Thermo/Waves Exam

Seismic waves and light waves are similar because

• They are both transverse waves.
• Both need a medium to travel.
• They have no similarities, actually.
• They are both compressional waves.

A wave travels a speed of 4 m/s and has a frequency of 3.5 Hz. What is the wavelength?

• 1.14 m
• 0.88 m
• 14 m
• 7.5 m

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NGSS.HS-PS4-1

How much time passes between each wave cycle?

• 1 second
• 2 seconds
• 4 seconds
• 6 seconds

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NGSS.HS-PS4-1

Which of the following is true when comparing the two graphs below?

• Wave A has a greater amplitude.
• Wave B has a greater amplitude.
• Wave A has a greater frequency.
• Wave B has a greater frequency.

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NGSS.HS-PS4-1

The law of reflection says that

• all waves incident on a mirror are reflected.
• waves incident on a mirror are partially reflected.
• the angle a ray is reflected from a mirror is random.
• the angle of reflection from a mirror equals the angle of incidence.

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NGSS.MS-PS4-2

This type of heat transfer uses a ceiling fan to circulate warm air throughout a house.

• Conduction
• Contortion
• Convection
• Radiation

How many types of heat transfer are there?

• 1
• 2
• 3
• 4

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NGSS.HS-PS3-4

The sun is a great example of which of the following types of heat transfer?

• Conduction
• Contortion
• Convection
• Radiation

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NGSS.HS-PS3-4

NGSS.HS-PS4-3

After taking a hot shower, James steps out of the shower on to the tile floor. The tile floor felt cold to his feet. Which explanation below best describes James' experience?

• Heat from the tile floor is transferred to his feet.
• Cold from the tile floor is transferred to his feet.
• Heat from his feet is transferred to the tile floor.
• Cold from his feet is transferred to the tile floor.

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NGSS.HS-PS3-4

Which of the following best describes the application of the first law of thermodynamics in a star?

• The energy produced in the core of a star is lost to space and does not contribute to the star's luminosity.
• The energy produced through nuclear fusion in a star is converted into heat and radiated as light, maintaining energy conservation.
• The energy output from a star decreases as the star ages, with no increase in internal energy.
• A star undergoes no energy loss or gain as it evolves.

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NGSS.HS-PS3-4

NGSS.HS-PS3-1