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Researchers identify 4.1 billion-year-old Martian meteorite found in Mali

The 800-gram rock, named Teghaza 001, provides rare evidence of Mars' early crust formation and historical interactions between water and rock.

By Hermes-Vector AI Desk

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Checked against 2 sourcesafrica.businessinsider.comcidrap.umn.edu
Illustration for: Researchers identify 4.1 billion-year-old Martian meteorite found in Mali

In brief

  • Teghaza 001 is an 800-gram Martian meteorite discovered in Mali's Sahara Desert in 2022.
  • The rock dates back over 4.1 billion years and contains volcanic minerals from cooling magma.
  • The meteorite shows evidence of being altered by water beneath the Martian surface.
  • Researchers have not yet identified the exact point of origin for the meteorite on Mars.

Researchers identify 4.1 billion-year-old Martian meteorite found in Mali

A meteorite discovered in the Sahara Desert of Mali has been identified as one of the oldest Martian rocks ever found on Earth. The 800-gram rock, named Teghaza 001 after the salt plain where it was discovered in 2022, dates back over 4.1 billion years, according to research published in the scientific journal Science.

Geological Significance

Teghaza 001 is among approximately 435 meteorites from Mars identified on Earth. However, its specific age and mineral composition make it particularly valuable to researchers. Unlike some other ancient Martian rocks, this discovery contains a mixture of volcanic minerals. These minerals provide clues regarding how the initial crust of Mars formed from cooling magma.

“It was only after we started looking closely that we realized this meteorite is really unique,” said Yang Liu of NASA’s Jet Propulsion Laboratory in Southern California, who is the lead author of the paper. One reviewer of the paper referred to the meteorite as a "Rosetta Stone for Mars."

Evidence of Water on Ancient Mars

Research indicates that the meteorite shows evidence of alteration by water beneath the Martian surface. This provides details about ancient interactions between water and rocks. A separate study published in Science Advances in June examined the water content of Teghaza 001, offering further insight into how water interacted with the Martian surface during the planet's early history.

“This is really our first piece of Martian crust from a part of Mars we’ve never had a sample of before,” said Lee Saper, the paper’s second author, who conducted research while at JPL as a postdoctoral scholar.

“It records interactions of water and rock and maybe even an imprint of the Martian atmosphere as it was losing water,” Lee added.

Evidence derived from chemical composition, microstructural features, and oxygen isotope ratios suggests that early Mars had a "substantially more active hydrological cycle."

Ongoing Research

While researchers have identified several possible locations on Mars that match the chemical and mineral composition of the meteorite, the exact point of origin for Teghaza 001 remains unknown. The report showed that the sample underwent modification by Martian water processes approximately 4.1 billion years ago, indicating its initial formation predated that period.

Further studies of the rock may help scientists understand how Mars developed more than four billion years ago and whether conditions on the planet were once more favorable to water and potentially life.


Sources

This article was drafted with AI assistance and checked against the sources above. Company claims are reported as claims. Cover image is AI-generated.

Questions readers ask

What is the name and age of the new Martian meteorite?
The meteorite is named Teghaza 001 and dates back over 4.1 billion years.
Where and when was the meteorite discovered?
It was discovered in 2022 in the Sahara Desert of Mali on a salt plain.
What does the meteorite reveal about ancient Mars?
It shows evidence of alteration by water beneath the Martian surface and suggests early Mars had a substantially more active hydrological cycle.
Who led the research and where was it published?
Yang Liu of NASA's Jet Propulsion Laboratory is the lead author, and the research was published in the scientific journal Science.

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