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Science lesson plan · 10th grade (Year 11 in England) · 45 minutes

The life cycle of stars

Space

CCSS NGSS.HS-ESS1-1CCSS NGSS.HS-ESS1-3England: KS3 Physics: Space physicsEngland: KS4 Physics: Space physics (separate science)

Objective and success criteria

Students will: The life cycle of stars.

  • I can answer questions on today's skill on my own, without help.
  • I can explain each step and say why it works.
  • I can check my answer and spot a mistake.

Before and after

Needs first: The scale of the universe

Leads to: The expanding universe and the Big Bang

Materials: Torch and ball for a Sun-Earth-Moon model, Space images, Mini whiteboards, A diagram or short video clip of the idea, Printed student sheet (below).

Warm-up · 5 min

  • Quick retrieval from earlier learning (The scale of the universe). Students answer on mini whiteboards.
  • Show answers together and note who needs support in the main task.
  1. Light travels about 300 000 km every second. How far does it travel in 60 seconds, in km? → 18000000 kmPrompt: distance = speed × time
  2. What is a light-year? (a very bright year / the time it takes to orbit the Sun / the distance light travels in one year / the time light takes to reach the Moon) → the distance light travels in one yearPrompt: Despite its name, it measures distance.
  3. The Sun is about 150 000 000 km away. Light travels at about 300 000 km/s. How many seconds does sunlight take to reach Earth? → 500 sPrompt: time = distance ÷ speed

Hook · 5 min

  • Ask why we see the Moon change shape over a month.
  • Share the objective: The life cycle of stars. Read the success criteria together.

I do: model it · 10 min

  • Work through the example out loud, saying why you do each step, not just what you do.
  • Example: In the life cycle of a star much more massive than the Sun, what comes straight after "nebula"?
  • Step 1: nebula → protostar → main sequence star → red supergiant → supernova → neutron star or black hole
  • Step 2: So the answer is: protostar
  • Answer: protostar
  • Pause after each step and ask a student to say what comes next.

We do: guided practice · 10 min

  • Do these together. Students try each step on whiteboards before you reveal it.
  • Use the hints as prompts rather than giving the answer.
  1. In the life cycle of a star like the Sun, what comes straight after "red giant"? (protostar / main sequence star / nebula (cloud of dust and gas) / white dwarf) → white dwarfPrompt: The Sun is in its main sequence stage now.
  2. What process releases energy in the core of a star? (nuclear fusion of hydrogen into helium / burning coal / chemical reactions with oxygen / nuclear fission of uranium) → nuclear fusion of hydrogen into heliumPrompt: Small nuclei join together to make bigger ones.

You do: independent practice · 10 min

  • Students work on the student sheet. Circulate and check the first two answers of every student early.
  • Students who finish: write a question of their own for a partner, with the answer.

The 8 questions are on the student sheet below, with answers in the key.

Exit ticket · 5 min

  • Two questions on their own. Sort answers into got it / nearly / not yet to plan the next lesson.
  1. In the life cycle of a star like the Sun, what comes straight after "nebula (cloud of dust and gas)"? (main sequence star / red giant / white dwarf / protostar) → protostarPrompt: The Sun is in its main sequence stage now.
  2. Why is a main sequence star stable for billions of years? (Gravity pulling in is balanced by pressure from fusion pushing out / It has no gravity / It stops fusion / It is cold inside) → Gravity pulling in is balanced by pressure from fusion pushing outPrompt: Two forces act in opposite directions.

Watch out for

  • Everyday meanings of words getting in the way of the science meaning: define key words explicitly.
  • Remembering facts without the reason: ask "why?" and "what is the evidence?"

Support and stretch

Support

  • Review first: The scale of the universe.
  • Use concrete materials: torch and ball for a sun-earth-moon model.
  • Give the first step of each question, or a partly worked example to finish.
  • Pair with a confident partner for the guided practice.

Stretch

  • Move on to: The expanding universe and the Big Bang.
  • Explain a common mistake in writing and how to fix it.
  • Write a word problem that uses today's skill, then solve a partner's.

Homework and more practice

Free online practice with hints and printable worksheets for this skill: eurekami.com/science/grade-10.

Free lesson plan from eurekami.com/lesson-plan-builder

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The life cycle of stars

Name

Date

Score/ 8

  1. Question 1

    In the life cycle of a star much more massive than the Sun, what comes straight after "main sequence star"?

    • A. nebula
    • B. red supergiant
    • C. neutron star or black hole
    • D. protostar
  2. Question 2

    What process releases energy in the core of a star?

    • A. burning coal
    • B. nuclear fission of uranium
    • C. nuclear fusion of hydrogen into helium
    • D. chemical reactions with oxygen
  3. Question 3

    In the life cycle of a star like the Sun, what comes straight after "red giant"?

    • A. main sequence star
    • B. protostar
    • C. white dwarf
    • D. nebula (cloud of dust and gas)
  4. Question 4

    What will the Sun become at the end of its life?

    • A. a planet
    • B. a white dwarf
    • C. a supernova
    • D. a black hole
  5. Question 5

    In the life cycle of a star like the Sun, what comes straight after "main sequence star"?

    • A. protostar
    • B. nebula (cloud of dust and gas)
    • C. red giant
    • D. white dwarf
  6. Question 6

    Where were elements heavier than iron made?

    • A. in supernova explosions and neutron-star collisions
    • B. by plants
    • C. in the Earth's oceans
    • D. in ordinary fires
  7. Question 7

    In the life cycle of a star much more massive than the Sun, what comes straight after "supernova"?

    • A. neutron star or black hole
    • B. main sequence star
    • C. nebula
    • D. red supergiant
  8. Question 8

    Why is a main sequence star stable for billions of years?

    • A. It is cold inside
    • B. It has no gravity
    • C. It stops fusion
    • D. Gravity pulling in is balanced by pressure from fusion pushing out

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Answer key: The life cycle of stars

  1. 1. B. red supergiant

  2. 2. C. nuclear fusion of hydrogen into helium

  3. 3. C. white dwarf

  4. 4. B. a white dwarf

  5. 5. C. red giant

  6. 6. A. in supernova explosions and neutron-star collisions

  7. 7. A. neutron star or black hole

  8. 8. D. Gravity pulling in is balanced by pressure from fusion pushing out