Astronomy Grade 6-8

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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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
    Sunlight reaching Earth and supporting plants and animals.

    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.

  2. 2
    Particles combining in the Sun’s core and releasing energy.

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

  3. 3
    Cross-section of the Sun showing its layers from core to corona.

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

  4. 4
    Different forms of solar energy reaching and affecting Earth.

    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.

  5. 5
    A dark sunspot on the Sun’s bright surface.

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

  6. 6
    Magnetic field lines looping between sunspots on the Sun.

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

  7. 7
    Sequence of Suns with increasing numbers of sunspots.

    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?

  8. 8
    A highly active Sun with many sunspots and flares.

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

  9. 9
    A visual trend showing sunspot counts increasing over time.

    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.

  10. 10
    Twisted magnetic field lines releasing energy as a solar flare.

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

  11. 11
    Solar activity affecting a satellite and communication signals near Earth.

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

  12. 12
    A solar flare shown as a bright flash and a coronal mass ejection shown as a plasma cloud.

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

  13. 13
    Charged particles following Earth’s magnetic field lines to create auroras near the poles.

    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.

  14. 14
    A ground telescope and a space telescope observing the Sun, with the spacecraft above the atmosphere.

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

  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.

LivePhysics™.com Astronomy - Grade 6-8

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