Geosphere; December 2006; v. 2; no. 7;
p. 324-332; DOI: 10.1130/GES00051.1
© 2006 Geological Society of America
Iron isotopes constrain the pathways and formation mechanisms of terrestrial oxide concretions: A tool for tracing iron cycling on Mars?
Marjorie A. Chan*1,
Clark M. Johnson*2,
Brian L. Beard*2,
John R. Bowman*3 and
W.T. Parry*3
1 Department of Geology & Geophysics, University of Utah, 719 WBB, 135 S. 1460 E., Salt Lake City, Utah 84112, USA
2 Department of Geology and Geophysics, University of Wisconsin, 1215 W. Dayton St., Madison, Wisconsin 53706, USA
3 Department of Geology & Geophysics, University of Utah, 719 WBB, 135 S. 1460 E., Salt Lake City, Utah 84112, USA

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Figure 2. Localities of Jurassic sampling for Fe isotope analyses: 1—Snow Canyon, 2—Sand Hollow, 3—Zion National Park, 4—Cedar City, 5–10—Grand Staircase Escalante National Monument, 11–13—Lake Powell area, and 14–18—Moab area. All samples are from the Lower Jurassic Navajo Sandstone (Ss) except for localities 12 and 17, which are from the Middle Jurassic Entrada Sandstone. Generalized stratigraphic column is at left (modified after Chan et al., 2005).
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