Researchers using the High Resolution Imaging Science Experiment
camera report the first measurement of a periodic signal in the rocks
of Mars. This pushes climate-cycle fingerprints much earlier in Mars"
history than more recent rhythms seen in Martian ice layers. It also
may rekindle debates about some patterns of rock layering on Earth.
Layers of similar thickness repeat dozens to hundreds of times in
rocks exposed inside four craters in the Arabia Terra region of Mars.
In one of the craters, Becquerel, bundles of a 10-layer pattern repeat
at least 10 times, which could correspond to a known 10-to-one pattern
of changes in the tilt of the planet"s rotation axis.
"Each layer has weathered into a stair step in the topography where
material that"s more resistant to erosion lies on top of material
that"s less resistant to erosion," said Kevin Lewis of the California
Institute of Technology, Pasadena, who is the lead author of a report
on the periodic layering published in the Dec. 5 edition of the journal
Science.
Some periodic change in the environment appears to have affected how
resistant the rock-forming sediments became, perhaps from changes in
what size of sand or silt particles were deposited by the wind, or from
how the particles were cemented together after deposition. Some of the individual layers are less than three feet thick.
The camera, called HiRISE for short, took pairs of images of each
site from slightly different angles in orbit, providing the stereo
information necessary for determining each layer"s thickness.
"It"s easy to be fooled without knowing the topography and measuring
the layers in three dimensions," said Alfred McEwen of the University
of Arizona, Tucson, principal investigator for the camera and a
co-author of the new report. "With the stereo information, it is clear
there"s a repeating pattern to these layers."
Geologists commonly find "rhythms," or repeating patterns, in
sedimentary layers on Earth. Determining the source of the rhythms can
be difficult. Some result from annual or tidal cycles, or from episodic
flooding that may not be periodic at all, but the role of longer-term
astronomical cycles has been debated. One step in showing that
astronomical cycles can leave their mark in sediments came from finding
repeating five-layer sets in some terrestrial bedrock, matching a known
five-to-one ratio of two cyclical variations in Earth"s orbit.
Lewis and colleagues found something similar on Mars: "Our findings
suggest that cycles of climate change led to the patterns we see
recorded in the Mars rock layers today, possibly as a result of similar
variations in Mars" orbit," he said. "Mars has a 10-to-one ratio in
cycles of how its tilt changes -- smaller wobbles within larger
packages. Sure enough, we see a 10-to-one ratio in one of these layered
deposits. It"s like trying to identify a song -- it"s easier if there
are multiple instruments playing different parts, rather than just a
single rhythm."
In addition to having rhythm of 10 beats to the bar instead of
Earth"s five-beat pattern, Mars has characteristics that make it a good
laboratory for studying how astronomical cycles affect climate. The
tilt of Mars" axis varies much more than the axis of Earth, because
Earth"s relatively large moon provides a stabilizing effect. And, at
least for most of its history, Mars has lacked the oceans and thick
atmosphere that, on Earth, modulate the effects of orbital variations
and add their own cyclical patterns.
The 10-beat pattern of Mars" wobble lasts about 1.2 million years.
If the 10-layer bundles in Becquerel crater are indeed signatures of
that cycle, the 10 or more bundles stacked on each other record about
12 million years when environmental conditions affecting sedimentation
were generally steady except for effects of the changing tilt.
NASA"s Jet Propulsion Laboratory, a division of Caltech, manages the
Mars Reconnaissance Orbiter for NASA"s Science Mission Directorate,
Washington. Lockheed Martin Space Systems, Denver, is the prime
contractor for the project and built the spacecraft. The HiRISE camera
was built by Ball Aerospace and Technologies Corp., Boulder, and is
operated by the University of Arizona.
Posted by Casey Kazan from materials submitted by NASA.