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Wold meteorite landing siteWatercolour showing an obelisk marking the landing site of the Wold Meteorite, Yorkshire, 1812. Image from the Sowerby Collection
The Murchison CM2 carbonaceous chondriteMurchison fell in September 1969, in Victoria, Australia. It is rich in indigenous (i.e. not terrestrial contaminant) amino acids and other organic molecules
Section of Chassigny meteoriteThin section of Chassigny in cross-polarized light, showing shocked and deformed olivine grains. The field of view is 3mm
Wold meteoriteWatercolour of the Wold meteorite, Yorkshire by Hariet Topham, 1797. Image from Sowerby Collection
Iron meteoriteThis meteorite is the product of atmospheric melting, as are stony achondrites. Specimen held at the Natural History Museum, London
Microscope image of the Pasamonte eucriteMicroscopic image of the Pasamonte eucrite showing a basaltic texture. Field of view is 2.5mm across
Wold Cottage meteoriteThe earliest surviving meteorite seen to land in the UK fell in Wold Cottage, Yorkshire, in 1795
The Stannern achondriteA piece of the Stannern achondrite which is thought to have originated on the asteroid Vesta
The Allende carbonaceous chondritePhotograph of the Allende carbonaceous chondrite, partly covered in jet-black fusion crust. This contains numerous white inclusions called CAIs. This stone is about 10cm across
Launton MeteoriteThe Launton meteorite fell on 15 February 1830 at approximately 7.30pm, Launton village in Oxfordshire. The meteorite is of the most common type of stony meteorite, known as an ordinary chondrite
Wold Cottage meteorite (detail)The earliest surviving meteorite seen to land in the UK fell in Wold Cottage, Yorkshire, in 1795
The Stannern achondrite see 35502A piece of the Stannern achondrite which is thought to have originated on the asteroid Vesta
The Beardsley H5 ordinary chondriteBeardsley fell in Kansas, U.S.A in 1929. Its fine-grained texture, with poor chondrule resolution indicate that it has experienced thermal metamorphism
The Abee EH4 enstatite chondriteAbee fell in Canada in 1953. The cut surface clearly shows the metal-rich and brecciated texture of Abee
Vigarano CV3 chondriteThis carbonaceous chondrite meteorite fell in Italy in 1910. It has clearly delineated chondrules or small granules
Parnallee LL3. 6 ordinary chondriteParnallee fell in India in 1857. The cut surface clearly shows well-delineated chondrules and slightly larger clasts
Brownfield (1973) H3. 7 ordinary chondriteThis meteorite fell in Texas in 1937. It has very small chondrules, plus highly-reflective metal and sulphide grains can easily be picked out
Cold Bokkeveld meteorite photomicrographThin section of the carbonaceous chondrite in the petrological microscope, showing a near circular chondrule about 1mm in diameter. The fall was in Cape Province in 1838
Stone meteoriteThis meteorite is unmelted and is therefore known as a chondrite. Specimen held at the Natural History Museum, London
Mayo Belwa, African meteoriteThis meteorite formed in a similar way to some igneous rocks in the Earth, and not by condensation of dust from nebular gas. Image from From Behind The Scenes (1987) by Dr Lawrence Mound
Microscope image of the Johnstown diogenite. Diogenites are coarse grained and composed primarily of one mineral, pyroxene. Field of view is 2.5mm across
Microscope image of chondrite showing chondrules, typical of primitive meteorites. Horizontal field of view, 3.3mm
Microscope image of the Brachina meteorite, the type specimen of the Brachinite meteorites. Brachinites are composed mostly of olivine with minor amounts of pyroxene and plagioclase
Microscope image of the Lodran meteorite. This meteorite is the type specimen of the Lodranite meteorites. The lodranites are related to the acaplucoites but are more course-grained
The Sioux County eucritePhotograph of the Sioux County eucrite, which is thought to have originated on the asteroid 4 Vesta. The sample weighs 153g
The Bustee aubritePhotograph of the Bustee aubrite, a light-coloured meteorite containing brown oldhamite crystals
Optical microscope image of the Barwell (Type 6) chondrite
Optical microscope image of the Parnallee (Type 3) chondriteAn optical microscope image of the Parnallee (Type 3) chondrite that has experienced little heating. The chondrules are clear and well-defined. The field of view is 5mm
The Beddgelert (H5) ordinary chondritePhotograph of the Beddgelert (H5) ordinary chondrite, clearly showing flecks of iron-nickel metal
The Parnalle ordinary chondriteThe Parnallee ordinary chondrite, part of the Parnallee meteorite that fell in India in 1857
The Barwell meteorite, showing a rock frgament formed by melting of a pre-existing planetary body; this indicates that plantesimals were present when chondrules formed
Textures of different chondrule types in the Etihudna (L4) ordinary chondrite (field of view 4mm)
Porphyritic olivine and pyroxene chondruleMicroscopic image of a porphyritic olivine and pyroxene chondrule from the Palmyra (L3) ordinary chondrite (the chondrule is about 1.8mm across)
Radial pyroxene chondruleMicroscope image of a radial pyroxene chondrule from the ALH 88036 (H3.4) ordinary chondrite. The chondrule is about 2mm across
Ivuna meteoriteThe Ivuna carbonaceous chondrite. This type of meteorite is the richest in volatile elements
Partially fusion-crusted stoneA 294g (10oz) partially fusion crusted stone from the Camel Donga eucrite strewn field. The orange/brown staining on the black, fusion crusted surface is staining from the local soil
Siena meteorite stoneOne of the stones of the Siena meteorite shower, which fell over Siena, Italy in 1794
Chergach meteorite
Meteoric Stone, Wold CottageOne of a series of 5 postcards featuring British meteorites produced and sold by the museum in the 1920s
British Meteorites, leafletLeaflet printed to accompany a set of 5 postcards published by the Natural History Museum in 1922
CarbonateThe formation of carbonate on the Allan Hills martian meteorite ALH84001
Glatton meteoriteMr Arthur Pettifor holding the Glatton meteorite which fell in Cambridgeshire on 5th May 1991