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Gravity at the Eyepiece: Jupiter's Moons and Beyond
Grade 8 gravity and orbits practice: analyze data on Jupiter's moons and the planets, use a string model, and connect gravity to the Milky Way.
Grade 8ScienceInteractive · Printable
Aligned toMS-ESS1-2
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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, Matching, Circle the answer, Sorting, Short answer
About this worksheet
What students practice
- Students use orbit data to describe how distance from a central body relates to orbital speed and period.
- Students use a model to explain how gravity keeps moons, planets and stars in orbit.
How to use
Demonstrate the ball-on-a-string model outdoors or in a gym before Part 1, then let students analyze both tables on their own.
Curriculum
NGSS standard covered
Model the role of gravity in the motions within galaxies and the solar system.
Preview
OwlSheets.com
Gravity at the Eyepiece: Jupiter's Moons and Beyond
Use orbit data and a string model to explain how gravity controls motion in space.
Part 1: Jupiter's moons
Read the passage and the first table, then answer the questions.
A Week of Observatory Nights
1Every October, the county observatory opens its large telescope to the Ridgecrest Middle School astronomy club. This year the club pointed it at Jupiter. Through the eyepiece, the planet looked like a small striped disk with four bright dots lined up beside it. Those dots are Jupiter's four largest moons: Io, Europa, Ganymede and Callisto. Galileo first saw them through a small telescope in 1610. Jupiter is about 11 times as wide as Earth and has more mass than all the other planets put together.
2Club member Shayla Okafor sketched the moons each clear night for a week. In her notes, each moon switched from one side of Jupiter to the other over a few nights, and on one night Io was missing until it came out from behind the planet. Bertrand Nakamura, an observatory volunteer, gave the club the data in the first table.
3Back at school, the club used a model. Outdoors, in an open area, Shayla swung a soft foam ball on a string in a flat circle above her head. She kept her hand pulling steadily on the string, and the ball kept circling. When she swung the ball faster in the same size circle, she felt that she had to pull harder on the string. When she let the string slip through her fingers, the ball flew off across the grass.
4Mr. Nakamura told the club that gravity also shaped the solar system itself. About 4.6 billion years ago, a huge cloud of gas and dust began to pull together. Most of the mass collected in the center and became the Sun, and smaller clumps that kept orbiting it formed the planets. The Sun is one of billions of stars in the Milky Way galaxy, and it carries the whole solar system along an orbit around the galaxy's center. One trip around takes about 230 million years, and the Sun moves along that path at roughly 230 km/s. On a dark night away from city lights, the club could see the Milky Way as a pale band across the sky, because we look out along the galaxy's flat disk from inside it.
| Moon | Distance from Jupiter | Time for one orbit | Orbital speed |
|---|---|---|---|
| Io | 422,000 km | 1.8 days | 17.3 km/s |
| Europa | 671,000 km | 3.6 days | 13.7 km/s |
| Ganymede | 1,070,000 km | 7.2 days | 10.9 km/s |
| Callisto | 1,883,000 km | 16.7 days | 8.2 km/s |
- A. Moons farther from Jupiter move more slowly and take longer to orbit.
- B. Moons farther from Jupiter move faster but take longer to orbit.
- C. Moons farther from Jupiter move faster and finish an orbit sooner.
- D. Moons farther from Jupiter move at about the same speed as closer moons.
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