Thaumasia Planum: Unusual Martian Region Leaves Clues to Planet’s Past

They also studied the chemistry of this area based on Gamma Ray Spectrometer data collected by the Mars Odyssey Orbiter, which was launched in 2001. What they found was the mountain ridge that outlines Greater Thaumasia was most likely created by a chain of volcanoes. The results were published recently in the Journal of Geophysical Research-Planets.

[Video] How did Greater Thaumasia, an oddly high elevation region of Mars, form? Don Hood talks Martian geology

“The chemical changes we see moving northwestward through the region is consistent with the mantle evolving on Mars. Our research supports that this whole area was built as a volcanic construct,” said Don Hood, LSU Department of Geology and Geophysics doctoral candidate and lead author of the paper.

The chemical composition changes throughout the region. Silica and H20 increase and potassium decreases from southeast to northwest.

“The chemical composition shifting is the key progression that tells us that this environment was most likely shaped by a series of volcanic events that continually erupted from a changing mantle composition,” Hood said.

LSU Mars researchers study the Kilauea Iki lava lake on Hawaii, which offers a similar geological environment to Mars.

Photo Credit: Don Hood, LSU

Hood and colleagues from Stony Brook University, University of Tokyo and Lehigh University ruled out another hypothesis that the abundance of H20 and potassium was caused by water interacting in rock.

“We looked for evidence of aqueous alteration through other geochemical means and didn’t find it,” he said.

The geography of the region has many shield volcanoes that are similar to the ones found in Hawaii. However from geochemical analyses, the researchers found that the sulfur that is present was most likely deposited as a volcanic ash. Volcanic ash from various areas could be evidence of explosive volcanism on Mars, which would be an important clue for piecing together the history of Mars. It is significant because explosive eruptions emit a lot of gas that can stay in the atmosphere and can cause global cooling and warming events.

“Whether there was explosive volcanism on Mars and how much of it there was is an important question in terms of finding out what the past climate was like,” Hood said.

Contacts and sources:
Alison Satake

Louisiana State University

Citation: “Assessing the geologic evolution of Greater Thaumasia, Mars,” Journal of Geophysical Research-Planets: http://onlinelibrary.wiley.com/doi/10.1002/2016JE005046/full