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Held by Gravity: Rubble-Pile Asteroids and a Racing Star

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Held by Gravity: Rubble-Pile Asteroids and a Racing Star

Use asteroid spin and escape-speed data to model what gravity holds together.

Part 1: Rubble piles and spin

Read the passage and Table 1, then answer questions 1 to 6.

Loose Rock, Here and in Space

1In the mountain town of Copper Notch, a week of heavy spring rain loosened a slope above the highway, and a landslide covered one lane with boulders, gravel and mud. A few days later, eighth grader Thandiwe Morrell went to a talk at the town library by Dr. Joaquín Ellery, a planetary scientist who grew up in the valley. He began with the landslide. Gravity pulls every rock on a slope downhill. Dry, loose rock can rest on a slope up to about 35° steep, but on a steeper slope gravity's pull wins and the rock slides.

2Then he turned to asteroids. Pictures from spacecraft show that many asteroids are rubble piles: boulders, gravel and dust resting together with gaps between them. One of these is Bennu, an asteroid about 490 m wide. When a spacecraft touched Bennu's surface to collect a sample, its arm sank into the loose rock like a hand pushed into a ball pit. Each body also has an escape speed, the speed a rock tossed straight up needs to fly off into space and not fall back. On Bennu, that speed is only about 0.2 m/s, slower than a slow walk.

3Asteroids spin, some slowly and some fast. As a pile spins faster, the rocks at its equator need a stronger inward pull to keep them moving in their circle. Telescope surveys have measured how fast thousands of asteroids spin, and Table 1 shows the fastest spin found in each size group. Pictures and radar show that some small asteroids are single solid boulders, and the strength of the rock holds each one together.

4Gravity pulls every piece of a body toward the body's center. Dr. Ellery compared Bennu with larger bodies in Table 2. Ceres, the largest object in the asteroid belt, is round, while Bennu is shaped like a lumpy spinning top. The same force reaches much farther. It holds the planets in their orbits around the Sun and holds the Sun and billions of other stars together in the Milky Way galaxy.

5Near the center of the Milky Way, astronomers have tracked a star called S2 as it circles an unseen object once every 16 years. At its closest, S2 is about 120 AU from that object (1 AU is Earth's distance from the Sun), and it moves at about 7,700 km/s. By comparison, Mercury, the fastest planet, moves at most about 59 km/s, when it is about 0.3 AU from the Sun.

Table 1: Fastest Spin Found in Each Size Group (simplified survey data)
Width of asteroidAsteroids measuredFastest spin found
Under 150 m1,0001 turn in 3 minutes
150 m to 1 km2,5001 turn in 2.2 hours
1 km to 5 km3,0001 turn in 2.2 hours
5 km to 20 km1,5001 turn in 2.3 hours
1.
Use paragraph 2. Which observation is the best evidence that Bennu is a loose pile of rubble, not one solid rock?
Question 1 options
2.
Use Table 1. One hour is 60 minutes.

The fastest turn in the 150 m to 1 km group takes times as long as the fastest turn in the under 150 m group.

3.
Which statement best describes the pattern in Table 1?
Question 3 options
4.
Use paragraph 3. Why do rubble-pile asteroids seldom spin faster than about one turn in 2.2 hours?
Question 4 options
5.
Use Table 1 and paragraph 3. Why can some asteroids under 150 m wide turn once in just a few minutes?
Question 5 options
6.
Over millions of years, sunlight can slowly speed up the spin of a small asteroid. Suppose a 1 km rubble pile speeds up until it turns once every 2 hours. What will most likely happen?
Question 6 options

Part 2: From asteroids to the galaxy

Use Table 2 and paragraphs 4 and 5 to answer questions 7 to 11. Then use the whole page for question 12.

Table 2: Four Bodies and Their Escape Speeds
BodyWidth (km)Escape speed (m/s)Shape
Bennu (asteroid)0.490.2Lumpy spinning top
Ceres (dwarf planet)940510Round
The Moon3,4752,380Round
Earth12,74211,200Round
7.
Use Table 2.

A rock must move times as fast to escape Ceres as to escape Bennu.

8.
Which statement best describes the pattern in Table 2?
Question 8 options
9.
Use Table 2 and paragraph 4. Which explanation best fits why Ceres is round but Bennu is lumpy?
Question 9 options
10.
Use Table 1 and the passage. Sort each object by what mainly holds it together.
11.
Use paragraph 5. At its closest, S2 is about 400 times as far from the object it circles as Mercury is from the Sun, yet it moves more than 100 times as fast. Which explanation fits best?
Question 11 options
12.
A town resident says, "Gravity matters for planets, but a small asteroid like Bennu is held together by its rocks sticking to each other. How fast it spins has nothing to do with gravity." Make a claim about this idea. Use evidence from both tables and the passage, and explain your reasoning.