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The Wyoming Craton
is no longer a craton
Part I
Suzan van der Lee
1997:
2005:
IRIS EMC
IRIS EMC
IRIS EMC
IRIS EMC
IRIS EMC
Wyoming, Part II
Heather Bedle and Suzan van der Lee
Bedle & Van der Lee,
includes early USArray
data from W US,
unpublished
Bedle & Van der Lee, unpublished
Bedle & Van der Lee, unpublished
Wyoming, Part III
Trevor Bollmann
Brad Sageman, Craig Jones
Suzan van der Lee
Motivation
• Overriding plate can flex and form foredeep.
• WIB is a textbook flexural basin until it widens
excessively.
• Flat Farallon “sucked” down a wide section of
overriding plate (WIB).
Questions
• Does WIB widening coincide with a change in the pattern of
volcanism?
• Does the crustal material beneath the basins have an effect
on the depth/width of the WIB?
• Did the point of maximum subsidence stay constant or
move with the Farallon plate over time?
1. Was the flat Farallon slab beneath the WIB during its
widening?
2. Was a particular oceanic plateau beneath Wyoming when
the WIB widened?
 Model sub-WIB slab fragments forwards in time and
compare to tomography.
 Model tomography backwards in time to find segment
placement in late Cretaceous
Cenomanian Turonian Coniacian-Santonian
Campanian I Campanian
II
Maastrichtian
Sedimentation vs. Pattern of Volcanism
WIB:
Cumulative depocenters not significantly
different from era depocenters.
Shatsky Rise Conjugate
(SRC)
Hess Rise Conjugate
(HRC)
Backwards
modeling
SRC tracks with Flat
Slab box
SRC tracks with
Oceanic Plateau box
SRC
Add shapes of
flat slab
segment
or
oceanic
plateau
HRC tracks with Flat
Slab box
HRC tracks with
Oceanic Plateau box
SRC
Add shapes of
flat slab
segment
or
oceanic
plateau
Turonian Slab Locations with Isopach
Flat Slab Oceanic Plateau
Coniacian-Santonian Slab Locations with Isopach
Flat Slab Oceanic Plateau
Campanian I Slab Locations with Isopach
Flat Slab Oceanic Plateau
Campanian II Slab Locations with Isopach
Flat Slab Oceanic Plateau
Maastrictian Slab Locations with Isopach
Flat Slab Oceanic Plateau
Campanian I Depo-center
80 m.y.a
Campanian II Depo-center
75 m.y.a
Point of Maximum Deposition
in Campanian I
Point of Maximum Deposition
in Campanian I
Forwards
modeling
Campanian I Depo-center
Campanian II Depo-center
Forwards
modeling
−125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚
25˚
30˚
35˚
40˚
45˚
50˚
−125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚
25˚
30˚
35˚
40˚
45˚
50˚
6.48
6.52
6.56
6.60
s(km/s)
S362ANI+M (Vs km/s) - 1200 km depth
*This model is in velocity, not velocity difference from
the background model like the previous examples.
Location of
modeled slab
−125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚
25˚
30˚
35˚
40˚
45˚
50˚
−125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚
25˚
30˚
35˚
40˚
45˚
50˚
−1.5
−1.0
−0.5
0.0
0.5
1.0
1.5
Vs%
GYPSUM (dVs %) - 1200 km depth
Location of
modeled slab
Conclusions
• The point of maximum subsidence and deposition
did not move significantly during the late
Cretaceous.
• There are slab fragments that were beneath the
basin at the right time to interact with the crust and
deepen the basin.
– The Seton et al. 2012 model is a better fit to the basins in
the isopach
– A Flat Slab window sized slab seems to be a better spatial
match to the isopachs
• Flat-slab fragments would have been effective at
hydrating/metasomatizing the Wyoming lithosphere
from below.
Further Work Needed (From others)
• Recreate the regional isopachs using all available
data
– The last were completed 20 years ago
• 3-D crustal flexural modeling
– Some 2-D modeling has been completed but 3-D with
crustal properties from different provinces could be
useful
• Plotting the reconstructed slab locations on a
palinspastic reconstruction of North America
– Would change the locations shown earlier. How much
is unclear.
References for workshop
• Bedle, PhD thesis
• Carlson 2014
• P. V. Doubrovine, B. Steinberger, and T. H. Torsvik. Absolute plate motions in a reference
frame defined by moving hot spots in the Pacific, Atlantic, and Indian oceans. Journal of
Geophysical Research: Solid Earth, 117(B9), 2012.
• R. Dietmar Müller, J.-Y. Royer, and L. A. Lawver. Revised plate motions relative to the hotspots
from combined atlantic and indian ocean hotspot tracks. Geology, 21:275, 1993.
• Hoffmann 1988
• Kirschbaum and Rogers
• Porter et al.
• M. Seton, R. Müller, S. Zahirovic, C. Gaina, T. Torsvik, G. Shephard, A. Talsma, M. Gurnis, M.
Turner, S. Maus, et al. Global continental and ocean basin reconstructions since 200Ma.
Earth-Science Reviews, 113(3):212–270, 2012.
• VdLee and Nolet JGR 1997
• Gypsum
• Sigloch? (Shatsky Rise?)

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Suzan VDZ WYCnWIB_sanitized.pptx

  • 1. The Wyoming Craton is no longer a craton Part I Suzan van der Lee
  • 8. Wyoming, Part II Heather Bedle and Suzan van der Lee
  • 9. Bedle & Van der Lee, includes early USArray data from W US, unpublished
  • 10. Bedle & Van der Lee, unpublished
  • 11. Bedle & Van der Lee, unpublished
  • 12. Wyoming, Part III Trevor Bollmann Brad Sageman, Craig Jones Suzan van der Lee
  • 13. Motivation • Overriding plate can flex and form foredeep. • WIB is a textbook flexural basin until it widens excessively. • Flat Farallon “sucked” down a wide section of overriding plate (WIB).
  • 14. Questions • Does WIB widening coincide with a change in the pattern of volcanism? • Does the crustal material beneath the basins have an effect on the depth/width of the WIB? • Did the point of maximum subsidence stay constant or move with the Farallon plate over time? 1. Was the flat Farallon slab beneath the WIB during its widening? 2. Was a particular oceanic plateau beneath Wyoming when the WIB widened?  Model sub-WIB slab fragments forwards in time and compare to tomography.  Model tomography backwards in time to find segment placement in late Cretaceous
  • 15. Cenomanian Turonian Coniacian-Santonian Campanian I Campanian II Maastrichtian Sedimentation vs. Pattern of Volcanism
  • 16. WIB: Cumulative depocenters not significantly different from era depocenters.
  • 17. Shatsky Rise Conjugate (SRC) Hess Rise Conjugate (HRC) Backwards modeling
  • 18. SRC tracks with Flat Slab box SRC tracks with Oceanic Plateau box SRC Add shapes of flat slab segment or oceanic plateau
  • 19. HRC tracks with Flat Slab box HRC tracks with Oceanic Plateau box SRC Add shapes of flat slab segment or oceanic plateau
  • 20. Turonian Slab Locations with Isopach Flat Slab Oceanic Plateau
  • 21. Coniacian-Santonian Slab Locations with Isopach Flat Slab Oceanic Plateau
  • 22. Campanian I Slab Locations with Isopach Flat Slab Oceanic Plateau
  • 23. Campanian II Slab Locations with Isopach Flat Slab Oceanic Plateau
  • 24. Maastrictian Slab Locations with Isopach Flat Slab Oceanic Plateau
  • 25. Campanian I Depo-center 80 m.y.a Campanian II Depo-center 75 m.y.a Point of Maximum Deposition in Campanian I Point of Maximum Deposition in Campanian I Forwards modeling
  • 26. Campanian I Depo-center Campanian II Depo-center Forwards modeling
  • 27. −125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚ 25˚ 30˚ 35˚ 40˚ 45˚ 50˚ −125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚ 25˚ 30˚ 35˚ 40˚ 45˚ 50˚ 6.48 6.52 6.56 6.60 s(km/s) S362ANI+M (Vs km/s) - 1200 km depth *This model is in velocity, not velocity difference from the background model like the previous examples. Location of modeled slab
  • 28. −125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚ 25˚ 30˚ 35˚ 40˚ 45˚ 50˚ −125˚ −120˚ −115˚ −110˚ −105˚ −100˚ −95˚ −90˚ −85˚ −80˚ −75˚ −70˚ 25˚ 30˚ 35˚ 40˚ 45˚ 50˚ −1.5 −1.0 −0.5 0.0 0.5 1.0 1.5 Vs% GYPSUM (dVs %) - 1200 km depth Location of modeled slab
  • 29. Conclusions • The point of maximum subsidence and deposition did not move significantly during the late Cretaceous. • There are slab fragments that were beneath the basin at the right time to interact with the crust and deepen the basin. – The Seton et al. 2012 model is a better fit to the basins in the isopach – A Flat Slab window sized slab seems to be a better spatial match to the isopachs • Flat-slab fragments would have been effective at hydrating/metasomatizing the Wyoming lithosphere from below.
  • 30. Further Work Needed (From others) • Recreate the regional isopachs using all available data – The last were completed 20 years ago • 3-D crustal flexural modeling – Some 2-D modeling has been completed but 3-D with crustal properties from different provinces could be useful • Plotting the reconstructed slab locations on a palinspastic reconstruction of North America – Would change the locations shown earlier. How much is unclear.
  • 31. References for workshop • Bedle, PhD thesis • Carlson 2014 • P. V. Doubrovine, B. Steinberger, and T. H. Torsvik. Absolute plate motions in a reference frame defined by moving hot spots in the Pacific, Atlantic, and Indian oceans. Journal of Geophysical Research: Solid Earth, 117(B9), 2012. • R. Dietmar Müller, J.-Y. Royer, and L. A. Lawver. Revised plate motions relative to the hotspots from combined atlantic and indian ocean hotspot tracks. Geology, 21:275, 1993. • Hoffmann 1988 • Kirschbaum and Rogers • Porter et al. • M. Seton, R. Müller, S. Zahirovic, C. Gaina, T. Torsvik, G. Shephard, A. Talsma, M. Gurnis, M. Turner, S. Maus, et al. Global continental and ocean basin reconstructions since 200Ma. Earth-Science Reviews, 113(3):212–270, 2012. • VdLee and Nolet JGR 1997 • Gypsum • Sigloch? (Shatsky Rise?)

Editor's Notes

  1. Craton = lithosphere with long-term stability
  2. Green circles: volcanism within the time period Blue dashed line: Sevier front (line of zero sedimentation)
  3. Replaces hidden slide 15