Worksheet
Behind the Forecast App: Sun Angle, Seasons and the Moon
Grade 8 Earth-Sun-Moon practice: analyze a school weather station's sun and distance data, and use lamp models to explain moon phases and eclipses.
Grade 8ScienceInteractive · Printable
Aligned toMS-ESS1-1
What’s included
- Single worksheet
- Auto-graded online
- 1 NGSS standard
- Printable answer key
- 11 questions
- Classroom-ready
Details
- Format
- Interactive · Printable
- Grade
- Grade 8
- Subject
- Science
- Question types
- Fill in the blank, Multiple choice, Matching, Short answer
About this worksheet
What students practice
- Students use sun angle, day length and distance data to explain what causes seasons.
- Students use a lamp-and-ball model to explain moon phases and when eclipses can happen.
How to use
If you can, act out the lamp-and-ball model in a darkened room before students answer Part 2; Part 1 works well as partner data analysis.
Curriculum
NGSS standard covered
Model the Earth-Sun-Moon system to explain moon phases, eclipses and seasons.
Preview
OwlSheets.com
Behind the Forecast App: Sun Angle, Seasons and the Moon
Use weather station data and two classroom models to explain seasons, moon phases and eclipses.
Part 1: The Sun data
Read the passage and the table, then answer the questions.
What the App Knows
1The weather club at Lakeview Middle School keeps a small weather station on the school roof. Its sensors send temperature, wind and sunlight readings to a forecast app the club built with their teacher, Ms. Farah Lindqvist. Lakeview is at 40° north latitude. Besides the forecast, the app shows how high the Sun climbs at noon, the length of the day, Earth's distance from the Sun and the phase of the Moon. Each Friday the club checks the app's forecasts against the station's real readings and posts how often they were right.
2Eighth grader Anouk Brandt pulled four dates from a full year of station data. The table shows them. The station's sunlight sensor also measures how much solar energy reaches each square meter of the flat roof. On a clear day at noon, it reads about twice as much in June as in December. Earth's axis is tilted about 23.5°, and all year the axis points toward the same place in space, close to the North Star.
3To test why the angle of sunlight might matter, the club shined the same flashlight at a sheet of graph paper from the same distance. With the beam pointing straight down, the bright spot covered 20 squares. With the beam tipped low, like a winter Sun, the bright spot covered 40 squares and looked dimmer.
4For the moon phase feature, the club built a model in a dark classroom. A bare lamp stood for the Sun. A student's head stood for Earth, and a foam ball on a stick, held at arm's length, stood for the Moon. The student turned slowly in a circle and watched how much of the ball's lit side faced her. The Moon's path around Earth is tilted about 5° compared with Earth's path around the Sun, so the club sometimes held the ball a little above or below the lamp's height. Over one month, the app showed the dates in the second table. The club also added eclipse dates from a public space agency calendar, and they noticed that only a few full moons each year had a lunar eclipse listed.
| Date | Noon Sun height | Day length | Average high | Earth–Sun distance |
|---|---|---|---|---|
| March 20 | 50° | 12.1 h | 10 °C | 149 million km |
| June 21 | 73° | 15.0 h | 29 °C | 152 million km |
| September 22 | 50° | 12.1 h | 24 °C | 150 million km |
| December 21 | 27° | 9.3 h | 4 °C | 147 million km |
How many degrees higher is the noon Sun on June 21 than on December 21? °
How many fewer hours of daylight does Lakeview get on December 21 than on June 21? h
- A. Earth is nearest the Sun in December, so distance does not explain winter.
- B. Earth's distance from the Sun stays the same all year, so it is not a cause.
- C. Earth is closest to the Sun in June, which is why June is warmest here.
- D. Earth is farthest from the Sun in December, which supports the idea.
The low beam spread the same light over how many times as many squares as the straight-down beam? times
- A. Earth's axis flips direction in June, so the north half moves closer to the Sun.
- B. The north half of Earth tilts toward the Sun, so sunlight is more direct and days are longer.
- C. The Sun gives off more energy in June, so its light covers more squares on the ground.
- D. Low-angle sunlight in June is spread over a larger area, so it heats the ground more.
Part 2: The Moon model
Use paragraph 4 and the moon table.
| Date | Phase | Part of Moon lit |
|---|---|---|
| October 2 | New moon | 0% |
| October 9 | First quarter | 50% |
| October 17 | Full moon | 100% |
| October 24 | Third quarter | 50% |
- Ball between the student's head and the lamp
- Ball a quarter turn away from the lamp
- Ball on the far side of the head from the lamp, a little above the head's shadow
- Ball on the far side of the head from the lamp, inside the head's shadow
- A. Lunar eclipse
- B. Full moon
- C. New moon
- D. Half of the ball looks lit
- A. Earth's shadow covers a different part of the Moon each night.
- B. Clouds in space block part of the Moon on different days of the month.
- C. The Moon makes less of its own light as it moves away from Earth.
- D. We see different amounts of the Moon's sunlit half as it orbits Earth.
- A. October 31
- B. November 9
- C. October 27
- D. November 16
- A. October 2
- B. October 24
- C. October 17
- D. October 9
- A. The Sun is too far from Earth during most months to make a shadow.
- B. The Moon moves too fast at full moon for Earth's shadow to reach it.
- C. Earth's shadow points toward the Sun, away from the Moon, during most months.
- D. The Moon's tilted path usually takes it a little above or below Earth's shadow.
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