Nebular Theory
Planetary Development
Impact and Surface Evo
Scale and Structure
ESSRT
100

What does the Nebular Theory describe?

The formation of the solar system from a spinning cloud of gas and dust about 4.6 billion years ago.

100

What is chemical fractionation?

The separation of materials within a planet based on density forms layers.

100

What is meant by the term 'bombardment'?

The period when planets were hit by leftover debris from solar system formation.

100

What is a scale factor?

The ratio between the real-life size of an object and its size in a model.

100

What page can you find solar system data on?

Page 2

200

During the first stage, what caused the early solar system to flatten into a disk?

Spinning

200

During the Hadean Eon, what process allowed scientists to date ancient rocks?

Radiometric dating using uranium-to-lead decay.

200

Why do the Moon and Mars have more visible craters than Earth?

Earth’s atmosphere, weathering, erosion, and tectonic activity erase craters.

200

In a model, what does 1 meter equal to 1.5 million kilometers represent?

A scale factor used to model distances between planets.

200

What is the density of the mantle? 

3.4-5.6 g/cm^3

300

What formed at the center of the spinning nebula?

The sun.

300

What mineral provides evidence of Earth's earliest history?

Zircon.

300

What term describes the depressions formed by impacts?

Impact craters

300

Which variable can be accurately represented in a model of the solar system: distances or diameters?

Usually one, not both—distance or size—because their scale differences are too large.

300

In what ERA did the Devonian Period occur? 

Paleozoic Era.

400

What evidence supports the Nebular Theory today? 

Observations of other star systems forming disks of gas and dust around young stars.

400

What do 'parent' and 'daughter' isotopes tell scientists about a rock?

The ratio reveals the rock's age.

400

Why do planets with more tectonic activity have fewer visible craters?

New crust replaces older, cratered surfaces.

400

What force caused planets to form spherical shapes during their formation?

Gravity pulling matter toward the center.

400

What is the parent isotope that has a half-life of 1.3 billion years?

Potassium-40 (K40)

500

Why do scientists use models to study the solar system's formation?

Because geological processes, such as erosion and plate tectonics, destroy direct evidence from early Earth.

Think Zircons

500

What do scientists notice about the absolute age of materials in our solar system?

Meteorites, lunar rocks, and Earth's oldest rocks all date to around 4.6 billion years ago.

500

What evidence shows that bombardment has decreased since the early solar system?

Younger surfaces, like Earth's, have fewer craters than older ones, like the Moon's.

500

Why is understanding planetary scale important in space science?

It helps visualize the immense distances and size differences in the solar system.

500

If 4.6 billion years have passed, how many half-lives of potassium-40 have occurred?

3 half-lives 

4.6/1.3\approx 3.5