TED-ED: The law of conservation of mass - Todd Ramsey

TED-ED: The law of conservation of mass - Todd Ramsey

Assessment

Interactive Video

Physics, Science, Other, Chemistry

KG - University

Hard

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The video explores the origin and transformation of atoms, starting with the Law of Conservation of Mass, which states that mass cannot be created or destroyed. It demonstrates chemical reactions, such as the formation of water and carbon dioxide, and explains how energy is stored and released. The video also covers combustion reactions with methane and propane, emphasizing the conservation of atoms. Finally, it traces the origin of atoms back to the Big Bang, explaining how stars formed heavier elements and scattered them across the universe, leading to the formation of Earth and life.

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5 questions

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1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does the Law of Conservation of Mass state about matter in an isolated system?

Matter can be created but not destroyed.

Matter can change forms but cannot be created or destroyed.

Matter can be created and destroyed.

Matter can be destroyed but not created.

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

In the context of chemical reactions, what happens to the atoms involved?

They lose their mass.

They rearrange to form new molecules.

They change into different elements.

They disappear after the reaction.

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a common use of methane besides being associated with cow flatulence?

As a building material

As a cleaning agent

As a rocket fuel

As a food preservative

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How are heavier elements like carbon and oxygen formed in the universe?

Through chemical reactions on Earth

By the fusion of light elements in stars

Through volcanic activity

By the splitting of atoms in space

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What significant event is believed to have led to the formation of hydrogen atoms?

The creation of the solar system

The first supernova

The Big Bang

The formation of Earth