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Figure 5. (A) The Chicxulub peak ring in 83-mm-diameter core is composed of granitic rocks, crosscut with cataclastic and hydrothermal veins, that
have also been shock-metamorphosed, as illustrated with planar deformation features with ~5 micron spacing in quartz (inset, with field of view 245
microns wide). Photomicrograph of quartz by expedition scientist Ludovic Ferrière. (B) Granitic basement (pink) was uplifted and then collapsed out-
ward over the pre-impact crust (yellow). The portion of the peak ring sampled in the core also contains shock-metamorphosed (blue) and melted (red)
components, which are consistent with a numerical model of dynamic collapse of a central uplift during the crater-forming event (Morgan et al., 2016).
While the numerical model treats the basement as a uniform unit of granite, which is the rock type that dominates the new IODP-ICDP core, the base-
ment also contains metaquartzite, mica schist, granitic gneiss, gneiss, amphibolite, dolerite dikes, dacite, felsite, and granodiorite (Kring, 2005;
Gulick et al., 2017).

Confidence in the dynamic collapse            CONCLUSIONS                                       (Mexico); M. Whalen (U.S.); A. Wittmann (U.S.);
model, finally tested with core samples,                                                        L. Xiao (China); K.E. Yamaguchi (Japan); and
has grown substantially.                        New IODP-ICDP borehole data indicate            W. Zylberman (France). The European
                                              that the peak-ring morphology of the              Consortium for Ocean Research Drilling
  The Chicxulub peak ring had an eleva-       Chicxulub crater was produced by the              (ECORD) implemented Expedition 364 with
tion below that of the crater rim. As         dynamic collapse of an uplifted central           contributions and logistical support from the
inferred from analogy with the                peak. Additional exciting expedition              Yucatán state government and Universidad
Schrödinger basin peak ring, and inferred     results are forthcoming. The impact gener-        Nacional Autónoma de México (UNAM). We
from seismic reflection data, the peak ring   ated an environmental calamity that extin-        thank Wright Horton and Christian Koeberl for
had a topographically complex surface.        guished life. It also induced a vast sub-         helpful reviews.
There were highs subject to erosion and       surface hydrothermal system that altered a
lows suitable for near-continuous sedimen-    portion of the Maya Block and serves as a         REFERENCES CITED
tation. Initial results suggest M0077A is     proxy for much larger and more frequently
located in a protected catchment with a       generated hydrothermal systems during             Claeys, P., Heuschkel, S., Lounejeva-Baturina, E.,
rich post-impact sedimentary and paleon-      the Hadean, when bombardment rates                   Sanchez-Rubio, G., and Stöffler, D., 2003, The
tologic record. The expedition members        were high. And, finally, the crater became           suevite of the Chicxulub impact crater:
are currently studying the sedimentation      an oasis for the recovery of life and                Meteoritics & Planetary Science, v. 38, p. 1299–
and biological processes that immediately     allowed expansion into momentarily                   1317, doi:10.1111/j.1945-5100.2003.tb00315.x.
followed the impact event, the nature of      vacant niches that, when filled, defined the
the sea that filled the basin, the chemical   modern world.                                     Collins, G.S., Melosh, H.J., Morgan, J.V., and
evolution of those waters as they were                                                             Warner, M.R., 2002, Hydrocode simulations of
affected by a venting impact-generated        ACKNOWLEDGMENTS                                      Chicxulub Crater collapse and peak-ring
hydrothermal system, and mixing with sea                                                           formation: Icarus, v. 157, p. 24–33, doi:10.1006/
water from outside the basin, up to and          The IODP-ICDP Expedition 364 Science Party        icar.2002.6822.
including sediments associated with the       is composed of co-authors S. Gulick (U.S.); J.V.
Paleocene-Eocene Thermal Maximum.             Morgan (UK); T. Bralower (U.S.); E. Chenot        Collins, G.S., Morgan, J.V., Barton, P., Christeson,
The underlying peak-ring basement sam-        (France); G. Christeson (U.S.); Ph. Claeys           G.L., Gulick, S., Urrutia-Fucugauchi, J., Warner,
ples of the Yucatán Peninsula will, in addi-  (Belgium); C. Cockell (UK); M.J.L. Coolen            M.R., and Wünnemann, K., 2008, Dynamic
tion to our evaluation of impact, be useful   (Australia); L. Ferrière (Austria); C. Gebhardt      modeling suggests terrace zone asymmetry in the
for assessing the tectonic evolution of the   (Germany); K. Goto (Japan); H. Jones (U.S.);         Chicxulub crater is caused by target
Maya Block and its assembly along the         D.A. Kring (U.S.); J. Lofi (France); C. Lowery       heterogeneity: Earth and Planetary Science
margins of both the Caribbean and Gulf of     (U.S.); C. Mellett (UK); R. Ocampo-Torres            Letters, v. 270, p. 221–230, doi:10.1016/j.epsl
Mexico basins. Measuring the ages of          (France); L. Perez-Cruz (Mexico); A. Pickersgill     .2008.03.032.
intrusive components within the core will     (UK); M. Poelchau (Germany); A. Rae (UK); C.
better refine those processes.                Rasmussen (U.S.); M. Rebolledo-Vieyra             Cornejo Toledo, A., and Hernandez Osuna, A.,
                                              (Mexico); U. Riller (Germany); H. Sato (Japan);      1950, Las anomalias gravimetricas en la cuenca
                                              J. Smit (Netherlands); S. Tikoo (U.S.); N.           salina del istmo, planicie costera de Tabasco,
                                              Tomioka (Japan); J. Urrutia-Fucugauchi               Campeche y Peninsula de Yucatán: Boletín de la
                                                                                                   Asociación Mexicana de Geólogos Petroleros,
                                                                                                   v. 2, p. 453–460.

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                                                                                                   impact structures, based on terrestrial data, in
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                                              www.geosociety.org/gsatoday                                                                               7
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