
THE MOON
LESSON 5: STRUCTURE | ORBITS | PHASES
INSIDE THE MOON
FOR YOUR NOTEBOOK:
Lesson 4: The Moon's Structure | Facts | Figures
Surface
Albedo- the percentage of incoming sunlight that its surface reflects (only about 7% compared to 31% on Earth)
Maria/Mare- dark, relatively smooth plains (about 3 km lower in elevation)
Rilles- valley-like structures that may be collapsed lava tubes
Impact craters- formed when objects from space crashed into the lunar surface
Ejecta- the material blasted out during these impacts that fell back to the Moon’s surface
Composition
Made up mostly of silicates
The highlands are predominantly lunar breccias (rocks formed by the fusion of smaller pieces of angular rock during impacts)
The maria are mainly basalt (does not contain water)
Crust- varies in thickness, is thickest on the far side of the moon (away from Earth)
Upper mantle- solid
Lower mantle- partially molten
Core- solid iron
Formation
Giant impact theory: the Moon formed as a result of a collision between Earth and a Mars-sized object about 4.5 billion years ago. Materials from the incoming body and Earth’s outer layers were ejected into space where they began to orbit (trapped by Earth’s gravity). Over time the materials merged to form the Moon.

FOR YOUR NOTEBOOK:
Lesson 4: Orbits and Phases
New Moon → Waxing Crescent → First Quarter → Waxing Gibbous → Full Moon → Waning Gibbous → Third Quarter → Waning Crescent → [restart cycle]
Earth’s gravity may have slowed the Moon’s spin to achieve synchronous rotation
Synchronous rotation- both the orbital and rotational periods of the Moon are equal
The Moon orbits counterclockwise around the Earth in a slightly elliptical (Oval) orbit
Apogee- most distant point from Earth during its orbit (Looks slightly smaller)
Perigee- closest point to Earth during its orbit (Looks slightly bigger)



