OwlSheets
Noon Shadows and Ring Eclipses: An Astronomy Club Year worksheet preview

WorksheetPremium

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

Buy this worksheet: $1.50

Or unlock every Premium worksheet with Premium

PrintUnlock to print
Answer keyUnlock to see answers
Assign to classUnlock to assign with a class code

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

MS-ESS1-1

Model the Earth-Sun-Moon system to explain moon phases, eclipses and seasons.

Preview

OwlSheets.com

Name Date

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.

Table 1: Noon Shadow of a 1 m Post (40° N)
DateNoon Sun heightNoon shadow (cm)Sunrise direction
September 2250°84Due east
October 2139°123South of east
December 2127°196Farthest south of east
February 2139°123South of east
March 2050°84Due east
April 2062°53North of east
June 2173°31Farthest north of east
1.
Use Table 1.

The noon shadow on December 21 was   cm longer than the noon shadow on June 21.

The preview shows the first questions. Unlock the worksheet to see all of it.

Related worksheets