Black Holes and Their Mysteries

Black Holes and Their Mysteries

Assessment

Interactive Video

1st - 10th Grade

Hard

Created by

Ethan Morris

FREE Resource

The video discusses the discovery of massive black holes, their locations, and their connection to quasars. It explains why black holes are not visible due to galactic dust and how they can be detected through light distortion. The potential threat of wandering black holes to our solar system is also explored, highlighting the possible disruptions they could cause.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the estimated mass of the black hole at the center of the Milky Way galaxy?

2 to 4 million times the mass of the Sun

2 to 4 million times the mass of the Moon

2 to 4 million times the mass of the Earth

2 to 4 million times the mass of Jupiter

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why can't we see the black hole at the center of the Milky Way clearly?

It is too far away

It is moving too fast

It is too small

It is obscured by clouds and galactic dust

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are quasars believed to be?

Distant planets

Old stars

Baby galaxies with raging black holes

Clusters of asteroids

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a possible reason we no longer see quasars in our galactic vicinity?

They have been destroyed

They have become quiet

They have moved to another galaxy

They have merged with other stars

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How can wandering black holes be detected?

By the distortion of light

By their smell

By their temperature

By their sound

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main characteristic of a wandering black hole?

It is stationary

It is visible

It emits light

It moves through the galaxy

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How is the detection of black holes similar to the function of glasses?

Both emit light

Both are visible

Both distort light

Both are heavy

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