Scientists Discover 4.1 Billion-Year-Old Martian Meteorite in Sahara Desert

Teghaza 001 Discovery Rewrites the Timeline of Early Mars

Discovered in the Sahara Desert by nomadic meteorite hunters in 2022, a nearly two-pound, rose-colored space rock designated Teghaza 001 has been identified as a 4.1-billion-year-old chunk of Mars, according to findings published in the journal Science. The study establishes the meteorite as one of the three most ancient Martian meteorites ever found on Earth, offering a rare window into the planet’s primordial crust and its early water cycle.

Unpacking the Unique Mineralogy of the Sahara Meteorite

When the 800-gram stone arrived at the laboratory, its physical characteristics immediately separated it from the approximately 435 known meteorites originating from the Red Planet. Most Martian meteorites recovered on Earth provide snapshots from the most recent 600 million years of the planet’s history. Teghaza 001 shatters that trend.

The rock formed at least 4.1 billion years ago, hailing from an era when Mars possessed a warmer, wetter, and more Earth-like environment. Yang Liu, a planetary scientist at NASA’s Jet Propulsion Laboratory and lead author of the study, noted the historical significance of the sample to Scientific American: “We’re holding a piece of a rock that’s dated even before the oldest Earth rock—a piece of Mars that’s so ancient, it existed when life had just started on Earth.”

UMaine researcher identifies 4.1-billion-year-old Martian meteorite

Unlike other ancient Martian samples such as Allan Hills 84001, Teghaza 001 displays a distinctive mix of volcanic minerals derived from cooling magma. Inside the rock, researchers discovered zircon crystals containing uranium, which allowed them to utilize uranium-lead decay dating. Further analysis of rubidium and strontium isotopes confirmed the timeline. One reviewer evaluating the research went so far as to call the specimen a “Rosetta stone for Mars.”

Water Alteration and the Search for Ancient Origins

The geochemical signature preserved inside the meteorite reveals aggressive interaction between liquid water and rock during the planet’s youth. Analyses of remnant hydrogen trapped within the minerals show that water percolated through the ancient crust. At the same time, the data indicates that Mars was already losing its atmosphere and transitioning toward its current freeze-dried state.

A rose-colored rock on a white background
Photo: NASA

The meteorite’s chemical composition aligns closely with observations made by NASA’s Mars Reconnaissance Orbiter in the planet’s cratered southern highlands. Researchers have pinpointed 13 potential origin locations in regions like the Noachian southern highlands that match the rock’s mineralogy. However, exact coordinates on the Martian surface remain unknown.

What Remains Unanswered in Martian Geology

While the meteorite provides a high-resolution glimpse into a part of the Martian crust scientists have never sampled before, the lack of a verified point of origin leaves critical gaps in planetary reconstruction. Lee Saper, a scientist at NASA’s Ames Research Center who co-authored the research, emphasized that the stone captures interactions of water, rock, and the escaping Martian atmosphere. Yet, researchers agree that analyzing impact-imported fragments on Earth cannot fully replace the need for dedicated sample-return missions to the Red Planet.

Photo of author

Sophie Lin - Technology Editor

Sophie is a tech innovator and acclaimed tech writer recognized by the Online News Association. She translates the fast-paced world of technology, AI, and digital trends into compelling stories for readers of all backgrounds.

Trainer Paul Traynor Secures Notable Victory with Staton at Down Royal

Vikings’ Kyler Murray Struggles in Loss to Lions