Back to the lesson plan builder
Lesson length30 min45 min60 min

Print the plan for yourself; the student sheet prints on its own page after it.

Science lesson plan · 10th grade (Year 11 in England) · 60 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 · 6 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 5 seconds, in km? → 1500000 kmPrompt: distance = speed × time
  2. What keeps the planets in orbit around the Sun? (gravity / wind / magnetism / friction) → gravityPrompt: The Sun has a huge mass.
  3. Light travels about 300 000 km every second. How far does it travel in 10 seconds, in km? → 3000000 kmPrompt: distance = speed × time

Hook · 6 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 · 12 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 · 12 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 "main sequence star"? (white dwarf / nebula (cloud of dust and gas) / protostar / red giant) → red giantPrompt: The Sun is in its main sequence stage now.
  2. What process releases energy in the core of a star? (chemical reactions with oxygen / nuclear fission of uranium / burning coal / nuclear fusion of hydrogen into helium) → nuclear fusion of hydrogen into heliumPrompt: Small nuclei join together to make bigger ones.

You do: independent practice · 17 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 · 7 min

  • Two questions on their own. Sort answers into got it / nearly / not yet to plan the next lesson.
  1. Why is a main sequence star stable for billions of years? (It stops fusion / It has no gravity / Gravity pulling in is balanced by pressure from fusion pushing out / It is cold inside) → Gravity pulling in is balanced by pressure from fusion pushing outPrompt: Two forces act in opposite directions.
  2. In the life cycle of a star much more massive than the Sun, what comes straight after "main sequence star"? (red supergiant / supernova / protostar / nebula) → red supergiantPrompt: Very massive stars end their lives far more violently than the Sun.

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

eurekami

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

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

    • A. a supernova
    • B. a black hole
    • C. a planet
    • D. a white dwarf
  3. Question 3

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

    • A. nebula
    • B. main sequence star
    • C. red supergiant
    • D. neutron star or black hole
  4. Question 4

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

    • A. nebula (cloud of dust and gas)
    • B. protostar
    • C. white dwarf
    • D. red giant
  5. Question 5

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

    • A. supernova
    • B. red supergiant
    • C. main sequence star
    • D. nebula
  6. Question 6

    Where were elements heavier than iron made?

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

    What process releases energy in the core of a star?

    • A. nuclear fusion of hydrogen into helium
    • B. burning coal
    • C. nuclear fission of uranium
    • D. chemical reactions with oxygen
  8. Question 8

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

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

Free from eurekami.com

for the adult only

Answer key: The life cycle of stars

  1. 1. D. red supergiant

  2. 2. D. a white dwarf

  3. 3. D. neutron star or black hole

  4. 4. D. red giant

  5. 5. C. main sequence star

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

  7. 7. A. nuclear fusion of hydrogen into helium

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

Lesson plan | Eurekami