Deltaic sediments on Mars

Post by Dr. Bethany Ehlmann

The Nili Fossae region of Mars has a diversity of minerals that include mafics and phyllosilicates. The mineral assemblage suggests widespread liquid water activity and a variety of alteration processes from surface weathering to hydrothermal processes (Mangold et al., 2007).

Nili Fossae, Mars

Image 1: CRISM infrared spectrometer data (wavelengths: 2.38 um (red), 1.80 um (green), 1.15 um (blue) acquired at 35 m/pixel have been used to colorize a Context Imager grayscale image, taken at 5 m/pixel resolution.

This region also boasts sapping channels and well-developed valley networks. Studies of these landforms suggest regional fluvial activity extending from the Noachian to the early Hesperian epochs (i.e. 3.96 to 3 Ga). The most well-developed valley system in this region is a network of tributaries that feed into and breach the Jezero crater rim. They create spectacular bedded sediments on the crater floor, most likely laid down in a crater lake (Fassett and Head, 2005). The western delta is particularly well preserved and is shown in Image 1 using data from the Mars Reconnaisance Orbiter .

Nili Fossae, Mars

Image 2: Mars Orbiter Laser Altimeter elevation map (Green=higher elevations, blue=lower elevations) of the Jezero crater watershed. Below a THEMIS Daytime infra-red image with clay detections from the OMEGA spectrometer on Mars Express overlain (Poulet et al., 2005). The tributaries feeding the main valleys (highlighted in blue) pass through clay-rich rock units.

The color data of the Compact Reconnaissance Imaging Spectrometer (CRISM) highlights the diverse mineralogy within the crater (Image 1). The crater walls (blue) are pyroxene-bearing while the uppermost surface of the delta and crater fill (purple) are mafic in composition. Olivine sands (yellow) fill in depressions in the crater and are blown in from the regional olivine deposits which are the largest on Mars (Hoefen et al., 2003; Hamilton and Christensen, 2005). While the crater and uppermost surfaces are mostly composed of primary igneous minerals, the bulk of the delta deposit and underlying crater fill is light-toned sediments, which are rich in iron-magnesium smectite clay (green) (Ehlmann et al., 2008). This is one of the few instances on Mars where geomorphic evidence of water and evidence for aqueous chemical alteration are found in the same place. It is likely that these clays were transported into Jezero crater as suspended sediments or bedload, sourced from the clay-rich rocks in the Nili Fossae region (Image 2; Mangold et al., 2007; Ehlmann et al., 2008).

Nili Fossae, Mars

Image 3: HiRISE camera images of epsilon cross-beds exposed in the wall of a crater, impacted into the delta. In plan view, meander loops are common in exposed light-toned sediments beneath the rocky cap unit.

High resolution data from the HiRISE camera (0.25 m/pixel) contain evidence of migrating distributary channels, which indicate that a significant portion of the delta plain sediment was deposited via lateral accretion (Ehlmann et al., 2008). Scroll bars in meander loops and epsilon cross-bedding provide evidence for the migration of distributory channels across the fan surface (Image 3). Discontinuous mesas with the same stratigraphic sequence as on the delta are found near the delta, and indicate that the delta was once more extensive and has subsequently eroded back, forming the over-steepened delta front that is observed in high resolution images.

Further Reading:

Ehlmann, B.L. et al. 2008. Clay minerals in delta deposits and organic preservation potential on Mars. Nature Geoscience 1, 355-358. [Abstract]

Fassett, C.I. and Head, J.W. 2005. Fluvial sedimentary deposits on Mars: Ancient deltas in a crater lake in the Nili Fossae region. Geophysical Research Letters 32, L14201, doi:10.1029/2005GL023456. [Abstract]

Hamilton, V.E, and Christensen, P. R. 2005. Evidence for extensive, olivine-rich bedrock on Mars. Geology 33, 433-436. [Abstract]

Hoefen, T.M., et al. 2003. Discovery of Olivine in the Nili Fossae Region of Mars. Science 302, 627-630. [Abstract]

Mangold, N., et al. 2007. Mineralogy of the Nili Fossae region with OMEGA/Mars Express data: 2. Aqueous alteration of the crust, J. Geophys. Res. 112, E08S04, doi:10.1029/2006JE002835. [Abstract]

Poulet, F. et al. 2005. Phyllosilicates on Mars and implications for early martian climate. Nature 438, 623-627. [Abstract]

Advertisements
Leave a comment

Leave a Reply

Fill in your details below or click an icon to log in:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out / Change )

Twitter picture

You are commenting using your Twitter account. Log Out / Change )

Facebook photo

You are commenting using your Facebook account. Log Out / Change )

Google+ photo

You are commenting using your Google+ account. Log Out / Change )

Connecting to %s

  • Enter your email address to follow this blog and receive notifications of new posts by email.

  • Blog Stats

    • 69,073 hits
  • Io

  • Mercury Tectonics

%d bloggers like this: