Solar Phenomena and Structure

Solar Phenomena and Structure

Assessment

Interactive Video

Physics, Science, Biology

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video provides an in-depth look at the Sun's structure, starting from the core where nuclear fusion occurs, through the radiative and convection zones, to the photosphere and chromosphere. It explains the corona's high temperatures and the solar winds that extend beyond the solar system. The Sun's role in the solar system and its comparison to other stars are also discussed.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary composition of the Sun?

Iron and Nickel

Oxygen and Nitrogen

Hydrogen and Helium

Carbon and Oxygen

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the initial mass of a star like the Sun affect its characteristics?

It determines the star's color

It dictates the star's energy output and structure

It influences the star's rotation speed

It affects the star's magnetic field

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What process in the solar core is responsible for the Sun's energy output?

Combustion

Chemical Reaction

Nuclear Fusion

Nuclear Fission

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which layer of the Sun is responsible for transferring heat through convection?

Convection Zone

Radiative Zone

Photosphere

Chromosphere

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are sunspots?

Areas of high magnetic activity in the corona

Hotter spots on the chromosphere

Regions of intense solar wind

Cooler spots on the photosphere

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What color is the chromosphere primarily observed as during a solar eclipse?

Blue

Green

Red

Yellow

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the temperature range of the Sun's corona?

10 million to 15 million Kelvin

100,000 to 500,000 Kelvin

5000 to 7000 Kelvin

1 million to 3 million Kelvin

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