Formation & Structure
Planets & Small Bodies
Moon Features & Phases
Eclipses & Mechanics
100

Define "nebula."

A cloud of gas and dust in space.

100

What are the two classifications of planets in our solar system?

Terrestrial and Jovian planets

100

What is "regolith" on the Moon?

Loose surface dust and broken rock produced by impacts.

100

During which lunar phase can a solar eclipse occur?

New Moon

200

State the Nebular Hypothesis (briefly).

Solar systems form from collapsing rotating clouds of gas and dust (nebulae).

200

Put these in order from the center outward: Kuiper Belt, Jovian Planets, Sun, Asteroid Belt, Oort Cloud, Terrestrial Planets.

Sun → Terrestrial Planets → Asteroid Belt → Jovian Planets → Kuiper Belt → Oort Cloud.

200

What are "maria" and how did they form?

Dark basalt plains formed when large impacts exposed molten material that filled basins and solidified.

200

During which lunar phase can a eclipse occur?

Full moon

300

What random astronomical event commonly triggers a nebula to begin collapsing into a star system?

A nearby supernova or other shock wave that compresses the nebula.

300

Give two primary compositional differences between terrestrial and Jovian planets.

Terrestrial: rocky composition, metal cores, smaller, denser, closer to Sun. Jovian: gaseous/icy, larger, low density, farther out, thick atmospheres.

300

Where on the Moon would you find anorthosite and why is it important?

Anorthosite is abundant in the lunar highlands (light crustal rock), indicating an early differentiated crust rich in plagioclase.

300

Explain why the Moon can cover the Sun in a solar eclipse even though the Sun is vastly larger.

Because the Moon is much closer to Earth, its apparent angular size can match the Sun's, allowing it to cover the Sun from some locations.

400

Explain how conservation of angular momentum affects a collapsing nebula.

As radius decreases, rotation rate increases (angular momentum conservation), causing flattening of the cloud.

400

Explain why there were originally many more planetesimals than final planets.

Many planetesimals formed; through collisions and accretion some combined into protoplanets and then planets, while others were ejected or remained as small bodies.

400

How long is one complete cycle of Moon phases? Give the value in days

29.5 days

400

Why does the Moon appear red during a total lunar eclipse? Provide an atmospheric explanation.

Earth's atmosphere scatters shorter wavelengths; refracted sunlight through the atmosphere is reddened and illuminates the Moon with red light.

500

Describe what the accretion disk is and why most mass ends up near the center.

The accretion disk is the flattened rotating disk of gas and dust around the forming protostar; most mass concentrates near the center forming the star.

500

Describe the significance of the Asteroid Belt, Kuiper Belt, and Oort Cloud to understanding solar system formation

They are reservoirs of leftover formation material; studying them gives clues about early solar system composition and processes

500

Explain why, at any given phase, the Moon is always half lit even though we see varying amounts. Use geometry of Sun–Moon–Earth positions.

Half the Moon is lit by the Sun at all times; phase differences come from our changing viewpoint of how much of that lit half faces Earth.

500

Why are eclipses infrequent events?

The moon's orbit is not directly in line with the plane that the Earth orbits the Sun. Only when the two line up during Full moons or New moons will an eclipse occur.