SC.5.11.3.c: Represent data in graphical displays to reveal patterns of daily…
Represent data in graphical displays to reveal patterns of daily changes in the length and direction of shadows, length of day and night, and the seasonal appearance of some stars in the night sky.
The Nebraska College and Career Ready Standards for Science (2024) outcome SC.5.11.3.c (Earth and Space Sciences) for Grade 5 says: “Represent data in graphical displays to reveal patterns of daily changes in the length and direction of shadows, length of day and night, and the seasonal appearance of some stars in the night sky.” These 3 Fieldbook units teach it hands-on, with everyday materials and a printable teacher guide and student sheet for every lesson. Official wording: Nebraska College and Career Ready Standards for Science (2024).
Stars and the Night Sky Grades 3–6 · partly supports this outcome
Where the stars go in the daytime, why they wheel across the sky all night and why Orion is a winter sight in Canada but a summer one in Australia. Students sort real star data, spin and orbit as human models and read a printed sky chart. No materials needed: just the printed sheets, in either hemisphere.
- Why do the stars seem to move across the sky? 45–60 min
Students spin slowly under star posters to feel why the stars rise and set, match star-trail pictures to Canada, Singapore and Australia, and use the Big Dipper and the Southern Cross to find north and south. They explain why Polaris barely moves and why the south has no bright pole star.
- Why do we see different stars in different seasons? 45–60 min
Students walk a year around a paper Sun, facing out into the night at each season, to find out why Orion fills the evening sky in some months and vanishes in others. They join the dots of a printed sky chart, invent their own star pattern and plan a star count that measures light pollution.
Sun, Earth and Moon Grades 4–5 · partly supports this outcome
Why it's breakfast time in Calgary and bedtime in Singapore, why your shadow swings round the stick, why the Moon changes shape and why some places barely have seasons. Students build models with balls and lamps, track real shadows and read real sky data from cities around the world.
- Why do we have day and night? 45–60 min
Teams spin a ball in the beam of a flashlight and follow a sticker 'person' through sunrise, noon, sunset and midnight. They use the model to explain why it's breakfast time in Calgary while it's bedtime in Singapore.
- Does the Sun really move across the sky? 45–60 min, plus 5 minutes once an hour across the school day
Teams set up a shadow stick in the schoolyard and mark the tip of its shadow across the day, then graph its length and direction. They use the pattern to explain the Sun's path across the sky as the Earth turning, and predict shadows in the other hemisphere.
- Why are there seasons, and why do some places barely have them? 60 min, or two 35-minute periods
Teams shine a flashlight on squared paper at different angles, then carry a tilted ball around a lamp to see how the Sun's height and day length change through the year. They graph real day lengths for London, Singapore and Cape Town and explain seasons with tilt, not distance.
The Reason for the Seasons: Tilt, Daylight and the Solstice Grades 5–8 · partly supports this outcome
Is summer when Earth is closest to the Sun? Students test the idea with real 2026 orbit distances and city temperatures from both hemispheres, walk a human orbit, graph real solstice day lengths from the Arctic to Tierra del Fuego and work out why a high Sun heats more than a low one. Nothing to buy: just the printed sheets and the room.
- Why are summer days longer? 45–60 min
The class lines up across the room from the Arctic to Tierra del Fuego, each team holding a real city's day lengths for the 2026 equinox and solstices, and acts out how daylight changes. Students graph day length against latitude and explain the long and short days, the steady equator and polar day and night with a tilted Earth.
- Why is sunlight stronger in summer? 45–60 min
Teams count squares of sunlight under printed beams arriving at different angles, then visit noon-Sun stations and show real solstice Sun heights with their arms. They explain why a high Sun heats more than a low one, what the December solstice means north and south, and why the tropics have wet and dry seasons instead.
Printable practice for SC.5.11.3.c
- Stars and the Night Sky workbook included with the unit
2 English-support pages, 2 practice pages, 2 readings, 1 word wall, 1 unit review, 1 unit test, with answer keys.
- Sun, Earth and Moon workbook included with the unit
2 English-support pages, 2 practice pages, 2 readings, 1 word wall, 1 unit review, 1 unit test, with answer keys.
- The Reason for the Seasons: Tilt, Daylight and the Solstice workbook included with the unit
2 practice pages, 2 readings, 1 word wall, 1 English-support page, 1 unit review, 1 unit test, with answer keys.
Need just this outcome? Build a custom pack from these pages, with its answer key, in about a minute. Custom packs come with All-access and school licences.
Compared with NGSS: 5-ESS1-2.
More Nebraska Grade 5 science outcomes we teach
Every Nebraska Grade 5 science standards outcome we teach
Every unit matched to Nebraska's curriculum · All places and curricula
Three full lessons, free
Make a free account and download any three Fieldbook lessons as printable PDFs. No card needed.