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Week 06 Β· A Disk of Dust and Gas

Monday

Where did all this come from?
// How a spinning cloud became a solar system
⏱ about 20 min

Monday: Where Did All This Come From?

Rocket lines up a lamp, a ball, an orange and a handful of pebbles on the Sky Deck step. "The Sun, Earth, the Moon, some asteroids."

Raven studies the row. "What do you notice? They all go around the lamp the same way. Why the same way?"

"Because that is how they started?" Rocket says, then stops. "Wait. How did they start?"

Nova hovers over the lamp. "Gravity pulls things together," she says. "Last week it held the system. Think about what it did first."

"Before there were planets," Raven says slowly, "there must have been just stuff. Dust. Gas."

Rocket sweeps the pebbles into a pile. "And gravity pulled the stuff into a pile." Nova glows. "A spinning pile. Find out what spinning does."

Rocket, Raven and Nova at the Sky Deck on a porch step. Rocket sweeps a handful of pebbles into a pile beside a lamp, a ball and an orange. Raven kneels with her Sky Log open. Nova the companion drone hovers above with her light on the pile.

A cloud that fell in on itself

Last week you learned that gravity holds the solar system together. This week you learn that gravity built it.

The Next Generation Science Standards say it this way. The solar system appears to have formed from a disk of dust and gas, drawn together by gravity.

NASA tells the story for students. It starts about 4.6 billion years ago with a cloud of dust that was part of a larger cloud called a nebula.

At some point the cloud collapsed. It fell in on itself, creating a disk of material around its center.

At the center, the pressure grew so great that hydrogen atoms began to fuse into helium, releasing a tremendous amount of energy. Our Sun was born.

Leftovers become planets

The Sun took in more than 99 percent of all the material in the disk. But there was still some left over.

Bits of this material clumped together because of gravity. Big objects joined bigger objects, forming still bigger objects.

Some grew big enough to become spheres. Those spheres became the planets and dwarf planets.

Rocky planets like Earth formed near the Sun, because icy and gaseous material could not survive close to all that heat.

Gas and ice collected farther away, creating the gas and ice giants.

A cloud of gas and dust
Gravity pulls it in on itself
It flattens into a spinning disk
The Sun forms at the hot center
Leftover bits clump into planets
HOW IT BEGAN
  • Read the question.
  • Tap your answer.
What did the solar system appear to form from?
About how long ago did the story begin?
Why did rocky planets form near the Sun?
StatementTrue or false?
The Sun took in more than 99 percent of the material in the disk.?
The planets formed before the cloud collapsed.?
Bits of leftover material clumped together because of gravity.?
Gas and ice giants formed close to the Sun.?
WHY THIS EXERCISEThe standard asks for a model of the solar system's formation with gravity doing the pulling.
Which force pulled the cloud in on itself and clumped the leftovers into planets? Type one word.
WHY THIS EXERCISEGravity both built the solar system and holds it together today.
Try it
Scatter ten small pebbles or buttons on a tray. Slowly slide them toward the middle with your hands. The pile is your Sun.
Leave three outside the pile. Those are your planets. Write what the pile and the three leftovers stand for.
For a grown-up
This week your student stirs a bowl of water with grains of sand to model a spinning disk. Please work over a sink or tray.
The facts this week come from NASA at science.nasa.gov and spaceplace.nasa.gov, from OpenStax Astronomy at openstax.org and from the NGSS at nextgenscience.org.
Try this
Hold a ball close to a lamp, then far away. Feel the warmth change on your hand, never touching the bulb.
Write why ice could gather far from the young Sun but not close to it.
Draw three pictures in a row. First a round cloud. Then a flat spinning disk with a bright center. Last, the Sun with planets around it.

Good start. Tomorrow you find out what spinning did to the cloud, and why that explains the planets' paths.