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Astronomy Grade 6-8 Answer Key

Astronomy: The Sun: Energy, Sunspots, and Solar Flares

Explore how the Sun makes energy and how solar activity affects space weather

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Astronomy: The Sun: Energy, Sunspots, and Solar Flares

Explore how the Sun makes energy and how solar activity affects space weather

Astronomy - Grade 6-8

Instructions: Read each problem carefully. Use complete sentences when explaining your thinking. Show your work in the space provided.
  1. 1

    The Sun is a star made mostly of hydrogen and helium. Explain why the Sun is the main source of energy for life on Earth.

    Think about plants, temperature, and weather.

    The Sun is the main source of energy for life on Earth because its light and heat warm the planet, drive weather and the water cycle, and provide energy for photosynthesis in plants.
  2. 2

    In the Sun's core, hydrogen atoms combine to form helium. What is this process called, and why is it important?

    This process is called nuclear fusion. It is important because it releases a huge amount of energy that travels outward from the Sun and eventually reaches Earth as sunlight.
  3. 3

    Put these layers of the Sun in order from the center outward: corona, core, photosphere, radiative zone, convective zone, chromosphere.

    Start with the region where nuclear fusion happens.

    The correct order from the center outward is core, radiative zone, convective zone, photosphere, chromosphere, and corona.
  4. 4

    The Sun gives off energy in many forms, including visible light, ultraviolet light, and infrared radiation. Describe one way each of these forms of energy affects Earth.

    Think about seeing, heating, and sun safety.

    Visible light helps us see and provides energy for photosynthesis. Ultraviolet light can cause sunburn and can damage living cells. Infrared radiation transfers heat and helps warm Earth's surface.
  5. 5

    A sunspot looks dark when viewed on the Sun's surface. Does that mean it is cold? Explain your answer.

    A sunspot is not cold. It looks dark because it is cooler than the surrounding photosphere, but it is still extremely hot compared with temperatures on Earth.
  6. 6

    Sunspots are linked to strong magnetic fields. Explain how magnetic fields are related to sunspot formation.

    Sunspots are cooler areas caused by changes in the movement of hot plasma.

    Sunspots form where strong magnetic fields block some of the hot gas rising from inside the Sun. This makes those areas cooler and darker than the surrounding surface.
  7. 7

    Scientists often count sunspots to study solar activity. If the number of sunspots is increasing over several months, what can scientists infer about the Sun's activity level?

    Scientists can infer that the Sun's activity level is increasing. More sunspots usually mean stronger magnetic activity and a greater chance of solar flares or other solar events.
  8. 8

    The Sun has an approximately 11-year sunspot cycle. What happens during a solar maximum?

    Maximum means the activity is near its highest level.

    During a solar maximum, the Sun has many sunspots and higher magnetic activity. Solar flares and coronal mass ejections are more likely during this part of the cycle.
  9. 9

    Study the data: Year 1 had 18 sunspots, Year 2 had 35 sunspots, Year 3 had 62 sunspots, and Year 4 had 80 sunspots. Describe the trend and identify whether the Sun may be moving toward solar minimum or solar maximum.

    The number of sunspots is increasing each year. This trend suggests that the Sun may be moving toward solar maximum.
  10. 10

    A solar flare is a sudden burst of energy from the Sun's atmosphere. What causes solar flares?

    Focus on magnetic energy being stored and then released.

    Solar flares are caused when twisted magnetic fields near the Sun's surface suddenly release stored energy. This release sends out radiation across space.
  11. 11

    Name two possible effects of strong solar flares on technology near Earth.

    Strong solar flares can disrupt radio communication and interfere with satellites. They can also affect GPS signals and increase radiation risks for astronauts.
  12. 12

    Explain the difference between a solar flare and a coronal mass ejection.

    A solar flare is a burst of radiation from the Sun. A coronal mass ejection is a huge cloud of charged particles thrown out from the Sun's corona. They can happen together, but they are not the same event.
  13. 13

    Charged particles from the Sun can interact with Earth's magnetic field and atmosphere to create auroras. Explain why auroras are often seen near the North and South Poles.

    Earth's magnetic field acts like a guide for charged particles.

    Auroras are often seen near the poles because Earth's magnetic field guides charged particles toward those regions. When the particles collide with gases in the atmosphere, the gases glow.
  14. 14

    Why do scientists monitor the Sun using telescopes and spacecraft instead of only looking at it from Earth's surface?

    Scientists use telescopes and spacecraft because they can observe forms of energy that Earth's atmosphere blocks, such as some ultraviolet and X-ray radiation. Spacecraft can also provide continuous views and early warnings of solar activity.
  15. 15

    A news report says a strong solar flare is aimed toward Earth. Write a short explanation for the public that describes what a solar flare is and one reason scientists track it.

    Use simple language and include an effect on technology or safety.

    A solar flare is a sudden burst of energy from the Sun caused by strong magnetic activity. Scientists track solar flares because they can affect radio signals, satellites, GPS systems, power grids, and astronaut safety.
LivePhysics™.com Astronomy - Grade 6-8 - Answer Key