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Nuclear Fusion in Stars

Nuclear Fusion in Stars

Assessment

Interactive Video

Physics

9th - 12th Grade

Practice Problem

Hard

Created by

Patricia Brown

FREE Resource

The video explains the proton-proton chain, a nuclear fusion process in stars, primarily the sun, where hydrogen is converted into helium. This process occurs in three steps, involving proton collisions, formation of helium-3, and finally, a helium nucleus. The energy generated from these reactions powers the sun, which has been converting hydrogen to helium for 4.6 billion years and will continue for another 5 billion years. The video also discusses the mass-energy conversion principle, as described by Einstein's equation E=mc².

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary purpose of the proton-proton chain in stars?

To convert helium into hydrogen

To convert hydrogen into helium

To generate iron from nickel

To produce carbon from oxygen

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is required for two protons to overcome their repulsive forces and collide?

Magnetic fields

High velocities

Low temperatures

Gravitational pull

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

In the first step of the proton-proton chain, what particle is emitted when a proton turns into a neutron?

Positron

Neutrino

Electron

Photon

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is formed when deuterium and a proton collide in the second step of the proton-proton chain?

Tritium

Lithium

Helium-3

Helium-4

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is released during the formation of helium-3 in the proton-proton chain?

Neutron

Gamma ray

Beta particle

Alpha particle

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

In the final step of the proton-proton chain, what is the result of two helium-3 nuclei colliding?

Helium-3 and two protons

Helium-4 and a neutron

Helium-3 and a neutron

Helium-4 and two protons

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main energy source for the sun's power output?

Gravitational contraction

Nuclear fusion

Nuclear fission

Chemical reactions

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