
Science • 30 • 20 students • Created with AI following Aligned with New Zealand Curriculum
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Planet Earth & Beyond Term 3 Science Overview Lesson 1: Categorize celestial bodies based on their physical composition and orbital behavior. Lesson 2: Investigate how mass determines the strength of gravitational pull and its effects on celestial objects. Lesson 3: Contrast the characteristics of stars with planets regarding luminosity and radiation.
Lesson 4: Model the hierarchical structure and scale of components within the universe.
Lesson 5: Explain how Kepler’s laws of planetary motion supported the shift to a heliocentric model.
LO: distinguish between planets (rocky or gaseous), dwarf planets, moons (rocky or icy), asteroids, and comets, using specific criteria like material composition and whether they can clear their orbital paths.
Classifying Solar System Objects.pptx
What is a Planet? Key Teaching Points A planet is a large object that orbits a star. Planets are nearly spherical because gravity pulls them into shape. A planet has enough gravity to clear its orbital path of most rocks and debris. There are two main types of planets: Rocky (terrestrial) – Mercury, Venus, Earth, Mars. Gaseous (gas giants/ice giants) – Jupiter, Saturn, Uranus, Neptune. Teacher Prompts & Questions "What do all planets have in common?" "Which planets have solid, rocky surfaces?" "Which planets are mostly made of gas?" "Complete the sentence: A planet must orbit a _____ and have enough gravity to _____ its orbit."
What is a Dwarf Planet? Key Teaching Points A dwarf planet orbits the Sun and is nearly spherical. Unlike a planet, it has not cleared its orbital path. Dwarf planets share their orbit with many other rocks and icy objects. Examples include Pluto, Ceres, Eris, Haumea, and Makemake. Teacher Prompts & Questions "How is a dwarf planet similar to a planet?" "What is the main difference between a planet and a dwarf planet?" "Why isn't Pluto classified as a planet anymore?" "Complete the sentence: A dwarf planet has not _____ its orbit."
What is a Moon? Key Teaching Points A moon is a natural satellite that orbits a planet, not a star. Moons can be: Rocky (e.g., Earth's Moon) Icy (e.g., Europa, Enceladus) Moons do not produce their own light—they reflect sunlight. Many planets have moons, while Mercury and Venus do not. Teacher Prompts & Questions "What does a moon orbit?" "Can a moon orbit the Sun directly?" "Why do we call the Moon a natural satellite?" "Can you think of any planets with many moons?"
What are Asteroids? Key Teaching Points Asteroids are small, rocky objects that orbit the Sun. Most asteroids are found in the Asteroid Belt between Mars and Jupiter. They are too small for gravity to pull them into a spherical shape. Asteroids have not cleared their orbital paths. Teacher Prompts & Questions "What are asteroids mostly made of?" "Why aren't asteroids round like planets?" "Where are most asteroids found?" "How are asteroids different from planets?"
What are Comets? Key Teaching Points Comets are made of ice, frozen gases, dust, and rock. They orbit the Sun in long, oval-shaped paths. As a comet gets close to the Sun, the ice heats up and forms a glowing tail. The tail always points away from the Sun because of the solar wind. Teacher Prompts & Questions "What are comets made of?" "Why do comets have tails?" "Does a comet always have a tail?" "What happens to a comet as it moves away from the Sun?"
Comparing Space Objects Key Teaching Points Scientists classify objects in space by: What they are made of. What they orbit. Whether they produce light. Whether they have enough gravity to become spherical. Whether they have cleared their orbital path. Teacher Prompts & Questions "Which object is made mostly of gas?" "Which object orbits a planet?" "Which objects have cleared their orbit?" "How can you tell the difference between a planet and a dwarf planet?"
LO: explain the relationship between mass and gravity, demonstrating how this force pulls large bodies into spherical shapes, dictates orbits, and clears debris from planetary paths. Gravity and Mass Cosmic Shapes.pptx
What is Gravity? Key Teaching Points Gravity is a force that pulls objects towards one another. Every object with mass has gravity. The more mass an object has, the stronger its gravitational pull. Gravity acts across space and keeps objects together. Teacher Prompts & Questions "What happens when you drop a pencil? Why does it fall instead of floating away?" "Does a basketball have gravity? What about a mountain?" "Which would have stronger gravity—a basketball or the Earth? Why?" "Complete the sentence: The more mass an object has, the ______ its gravity."
Mass and Gravity Key Teaching Points Mass is the amount of matter in an object. Gravity depends on mass—the greater the mass, the stronger the gravitational pull. Mass stays the same wherever you go, but your weight changes because gravity changes. The Sun has much more mass than Earth, so it has much stronger gravity. Teacher Prompts & Questions "If you travelled to the Moon, would your mass change? Why or why not?" "Why do astronauts appear to weigh less on the Moon?" "Which has more mass—the Moon or Earth? How does this affect gravity?" "How are mass and gravity connected?"
Why Are Planets Round? Key Teaching Points Gravity pulls matter equally towards the centre of a planet. When an object becomes large enough, gravity overcomes sharp edges and pulls it into a spherical shape. Small asteroids often have irregular shapes because they do not have enough gravity. Planets, stars and many moons are spherical because of their strong gravity. Teacher Prompts & Questions "Why do you think planets are round instead of cube-shaped?" "Why aren't all asteroids perfectly round?" "What do Earth, Jupiter and the Sun all have in common?" "How does gravity affect the shape of large objects in space?"
Gravity and Orbits Key Teaching Points Gravity keeps planets orbiting the Sun. Gravity also keeps moons orbiting planets. Without gravity, planets would travel in straight lines through space. An orbit is the curved path an object follows because gravity continually pulls it inward. Teacher Prompts & Questions "Why doesn't Earth fly away from the Sun?" "Why doesn't the Moon fall into Earth?" "Can you think of something on Earth that moves in a circle because it's being pulled inward?" (e.g. swinging a ball on a string) "What would happen if gravity suddenly disappeared?"
Clearing a Planet's Orbit Key Teaching Points A planet's gravity attracts nearby rocks, dust and other space objects. Over millions of years, planets collect, push away or capture most debris near their orbit. This is called clearing the orbit. Pluto has not cleared its orbit, which is why it is classified as a dwarf planet. Teacher Prompts & Questions "What do you think 'clearing an orbit' means?" "Why is Earth called a planet but Pluto is called a dwarf planet?" "How does gravity help planets clear their paths?" "Complete the sentence: A planet's gravity helps it ______ its orbit."
Bringing It All Together Key Teaching Points Gravity is caused by mass. More mass creates stronger gravity. Gravity pulls large bodies into spheres. Gravity keeps planets and moons in orbit. Gravity helps planets clear debris from their orbital paths. Teacher Prompts & Questions "How are mass and gravity connected?" "Why are planets round?" "How does gravity keep Earth in orbit?" "What are the three main jobs of gravity in our Solar System?"
LO: identify stars (including our Sun) as large, luminous bodies that emit vast amounts of radiation, and differentiate them from the non-luminous planets that orbit them
Stars and Planets Distinguishing Luminous from Non-luminous.pptx
What is a Star? Key Teaching Points A star is a large, hot ball of gas made mostly of hydrogen and helium. Stars produce their own light and heat through nuclear fusion. Because they produce their own light, stars are luminous. The Sun is the closest star to Earth. Teacher Prompts & Questions "When you look at the sky during the day, what is the brightest object you can see?" "Is the Sun a planet or a star? How do you know?" "What does the word luminous mean?" "Complete the sentence: A star is a large, hot ball of _____ that produces its own _____ and _____."
Why Do Stars Shine? Key Teaching Points Stars release huge amounts of energy through a process called nuclear fusion. This energy is released as light and heat (radiation). The Sun provides the light and warmth needed for life on Earth. Without the Sun's energy, Earth would be dark and extremely cold. Teacher Prompts & Questions "Where does the Sun's light come from?" "What would happen if the Sun stopped producing energy?" "Why is the Sun important for life on Earth?" "Can you think of ways we use the Sun's energy every day?"
What is a Planet? Key Teaching Points Planets do not produce their own light. Planets are non-luminous because they only reflect light from a star. Planets orbit (travel around) a star due to gravity. Earth is a planet that orbits the Sun. Teacher Prompts & Questions "If planets don't make their own light, why can we sometimes see them in the night sky?" "What does non-luminous mean?" "Why can we see the Moon if it doesn't produce light?" "Complete the sentence: Planets _____ light, but stars _____ light."
Stars vs Planets Key Teaching Points Stars are much larger than planets. Stars are luminous; planets are non-luminous. Stars produce energy, while planets reflect energy from stars. Planets orbit stars because of gravity. Teacher Prompts & Questions "How are stars and planets different?" "Which object produces its own light?" "Which object travels around the other?" "Would Earth still be a planet if it produced its own light? Why or why not?"
Our Solar System Key Teaching Points The Sun is the only star in our Solar System. Eight planets orbit the Sun. Gravity keeps the planets moving in their orbits. Other stars are much farther away than the Sun. Teacher Prompts & Questions "How many stars are in our Solar System?" "Can you name the eight planets?" "Why don't the planets fly off into space?" "What is at the centre of our Solar System?"
Bringing It All Together Key Teaching Points Stars produce their own light and heat. The Sun is our nearest star. Planets do not produce light; they reflect light from stars. Planets orbit stars because of gravity. The Sun's radiation provides Earth with light and warmth. Teacher Prompts & Questions "What makes the Sun different from Earth?" "Why is the Sun called a luminous object?" "How do planets get the light that we see?" "Complete the sentence: Stars are _____, while planets are _____."
LO: describe the universe's vast scale by mapping how planetary systems fit into billions of stars, which form galaxies (alongside gas, dust, and dark matter), which ultimately make up trillions of galaxies in the universe.
Scale of the Universe A Hierarchy tour.pptx
What is a Planetary System? Key Teaching Points A planetary system consists of a star and all the objects that orbit it. These objects can include planets, dwarf planets, moons, asteroids, and comets. Our Solar System is a planetary system with the Sun at its centre. Gravity keeps all objects moving in their orbits around the star. Teacher Prompts & Questions "What is at the centre of our Solar System?" "Besides planets, what other objects orbit the Sun?" "Why don't the planets drift away into space?" "Complete the sentence: A planetary system is made up of a _____ and everything that _____ it."
What is a Galaxy? Key Teaching Points A galaxy is a huge collection of stars held together by gravity. Galaxies also contain gas, dust, planets, planetary systems, and dark matter. Most stars belong to galaxies. Our Solar System is part of the Milky Way Galaxy. Teacher Prompts & Questions "Is the Solar System the same thing as a galaxy?" "Approximately how many stars are in the Milky Way?" (Billions) "Besides stars, what else is found in galaxies?" "Complete the sentence: The Solar System is located inside the _____ Galaxy."
The Milky Way Galaxy Key Teaching Points The Milky Way is a spiral galaxy. It contains billions of stars. The Sun is just one ordinary star among billions. Our Solar System is located in one of the Milky Way's spiral arms. Teacher Prompts & Questions "If the Milky Way contains billions of stars, how special is our Sun?" "Can we see all the stars in the Milky Way from Earth?" "Where is our Solar System located within the Milky Way?" "Why do you think the Milky Way looks like a band of light in the night sky?"
What is the Universe? Key Teaching Points The Universe includes everything that exists: Galaxies Stars Planets Gas Dust Dark matter Space and time Scientists estimate there are trillions of galaxies in the observable universe. Each galaxy contains millions to billions of stars. Teacher Prompts & Questions "What is larger—a galaxy or the Universe?" "How many galaxies do scientists estimate exist?" "Can the Universe contain more than one galaxy?" "Complete the sentence: The Universe contains _____ of galaxies."
Understanding the Scale of the Universe Key Teaching Points The Universe is organised in levels: Moon Planet Planetary System (Solar System) Galaxy (Milky Way) Universe Each level becomes much larger than the one before it. Our Solar System is only a tiny part of the Milky Way, and the Milky Way is only one of trillions of galaxies. Teacher Prompts & Questions "Which is larger: the Solar System or the Milky Way?" "How many Solar Systems could fit inside a galaxy?" "What is the largest structure we have learned about today?" "Can you put these in order from smallest to largest?"
Bringing It All Together Key Teaching Points A planetary system contains a star and everything orbiting it. Billions of stars make up a galaxy. Galaxies also contain gas, dust, planets, and dark matter. Trillions of galaxies make up the observable universe. Gravity plays a key role in holding planetary systems and galaxies together. Teacher Prompts & Questions "How are planetary systems, galaxies and the Universe connected?" "Why is the Universe difficult to imagine?" "Where do humans fit within this scale?" "Complete the sequence: Planet → __________ → Galaxy → Universe."
LO: explain how Johannes Kepler used elliptical orbits to describe planetary movement, providing crucial evidence that supported the Sun-centred model of our solar system.
Elliptical Orbits and the Sun-Centered Solar System.pptx
Who Was Johannes Kepler? Key Teaching Points Johannes Kepler was a German astronomer and mathematician who lived over 400 years ago. He used careful observations of the planets to understand how they move. Kepler built on the work of earlier astronomers, especially Tycho Brahe, who collected detailed observations of the planets. His discoveries changed our understanding of the Solar System. Teacher Prompts & Questions "What do you think an astronomer studies?" "Why would scientists spend years observing the night sky?" "How do you think observations can help us understand space?" "Complete the sentence: Johannes Kepler was an __________ who studied how __________ move."
What is an Ellipse? Key Teaching Points An ellipse is an oval-shaped path. Before Kepler, many people believed planets travelled in perfect circles. Kepler discovered that planets move in elliptical orbits, not perfect circles. The Sun is not in the centre of the ellipse—it is slightly off-centre at one of the ellipse's foci. Teacher Prompts & Questions "How is an ellipse different from a circle?" "Do you think planets move in perfect circles? Why or why not?" "Where is the Sun located in an elliptical orbit?" "Why might an oval path better match what astronomers observed?"
Kepler's First Law Key Teaching Points Kepler's First Law of Planetary Motion states:
Planets move around the Sun in elliptical orbits.
This explained why planets are sometimes closer to the Sun and sometimes farther away. The shape of the orbit affects the planet's distance from the Sun throughout the year. Teacher Prompts & Questions "What shape is a planet's orbit?" "Does a planet stay the same distance from the Sun all year?" "How might being closer to the Sun affect a planet?" "Complete the sentence: Planets orbit the Sun in __________."
Supporting the Sun-Centred Model Key Teaching Points Before Kepler, many people believed Earth was the centre of the Solar System (geocentric model). Kepler's work supported the heliocentric model, where the Sun is at the centre of the Solar System. His mathematical calculations matched real observations of planetary movement. His work provided strong evidence that the planets orbit the Sun. Teacher Prompts & Questions "What does heliocentric mean?" "Why was Kepler's discovery important?" "How did Kepler's observations support the Sun-centred model?" "Which object is at the centre of our Solar System?"
Why Was Kepler's Discovery Important? Key Teaching Points Kepler's ideas helped explain the movement of planets much more accurately. His work became the foundation for later scientists, including Isaac Newton, who explained why planets stay in orbit using gravity. Kepler showed that science improves when ideas are tested using evidence and observations. Teacher Prompts & Questions "Why is evidence important in science?" "How did Kepler improve our understanding of space?" "Which scientist later explained why planets stay in orbit?" "What can we learn about science from Kepler's discoveries?"
Bringing It All Together Key Teaching Points Johannes Kepler discovered that planets travel in elliptical orbits. His discoveries supported the Sun-centred (heliocentric) model of the Solar System. Careful observations and mathematical evidence helped replace older ideas. Kepler's work laid the foundation for our modern understanding of planetary motion. Teacher Prompts & Questions "What shape are planetary orbits?" "How did Kepler change people's understanding of the Solar System?" "Why is the heliocentric model accepted today?" "Complete the sequence: Observation → Evidence → Discovery → Better Scientific Understanding"
Students consolidate the unit by using evidence cards and a visual model to classify Solar System objects, connect mass with gravity, distinguish stars from planets, order the scale of the Universe, and explain how Kepler’s observations supported a heliocentric model. The lesson is designed as a fast-paced team challenge so students revisit key ideas through discussion, movement and justification.
0–4 min · Hook: “Who am I?” Teacher opens the mystery-object hook and displays four clues: “I orbit a star”, “I make my own light”, “I am mostly hydrogen and helium”, and “I give Earth heat and light”. Students silently identify the object, then pair-share which clue is strongest evidence. Reveal “star” and briefly establish that the lesson is a retrieval challenge, not a new topic.
4–9 min · Rapid retrieval. Teacher uses the unit retrieval questions to ask one question from each part of the unit: What does a planet clear? What makes an object luminous? What keeps planets in orbit? Where does the Solar System fit? What shape did Kepler identify? Students answer on mini-whiteboards or fingers, then correct answers through brief whole-class discussion. Address the misconception that planets produce light: they reflect light from stars.
9–18 min · Team classification challenge. Teacher places six headings around the room—star, planet, dwarf planet, moon, asteroid and comet—and gives each group of four a mixed set of object and clue cards represented on the classification challenge instructions. Students move to the heading they think fits each clue, then agree on a justification using at least two criteria: what it is made of, what it orbits, whether it produces light, whether gravity makes it spherical, or whether it has cleared its orbital path. Groups must challenge one placement respectfully and explain their reasoning. Clarify that a moon orbits a planet or dwarf planet, while the whole planetary system orbits its star.
18–24 min · Gravity and scale model. Teacher shows the gravity and universe-scale diagrams and assigns students roles in a quick human model: one student is the Sun, one Earth, one Moon, and the remaining students form a “debris field”, then regroup as Solar System, Milky Way and Universe. Students explain: “More mass means stronger gravity”; “gravity pulls large bodies towards a spherical shape”; “gravity bends moving objects into orbits”; and “a planet’s gravity helps clear nearby debris”. They then arrange the hierarchy from smallest to largest: moon/planet → planetary system → galaxy → Universe. Emphasise that the model shows relationships, not accurate distances or sizes.
24–28 min · Kepler evidence talk. Teacher displays the Kepler ellipse comparison showing a circular path beside an ellipse with the Sun at one focus. Students use the sentence frame, “Kepler’s observations supported the heliocentric model because …” to explain that planets travel in elliptical orbits and that the observed movement matched a Sun-centred model more accurately than an Earth-centred model. Invite two students to connect Kepler’s work with gravity: observations described the motion, while later work explained why the motion occurs.
28–30 min · Exit synthesis. Teacher distributes the Planet Earth and Beyond synthesis grid and asks students to complete the three short prompts before leaving: classify one unfamiliar object and justify it; explain two effects of gravity; complete “Moon → planetary system → galaxy → Universe” and state how Kepler changed the model. Collect responses for next-step planning. If time is short, students complete the first two prompts and verbally answer the hierarchy question.
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