Category PHYS P24 Tharsis Montes:The Search for Palagonite and Its Implications

for Martian Life

Abstract The Tharsis Montes are a group of three shield volcanoes located

near the equator of Mars, centered around 332°E, -40°N. This region

has been described as having glacial and volcanic activity during the

Amazonian Era. These glaciovolcanic interactions could have created

habitable aqueous environments in the late history of Mars.

Palagonite is an alteration mineral that is often formed from volcanic

glass. Researchers believe that palagonite on Earth is often biogenic in

its origin. One goal of this research was to find if palagonite exists on

Mars. Investigators have not yet found palagonite on the surface of

Mars. The spectrum of palagonite is hard to distinguish as it closely

resembles the spectra of other hydrated silicates. So, another research

goal is to create a set of criteria to distinguish palagonite spectra from

its look-alikes.

A total of 364 HiRISE images were examined for indicators of ice-

volcanic interactions, such as inverted terrain, ice cauldrons, and

glaciovolcanic edifices. These areas were then analyzed using online

spectral libraries and spectra from the CRISM instrument to find

possible spectra of palagonite in the given area.

Out of 40 spectra examined, 3 putative palagonite spectra were found

in three different areas in the Tharsis Region as a result of this

research. Along with this discovery, an algorithm was set to determine

palagonite from look-alikes so future researchers will have a more

streamlined process when searching for palagonite. This algorithm

includes looking at the overall form of a certain spectrum and its major

absorption bands in relation to the spectra of palagonite and its mineral

associates.

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