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Shergottites

The most common Martian meteorites: young basaltic and olivine-rich rocks.

Shergottite
Zagami, Martian (shergottite), Nigeria
Classification
Stony meteorites › Achondrites › Planetary achondrites › Martian meteorites › Shergottites
Share of witnessed falls
about 0.3%
In our catalogue
99 meteorites, 3 seen to fall
Heaviest
Zagami, 18 kg
Earliest recorded fall
Shergotty, 1865
Most recent fall
Tissint, 2011
Type specimen
Shergotty, fell in India in 1865

Shergottites, named after Shergotty in India (fell 1865), make up about three-quarters of Martian meteorites. They are basaltic, olivine-phyric or 'lherzolitic' (poikilitic) igneous rocks that crystallised surprisingly recently, mostly between about 150 and 600 million years ago. Their minerals are often converted to glass (maskelynite) by the shock of being blasted off Mars.

Mineralogy and chemistry

Basaltic shergottites, such as Shergotty, Zagami and Los Angeles, are made mostly of pyroxene (pigeonite and augite) and plagioclase turned to maskelynite glass by shock. Olivine-phyric shergottites, such as Tissint, Dhofar 019 and Elephant Moraine A79001, contain large olivine crystals in a fine basaltic groundmass. Poikilitic shergottites, such as Allan Hills A77005 and Yamato 793605, have olivine enclosed in large pyroxene crystals and formed as cumulates; they were formerly called lherzolitic.

Shergottites are also divided by trace elements and isotopes into depleted, intermediate and enriched kinds, depending on how much of the incompatible elements their source in the Martian mantle contained. This variety shows that Mars's mantle has had distinct reservoirs since it formed.

Origin and formation

Shergottites are lavas and shallow intrusions from Mars's volcanic regions, perhaps from the great volcanic provinces of Tharsis or Elysium. Most crystallised between about 150 and 600 million years ago, though a few are about 2.4 billion years old. Many show strong shock and pockets of impact melt; it was in such glass in Elephant Moraine A79001 that Martian atmospheric gas was found in 1983. They were launched from Mars in several separate impacts, with cosmic-ray exposure ages ranging from about 1 to 20 million years.

Shergottites are the main source of what we know about the Martian mantle and its volcanoes. Their minerals record water and chlorine in Martian magmas, and their isotopes show that Mars separated into core, mantle and crust within a few tens of millions of years of forming.

Abundance, type specimen and famous examples

Shergottites make up about three-quarters of Martian meteorites. Shergotty, the type specimen, fell near Sherghati in Bihar, India, on 25 August 1865; about 5 kg was recovered. Zagami fell in Nigeria in 1962 as a single stone of about 18 kg, the largest Martian meteorite seen to fall. Tissint fell in Morocco on 18 July 2011, and its fresh stones, collected within months, preserve Martian gases and minerals uncontaminated by long exposure on Earth. Los Angeles was found among a collector's rocks in California and recognised in 1999.

How to recognise one

Shergottites are greenish-grey to black basalts, often with clear or white maskelynite and dark shock veins. Olivine-phyric ones show yellow-green olivine crystals. Fresh Tissint stones have a shiny black crust. They are weakly to moderately magnetic and need laboratory confirmation.

Famous examples

Related groups

Photos shared under Creative Commons licences (Wikimedia Commons).