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Martian Rocks Make Geological Clocks

The rock that paves Mars's vast Arabia Terra region is very ancient and cratered. Now, the powerful HiRISE camera on the Mars Reconnaissance Orbiter has taken striking images of wind-eroded outcrops on some of the crater floors. The outcrops' sedimentary layers appear to have built up with rhythmic regularity, suggesting that random, catastrophic events such as floods or volcanic eruptions did not create them.

Periodic layering in Becquerel Crater, Mars

Periodic layering in Becquerel Crater, Mars (NASA/JPL-Caltech/ University of Arizona)

So what did? HiRISE's high-resolution images allowed Mars researchers to use investigative techniques practiced by Earth geologists. A team of scientists from the California Institute of Technology, the U.S. Geological Survey, and the University of Arizona reconstructed a 3D topographic map of a hilly region in Arabia Terra. They used this map to measure the height and pattern of the rock layers.

The results suggest that regular climate events built up the layers in stages. The best candidate for what would set off such cycles is the shift of Mars's tilt on its axis, which varies by a few degrees on a 100,000-year rhythm. These types of orbital changes on Earth induce periodic ice ages due to the planet's position relative to the Sun.

See more of HiRISE's images—including a movie of the 3-D map—in the latest AMNH Astro Bulletin.

Rhythmic Pattern of Sedimentary Rock in Becquerel Crater

What if the rhythmic clastic rock has been laid down in the core of a comet within a comet cluster of the Outer Oort Belt and delivered in an icy package that protected the sedimentary rock from the perils of impact? Quickly, granitoid rock might form in aqueous comet cores when chemoautotrophic bacteria oxidize nebular dust and the saturated oxides precipitate to the center forming a granite core. Later in the Late Heavy Bombardment when our birth nebular cluster broke up, the close encounter of a sister star may have wrecked the Hills Cloud comet belt scattering comets as far out as the Outer Oort Belt. These comets could have organized into clusters with the low solar gravity at a distance of 1 light year from the sun, and when comets collide, the granite cores grind together within an aqueous ocean, creating clastic material which is deposited in rhythmic patterns caused by the complicated tidal effects of nearby orbiting comets within the comet cluster.