I. Publications
Papers
McEwen,
A., C.
Hansen, A. Delamere, E. Eliason, K. Herkenhoff, L. Keszthelyi, V. Gulick, R.
Kirk, M. Mellon, J. Grant, N. Thomas, C. Weitz, S. Squyres, N.
Bridges, S. Murchie, F. Seelos, K. Seelos, C. Okubo, M. Milazzo, L. Tornabene,
W. Jaeger, S. Byrne, P. Russell, J. Griffes, S. Martinez-Alonso, A. Devatzes,
F. Chuang, B. Thomson, K. Fishbaugh, C. Dundas, K. Kolb, M. Banks, J. Wray, A
closer look at water-related geologic activity on Mars, Science, 317, 1706-1709, 2007.
Minitti, M. E., C. M. Weitz, M. D. Lane and J. L.
Bishop, Morphology, Chemistry and Spectral Properties of Hawaiian Rock Coatings
and Implications for Mars, J. Geophys. Res., 112, E05015, doi:10.1029/2006JE002839,
2007.
McEwen, A.S., E.M. Eliason, J.W.
Bergstrom, N.T. Bridges, C.J. Hansen, W. A. Delamere, J.A. Grant, V.C. Gulick,
K.E. Herkenhoff, L/ Keszthelyi, R.L. Kirk, M.T. Mellon, S.W. Squyres, N.
Thomas, and C.M. Weitz, Mars Reconnaissance OrbiterŐs High Resolution Imaging
Science Experiment (HiRISE), J. Geophys. Res., 112, E05S02,
doi:10.1029/2005JE002605, 2007.
Abstracts
Weitz, C.M., A.S. McEwen, R.E.
Milliken, J.A. Grant, and the HiRISE team, MRO observations of light-toned layered deposits along
the plains adjacent to Valles Marineris, Fall AGU, 2007.
Weitz,
C.M., A. S. McEwen, and
the HiRISE team, HiRISE
observations of layered deposits in and around Valles Marineris, Spring AGU, Acapulco, 2007.
Beyer,
R.A., C. M. Weitz, B. J. Thompson,
J. M. Moore, A. S. McEwen, and the HiRISE team, HiRISE observations of Valles
Marineris layering, 7th International Conference on Mars, Abstract 3310, 2007.
L.H.
Roach, J.F. Mustard, S.L. Murchie, J.L. Bishop, C.M. Weitz, A.T. Knudson, J.P. Bibring, S.M. Pelkey, B.L.
Ehlmann, and the CRISM team, Magnesium and iron sulfate variety and
distribution in East Candor and Capri Chasma, Valles Marineris, 7th
International Conference on Mars, Abstract 3223, 2007.
Knudson,
A.T., R.E. Arvidson, P.R. Christensen, S.L. Murchie, J.F. Mustard, L.H. Roach, C.M.
Weitz, S.M. Wiseman,
and the CRISM team, Aqueous geology in Valles Marineris: New insights in the
relationship of hematite and sulfates from CRISM and HiRISE, 7th
International Conference on Mars, Abstract 3370, 2007.
Weitz,
C. M., A. S. McEwen, C.
H. Okubo, P. Russell, J. A. Grant, C. Dundas, N. Bridges, and the HiRISE team,
Early HiRISE observations of light-toned layered deposits, In Lunar and
Planetary Science XXXVIII,
Abstract 1442, Lunar and Planetary Institute, Houston (CD-ROM), 2007.
II. Ongoing research
(A) Weitz is a
Co-Investigator on the HiRISE camera that is now orbiting around Mars on the
MRO spacecraft. HiRISE is taking images at the highest resolution of any camera
around Mars, with 30 cm/pixel resolution. Weitz is interested in the
light-toned layered rocks on Mars and has been using the HiRISE images to
explore the morphologies and origins for these deposits (Figure 1). She is also
busy targeting the camera and prioritizing targets entered by anyone on
sedimentary and layered deposits.

Figure 1. Portion of HiRISE
false-color image showing layering along the plains adjacent to Juventae
Chasma, Mars.
(B) Weitz has continued her
work in support of a Mars Data Analysis Program grants where she is the PI. Her
work on Valles Marineris is now focusing on small areas in Valles Marineris
where the Thermal Emission Spectrometer (TES) has identified gray hematite
(Figure 2). She has completed a plublication with other PSI scientists Melissa
Lane, Mathew Staid, and Eldar Noe on the hematite-bearing units within Ophir
and Candor Chasmata. Our conclusions from this research are that the hematite
is concentrated in lag deposits in a similar manner to what has been seen at
the Opportunity landing site in Meridiani Planum. The team hopes to continue
these studies on other hematite regions in eastern Valles Marineris.

Figure 2. Portion of HRSC image that shows the TES-derived
hematite abundance in Ophir Chasma. Colors indicate different abundances of
gray hematite with red and yellows higher abundances than blues and green. The
hematite correlates strongly to dark debris concentrated in a topographic basin
within Ophir Chasma.