Cosmic Structures and Star Formation

Cosmic Structures and Star Formation

Assessment

Interactive Video

Physics, Science, Other

9th - 12th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video explores the formation of the universe from the Big Bang, focusing on the cosmic microwave background and density fluctuations that led to the formation of stars and galaxies. It describes the universe's structure using a soap bubble analogy, highlighting regions of high density where galaxies formed. The early universe was much denser, facilitating rapid star and galaxy formation, unlike the slower processes observed today.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What significant event allowed radiation to move freely in the universe?

The Big Bang

Decoupling

Formation of galaxies

Expansion of the universe

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What did scientists discover by studying the cosmic microwave background?

The speed of light

The presence of black holes

The exact age of the universe

Density fluctuations in the universe

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How are the filament-like structures in the universe described?

As spiral arms

As string-like objects

As flat sheets

As spherical clusters

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Where do stars and galaxies primarily form in the universe?

In isolated regions

At the center of black holes

Along the edges of soap bubble-like structures

In the voids

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What analogy is used to describe the structure of the universe?

A crystal lattice

Soap bubbles

A honeycomb

A spider web

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does a redshift of 20 indicate about the universe's size?

It was 1/20th its current size

It was 1/10th its current size

It was half its current size

It was twice its current size

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How much denser was the universe when it was 150 million years old compared to today?

500 times denser

100 times denser

10,000 times denser

8,000 times denser

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