Seasons, day length and the light year
The Earth's tilt, not its distance from the Sun, is why summer days are long and warm while winter days are short and cold.
Part of your national curriculum
- Physics: space physics: Understand the seasons and the Earth's tilt, day length at different times of year, and the light year as a unit of astronomical distance
Lesson overview
What you'll learn in this lesson
Understand the seasons and the Earth's tilt, day length at different times of year, and the light year as a unit of astronomical distance
Key learning points
- • Earth's tilt and the seasons
- • Day length through the year
- • The light year
This lesson at a glance
- 26 minutes
- 14 parts to scroll through
- 3 quick checks
- Marked quiz at the end
- Gentle pace: short sittings with pauses
Words to know
Scroll down — the lesson carries on below
Watch & discover
Part 1 of 14
Watch first
Seasons, day length and the light year
An English teaching video on this topic from Lammas Science. Watch it, then scroll down for the lesson.
In a nutshell
Understand the seasons and the Earth's tilt, day length at different times of year, and the light year as a unit of astronomical distance
Learning cycle
Part 2 of 14
Learning cycle 1 of 2
Part 1 · Earth's tilt and the seasons
A short piece of teaching, then a check to make sure it has landed.
Explore the idea
Part 3 of 14
Learn
Earth's tilt and the seasons
Earth's axis is tilted at about 23.5° from vertical. As Earth orbits the Sun over a year, this tilt means different hemispheres lean towards or away from the Sun at different times, causing the seasons — not changes in distance from the Sun.
Explore the idea
Part 4 of 14
Learn
Day length through the year
When the Northern Hemisphere is tilted towards the Sun (summer), it receives more direct sunlight for longer, giving long days and short nights. In winter, tilted away from the Sun, days are short with more indirect, weaker sunlight.
Quick check
Part 5 of 14
Quick check
What mainly causes the seasons on Earth?
Reset break
Part 6 of 14
Pause
That's sitting 1 of 2 done
Stretch, get a drink, look out of the window. There is no timer and nothing is counting down — your place is saved, so you can come back in five minutes or tomorrow.
Quick check
Part 7 of 14
Quick check
What is a light year a measure of?
Learning cycle
Part 8 of 14
Learning cycle 2 of 2
Part 2 · The light year
A short piece of teaching, then a check to make sure it has landed.
Explore the idea
Part 9 of 14
Learn
The light year
A light year is the distance light travels in one year — about 9.46 trillion kilometres. It is used to measure vast astronomical distances because using kilometres would produce impossibly large numbers; the nearest star beyond the Sun is over 4 light years away.
Quick check
Part 10 of 14
Quick check
During Northern Hemisphere summer, why are days longer?
Challenge round
Part 11 of 14
Game · Sort it
Which of these are true?
Drag each card into the right column. Tap a card first if dragging is fiddly.
True
Not true
Challenge round
Part 12 of 14
Game · Fill the gaps
Finish the sentences
Choose the word that belongs in each gap.
As Earth orbits the Sun over a year, this tilt means different hemispheres lean towards or away from the Sun at different times, causing the ____ — not changes in distance from the Sun.
A light year is the ____ light travels in one year — about 9.46 trillion kilometres.
It is used to measure vast ____ distances because using kilometres would produce impossibly large numbers; the nearest star beyond the Sun is over 4 light years away.
Mastery quiz
Part 13 of 14
Marked quiz
End of lesson quiz: Seasons, day length and the light year
3 questions, marked with the reasoning shown. No timer.
1. What mainly causes the seasons on Earth?
2. What is a light year a measure of?
3. During Northern Hemisphere summer, why are days longer?
Lesson round-up
Part 14 of 14
Lesson round-up
Ready when you are
Quiz score
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Games
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Points this lesson
0
Best run
0 in a row
Luna: 0 out of 3 on the practice checks. Only if you feel up to it — one more?
Ask LunaDo the work
Your written work for this lesson
This is the part you'd do in your book at school. Pick the pieces below, write here or on paper, and photograph anything you draw or work out.
Why the school greenhouse failed
A science club grew tomato plants in the school greenhouse. In June the plants grew well: leaves were dark green and the fruit set quickly. In July the club went away for two weeks and left the greenhouse door shut. When they came back, the leaves were curled and pale and most of the fruit had dropped.
The club had a data logger inside. It showed the temperature reached 46 °C on several afternoons and the soil moisture fell close to zero. The club knew photosynthesis needs light, water and carbon dioxide, and that enzymes in a plant work best in a narrow range of temperature. Above that range the enzymes stop working properly.
The club repeated the summer with the door propped open and a water bottle drip on each pot. Temperature peaked at 31 °C and the plants survived.
Written for Good Learning Co.
Reading questions
- Name the variable the club changed the second time, and one variable they kept the same.
- Explain, using the words photosynthesis and enzymes, why the plants were damaged in July.
- Write a conclusion for the club's report, saying how far the evidence supports it.
Method and results
WritingWrite the aim, what you changed, what you measured and what you kept the same, then record your results in a table.
1 page + results table
Conclusion
WritingExplain what your results show and why, using the scientific words from the lesson. Say how you know you can trust them.
6–8 sentences
Labelled diagram
DiagramDraw the apparatus or the process in pencil, label it fully, and photograph it.
1 labelled diagram
Reading and notes
ReadingRead the lesson text again and write the key ideas in your own words.
Half a page of notes
Saved as you type.
Part 1 of 14 · Watch & discover
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Understand the seasons and the Earth's tilt, day length at different times of year, and the light year as a unit of astronomical distance
