Worksheet
Behind the Ridge: A Valley Town's Winter Without Sun
Grade 8 Earth-Sun-Moon practice: explain why a valley town's square gets no winter sun, then use the model to predict full moons and a noon eclipse there.
Grade 8ScienceInteractive · Printable
Aligned toMS-ESS1-1
What’s included
- Single worksheet
- Auto-graded online
- 1 NGSS standard
- Printable answer key
- 10 questions
- Classroom-ready
Details
- Format
- Interactive · Printable
- Grade
- Grade 8
- Subject
- Science
- Question types
- Fill in the blank, Multiple choice, Circle the answer, Short answer
About this worksheet
What students practice
- Students use noon Sun data and a tilted-globe model to explain why a valley town is shaded in winter.
- Students use the Earth-Sun-Moon model to predict how high full moons ride and when an eclipse can be seen.
How to use
If possible, act out the lamp-and-globe model before Part 1; let students point to the globe position for each date before they answer.
Curriculum
NGSS standard covered
Model the Earth-Sun-Moon system to explain moon phases, eclipses and seasons.
Preview
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Behind the Ridge: A Valley Town's Winter Without Sun
Use Sun data and a lamp-and-globe model to explain shade, seasons and the Moon.
Part 1: Twelve weeks of shade
Read the passage and Table 1, then answer questions 1–5.
The Sun Return Festival
1Greyhaven Hollow is a small mountain town at 47° north latitude. It sits at the bottom of a deep valley that runs from east to west. Just south of town, a steep forested ridge rises high above the rooftops. Seen from the town square, the top of the ridge is 26° above the horizon due south. Each winter, for about twelve weeks, the noon Sun stays behind the ridge and no direct sunlight reaches the square, although the sky above is still bright. In summer, by contrast, sunlight floods the square from late morning until late afternoon. The town marks the first day the Sun peeks over the ridge again with a Sun Return festival.
2Eighth grader Zsófia Szántó-Obi and her science class wrote a page for the festival's website. They used a sky app to record the height of the noon Sun and the length of the day on flat ground at 47° N (Table 1). They also looked up Earth's distance from the Sun: about 147 million km in early January and about 152 million km in early July.
3To explain the data, the class built a model. A lamp in the middle of a dark room stood for the Sun. A globe with its axis tilted 23.5° was carried in a big circle around the lamp, and its axis always pointed toward the same corner of the room. A sticker marked Greyhaven Hollow. At one spot on the circle, the north end of the axis leaned toward the lamp, and the light struck the sticker from high above. Half a circle later, the north end leaned away from the lamp, and the light struck the sticker at a low slant.
4Next, the class added a small white ball for the Moon and carried it around the globe once for each trip of a month. Like the globe, the ball was always half lit by the lamp. Their teacher, Mr. Osvaldo Okoro-Haldane, added one more fact: the Moon's orbit is tipped only about 5° from the path of Earth around the Sun, so the Moon moves across the sky along nearly the same paths that the Sun takes at different times of year.
| Date | Noon Sun height | Day length (h) |
|---|---|---|
| September 22 | 43° | 12.1 |
| October 21 | 32° | 10.4 |
| November 21 | 23° | 9 |
| December 21 | 19.5° | 8.4 |
| January 21 | 23° | 9.1 |
| February 21 | 32.5° | 10.6 |
| March 20 | 43° | 12.1 |
| June 21 | 66.5° | 16 |
October 21November 21December 21January 21February 21March 20
On December 21, the noon Sun is ° below the top of the ridge. On flat ground, the June 21 day is about times as long as the December 21 day (round to the nearest tenth).
- A. North end leaning toward the lamp, because the ridge then blocks the light
- B. Axis standing straight up, because the tilt goes away for part of each winter
- C. North end leaning away from the lamp, because light then reaches the town at a low slant
- D. North end leaning toward the lamp, because the town is then closest to the Sun
- A. The noon Sun is 43° high on both September 22 and March 20.
- B. The ridge top is 26° above the horizon as seen from the square.
- C. Earth is about 147 million km from the Sun in January and 152 million km in July.
- D. The June 21 day lasts 16 h on flat ground at 47° N.
- A. From about February to April, while Earth moves closer to the Sun
- B. From about May to July, when the south end of the axis leans away
- C. From about November to January, the same weeks as Greyhaven Hollow
- D. From about August to October, when Earth is farthest from the Sun
Part 2: The Moon over the ridge
Use the model in paragraphs 3 and 4 and Table 1 to answer questions 6–10.
- A. Yes. It is opposite the Sun, so it rides high, near the June noon Sun's path.
- B. Yes. The Moon is closer to Earth in winter, so it looks higher in the sky.
- C. No. At midnight a full moon sits inside Earth's shadow, so it is hidden.
- D. No. Like the December noon Sun, it stays about 20° high, below the ridge.
- A. In June the Moon's orbit tips 23.5° away from Earth, so it stays near the horizon.
- B. June nights are short, so the full moon sets before it has time to climb high.
- C. The June full moon is farther from Earth, so it sinks lower in the sky than in winter.
- D. The June full moon is opposite the Sun, so it follows a low path like the December Sun's.
A solar eclipse can happen only at , when the Moon is between the Sun and Earth. A lunar eclipse can happen only at , when Earth is between the Sun and the Moon.
- A. No Sun at all; they must climb the ridge or leave the valley
- B. A reddish Moon, since Earth's shadow falls on the town
- C. A full moon covering part of the Sun high in the southern sky
- D. The Sun with a bite out of it, low over the top of the ridge
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