Daily Read / Everyday Physics
Everyday Physics · Integrate text and table evidence to explain a pattern
Why Do Shadows Change Length During the Day?
Combine an explanation of the Sun’s apparent daily path with an illustrative shadow-length table to explain why a fixed object can cast different shadows through one day.
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One object, many shadows
A straight stick can stay in one place while its shadow changes through the day. The stick does not need to change height; the direction of incoming sunlight changes.
NASA explains that the Sun’s apparent position in our sky changes through the day because Earth rotates. That apparent motion changes the angle at which sunlight reaches the ground.[1]
Low Sun, long shadow
When the Sun is low in the sky, light reaches the ground at a shallow angle. A vertical object then blocks light across a longer stretch of ground.
NASA visualizations show that a low Sun angle can produce very long shadows. The geometry matters: a shallower light path stretches the shadow farther from the object.[2]
Higher Sun, shorter shadow
As the Sun appears higher, the light arrives more steeply. The same object still blocks the light, but the shadow does not extend as far across the ground.
The exact time of the shortest shadow depends on location and date, so a careful explanation focuses on the pattern instead of inventing one universal clock time.[1]
Read the table as evidence
The table below is an original illustrative classroom dataset for a one-metre stick. It is not a record from a particular city or date. The stick height stays fixed while the listed time and shadow length change.
The illustrative shadow is 2.4 m at 9:00, 1.3 m at 11:00, 1.0 m at 13:00 and 1.6 m at 15:00. Those values show a down-then-up pattern.[1]
Numbers show the pattern; prose explains it
The table can show that the shadow changes, but it does not by itself explain why. The prose supplies the mechanism: Earth’s rotation changes the Sun’s apparent position and therefore the light angle.
A strong reader combines both forms of evidence instead of repeating only the numbers or only the explanation.[1]
A fair comparison keeps important things the same
The same object, location and measuring method should be used across rows. If the stick height changed, the rows would no longer isolate the effect of time and Sun position.
That is the reading skill: identify the claim, find numerical evidence that fits it, and check whether the comparison is fair.[1]
Fast lesson
Use these checks before you answer the practice questions.
Identify what each column means before describing a pattern.
The table assumes the same one-metre stick across all rows.
Cite at least two values when describing the pattern.
Common mistakes
Why this fails: Real shadow lengths depend on date, location, object height and surface geometry.
Why this fails: The table shows a pattern; the prose explains the mechanism.
Why this fails: The illustrative value rises from 1.0 m at 13:00 to 1.6 m at 15:00.
Word Lab
Use the meaning, hear the word, then try it in your own sentence.
shadow
nounA darker area where an object blocks light.
The tree cast a long shadow.
apparent
adjectiveSeeming to be a certain way from an observer’s point of view.
The Sun’s apparent path changes across the sky.
angle
nounThe amount of turn between two directions or lines.
A low sunlight angle can make a long shadow.
vertical
adjectiveStraight up and down.
The class used a vertical stick.
pattern
nounAn organized way values change.
The table shows a down-then-up pattern.
controlled
adjectiveKept the same so a comparison is fairer.
The stick height was controlled across rows.
Check your understanding
Choose an answer, explain your choice, and then check. Hints and retries are welcome.
| Time | Shadow length |
|---|---|
| 9:00 | 2.4 m |
| 11:00 | 1.3 m |
| 13:00 | 1.0 m |
| 15:00 | 1.6 m |
Try the questions here. Public practice does not save a learning record.
Foundation
Foundation practice
Read exact values and variables.
1. What is the illustrative shadow length at 9:00?
- 2.4 m
- 1.3 m
- 1.0 m
- 1.6 m
2. What is the illustrative shadow length at 15:00?
- 2.4 m
- 1.3 m
- 1.0 m
- 1.6 m
3. What stays the same in the table?
4. What short phrase describes all four rows?
Core
Core practice
Connect numerical evidence to the explanation.
5. How much shorter is the 13:00 shadow than the 9:00 shadow?
6. From 13:00 to 15:00, does the shadow shorten or lengthen?
7. How do the prose and table work together?
8. Does the table prove that 13:00 is always the shortest-shadow time everywhere?
Think
Think practice
Use calculations, limitations and causal reasoning to combine the table with the text.
9. Put the illustrative shadow lengths in order from shortest to longest.
10. How much longer is the 9:00 shadow than the 11:00 shadow?
11. Which two rows show the shadow beginning to lengthen again?
12. Why does a lower Sun angle make a longer shadow?
13. Are the four table values NASA measurements?
14. Name two conditions that should stay the same while comparing times.
15. Why is 'shadows are always shortest at exactly 13:00' too strong?
16. Complete the reasoning: Earth rotates → the Sun’s apparent position changes → ______.
17. Which sentence is strongest evidence language?
- The shadow changes a lot.
- The shadow is shorter sometimes.
- In the illustrative table, the shadow falls from 2.4 m at 9:00 to 1.0 m at 13:00 before rising to 1.6 m at 15:00.
- The Sun makes shadows.
Practice answer key
- 1. 2.4 m
Read the first row. - 2. 1.6 m
Read the last row. - 3. The one-metre stick and assumed setup.
Keeping the object fixed makes the comparison stronger. - 4. The shadow gets shorter, reaches the shortest listed value, then gets longer.
The values are 2.4, 1.3, 1.0 and 1.6 m. - 5. 1.4 m shorter.
2.4 − 1.0 = 1.4. - 6. It lengthens by 0.6 m.
The value rises from 1.0 m to 1.6 m. - 7. The prose explains changing sunlight angle; the table gives numerical examples of the shadow pattern.
Mechanism plus data makes a stronger explanation. - 8. No.
The data are illustrative, and real solar timing depends on place and date. - 9. 1.0 m, 1.3 m, 1.6 m, 2.4 m.
Ordering the values helps reveal the shape of the pattern. - 10. 1.1 m.
2.4 − 1.3 = 1.1. - 11. 13:00 at 1.0 m and 15:00 at 1.6 m.
The later value is larger, showing the turn upward. - 12. The light reaches the ground more shallowly, so the blocked region stretches farther.
The geometry in the text links shallow light angle with longer ground distance. - 13. No. They are original illustrative Study Commons data.
The lesson explicitly labels the dataset as illustrative. - 14. For example, object height and location.
Holding important conditions constant makes the rows more comparable. - 15. The exact timing depends on date and location, and the table is illustrative.
The data support the lesson pattern, not a universal clock rule. - 16. the sunlight angle changes, so the shadow length changes.
This connects cause, mechanism and observed result. - 17. In the illustrative table, the shadow falls from 2.4 m at 9:00 to 1.0 m at 13:00 before rising to 1.6 m at 15:00.
It cites several exact values and describes the full pattern.
Related skills
Put it in your own words
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Check your own explanation
This is self-review, not automatic marking.
Compare with a model response
Earth’s rotation makes the Sun appear to change position across the sky, so the sunlight angle changes. In the illustrative table, the shadow drops from 2.4 m at 9:00 to 1.0 m at 13:00, then rises to 1.6 m at 15:00. This fits the explanation that a higher Sun makes a shorter shadow. Exact times and lengths vary by place and date.
Sources and revision notes
Source check: 2026-10-01. Grade guidance is an editorial suggestion, not a standardised reading score.
What changed in this edition?
Initial release. Claims about the Sun’s apparent position, Earth’s rotation and low-Sun-angle shadows were checked against NASA Science on 2026-10-01. The four-row shadow table is an original illustrative dataset, not a real measurement series.