Title:
Isotope provinces in Laramide and mid-Tertiary igneous rocks of northwestern Mexico (Chihuahua and Sonora) and their relation to basement configuration 
Reference Number:
2003 
ISSN:
0072-1077
Publication Year:
2005
Book Editors:
Anderson, Thomas H; Nourse, Jonathan A; McKee, James W; Steiner, Maureen B
GeoREF Number:
2006-010959 (View Original Data File)
Authors:
Housh, Todd B; McDowell, Fred W
Descriptors:
absolute age; alkaline earth metals; Arizona; basement; Cenozoic; Chihuahua Mexico; Cretaceous; dates; deformation; faults; geochemistry; Grenvillian Orogeny; igneous rocks; intrusions; isotope fractionation; isotope ratios; isotopes; Jurassic; K/Ar; Laramide Orogeny; lead; magma contamination; magmatism; Mesozoic; metals; Mexico; Mojave-Sonora Megashear; Nd-144/Nd-143; neodymium; Oligocene; orogeny; Paleogene; Pb-206/Pb-204; Precambrian; Proterozoic; radioactive isotopes; rare earths; Rb/Sr; shear zones; Sierra Madre Occidental; Sonora Mexico; Sr-87/Sr-86; stable isotopes; strontium; systems; tectonics; Tertiary; Texas; U/Pb; United States; Upper Cretaceous; upper Precambrian
Source:
Special Paper - Geological Society of America, vol.393, pp.671-692, 2005
Abstract:
We have identified five distinct isotope provinces in northwestern Mexico in a study of the Sr, Nd, and Pb isotope geochemistry of Laramide and mid-Tertiary igneous rocks in Sonora and Chihuahua as well as adjacent portions of southwestern United States. Province A, in northern Sonora, is characterized by very unradiogenic Nd and Pb isotopic compositions and radiogenic Sr isotopic compositions. Unradiogenic Nd and radiogenic Sr and Pb isotopic compositions characterize Province B, in central Sonora. Provinces A and B are flanked to the east and south by Provinces C, D, and E, which are characterized by more radiogenic Nd and less radiogenic Sr isotopic compositions than observed in Provinces A and B. Rocks from Provinces C, D, and E have similar Sr and Nd isotopic compositions, although the variation observed in rocks from Province E is more restricted than in Provinces C and D. These provinces are unique, however, in their Pb isotopic compositions; rocks from Province C are the least radiogenic whereas those from Province E are the most radiogenic. The identified isotope provinces correlate well with the constraints imposed by the geology of the southwestern United States and northwestern Mexico. The primary factor controlling the geographic distribution of isotope provinces in northwestern Mexico appears to be the age of the crust that the magmas passed through and with which they interacted. Provinces A and B are interpreted to reflect the area underlain by old, early Proterozoic basement in northwestern Sonora; the significance of the difference in Pb isotopic compositions between rocks in Provinces A and B is not clear. We interpret Province C, located in northern Chihuahua and adjacent regions of Texas, to reflect the distribution of mid-Proterozoic crust of the North American craton that has been overprinted by Grenvillian deformation. Province D is located in a belt running from central Chihuahua into southwestern Texas and is interpreted to reflect the distribution of exotic crust that was accreted to the southern margin of the North American craton during Ouachita convergence; this crustal block consists of a Paleozoic arc sequence developed on Proterozoic basement. Lastly, we interpret Province E, located in southern Sonora and Chihuahua, as exotic Jurassic-Cretaceous arc crust accreted during the late Mesozoic. The observed distribution of isotope provinces in northwestern Mexico is not consistent with the Mojave-Sonora megashear hypothesis. In particular, the NNE-trending eastern boundary of the two western isotope provinces (Provinces A and B) does not show the 700-800 km of left-lateral offset that would be expected if this boundary was intersected by the Mojave-Sonora megashear.
Copyright:
GeoRef, Copyright 2006, American Geological Institute.

Sample Summary:
Sample ID: Major Data: Trace Data: Isotope Data:
3--25--3 No No Yes
C1 No No Yes
C2 No No Yes
11--14--1 No No Yes
MA-1 No No Yes
3--21--2 No No Yes
SAD-6 No No Yes
CM-38 No No Yes
CM-636 No No Yes
SGD 2 No No Yes
SGD 5 No No Yes
SGC 4 No No Yes
SGC 5 No No Yes
SGD 6 No No Yes
SGD 12 No No Yes
CM-44 No No Yes
MEX-3 No No Yes
CH97-3 No No Yes
CH97-5 No No Yes
CH97-6 No No Yes
CH97-9 No No Yes
CH97-11 No No Yes
CH97-11d No No Yes
CH97-12 No No Yes
CH97-13 No No Yes
CH97-14 No No Yes
CH97-15 No No Yes
CH97-16 No No Yes
CH97-17 No No Yes
CH97-18 No No Yes
CH97-20 No No Yes
CH97-21 No No Yes
M21 No No Yes
M28 No No Yes
M35 No No Yes
M38 No No Yes
M48 No No Yes
M51 No No Yes
M53 No No Yes
M56 No No Yes
M58 No No Yes
M60 No No Yes
M61 No No Yes
C-16 No No Yes
D75A No No Yes
I521 No No Yes
Per No No Yes
J369 No No Yes
W 200 No No Yes
W 300 No No Yes
DZ 31 No No Yes
PLM No No Yes
I 532 No No Yes
RND No No Yes
C10 No No Yes
D70D No No Yes
D76A No No Yes
D53D No No Yes
W176 No No Yes
I133 No No Yes
PC-1 No No Yes
ECD No No Yes
4RSRB No No Yes
SO 106 No No Yes
SO 35 No No Yes
SO 15 No No Yes
SO 2 No No Yes
SO 7 No No Yes
SO 8 No No Yes
SO 26 No No Yes
SO 64 No No Yes
SO 3 No No Yes
SO 5 No No Yes
SO 14 No No Yes
SO 25 No No Yes
SO 28 No No Yes
SO 40 No No Yes
SO 41 No No Yes
SO 48 No No Yes
SO 60 No No Yes
SO 63 No No Yes
CH98-2d No No Yes
CH98-3 No No Yes
CH98-5d No No Yes
CH98-5 No No Yes
CH98-6 No No Yes
CH98-7d No No Yes
CH98-7 No No Yes
CH98-8 No No Yes
CH98-10 No No Yes
CH98-11d No No Yes
CH98-11 No No Yes
CH98-17d No No Yes
CH98-17 No No Yes