How do meteorites give evidence for the composition of the Earth's interior?
Meteorites are fragments of asteroids and other bodies that fall to Earth; the main types (stony, iron and stony-iron) are thought to sample the interiors of broken-up rocky bodies, so they give evidence for the composition of the Earth's deep interior; iron meteorites support an iron-rich core and stony meteorites a silicate mantle, because we cannot sample the deep Earth directly.
A focused answer to the Eduqas GCSE Geology statement on meteorites. Covers what meteorites are, the three main types (stony, iron, stony-iron), and how they provide evidence for the composition of the Earth's deep interior (an iron core and a silicate mantle) when we cannot sample it directly.
Reviewed by: AI editorial process; not yet individually human-reviewed
Have a quick question? Jump to the Q&A page
Jump to a section
What this dot point is asking
Eduqas wants you to explain what meteorites are, to name the three main types (stony, iron and stony-iron) and what each is made of, and to explain how they give evidence for the composition of the Earth's deep interior. The key argument is that we cannot sample the deep Earth directly, so meteorites, thought to be fragments of broken-up rocky bodies like the early Earth, act as samples of the kind of material the interior is made of: iron meteorites support an iron-rich core and stony meteorites a silicate mantle.
The answer
What meteorites are
A meteorite is a piece of rock or metal from space that survives its fall through the atmosphere and lands on the Earth's surface. Most meteorites are fragments of asteroids, and a few come from the Moon or Mars. Many asteroids are the broken-up remains of small rocky bodies that formed early in the Solar System, at the same time as the Earth and from the same kind of material.
The three main types
Meteorites are classified by what they are made of:
- Stony meteorites are made mainly of silicate minerals (rock). They are the most common type and resemble the rocks of the Earth's mantle.
- Iron meteorites are made mainly of iron and nickel metal. They are dense and metallic.
- Stony-iron meteorites are a mixture of silicate minerals and iron-nickel metal.
Why the types matter: sampling a broken planet
Early in the Solar System, bodies large enough to heat up differentiated: the dense metal sank to form a metallic core and the lighter silicates formed a rocky mantle around it, exactly as the Earth did. When such a body was later smashed apart by collisions, its fragments sampled different depths:
- fragments from the metallic centre became iron meteorites;
- fragments from the rocky outer part became stony meteorites;
- fragments from the boundary between the two became stony-iron meteorites.
So the three meteorite types are thought to be samples of the core, mantle and core-mantle boundary of broken-up planet-like bodies.
Evidence for the Earth's interior
This is the link Eduqas is after. We cannot drill to the deep Earth: even the deepest boreholes barely scratch the crust, and the core lies thousands of kilometres down. Meteorites give us actual samples of the kind of material that makes up a differentiated rocky body like the Earth:
- Iron meteorites show that broken bodies had iron-nickel metallic cores, supporting the idea that the Earth has an iron-rich (iron-nickel) core.
- Stony meteorites show silicate outer layers, supporting a silicate mantle around that core.
Combined with other evidence (the Earth's overall density and the behaviour of earthquake waves), meteorites help confirm the layered, iron-core, silicate-mantle structure of the Earth.
Examples in context
Example 1. Iron meteorites in museums. The large iron meteorites on display are slices of the metallic cores of asteroids. Their iron-nickel composition is direct evidence of the metal-rich centres that differentiated bodies, including the Earth, possess.
Example 2. Meteorites and the age of the Earth. Because meteorites formed at the same time as the rest of the Solar System, radiometric dating of them gives the age of the Earth (about 4.5 billion years), which we cannot get from Earth rocks alone because the oldest crust has been recycled.
Try this
Q1. Name the type of meteorite made mainly of iron and nickel. [1 mark]
- Cue. An iron meteorite.
Q2. Explain why meteorites are useful evidence for the Earth's deep interior. [2 marks]
- Cue. We cannot sample the deep Earth directly, and meteorites are fragments of differentiated bodies, so they provide samples of core-like (iron) and mantle-like (silicate) material.
Q3. State what an iron meteorite suggests about the composition of the Earth's core. [1 mark]
- Cue. That the core is iron-rich (made of iron and nickel metal).
Exam-style practice questions
Practice questions written in the style of WJEC Eduqas exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.
Eduqas 20205 marksExplain how the different types of meteorite provide evidence for the layered structure and composition of the Earth's interior.Show worked answer →
Link the meteorite types to the layers they are thought to sample, and explain why this matters.
- Meteorites sample broken-up rocky bodies
- Many meteorites are fragments of asteroids that, like the Earth, separated into a metal-rich centre and a rocky outer part before breaking apart. So the pieces sample different depths of a planet-like body.
- Iron meteorites and the core
- Iron meteorites are made largely of iron and nickel metal. They are thought to sample the metallic cores of broken bodies, supporting the idea that the Earth too has an iron-rich (iron-nickel) core.
- Stony meteorites and the mantle
- Stony meteorites are made of silicate minerals, like the Earth's mantle rocks. They support a silicate mantle surrounding the core.
- Why it matters
- We cannot drill to the deep Earth, so meteorites give us samples of the kind of material that makes up the interior. Markers reward matching iron meteorites to an iron core and stony meteorites to a silicate mantle, and the point that we cannot sample the deep Earth directly.
Eduqas 20183 marksState the three main types of meteorite and describe what each is mainly made of.Show worked answer →
Name the three types and give the composition of each. One mark each.
Stony meteorites are made mainly of silicate minerals (rock), similar to the rocks of the Earth's mantle. They are the most common type.
Iron meteorites are made mainly of iron and nickel metal.
Stony-iron meteorites are a mixture, containing both silicate minerals and iron-nickel metal, thought to come from the boundary between a body's rocky and metallic parts.
Markers reward the three named types each correctly paired with its composition (silicate rock; iron-nickel metal; a mixture of both).
Related dot points
- The Earth can be compared with its planetary neighbours (the other rocky planets and the Moon) in terms of their rocks and surface materials, surface landforms, atmosphere, surface temperature, pressure and gravity; differences in size, distance from the Sun and the presence of an atmosphere and liquid water explain why the Earth is geologically active and habitable while the Moon and Mars are not, and why some bodies preserve an ancient cratered surface.
A focused answer to the Eduqas GCSE Geology statement on comparing Earth with the rocky planets and the Moon. Covers the comparison of rocks and landforms, atmosphere, surface temperature, pressure and gravity, and why size, distance from the Sun and the presence of an atmosphere and water make the Earth uniquely active and habitable.
- Uniformitarianism (the principle that the present is the key to the past, so the same physical processes operate everywhere and at all times) lets geologists interpret the surfaces of other planetary bodies; by comparing landforms seen in space imagery (craters, volcanoes, channels, dunes) with landforms made by known processes on Earth, geologists infer the processes (impact, volcanism, flowing water, wind) that shaped other worlds, even though we have never seen them happen there.
A focused answer to the Eduqas GCSE Geology statement on uniformitarianism applied to planetary geology. Covers the principle that the present is the key to the past, how comparing landforms in space imagery with Earth landforms lets geologists infer the processes (impact, volcanism, water, wind) that shaped other planets, and the limits of the approach.
- The surfaces of the Moon and Mars record their geological histories: the Moon has heavily cratered highlands and smoother dark maria (ancient basalt plains), showing impact and volcanism on a body that is now dead; Mars shows giant volcanoes, a vast canyon system, dried-up channels and polar ice, showing past volcanism and flowing water; the relative density of impact craters is used to work out the relative ages of different surfaces (more craters means an older surface).
A focused answer to the Eduqas GCSE Geology statement on the Moon and Mars. Covers the lunar highlands and maria and what they record, the volcanoes, canyons, channels and ice of Mars, and how the density of impact craters is used to date planetary surfaces relatively.
- Minerals are identified using physical properties: colour, crystal size, hardness (tested against fingernail, copper coin, steel and glass), cleavage and fracture, lustre, streak, and the reaction of carbonates with dilute hydrochloric acid; common minerals include quartz, feldspar, mica, calcite, halite, galena and haematite.
A focused answer to the Eduqas GCSE Geology statement on identifying minerals. Covers the physical properties used (colour, crystal size, hardness, cleavage and fracture, lustre, streak and the acid test) and the diagnostic features of quartz, feldspar, mica, calcite, halite, galena and haematite.
- The rock cycle links igneous, sedimentary and metamorphic rocks through the processes of weathering, erosion, transport, deposition, burial and lithification, melting and crystallisation, and metamorphism; the cycle is driven by energy from the Sun (at the surface) and from the Earth's interior (at depth), and any rock can be changed into any other given time and the right conditions.
A focused answer to the Eduqas GCSE Geology statement on the rock cycle. Covers the three rock families and the processes that connect them (weathering, erosion, transport, deposition, lithification, melting, crystallisation and metamorphism), the two energy sources that drive the cycle, and how any rock can become any other.
Sources & how we know this
- WJEC Eduqas GCSE (9-1) Geology specification (teaching from 2017) — WJEC Eduqas (2017)