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Carbon Rocks Deep Underground Could Hold the Evidence of Mars' Watery Past.
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Carbon Rocks Deep Underground Could Hold the Evidence of Mars' Watery Past.

A new geochemical modeling study led by researchers at JAXA and the University of Tokyo addresses Mars' "missing" stores of carbonate rocks.

Original source cited and editorially framed by Cosmos Week. Universe Today
Editorial signatureCosmos Week Editorial Desk
Published26 Sep 2026 22: 53 UTC
Updated2026-09-26
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: A new geochemical modeling study led by researchers at JAXA and the University of Tokyo addresses Mars' "missing" stores of carbonate rocks
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

A new geochemical modeling study led by researchers at JAXA and the University of Tokyo addresses Mars' "missing" stores of carbonate rocks. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

That matters because chemistry gains force when a claimed structure or process can be described with enough precision to be reproduced by others. Synthetic routes, spectroscopic signatures, yield under defined conditions and stability under realistic operating parameters are the currency of credibility in chemistry, and a result that lacks these details cannot be evaluated independently. The distance between a discovery on a laboratory bench and a process that works reliably at scale is measured in years of optimization, and each step reveals constraints that were invisible at smaller scale. And yet, orbiters and rovers have found only small amounts of carbonate rocks on its surface, far less than what scientists would expect from a planet that is believed to have. But a new geochemical study led by researchers from the Japan Aerospace Exploration Agency (JAXA) shows two things that could resolve the mystery.

This study was led by doctoral student Chang-Chin Wang with Professor Tomohiro Usui of the Institute of Space and Astronautical Science at JAXA and the University of Tokyo, and. Previous research on water-rock interactions on Mars billions of years ago has assumed that water interacted with the planet's most common rock types, which are composed of mafic.

These rock-forming minerals are also the most abundant group on Earth, accounting for 60% of the Earth's crust. On Mars, these rocks are distinguished by higher calcium, sodium, and aluminum content, with strong indications that they may have once been widespread.

To this end, the team built one-dimensional thermochemical models that tracked how water dissolved minerals and created new ones (altering the chemistry of both) as it percolated. The simulations were based on the PHREEQC Version 3 geochemical code, which performs a wide variety of aqueous geochemical calculations.

The broader interest lies in whether the claimed property or reaction pathway can be characterized with enough precision to support replication by other groups. Chemistry has a replication problem that is less discussed than the one in psychology or medicine, but it is real: synthetic procedures that work reliably in one laboratory sometimes fail to transfer, for reasons ranging from impure starting materials to undocumented temperature sensitivities. A result that comes with full experimental detail and a clear characterization of the product is far more valuable than one that reports a discovery without the procedural backbone.

The simulations ranged from short bursts of alteration that lasted for a few years to longer episodes lasting up to 100, 000 years. ESA/Medialab The results showed that feldspar-rich rock readily produces calcium/iron-rich carbonates under most conditions.

Because this item comes through Universe Today as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to see whether independent groups working with orthogonal techniques reach compatible conclusions, and whether the result scales beyond the conditions used in the original study. Chemical discoveries that matter tend to be ones whose key properties can be measured by multiple spectroscopic, crystallographic or computational methods that are unlikely to share the same blind spots. Scalability, cost and long-term stability under realistic operating conditions are additional filters that come into play before any practical application becomes viable.

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