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Noon Shadows and Ring Eclipses: An Astronomy Club Year
Grade 8 Earth-Sun-Moon practice: analyze a year of noon shadow data, then use Moon distances and a scale model to explain total and annular eclipses.
Grade 8ScienceInteractive · Printable
Aligned toMS-ESS1-1
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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, Circle the answer, Short answer
About this worksheet
What students practice
- Students use noon shadow data and a tilted-axis model to explain the pattern of seasons.
- Students use Moon distance data and a scale model to explain why some solar eclipses are total and others annular.
How to use
If possible, measure a real noon shadow before class; read paragraph 1 and Table 1 together, then let students work through both parts.
Curriculum
NGSS standard covered
Model the Earth-Sun-Moon system to explain moon phases, eclipses and seasons.
Preview
OwlSheets.com
Noon Shadows and Ring Eclipses: An Astronomy Club Year
Use a year of shadow data and a scale model to explain seasons and two kinds of solar eclipse.
Part 1: A year of noon shadows
Read the passage and Table 1, then answer the questions.
The Shadow Post
1The astronomy club at Ridgeview Middle School, at 40° north latitude, spent a whole school year on one simple tool: a straight post exactly 1 m tall, set upright in flat ground beside the school's front walk. On about the 21st of each month, club members measured the post's shadow at local noon, when the Sun is highest, and used a sky app to record how high the Sun was in degrees above the horizon. Early in the morning, they also noted the direction where the Sun came up. Club president Ayaan Whitfield made Table 1 from their notes.
2The club's advisor, Mr. Leopold Ferrante, set up a model in the gym. A lamp in the center stood for the Sun. A student carried a globe in a big circle around it to stand for one year. The globe's axis was tilted 23.5° and pointed toward the same wall the whole time, the way Earth's axis keeps pointing toward the same place in space. The club stuck a short toothpick upright on the globe at 40° N and watched its tiny shadow at four spots around the lamp.
| Date | Noon Sun height | Noon shadow (cm) | Sunrise direction |
|---|---|---|---|
| September 22 | 50° | 84 | Due east |
| October 21 | 39° | 123 | South of east |
| December 21 | 27° | 196 | Farthest south of east |
| February 21 | 39° | 123 | South of east |
| March 20 | 50° | 84 | Due east |
| April 20 | 62° | 53 | North of east |
| June 21 | 73° | 31 | Farthest north of east |
The noon shadow on December 21 was cm longer than the noon shadow on June 21.
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