91¶¶Ňő

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91¶¶Ňő

Last updated

31 May 2026

docx, 1.37 MB
docx, 1.37 MB
pptx, 2.89 MB
pptx, 2.89 MB

Explain how gravity keeps objects in orbit using clear modelling that shows how forward motion and gravitational pull work together to create stable paths around planets.

  • Distinguish between natural and artificial satellites with simple comparisons that help pupils understand the difference between moons, space stations, and man‑made satellites.
  • Understand the physics of circular motion through accessible explanations of centripetal force and why orbiting objects constantly “fall around” the body they orbit.
  • Identify the many uses of satellites in our daily lives including communication, GPS, weather forecasting, imaging and scientific research.
  • Built with clean diagrams, engaging modelling, and student‑friendly explanations, this lesson makes orbital mechanics feel intuitive and exciting for Year 7 learners.

Why teachers love this resource

  • ¸é±đ˛ą»ĺ˛â‑t´Ç‑t±đ˛ął¦łó — fully sequenced and ideal for specialists and non‑specialists.
  • Misconception‑free explanations that tackle classic errors like “gravity stops working in space”.
  • High‑impact visuals that make orbits, centripetal force and satellite motion easy to demonstrate.
  • Worksheet included — perfect for assessment, homework or retrieval practice.
  • Real‑world relevance that boosts engagement by linking learning to phones, weather apps and navigation.

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