why is the absence of intermediate-mass black holes puzzling?

Because they emit no radiation.

Because they are only found in certain galaxies.

Because they are too small to be detected.

Because they should exist if supermassive black holes grew from stellar black holes.

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does the heavy seed model propose?

Black holes form from the collapse of stars.

Black holes form directly from gas clouds.

Black holes form from dark matter.

Black holes form from the collision of galaxies.

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is an OBG in the context of black holes?

An overly-massive black hole galaxy.

A new type of quasar.

A black hole formed from dark matter.

A type of star cluster.

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