Space Science & Education

The Moon’s Secret Anatomy

Rabaka Sultana5 months ago5 months ago705 mins

Although the Moon appears calm and simple from Earth, its interior hides a complex and fascinating structure shaped by ancient cosmic events. Scientists have uncovered the Moon’s internal layers using seismic data from Apollo missions, lunar rock samples, gravity measurements and modern spacecraft observations. The Moon’s anatomy reveals clues about its violent origin, thermal history and ongoing evolution.

1. Lunar Crust — The Scarred Outer Shell

The Moon’s crust is its outermost layer, averaging 30–50 km thick but it varies greatly. The far side crust is significantly thicker than the near side explaining why the near side has vast dark plains called lunar maria while the far side is heavily cratered.

Composed mainly of anorthosite a light-colored rock rich in calcium and aluminum
Formed over 4 billion years ago as the Moon’s surface cooled
Heavily bombarded by asteroids preserving an ancient record of the early Solar System
Contains regolith a fine dust layer created by billions of years of impacts

Secret clue: The crust’s uneven thickness supports the theory that internal heat and early tidal forces shaped the Moon differently on each side.

2. Lunar Mantle — The Silent Interior Engine

Beneath the crust lies the mantle extending roughly 1,300 km deep. This layer once contained partially molten rock that fueled ancient volcanic eruptions.

Made of dense silicate minerals like olivine and pyroxene
Source of basaltic lava that flooded impact basins and formed maria
Evidence suggests parts of the mantle were molten billions of years ago
Today, it is mostly solid and geologically quiet

Hidden past: The mantle was once active, driving volcanism long after the Moon formed far longer than scientists once believed.

3. Lunar Core — Small but Surprising

At the Moon’s center lies a small metallic core surprisingly complex for such a small body.

Radius of about 350 km
Consists of iron, nickel, and sulfur
Divided into:
- Solid inner core
- Liquid outer core
- A partially molten boundary layer

Although the Moon lacks a global magnetic field today, ancient rocks show it once had one evidence that the core was once active possibly powered by early rotation and cooling.

4. Temperature & Heat Flow — A Cooling World

The Moon is slowly losing heat.

Interior temperatures reach 1,600–1,700°C near the core
Heat escapes extremely slowly due to lack of tectonic activity
No plate tectonics like Earth
Small, shallow moonquakes still occur mostly due to tidal forces from Earth

Ongoing change: The Moon is shrinking slightly as it cools, causing surface fractures called lobate scarps.

5. What the Moon’s Anatomy Reveals About Its Origin

The Moon’s internal structure strongly supports the Giant Impact Hypothesis:

A Mars-sized body (Theia) collided with early Earth
Debris formed the Moon
Explains:
- Small iron core
- Similar isotopic composition to Earth
- Early global magma ocean

The layered anatomy is a fossil record of this catastrophic birth.