5.9Chapter 5: The Earth in Space
Using planetary data — Alhussan Physics - Stage 7 Revision Notes & Topical Questions
5 min read 9 parts Lesson 9 of 11 1 quiz
Lesson summary
Physics 5.9 Using planetary data — Day Length, Year Length and Axis Tilt — Alhussan International Academy — Physics (Stages 7–9) notes: Distinguish primary from secondary sources of data and use planetary data tables to answer questions.Data = observations or measurements recorde…
- Primary source
- Use in astronomy
- Importance
- Similar tilt
- Small tilt
- Large tilt
Part 1 of 7Primary and secondary sources
Data
Data observations or measurements recorded in an experiment
Recording
- Recording scientists record data in tables and display them using charts or graphs
Primary source
- Primary source experiments and fieldwork are primary sources, where you collect the data yourself
Secondary source
- Secondary source a book or the Internet contains data that other people have collected
Use in astronomy
- Use in astronomy questions about planets cannot be answered by experiments in a laboratory, so secondary data are used
Part 2 of 7Checking data
Importance
- Importance data must be checked whether they are primary or secondary
Methods of checking
- Repeat an experiment.
- Look at more than one secondary source to check that the data are the same.
Part 3 of 7Day length and year length
1Day
Day the time a planet takes to spin once on its axis, which is 24 hours on Earth
2Year
Year the time a planet takes to go once around the Sun, which is 365 days (1.00 year) on Earth
3Question
- Question the data can be used to find whether day length on other planets is related to year length
Part 4 of 7Spin time and orbit time of the planets
| Planet | Time to spin once on its axis (hours) | Time to go once around the Sun (years) |
|---|---|---|
| Mercury | 1416 (59 days) | 0.24 |
| Venus | 244 days | 0.69 |
| Earth | 24 | 1.00 |
| Mars | 25 | 1.88 |
| Jupiter | 10 | 11.86 |
| Saturn | 11 | 29.46 |
| Uranus | 17 | 84.01 |
| Neptune | 16 | 164.80 |
1Year length
- Year length it increases from Mercury to Neptune, so planets further from the Sun take longer to go once around it
2Day length
- Day length there is no simple relationship between the time to spin once and the time to go once around the Sun
Part 5 of 7Seasons and axis tilt
Cause
- Cause seasons on Earth are due to the tilt of the Earth's axis
Tilt data
- Tilt data the angle at which the axis of each planet is tilted can be found on websites and compared
No tilt
- No tilt a planet with no tilt, such as Mercury (0°), has no seasons
Similar tilt
- Similar tilt planets with a tilt close to the Earth's 23.5° have seasons similar to Earth's
Small tilt
- Small tilt a planet with a small tilt, such as Jupiter (3.1°), has seasons that are hardly noticeable
Large tilt
- Large tilt a planet with a very large tilt, such as Uranus (97.9°), has seasons very different from the Earth's
Part 6 of 7Axis tilt of the planets
| Planet | Angle of tilt (°) |
|---|---|
| Mercury | 0 |
| Venus | 177.4 |
| Earth | 23.5 |
| Mars | 24.0 |
| Jupiter | 3.1 |
| Saturn | 26.7 |
| Uranus | 97.9 |
| Neptune | 28.8 |
Retrograde spin
- Venus (177°) and Uranus (98°) have tilts shown with a second angle of −3° and −82° in the diagram
Not to scale
- Not to scale a diagram that is not to scale cannot show real sizes or distances
Part 7 of 7Presenting secondary data
Diagrams
- Diagrams data are not always presented in a table, so numbers taken from a diagram can be put into a table
Re-displaying
- Re-displaying secondary data may need to be shown in a different way, such as on a chart or a graph
Units
- Units table headings should include units such as hours, days and years
Key terms
| Term | Meaning |
|---|---|
| Data | Observations or measurements recorded in an experiment. |
| Primary source | Experiments and fieldwork, where you collect the data yourself. |
| Secondary source | A book or the Internet, containing data other people collected. |
| Day | Time for a planet to spin once on its axis. |
| Year | Time for a planet to go once around the Sun. |
| Axis tilt | Angle at which a planet's axis is tilted, which causes seasons. |
Avoid these mistakes
1
Thinking a year is the time to spin once — a day is one spin and a year is one orbit.
2
Assuming data in a book are always correct — check more than one source.
3
Thinking a diagram that is not to scale shows real sizes or distances — it does not.
4
Thinking only experiments give data — fieldwork is also a primary source, and books and websites are secondary sources.
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