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The largest cross-sectional slice of the NWA 7397 main mass. It is a Martain Shergottite (poikilitic), the result of a significant impact on a volcanic magma chamber on Mars.

Meteorites from Mars are among the most exotic substances on Earth. Martian meteorites share the following fundamental characteristics: they exhibit an unusually young crystalline age (so they cannot be from Earth); they contain water-bearing minerals (so they cannot be from the asteroid belt – the origin of 99.9 percent of all meteorites); there is evidence of a planetary sized gravitational field on their crystalline structure (which then makes the most likely candidates of origin our two closest neighbors – Venus and Mars). The link to Mars was speculative until an analysis was conducted on the glassy inclusions of two suspected Martian meteorites. In this glass were tiny voids, and in these voids were tiny volumes of gas. In 1997, the technology existed to analyze the gas – and it matched perfectly with the signature of the Martian atmosphere as reported by NASA’s Viking Missions to Mars. The delivery mechanism was an asteroid impact which jettisoned material off the Martian surface into an Earth intersecting orbit. This is a select slice of a rock from the planet Mars.

NWA 7397 contains large ovoid crystals – many of which are chatoyant. The large salmon-hued oikocrysts (crystals that contain other crystals) are composed of low calcium pyroxene, which enclose crystals of olivine and chromite. The reverse is blanketed in fusion crust, an artifact of the meteorite’s fiery descent through Earth’s atmosphere (where temperatures reached during frictional heating are hotter than the surface of the sun!).

NWA 7397 shares the compositional and isotopic fingerprint of other Martian meteorites. The determination of Martian origin is the result of research having been conducted by hundreds of scientists throughout the world. The lead author of the scientific abstract on NWA 7397 is Dr. Anthony Irving, the world’s foremost classifier of planetary meteorites.

5.5″ x 3.5″ x 1.5mm, 51.4g
SNC – Shergottite / Mars Rock
Found in Morocco in 2012.

3 responses to “A Large Slice of Mars”

  1. Thanks for sharing this series.

    It’s absolutely remarkable that impactors traveling at dozens of kilometers per second can spall unshocked material from planetary surfaces for express delivery to other Solar System bodies.

    http://www.flickr.com/photos/oklo/49810211101/in/photostream/

    We’re about to publish a study showing that Venusian meteorites (and specifically zircons) should be recoverable from lunar regolith. This is potentially a game-changer in permitting determination of when Venus lost its oceans, and by extension, its status as a habitable planet.

    http://www.flickr.com/photos/oklo/49810510522/in/photostream/

  2. fascinating! Please point me to it, and if you can share the isotopes to look for, I’d love to check some of my lunars… especially NWA5000A Huge Slice of the Moon

  3. I also a complete rock from MarsThe second-largest Mars rock in private hands, Dar al Gani 1037 It is awe-inspiring to contemplate how it got here: an asteroid impacts Mars long ago and dislodges a rock from the Martian surface. The rock orbits the sun for millions of years in an elliptical orbit, and by luck, lands on Earth. Most of the Martian material remains in roughly a Martian orbit (for most impact angles). Interestingly, there are a similar number of meteorites from our moon and from Mars. Mars is larger, but it is in a different orbit, and its atmosphere and gravity make it more difficult for ejecta to leave the planet. Nevertheless, if you include dust, Mars and Earth exchange a ton of ancient material per year.

    And maybe that’s how life spreads across the planets.

    The formation ages of meteorites can come from their cosmic-ray exposure (CRE), measured from the nuclear products of interactions of the meteorite in space with energetic cosmic ray particles. The one i have is particularly young, having crystallized only 180 million years ago, suggesting that volcanic activity was still present on Mars at that time. Volcanic flows are the youngest part of a planet, and this one happened to be hit by an meteor impact, ejecting the youthful Mars (in the same sense that parts of Kona are the newest Earth on Earth).

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