Finding Buried Treasure on Mars: Radar Map Confirms Climate Cycles
Written by Nancy Atkinson
A radar-generated map of the thickness of the layered deposits. Image credit: NASA/JPL-Caltech/University of Rome/Southwest Research Institute/University of Arizona
A radar instrument on the Mars Reconnaissance Orbiter has essentially looked below the surface of the Red Planet's north-polar ice cap, and found data to confirm theoretical models of Martian climate swings during the past few million years. The new, three-dimensional map using 358 radar observations provides a cross-sectional view of the north-polar layered deposits. "The radar has been giving us spectacular results," said Jeffrey Plaut of JPL, a member of the science team for the Shallow Radar instrument. "We have mapped continuous underground layers in three dimensions across a vast area."
Alignment of the layering patterns with the modeled climate cycles provides insight about how the layers accumulated. These ice-rich, layered deposits cover an area one-third larger than Texas and form a stack up to 2 kilometers (1.2 miles) thick atop a basal deposit with additional ice.
"Contrast in electrical properties between layers is what provides the reflectivity we observe with the radar," said Nathaniel Putzig of Southwest Research Institute, Boulder, CO, who led the science team. "The pattern of reflectivity tells us about the pattern of material variations within the layers."
Earlier radar observations indicated that the Martian north-polar layered deposits are mostly ice. Radar contrasts between different layers in the deposits are interpreted as differences in the concentration of rock material, in the form of dust, mixed with the ice. These deposits on Mars hold about one-third as much water as Earth's Greenland ice sheet.
Their radar results show that high-reflectivity zones, with multiple contrasting layers, alternate with more-homogenous zones of lower reflectivity. Patterns of how these two types of zones alternate can be correlated to models of how changes in Mars' tilt on its axis have produced changes in the planet's climate in the past 4 million years or so, but only if some possibilities for how the layers form are ruled out.
"We're not doing the climate modeling here; we are comparing others' modeling results to what we observe with the radar, and using that comparison to constrain the possible explanations for how the layers form," Putzig said.
The most recent 300,000 years of Martian history are a period of less dramatic swings in the planet's tilt than during the preceding 600,000 years. Since the top zone of the north-polar layered deposits — the most recently deposited portion — is strongly radar-reflective, the researchers propose that such sections of high-contrast layering correspond to periods of relatively small swings in the planet's tilt.
They also propose a mechanism for how those contrasting layers would form. The observed pattern does not fit well with an earlier interpretation that the dustier layers in those zones are formed during high-tilt periods when sunshine on the polar region sublimates some of the top layer's ice and concentrates the dust left behind. Rather, it fits an alternative interpretation that the dustier layers are simply deposited during periods when the atmosphere is dustier.
The new radar mapping of the extent and depth of five stacked units in the north-polar layered deposits reveals that the geographical center of ice deposition probably shifted by 400 kilometers (250 miles) or more at least once during the past few million years.
The Italian Space Agency operates the Shallow Radar instrument.
More information about the MRO mission.
Source: JPL
Filed under: Astronomy
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September 23rd, 2009 at 11:10 am
Ah, so the bimodal ice distribution is indicative of polar shift, not asymmetry of climate due to Mars asymmetry of geology. One less mystery.
Now I would love for the climate modelers to step in and tell us if the dust deposit rate overwhelming dust concentration at all times mean that the ice is fairly protected from sublimation. If it's because of the dust cover, then Mars is dry because Mars is dry.