The Sun's Role and Structure in Our Solar System

The Sun's Role and Structure in Our Solar System

Assessment

Interactive Video

Physics, Science, Biology

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video explains the formation and structure of the Sun, its role in the solar system, and its eventual fate. The Sun formed 4.5 billion years ago from a solar nebula and became the center of our solar system due to its gravitational pull and magnetic field. It consists of six layers and is primarily composed of hydrogen and helium. The Sun's energy is produced through thermonuclear fusion in its core. Its gravity holds the solar system together, while its magnetic field protects planets from cosmic radiation. In 6.5 billion years, the Sun will exhaust its hydrogen fuel and become a white dwarf.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary role of the Sun in our solar system?

To absorb cosmic radiation

To provide light and heat

To orbit around Earth

To create new stars

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How many layers or regions can the Sun be divided into?

Four

Five

Six

Seven

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary fuel for the Sun's thermonuclear fusion?

Carbon

Nitrogen

Helium

Hydrogen

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What percentage of the solar system's mass does the Sun contain?

99.8%

90%

75%

50%

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the heliosphere?

The Sun's gravitational field

A region of intense heat

A layer of the Sun

The Sun's magnetic field

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What causes the Sun to act like a giant magnet?

Its heat and light

Its plasma pushing charged particles

Its gravitational pull

Its size and mass

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are sunspots?

Bright areas on the Sun

Dark areas indicating strong magnetism

Areas of high solar wind

Regions of intense heat

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