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Solar Energy on Earth

Solar Energy on Earth

Assessment

Flashcard

Science

6th - 8th Grade

Hard

Created by

Barbara White

FREE Resource

Student preview

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13 questions

Show all answers

1.

FLASHCARD QUESTION

Front

Radiation Noun

[ray-dee-ay-shun]

Back

Radiation


The transfer of thermal energy by electromagnetic waves, which can travel through the vacuum of space.

Example: Sun's radiation transfers thermal energy to Earth through space.
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2.

FLASHCARD QUESTION

Front

Electromagnetic Waves Noun

[uh-lek-troh-mag-net-ik wayvs]

Back

Electromagnetic Waves


Waves capable of transmitting energy through a vacuum, such as the solar energy that travels from the Sun to Earth.

Example: Solar energy from the Sun travels through space to Earth as electromagnetic waves.
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3.

FLASHCARD QUESTION

Front

Thermal Energy Noun

[thur-muhl en-er-jee]

Back

Thermal Energy


Energy related to the temperature of a substance, which is the total kinetic energy of its atoms or molecules.

Example: Molecules move faster in a warmer liquid, showing increased thermal energy.
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4.

FLASHCARD QUESTION

Front

Vacuum Noun

[vak-yoom]

Back

Vacuum


A space that is completely empty of matter, through which radiation can travel without a medium to carry it.

Example: A balloon in a vacuum chamber shows how the absence of air affects pressure.
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5.

FLASHCARD QUESTION

Front

Latitude Noun

[lat-i-tood]

Back

Latitude


The distance of a location on Earth, measured in degrees north or south of the equator, affecting sunlight angle.

Example: Sunlight hits Earth at different angles due to latitude, affecting solar energy received.
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6.

FLASHCARD QUESTION

Front

Equator Noun

[i-kway-ter]

Back

Equator


The imaginary line at 0 degrees latitude that circles the middle of Earth, receiving the most direct solar energy.

Example: The equator is shown as the line receiving the most direct sunlight, demonstrating its role in solar energy distribution.
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7.

FLASHCARD QUESTION

Front

Specific Heat Noun

[spuh-sif-ik heet]

Back

Specific Heat


The amount of heat energy needed to raise the temperature of one kilogram of a material by one degree Celsius.

Example: Heat moves from the hot side to the cool side, showing energy transfer.
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