theory

lunar formation giant impact

The Moon formed from debris after a Mars-sized body collided with Earth.
31 related articles

Description

The leading explanation for the Moon's origin is the giant-impact hypothesis: a Mars-sized body, sometimes called Theia, struck the young Earth about 4.5 billion years ago. The collision vaporized part of Earth's mantle and the impactor, forming a disk of debris around Earth that eventually coalesced into the Moon. This idea elegantly explains the Moon's large size relative to Earth, its lack of a substantial iron core, and the similar isotopic composition of lunar and terrestrial rocks — a geochemical puzzle that older capture or fission models struggled with.

History

The hypothesis was proposed in the mid-1970s by William Hartmann and Donald Davis, and independently by Alastair Cameron and William Ward, following the Apollo missions that revealed the Moon's geochemical similarity to Earth.

How it works

The impactor's iron core merged with Earth's core, while the lighter rocky material from both bodies was ejected into orbit. This debris formed a hot, partially molten ring around Earth. Over thousands of years, gravitational clumping assembled the debris into the Moon. Because the material came mostly from the mantles of both bodies, the Moon is depleted in iron and has a composition close to Earth's outer layers, matching observations.

In practice

It guides planetary formation models and helps interpret the early history of the Earth-Moon system, including the timing of Earth's core formation and the onset of plate tectonics.

Fun fact

The Moon is actually older than its oldest surface rocks — the lunar crust crystallized about 150 million years before the oldest samples brought back by Apollo astronauts.

Concept graph →

Related articles · 31

Exoplanets2026-08-151 minarXiv:2608.15068express
Laser Instead of Meteorite: How Melted Craters Are Born
On the surface of the Moon and asteroids, you can find pits smaller than a pinhead but with shiny, melted rims. Such marks are left by tiny meteorites, but the exact impact speed at which melting occurs remained unclear.
Fountain of Debris: Where the Dust Settled After the DART Impact
On September 26, 2022, the DART probe slammed into the natural satellite at a speed of 6,6 km/s. A fountain of debris burst into space. Rocks, dust, sand grains — everything erupted in a silent flash. Two years later, a numerical simulation of 20 million trajectories revealed the fate of each particle.
Exoplanets2026-07-112 minarXiv:2607.10403express
Lunar muons could illuminate subsurface voids
The Moon is an airless sphere of dense rocky grit called regolith. When fast particles from space slam into it, muons are born in the soil — unstable relatives of electrons, but two hundred times heavier. Most fly downward and fade away in the depths. But those that pop upward into the vacuum can travel tens of kilometers before decaying.
Cosmic Carving: Birth of a Bloated Neptune from a Jupiter
A ball, almost weightless for its size, circles its star every four days. Planet TOI-2195 A b is a real riddle: by mass it's slightly heavier than Neptune, yet bloated to Jovian volumes. If there were an ocean big enough, this exoplanet would float on its surface like a giant inflatable ball.
Exoplanets2026-06-181 minarXiv:2606.20398express
Why the Moon Is a Copy of Earth? The Fluidity Clue
Young Earth was a boiling sphere of liquid rock, while Theia, which crashed into it, had had time to cool and solidify. It’s like dropping a chunk of cold butter into a pot of soup: the soup splashes out, but the butter barely moves. Similarly, Earth’s interior spewed into space, forming a cloud of cosmic dust and debris.
Popular Physics2026-06-141 minarXiv:2606.17105express
Gravitational Visitors: How Passing Planets Rewrote Earth's History
On the periphery of the Solar System lurk thousands of objects comparable in size to an exoplanet — a body of planetary mass not bound to our star. Their orbits are chaotic, and from time to time the trajectory of such a wanderer crosses Earth's path.
Shattered Inkwell: Impact Downpour 800 Million Years Ago
Eight hundred million years ago, in the main asteroid belt, a giant inkwell shattered. The parent body, over a hundred kilometers in diameter, made of primitive carbonaceous chondrites, suddenly broke apart near the J3:1 resonance with Jupiter.
Exoplanets2026-05-151 minarXiv:2605.15595express
Martian Spores: How Life Could Have Flown to Earth
The idea of extraterrestrial origin of life has long excited minds. Fred Hoyle believed bacteria travel between stars. A new study tested a similar but closer route: from Mars to Earth. In ancient times, Mars had water, and asteroid impacts knocked rocks with microbes into space.
Exoplanets2026-05-131 minarXiv:2605.13960express
Moon Bell: How Gravitational Waves Unveil Lunar Secrets
Back in the 1960s, physicist Joseph Weber tried to catch gravitational waves using aluminum cylinders: they were supposed to tremble like tuning forks from the ripples of spacetime.
Exoplanets2026-05-061 minarXiv:2605.04840express
Mars's dense layer reveals the fate of rocky planets
If you don’t stir a layered cocktail, the heavy syrup sinks to the bottom. A young planet is much the same — a seething ocean of molten rock. As it cools, minerals crystallize: some, like iron, get heavy and sink, while others float. You’d think a dense layer would pile up at the core.
General Relativity2026-04-141 minarXiv:2604.12787express
Planet Nine Heats Up with Dark Matter
At the edge of the solar system, far beyond Neptune's orbit, something is knocking icy chunks off their paths. Their orbits are stretched and tilted in the same way, as if an invisible hand arranged them in a pattern.
Exoplanets2026-04-062 minarXiv:2604.05235express
Moons of Distant Planets: What's Keeping Us from Seeing Them
The light from a distant star is never steady. It shimmers like heat over hot asphalt. When astronomers pointed JWST at the star TOI 700, they saw this shimmer especially clearly: every 16 minutes, the brightness changed by a tiny fraction, just 46 parts per million.For comparison: if you placed a light bulb a kilometer away, this change would be…
Instrumentation2026-04-021 minarXiv:2604.01927express
Europa's Ice Under Electron Fire
Europa's surface is an icy armor continuously bombarded by charged particles from Jupiter's magnetosphere. Electrons slam into the ice's crystal lattice, lose energy, and kick off chemical reactions. Until now, there was no tool to show how deep such bombardment pierces the ice.
Exoplanets2026-03-221 minarXiv:2603.21360express
Where Earth's Iron Came From
When a baker kneads dough, the grains of flour can tell you which mill they came from. It's the same with Earth: the composition of iron in its depths preserves a memory of where the pieces that assembled the planet were born.
Exoplanets2026-03-182 minarXiv:2603.17961express
Why Earth Didn't Absorb the Gifts from Space
In its youth, Earth resembled a beehive: it grew by sticking together from countless rocky chunks. When the main construction was over, a late swarm of meteorites rained down on the young planet — the so-called late veneer. These impacts, scientists thought, brought platinum, gold, and other rare metals to Earth's upper layers.
Stellar2026-03-042 minarXiv:2603.03732express
Stellar Passports: How a Neural Network Reads Age and Mass from Light
The light of every star is its unique passport, but the entries are written in the language of spectra and colors. For old giants, such documents are almost indistinguishable: their spectra overlap, and deciphering the details by hand was practically impossible.
Exoplanets2026-02-091 minarXiv:2602.09281express
Saturn's Rings: Trace of a Cosmic Collision
Saturn's system 300 million years ago resembled a crowded dance floor. The most massive moon, Titan, began to migrate, and this movement threw its neighbors off balance. One moon crashed into Titan; the debris swirled into a vortex, gathering into Hyperion.
Geophysics2026-01-301 minarXiv:2601.22606express
Mars's Brain-Like Terrain Tells a Tale of Climate Shifts
In the northern part of Arabia Terra, there are fields that look like a giant brain: ridges and troughs wind like convolutions. On Earth, similar patterns form in cold regions when water in the soil freezes and thaws, causing stones to sort themselves into stripes. But the Martian ridges are taller — averaging 3.29 meters — while Earth's mechanisms produce less than half a meter.
General Relativity2026-01-231 minarXiv:2601.16567express
The Moon as a Gravitational Wave Detector
Gravitational waves are ripples in spacetime curvature that imperceptibly stretch and squeeze everything around. But the Moon, like a bell, catches these waves: as a gravitational wave passes through it, it makes our satellite vibrate.
Exoplanets2026-01-131 minarXiv:2601.08306express
Titan's Age: Icy Moon Turns Out Younger Than Thought
Titan, discovered by Christiaan Huygens in 1655, resembles a canvas that is constantly being repainted. Impacts from cosmic dust and asteroids leave crater marks on it. But an invisible artist, the moon's own forces, time and again covers everything with a fresh layer, erasing old strokes.
Exoplanets2026-01-131 minarXiv:2601.08923express
The Mystery of Asteroid Kamo'oalewa: Why It's Not from the Moon
Kamo'oalewa is Earth's partner in a peculiar gravitational dance: it orbits the Sun almost in unison with us, edging closer and then pulling away. Its color — the palette of reflected light — matches the lunar surface. Hence the initial thought: it's a chunk of the Moon from the Giordano Bruno crater.
Exoplanets2026-01-121 minarXiv:2601.07159express
The Climate Swings of Ancient Mars
For a long time, the climate of ancient Mars remained a mystery: the beds of dried-up rivers spoke of water, but models couldn't explain how it got there — after all, 4 billion years ago the Sun shone 30% dimmer. New research shows that the planet swayed, as if on a swing, between long glaciations and short wet epochs.
Exoplanets2026-01-052 minarXiv:2601.02548express
Oxygen Dead End in a Red Dwarf System
On the exoplanet TRAPPIST-1, oxygenic photosynthesis, the process by which light energy is converted into chemical energy with oxygen as a byproduct, is losing the race for survival. This M-dwarf star emits mostly in the infrared, not in the visible range like the Sun.
Exoplanets2025-12-311 minarXiv:2601.00057express
A Cosmic Wanderer Steps on the Scales for the First Time
In the darkness of interstellar space drift millions of rogue planets — worlds not bound to any star. They are almost impossible to see, but when such a wanderer passes in front of a distant star, its gravity bends the light and momentarily creates a cosmic magnifying glass.
Exoplanets2025-12-261 minarXiv:2512.22375express
The Moon Assembled from a Swarm of Earth's Fragments
When countless asteroids pummeled the young Earth, they tore chunks from its mantle. These fragments spiraled in a cosmic disk around the planet and, like a snowball in a blizzard, fused into the Moon.
Exoplanets2025-11-251 minarXiv:2511.19946express
The Moon Is Older Than Its Rocks: Why 4.35 Billion Years?
Lunar rocks brought a puzzle: their age is 4.35 billion years, but the Moon itself should have appeared 150 million years earlier. The missing time is hidden in tidal heating. When the Moon hung closer to Earth, Earth's gravity acted like tireless hands: it constantly kneaded and bent the satellite.
Exoplanets2025-11-061 minarXiv:2511.04067express
The Moon — a Giant Gravitational Bell
The Moon is not just a rocky sphere, but a giant bell. Passing through it, gravitational waves cause it to vibrate almost imperceptibly. This tremor was predicted by Einstein, and Weber was the first to try to hear it with Earth-based detectors.
Exoplanets2025-11-051 minarXiv:2511.03392express
Warm Moons of Rogue Planets
The planet's gravity rhythmically squeezes and kneads the moon like dough: from this constant 'kneading', the interior heats up, and oceans of water can persist under the icy crust for ages. In the Galaxy, there are plenty of rogue planets, thrown out by supernova explosions.
Exoplanets2025-11-021 minarXiv:2511.00952express
Lunar Heating: How Tides Prolonged Earth's Magma Ocean
After the Moon's birth, Earth resembled a sizzling lump of dough: a continuous liquid magma and a dense shroud of gases. The Moon acted like a giant spoon, constantly kneading this lump with its gravity. Friction generated heat, delaying cooling.
Exoplanets2025-10-111 minarXiv:2510.10344express
Can the Moon have its own moon?
The Moon can have its own tiny moon — like a nesting doll, but in space. The outer doll is a planet, the middle one is a moon, the inner one is a small moon-satellite, or submoon. Ньютон showed that all bodies attract each other, and gravity holds them together.
A Layered Lunar Magma Ocean Explains the Moon's Isotopic Crisis
The Moon harbors a secret that has puzzled planetary scientists for decades: its isotopic composition is almost indistinguishable from Earth's. According to the canonical giant impact model, the Moon should have inherited most of its material from the impactor Theia, a Mars-sized planet that slammed into the young Earth.