
Science • 60 • 25 students • Created with AI following Aligned with New Zealand Curriculum
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This is lesson 3 of 17 in the unit "Journey to the Cosmos". Lesson Title: Gravity: The Force That Binds Us Lesson Description: Learn about gravity and its role in the universe. Students will conduct experiments to understand gravitational forces and how they affect celestial bodies.
Lesson 3 of 17 in Journey to the Cosmos. Students investigate gravity as an attractive force between objects with mass, then use evidence and models to explain how gravity affects falling objects, planets and moons. The lesson builds on prior learning about forces, motion and free-body diagrams.
0–5 min · Hook and retrieval. Teacher opens with the hook and retrieval slides, showing an image of an astronaut, Earth and the Moon, and asks: “If gravity pulls everything down, why does the Moon not crash into Earth?” Students discuss with a partner, then share one idea and one question. Briefly revisit balanced and unbalanced forces from the previous lesson.
5–15 min · Direct teaching. Teacher uses the gravity teaching slides to establish that gravity is an attractive force between objects with mass, that larger masses produce stronger gravitational attraction, and that gravitational force acts towards the centre of a body. Students annotate the gravity investigation worksheet with a definition, a labelled Earth–object force diagram and the terms mass, gravity and attraction. Clarify that weight is the force of gravity on an object, while mass is the amount of matter in it.
15–30 min · Falling-object investigation. In groups of four, students use a tennis ball and a sheet of paper to compare drops from the same height. They first predict which will reach the ground first, then repeat the test with the paper flat and tightly crumpled. Teacher stresses a fair test: same release height, no throwing, several trials, and one variable changed at a time. Students record observations and trial results on the results table and investigation questions. Groups consider whether air resistance, rather than different gravitational forces, explains the flat paper’s slower fall.
30–42 min · Modelling gravity and orbits. Teacher demonstrates with a ball-on-string model or a projected simulation, using the orbit modelling slides. Explain that gravity continually pulls an orbiting object towards the central body while its forward motion carries it onwards; together these motions produce a curved path. In pairs, students use the labelled force arrow cards to arrange and draw arrows showing gravity acting on a falling object, the Moon and an orbiting satellite. They add captions explaining the direction of each force.
42–53 min · Apply and explain. Teacher displays three scenarios through the application discussion slides: a dropped object near Earth, the Moon orbiting Earth and a planet orbiting the Sun. Students complete the explanation section of the scenario questions, using the structure: “The object is affected by gravity because… The evidence/model shows… Therefore…” Groups compare answers and identify where gravity is the central idea. Challenge students to explain why astronauts appear weightless while still being affected by Earth’s gravity.
53–60 min · Plenary and assessment. Teacher returns to the opening question using the plenary slides. Students independently complete the final reflection on the exit response: “Explain how gravity can make an object fall and also help keep the Moon in orbit.” Invite two students to share answers, then collect worksheets to identify misconceptions for the next lesson.
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