Worksheet
Nudging a Moonlet: Gravity and the Asteroid Impact Test
Grade 8 gravity practice: compare moons around Earth, Mars, Pluto and an asteroid, analyze the DART impact's orbit change and simulator runs, and link to the galaxy.
Grade 8ScienceInteractive · Printable
Aligned toMS-ESS1-2
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, Matching, Sorting, Short answer
About this worksheet
What students practice
- Students use orbit data to explain how mass and distance affect the gravity that holds a moon in orbit.
- Students use impact and simulator data to explain how a change in speed changes an orbit.
- Students connect gravity in a tiny asteroid system to orbits around the Sun and the Milky Way.
How to use
Read the passage aloud and review how to read numbers like 6.0 × 10²⁴ kg. Students answer Part 1 in pairs and Part 2 on their own.
Curriculum
NGSS standard covered
Model the role of gravity in the motions within galaxies and the solar system.
Preview
OwlSheets.com
Nudging a Moonlet: Gravity and the Asteroid Impact Test
Use orbit data and simulator runs to explain how gravity holds a tiny moon in place.
Part 1: Four moons and one small push
Read the passage, Table 1 and Table 2, then answer questions 1–6.
The Planning Briefing
1Saoirse Nakamura-Ruiz spent a week of her summer in a space science program for eighth graders. On the last day, the group sat in on a planning briefing with Dr. Emeka Lindahl, a scientist who helps plan spacecraft visits to asteroids. His team is getting ready for data from a follow-up spacecraft that will study a pair of asteroids up close. Before the spacecraft arrives, the team plans which measurements to take first, so Dr. Lindahl walked the students through what is already known about the pair and asked them to explain it.
2The pair is called Didymos and Dimorphos. Didymos is a rocky asteroid about 780 m wide, and Dimorphos, about 150 m wide, circles it like a tiny moon. Together they travel around the Sun about once every 2.1 years. Dr. Lindahl compared Dimorphos with three other moons in Table 1. Dimorphos moves at about 0.17 m/s, which is much slower than a person walks.
3In 2022, a NASA spacecraft called DART, with a mass of about 580 kg, crashed into Dimorphos at about 6 km/s on purpose. The test asked a planetary defense question: could hitting a small asteroid change its path? Telescopes on Earth timed Dimorphos as it passed in front of and behind Didymos, before and after the crash (Table 2). The crash slowed Dimorphos down by only a few millimeters per second.
4Next, Dr. Lindahl showed runs from his team's orbit simulator. In each run, Dimorphos started 1,190 m from the center of Didymos, moving sideways at a different speed (Table 3). Everything else stayed the same, including the masses of both asteroids. The simulator then drew the path Dimorphos would follow for several days. In one extra run, the team switched gravity off to see what Dimorphos would do with no pull at all.
5At the end, he zoomed out on the screen. The Sun holds Didymos, Dimorphos, Earth and every other planet in their orbits. The Sun itself travels at about 230 km/s around the center of the Milky Way galaxy and takes about 230 million years to go around once. The galaxy holds hundreds of billions of stars and huge clouds of gas and dust.
| Main body | Its moon | Main body mass (kg) | Center to center | Time for one orbit | Moon's speed |
|---|---|---|---|---|---|
| Earth | Moon | 6.0 × 10²⁴ | 384,000 km | 27.3 days | 1.0 km/s |
| Mars | Phobos | 6.4 × 10²³ | 9,400 km | 7.7 h | 2.1 km/s |
| Pluto | Charon | 1.3 × 10²² | 19,600 km | 6.4 days | 0.2 km/s |
| Didymos | Dimorphos | 5.4 × 10¹¹ | 1.19 km | 11.9 h | 0.00017 km/s |
| Measurement | Before | After |
|---|---|---|
| Time for one orbit | 11 h 55 min | 11 h 23 min |
| Center to center | about 1,190 m | about 1,150 m |
- A. Phobos has more mass than our Moon, so it falls around Mars faster.
- B. Phobos is about 40 times closer to its planet, where the pull is far stronger.
- C. Mars is farther from the Sun, so the Sun pulls Phobos forward faster.
- D. Mars spins faster than Earth, and its spin drags Phobos along with it.
- A. Didymos has so little mass that its weak pull can hold only a slow-moving moon.
- B. Dimorphos moves slowly because it is farther from Didymos than Phobos is from Mars.
- C. Earth's gravity holds Dimorphos in place, so it does not need to move fast.
- D. Dimorphos is too small to feel any gravity, so it drifts next to Didymos.
After the crash, one orbit took minutes less. That is about % shorter than before.
- A. The crash sped Dimorphos up, so it now circles farther out from Didymos than before.
- B. The crash added DART's mass to Dimorphos, so Dimorphos fell out of orbit and is drifting away.
- C. The crash slowed Dimorphos, so Didymos's gravity pulled it into a slightly smaller, shorter orbit.
- D. The crash turned off Didymos's gravity for a moment, so Dimorphos moved in a straight line.
Part 2: The orbit simulator and the bigger picture
Use Table 3 and paragraphs 4 and 5 to answer questions 5–10.
| Run | Sideways speed (m/s) | What happened |
|---|---|---|
| 1 | 0.1 | Curved inward and hit Didymos |
| 2 | 0.17 | Circled at 1,190 m |
| 3 | 0.21 | Stretched oval, out to 3,800 m and back |
| 4 | 0.3 | Curved a little, then left for good |
| 5 | 0.17, gravity off | Moved in a straight line |
- A. Dimorphos needs both its sideways speed and Didymos's pull to keep circling.
- B. Turning off gravity makes Dimorphos speed up and spiral away from Didymos.
- C. Gravity pushes Dimorphos forward along its path, which keeps its speed at 0.17 m/s.
- D. Dimorphos's speed keeps it circling, and gravity shrinks the circle by a few meters.
- Run 1 (0.1 m/s)
- Run 3 (0.21 m/s)
- Run 4 (0.3 m/s)
- A. Gravity bent its path, but it was too fast to be pulled back.
- B. Gravity slowed it as it moved out, then pulled it back in.
- C. It was too slow to miss Didymos as gravity pulled it inward.
In Run 3, the farthest point of the oval was m farther from Didymos's center than the starting point.
- A. Hit the main asteroid so its gravity turns off for a short time.
- B. Hit the moon from the front to slow it down to about 0.1 m/s.
- C. Hit the moon from behind to speed it up by about 0.13 m/s.
- D. Hit the moon from the front to slow it by a tiny amount.
| Didymos's gravity | The Sun's gravity | Gravity of the Milky Way's mass |
|---|---|---|
Related worksheets
WorksheetGrade 8
Bending the Path: Gravity Checks for a Space Game
Earth & Space Science · MS-ESS1-2
Free10 questions
WorksheetGrade 8
Who Pulls Hardest? Gravity, Asteroids and a Museum Meteorite
Earth & Space Science · MS-ESS1-2
Premium11 questions
WorksheetGrade 8
Mission Briefing: How Fast Must an Orbiter Go?
Earth & Space Science · MS-ESS1-2
Premium11 questions
WorksheetGrade 8
Fast Near the Sun, Slow Far Away: A Comet's Orbit
Earth & Space Science · MS-ESS1-2
Premium10 questions
WorksheetGrade 8
The Satellites Watching the Storm
Earth & Space Science · MS-ESS1-2
Premium10 questions
WorksheetGrade 8
Gravity at the Eyepiece: Jupiter's Moons and Beyond
Earth & Space Science · MS-ESS1-2
Premium11 questions