ATHABASCA VALLES:
FOLLOWING THE WATER
JIM RICE
and
TIM PARKER
Contributors: A. McEwen, D. Burr,
S. Sakimoto, and A. Haldemann

SCIENTIFIC OBJECTIVES
DRIVING SITE SELECTION
The landing sites will be selected so that they show two different types of evidence for the action of liquid water,
such as mineralogic or geomorphologic
(outflow sediments or hydrothermal deposits) and where hypotheses related to aqueous activity can be further tested using
the rovers and their payloads.
The target composition data combined
with the context and
landing site information are intended to
support the testing of
hypotheses regarding the geologic history and the nature of past aqueous
processes.

Scientific
Rationale for
Athabasca
Valles Sites
Follows the Water:
Diversity
of Geologic Processes
Hydrothermal: fissure
vents for water/ lava
Ground
Ice: rootless cones, patterned
ground
Volcanic: lava flows, fissure vents
for lavas
Elysium Regional Geology Overview
VOLCANIC
Elysium Volcanic Province: 2nd largest volcanic region on Mars
(Elysium Mons, Albor Tholus, Hecates Tholus, Cerberus Rupes).
Geomorphology: volcanic edifices, fissure vents, lava plains, flow fronts
Eruption style: low viscosity flood volcanism followed by central construct building
then back to flood eruptions.
Timing: Young or older? Crater counts suggest very young ages (~10 ma) but it
appears that in many regions this surface is being exhumed.
Implications: on thermal history of Mars, indicates that sufficient heat in upper
mantle generated large quantities of lava with high eruption rates possibly
very late in history (geothermally still active??). Water and heat: Exobiology?
Outflow
Channel Complex: Extensive network of channels
associated with volcanoes and fissures (Athabasca, Marte, Granicus, Iberus,
Ituxi, and Patapsco Valles).
Geomorphology:
channels,
streamlined islands, scour, collapsed terrain (Water); rootless cones,
patterned ground (Ice). Note: Rice and
Parker suggest that the “platy flows” may be flood deposits (jökulhlaups) and not lava flows. These sediments “froze up” forming a debris
mantled ice rich deposit. The analogy
is polar pack ice with pressure ridges. Alternatively, this ice choked flood
deposit would undergo sublimation leaving behind ice casts and crevasse fills.
Flood Sources:
volcano-ground
ice interactions, fissures, eroded or buried outflow channel.
Timing: Young or ancient? Crater
counts suggest very young ages (~10 ma) but it appears that in many regions
this surface is being exhumed.
Implications: near surface ice lenses/ice
rich permafrost or deep seated aquifers were preserved for extended periods of
time in equatorial regions and that specific local geologic conditions caused
the release of water (hydrothermal) to the surface in recent times or that an
ancient buried or eroded outflow channel flowed across this region. Exobiology?
Observation: Extensive region of fine scale layered, friable, stripped
material. This unit is currently being
stripped off the underlying rougher plains unit (volcanic or flood deposit?).
Ground Ice
Observation: rootless cones, patterned ground.
ATHABASCA VALLES:
WHAT ATHENA CAN do
1.
Observe morphology and stratigraphy of large and small scale landforms
2.
Spatial distribution of rocks and soils
3.
Textures and structures of rocks and soils
Results:
1. The above observations and
measurements will aid in determining if MER is on fluvial, lacustrine,
hydrothermal, or volcanic terrain based on morphology, grain size, shape,
sorting, cements and sedimentary structures such as bedding, imbrication,
ripple marks, and veins, and distribution and texture of rocks and soils.
2. Extract
clues from the geologic investigation, related to the environmental conditions
when liquid water was present and assess whether those environments were
conducive for life.
3. Calibrate and validate orbital remote sensing data and assess the amount and scale of heterogeneity at each landing site and put them in geologic context.
ATHABASCA VALLES:
WHAT ATHENA CAN do
Instrument(s):
Mini-TES, APXS, Mössbauer, Pancam, RAT
1.
Mineral identification and abundance determination
(carbonates,clays,oxides,silicates)
2. Iron-bearing mineralogy of rocks and soils and iron oxidation state
3. Detailed
analyses of selected rocks and soils to determine their elemental composition
Results:
1. Determine
rock and soil mineralogy, specifically identify water-bearing minerals and
minerals deposited by precipitation, evaporation, sedimentary cementation, or
hydrothermal activity.
2. Extract clues from the geologic investigation, related to the environmental conditions when liquid water was present and assess whether those environments were conducive for life.
3. Calibrate and validate orbital remote sensing data and assess the amount and scale of heterogeneity at each landing site and put them in geologic context.