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Solar activity: How it evolves with time

Solar activity: How it evolves with time

Feb 5, 2026 | Big Ideia 11, Big Ideia 2, Big Ideia 4, Big Ideia 5, Big Ideia 8, IAC, Resource, Sun

Understanding solar activity is relevant because the physical phenomena that cause it cannot be studied on Earth, and also because it allows us to predict space weather. Solar storms (coronal mass ejections) carry large amounts of charged particles that form auroras...
Solar activity: How it evolves with time

Finding a number to measure Solar activity (Wolf number)

Feb 5, 2026 | Big Ideia 1, Big Ideia 2, Big Ideia 4, Big Ideia 5, Big Ideia 8, IAC, Resource, Sun

The Sun may seem like a static object, resting in the center of the Solar System while the planets orbit around it. But this is not the case. Our star is constantly undergoing processes of change that release large amounts of energy. In fact, the stability of its...
Laws of Planetary Motion – Mass of the Sun

Laws of Planetary Motion – Mass of the Sun

Feb 5, 2026 | Big Ideia 1, Big Ideia 4, IAC, Resource, Solar System, Sun

This activity is part of teaching unit 5, Laws of Planetary Motion. You can find the introduction and teaching guide here. Laws of Planetary Motion – Mass of the Sun This activity is part of teaching unit 5, Laws of Planetary Motion. You can find the introduction and...
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Astro-Journeys is an Erasmus+ funded project under Action Type: KA220-SCH – Cooperation partnerships in school education. Grant Agreement nº: 2024-1-FR01-KA220-SCH-000251302.
Period: September 2024 – August 2027

Co-funded by the European Union

Funded by the European Union. However, the views and opinions expressed are those of the authors only and do not necessarily reflect those of the European Union or the European Education and Culture Executive Agency (EACEA). Neither the European Union nor EACEA can be held responsible for them.

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