Martian Meteorites List
This page provides a reference overview of recognized Martian meteorites and their scientific importance. Martian meteorites are genuine samples of Mars found on Earth, and together they reveal the remarkable diversity of Martian volcanic, cumulate, crustal, and brecciated materials.
What Is a Martian Meteorites List?
A Martian meteorites list is a reference overview of meteorites officially recognized as having originated from Mars. Such a list is useful not only for identifying individual Martian meteorites, but also for understanding the diversity of Martian lithologies represented among samples recovered on Earth.
Martian meteorites are exceptionally important because they are the only direct samples of Mars currently available for laboratory study on Earth. Each recognized specimen contributes to a broader scientific understanding of Martian geology, volcanism, crustal evolution, and impact history.
Why Martian Meteorites Are Important
Martian meteorites provide direct evidence about the geological evolution of Mars. They preserve information about magmatic activity, mantle-derived rocks, crustal processes, shock events, aqueous alteration, and regolith formation. Together, they offer a uniquely valuable complement to data obtained by orbiters, landers, and rovers.
As a group, Martian meteorites form one of the most important categories of planetary material available to science, museums, and advanced collectors.
What a Martian Meteorites List Reveals
A reference list of Martian meteorites is not simply a catalog of names. It reveals the range of recognized Martian lithologies, the historical growth of the field, and the classification framework used to organize these meteorites. It also helps distinguish between individual meteorites, paired stones, and the main families of rocks represented among known Martian samples.
As new Martian meteorites are classified, the list reflects the expanding geological picture of Mars and helps place each specimen within a broader scientific context.
The SNC Framework
Martian meteorites are traditionally organized within the SNC classification, named after three historic meteorites: Shergotty, Nakhla, and Chassigny. These meteorites represent distinct Martian rock types and form the historical basis of Martian meteorite classification.
Today, the SNC framework remains useful because it provides a practical structure for the principal Martian groups, even though the known diversity of Martian meteorites now extends beyond the simplicity of the original three-part naming scheme.
Recognized Types of Martian Meteorites
The Martian meteorites recognized to date represent a range of igneous and brecciated lithologies. These include:
- basaltic shergottites,
- olivine-phyric shergottites,
- lherzolitic shergottites,
- nakhlites,
- chassignites,
- orthopyroxenites,
- Martian crustal and regolith breccias.
This diversity shows that Martian meteorites are not a single uniform category, but a complex family of rocks derived from different geological settings and processes on Mars.
Pairings, Fragments, and Individual Meteorites
When reading any Martian meteorites list, it is important to distinguish between officially recognized meteorites and paired fragments. Some stones recovered separately may in fact belong to the same original meteoritic mass or terrestrial find event. For that reason, the total number of recognized Martian meteorites is not always identical to the number of truly separate Martian source stones represented in collections.
This is one reason why a Martian meteorites list should always be interpreted as a scientific reference framework rather than a simple count of independent falls or finds.
Why the Discovery of Martian Meteorites Was So Important
The identification of Martian meteorites marked a major turning point in planetary science. Their relatively young crystallization ages and unusual isotopic characteristics distinguished them from most other achondrites and suggested a planetary source rather than a small asteroid parent body.
A decisive line of evidence came from trapped gas inclusions found in some Martian meteorites, especially the shergottite EETA 79001. These gases closely matched the composition of the Martian atmosphere measured by spacecraft, providing one of the strongest demonstrations that these meteorites truly originated on Mars.
Martian Meteorites as a Scientific Resource
Beyond their rarity, Martian meteorites are scientifically essential because they provide direct hand samples of another planet. They help researchers study Martian volcanic rocks, cumulate lithologies, ancient crustal components, and water-related alteration features under laboratory conditions not possible with remote sensing alone.
They are also important in the broader context of astrobiology, because some Martian meteorites preserve evidence of water-related processes and geochemical environments relevant to the history of habitability on Mars.
Classification and Official Recognition
Martian meteorites are formally recognized through detailed laboratory analyses involving mineralogy, chemistry, petrography, and isotopic composition. Once approved, their names and classifications are recorded in the Meteoritical Bulletin Database, which remains the principal reference source for officially recognized meteorites.
A serious Martian meteorites list should therefore be understood as a scientific reference guide rather than a simple historical catalog.
Explore Martian Meteorites
This page is intended as a reference overview of recognized Martian meteorites. To explore specimens selected for collectors, museums, and research institutions, please visit our main page on Martian Meteorites.
List of mars meteorites, catalog of worldwide meteorite finds identified as originating from the red planet Mars.
List of Martian Meteorite courtesy of:
Ron Baalke
Jet Propulsion Laboratory
Martian meteorites are of major scientific importance because they represent the only known samples of another planet available for research. From a geological point of view, they are most intriguing, but more importantly, they provide tantalizing clues to the question of the possibility of life on other planets.
If we exclude all probable pairings, 34 different Mars meteorites have been recovered to date, comprising a total weight of about 94 kg, with about 66 kg recovered from out of Antarctica. Based on their mineral compositions, the Mars meteorites are further divided into six related subgroups: basaltic shergottites, olivine-phyric shergottites, lherzolitic shergottites, nakhlites, chassignites, and orthopyroxenites, the latter subgroup consisting of just one single member.
| Meteorite Name | Location Found | Date Found | Mass (g) | Type |
| Chassigny | France, Haute-Marne province, village of Chassigny |
October 3, 1815 | ~4,000 | dunite (chassignite) |
| Shergotty | India, Bihar State, town of Shergahti | August 25, 1865 | ~5,000 | basaltic shergottite |
| Nakhla | Egypt, El-Baharnya, village of El-Nakhla | June 28, 1911 | ~10,000 | clinopyroxenite (nakhlite) |
| Lafayette | United States, Indiana, Lafayette | 1931 | ~800 | clinopyroxenite (nakhlite) |
| Governador Valadares | Brazil, state of Minas Gerais, city of Governador Valadares |
1958 | 158 | clinopyroxenite (nakhlite) |
| Zagami | Nigeria, Katsina Province, Zagami Rock | October 3, 1962 | ~18,000 | basaltic shergottite |
| ALHA 77005 | Antarctica, Victoria Land, Allan Hills | December 29, 1977 | 482 | peridotite (lherzolitic shergottite) |
| Yamato 793605 | Antarctica, Victoria Land, Yamato Mountains | 1979 | 16 | peridotite (lherzolitic shergottite) |
| EETA 79001 | Antarctica, Victoria Land, Elephant Moraine | January 13, 1980 | 7,900 | olivine-phyric shergottite |
| ALH 84001 | Antarctica, Victoria Land, Allan Hills | December 27, 1984 | 1,939.9 | orthopyroxenite |
| LEW 88516 | Antarctica, Victoria Land, Lewis Cliff | December 22, 1988 | 13.2 | peridotite (lherzolitic shergottite) |
| QUE 94201 | Antarctica, Victoria Land, Queen Alexandra Range |
December 16, 1994 | 12.0 | basaltic shergottite |
| Dar al Gani 476 Dar al Gani 489 Dar al Gani 735 Dar al Gani 670 Dar al Gani 876 Dar al Gani 975 Dar al Gani 1037 |
Libya, Sahara Desert | May 1, 1998 1997 1996-1997 1998-1999 May 7, 1998 August 21, 1999 1999 |
2,015 2,146 588 1,619 6.2 27.55 4012.4 |
olivine-phyric shergottite |
| Yamato 980459 | Antarctica, Yamato Mountains | December 4, 1998 | 82.46 | basaltic shergottite |
| Los Angeles 001 Los Angeles 002 |
United States, California, Mojave Desert | October 30, 1999 October 30, 1999 |
452.6 245.4 |
basaltic shergottite |
| Sayh al Uhaymir 005 Sayh al Uhaymir 008 Sayh al Uhaymir 051 Sayh al Uhaymir 094 Sayh al Uhaymir 060 Sayh al Uhaymir 090 Sayh al Uhaymir 120 Sayh al Uhaymir 150 Sayh al Uhaymir 125 Sayh al Uhaymir 130 Sahy al Uhaymir 131 |
Oman, Sayh al Uhaymir | November 26, 1999 November 26, 1999 August 1, 2000 February 8, 2001 June 27, 2001 January 19, 2002 November 17, 2002 October 8, 2002 November 19, 2003 January 11, 2004 January 11, 2004 |
1,344 8,579 436 233.3 42.28 94.84 75 107.7 31.7 278.5 168 |
olivine-phyric shergottite |
| Dhofar 019 | Oman, Dhofar | January 24, 2000 | 1,056 | olivine-phyric shergottite |
| GRV 99027 | Antarctica, Grove Hill | February 8, 2000 | 9.97 | peridotite (lherzolitic shergottite) |
| Dhofar 378 | Oman, Dhofar | June 17, 2000 | 15 | basaltic shergottite |
| Northwest Africa 2737 | Morocco | August 2000 | 611 | dunite (chassignite) |
| Northwest Africa 480 Northwest Africa 1460 |
Morocco | November 2000 December 2001 |
28 70.2 |
basaltic shergottite |
| Y000593 Y000749 Y000802 |
Antarctica, Yamato Mountains | November 29, 2000 December 3, 2000 ?? |
13,700 1,300 22 |
clinopyroxenite (nakhlite) |
| Northwest Africa 817 | Morocco | December 2000 | 104 | clinopyroxenite (nakhlite) |
| Northwest Africa 1669 | Morocco | January 2001 | 35.85 | basaltic shergottite |
| Northwest Africa 1950 | Morocco | January & March 2001 | 797 | peridotite (lherzolitic shergottite) |
| Northwest Africa 856 | Morocco | March 2001 | 320 | basaltic shergottite |
| Northwest Africa 1068 Northwest Africa 1110 Northwest Africa 1775 Northwest Africa 2373 |
Morocco, Maarir Morocco, Erfoud |
April 2001 January 2002 2002 August 2004 |
654 118 25 18.1 |
olivine-phyric shergottite |
| Northwest Africa 998 | Algeria or Morocco | September 2001 | 456 | clinopyroxenite (nakhlite) |
| Northwest Africa 1195 | Morocco, Safsaf | March 2002 | 315 | olivine-phyric shergottite |
| Northwest Africa 2046 | Algeria, Lakhbi | September 2003 | 63 | olivine-phyric shergottite |
| MIL 03346 | Antarctica, Miller Range of the Transantarctic Mountains | December 15, 2003 | 715.2 | nakhlite |
| Northwest Africa 3171 | Algeria | February 2004 | 506 | basaltic shergottite |
| Northwest Africa 2626 | Algeria | November 2004 | 31.07 | olivine-phyric shergottite |
| YA1075 | Antarctica | ?? | 55 | peridotite (lherzolitic shergottite) |
Frequently Asked Questions About Martian Meteorites List
What is a Martian meteorites list?
A Martian meteorites list is a reference overview of meteorites officially recognized as originating from Mars.
Why is a Martian meteorites list scientifically important?
It helps document the diversity of Martian rocks found on Earth and places individual meteorites within a broader geological and classification framework.
Are all Martian meteorites the same?
No. Martian meteorites include several lithologies such as shergottites, nakhlites, chassignites, orthopyroxenites, and Martian crustal breccias.
What does SNC mean?
SNC refers to the traditional framework based on Shergotty, Nakhla, and Chassigny, the three historic meteorites that gave their names to the main Martian meteorite groups.
Does the number of Martian meteorites equal the number of separate Martian stones?
Not always. Some recognized Martian meteorites are paired fragments belonging to the same original meteoritic mass, so reference lists must be interpreted carefully.
How do scientists know a meteorite comes from Mars?
Martian meteorites are identified through mineralogy, chemistry, isotopic composition, and in some cases trapped gases that match the Martian atmosphere measured by spacecraft.
Who officially recognizes Martian meteorites?
Martian meteorites are officially recognized through classification work recorded in the Meteoritical Bulletin Database.
Where can I see available Martian meteorites?
You can explore available specimens on our main Martian Meteorites page.