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TEACHER MATERIALS 
ACTIVE ACCRETION 
Purpose 
This activity simulates accretion. The process of accretion is responsible for the formation of planets, so it is critical that students understand how this process 
works. Previous resources have introduced the idea, but this activity asks students to experience the process in a more hands-on way, through role play. 
Process 
BIG HISTORY PROJECT / LESSON 4.0 ACTIVITY 
Go to a large open space such as a football field or park. Pass out one copy 
of the dust particle sign to each student—they’ll each play the role of “dust 
particle.” You, playing the role of the Sun, should stand in the center of the 
area (your “Solar System”). Have each student (“dust particle”) take their dust 
particle sign and choose a spot around the “Sun.” 
When the Sun yells “Go!” all of the dust particles should start moving around it, 
walking in the same direction at a brisk walking pace. As they move, they have 
to follow a few rules: 
1. They must move towards closer objects. (The word object refers to a 
student or group of students.) 
2. They must move towards larger objects. 
3. They must always move around a center point (the Sun). 
4. When they’re close enough to someone else that their hands can reach 
each other, they must link hands (or arms) and then move as a unit, 
following the same rules as before. 
As the students link up with other students, their “object” size will grow. 
Periodically, you (again, you’re the Sun!) should yell, “Stop!” Once they’ve 
stopped, one student from each group should run to the Sun to swap out their 
sign for one that reflects their group’s new role, which is, of course, determined 
by their new group size: 
Number of Students in Group Object 
1 dust particle 
2 chondrule 
3–10 meteoroid 
11–14 asteroid 
15–17 planetesimal 
18+ planet 
Continue the process until there is at least one planet orbiting the Sun. You 
might want to repeat the game more than once to see if there are differences in 
the resulting Solar System each time.
STUDENT MATERIALS 
ACTIVE ACCRETION 
Purpose 
This activity simulates accretion. The process of accretion is responsible for the formation of planets, so it’s really important that you understand how this process 
works. You’ve already been introduced to the idea, but this activity illustrates the process in a hands-on way that gets you out of your chair. 
Process 
BIG HISTORY PROJECT / LESSON 4.0 ACTIVITY 
Your teacher will take you to a large open space such as a football field or park 
and give you a “dust particle” sign. Yes, that’s your role: dust particle. Your 
teacher—or a lucky substitute—will be the Sun and will stand at the center of 
the “Solar System.” Take your dust particle sign and move to a spot somewhere 
around the “Sun.” 
When the Sun yells “Go,” all of the “dust particles”—that’s you and your 
classmates—are going to move around the Sun. You should all move in the 
same direction at a brisk walking pace. As you move, you have to follow a few 
rules: 
1. You must move towards closer objects. (The word object refers to you or a 
group of you.) 
2. You must move towards larger objects. 
3. You must always move around a center point (the Sun). 
4. When you’re close enough to someone else that your hands can reach each 
other, you must link hands (or arms) and then move as a unit, following the 
same rules as before 
As you link up with other students and groups of students, your “object” size 
will grow. Periodically, the Sun will yell, “Stop!” Once you’ve stopped, one 
student from each group must run to the Sun to swap out your object sign for 
one that reflects your group’s new role, which is, of course, determined by your 
new group size: 
Number of Students in Group Object 
1 dust particle 
2 chondrule 
3–10 meteoroid 
11–14 asteroid 
15–17 planetesimal 
18+ planet 
Continue the process until there is at least one planet orbiting the Sun. Your 
teacher might have you repeat the simulation more than once to see if there are 
differences in the resulting Solar System each time.
DUST PARTICLE 
< 0.1 MICROMETERS 
about the size of a virus
CHONDRULE 
< 0.5 IN 
smaller than a marble
METEOROID 
< 1 METER 
the size of a large beach ball
ASTEROID 
10 - 1000 KILOMETERS 
the size of Mount Everest - the size of California
PLANETESIMAL 
> 1000 KILOMETERS 
about the size of Earth’s moon
PLANET 
> 4500 KILOMETERS 
at least the size of Mercury

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Lesson 4.0 Activity: Active Accretion

  • 1. TEACHER MATERIALS ACTIVE ACCRETION Purpose This activity simulates accretion. The process of accretion is responsible for the formation of planets, so it is critical that students understand how this process works. Previous resources have introduced the idea, but this activity asks students to experience the process in a more hands-on way, through role play. Process BIG HISTORY PROJECT / LESSON 4.0 ACTIVITY Go to a large open space such as a football field or park. Pass out one copy of the dust particle sign to each student—they’ll each play the role of “dust particle.” You, playing the role of the Sun, should stand in the center of the area (your “Solar System”). Have each student (“dust particle”) take their dust particle sign and choose a spot around the “Sun.” When the Sun yells “Go!” all of the dust particles should start moving around it, walking in the same direction at a brisk walking pace. As they move, they have to follow a few rules: 1. They must move towards closer objects. (The word object refers to a student or group of students.) 2. They must move towards larger objects. 3. They must always move around a center point (the Sun). 4. When they’re close enough to someone else that their hands can reach each other, they must link hands (or arms) and then move as a unit, following the same rules as before. As the students link up with other students, their “object” size will grow. Periodically, you (again, you’re the Sun!) should yell, “Stop!” Once they’ve stopped, one student from each group should run to the Sun to swap out their sign for one that reflects their group’s new role, which is, of course, determined by their new group size: Number of Students in Group Object 1 dust particle 2 chondrule 3–10 meteoroid 11–14 asteroid 15–17 planetesimal 18+ planet Continue the process until there is at least one planet orbiting the Sun. You might want to repeat the game more than once to see if there are differences in the resulting Solar System each time.
  • 2. STUDENT MATERIALS ACTIVE ACCRETION Purpose This activity simulates accretion. The process of accretion is responsible for the formation of planets, so it’s really important that you understand how this process works. You’ve already been introduced to the idea, but this activity illustrates the process in a hands-on way that gets you out of your chair. Process BIG HISTORY PROJECT / LESSON 4.0 ACTIVITY Your teacher will take you to a large open space such as a football field or park and give you a “dust particle” sign. Yes, that’s your role: dust particle. Your teacher—or a lucky substitute—will be the Sun and will stand at the center of the “Solar System.” Take your dust particle sign and move to a spot somewhere around the “Sun.” When the Sun yells “Go,” all of the “dust particles”—that’s you and your classmates—are going to move around the Sun. You should all move in the same direction at a brisk walking pace. As you move, you have to follow a few rules: 1. You must move towards closer objects. (The word object refers to you or a group of you.) 2. You must move towards larger objects. 3. You must always move around a center point (the Sun). 4. When you’re close enough to someone else that your hands can reach each other, you must link hands (or arms) and then move as a unit, following the same rules as before As you link up with other students and groups of students, your “object” size will grow. Periodically, the Sun will yell, “Stop!” Once you’ve stopped, one student from each group must run to the Sun to swap out your object sign for one that reflects your group’s new role, which is, of course, determined by your new group size: Number of Students in Group Object 1 dust particle 2 chondrule 3–10 meteoroid 11–14 asteroid 15–17 planetesimal 18+ planet Continue the process until there is at least one planet orbiting the Sun. Your teacher might have you repeat the simulation more than once to see if there are differences in the resulting Solar System each time.
  • 3. DUST PARTICLE < 0.1 MICROMETERS about the size of a virus
  • 4. CHONDRULE < 0.5 IN smaller than a marble
  • 5. METEOROID < 1 METER the size of a large beach ball
  • 6. ASTEROID 10 - 1000 KILOMETERS the size of Mount Everest - the size of California
  • 7. PLANETESIMAL > 1000 KILOMETERS about the size of Earth’s moon
  • 8. PLANET > 4500 KILOMETERS at least the size of Mercury