J. Urrutiafucugauchi et al., UNAM SCIENTIFIC DRILLING PROGRAM OF CHICXULUB IMPACT STRUCTURE - EVIDENCE FOR A 300 KILOMETER CRATER DIAMETER, Geophysical research letters, 23(13), 1996, pp. 1565-1568
As part of the UNAM drilling program at the Chicxulub structure, two 7
00 m deep continuously cored boreholes were completed between April an
d July, 1995. The Peto UNAM-6 and Tekax UNAM-7 drilling sites are simi
lar to 150 km and 125 km, respectively, SSE of Chicxulub Puerto, near
the crater's center. Core samples from both sites show a sequence of p
ost-crater carbonates on top of a thick impact breccia pile covering t
he disturbed Mesozoic platform rocks. At UNAM-7, two;impact breccia un
its were encountered: (1) an upper breccia, mean magnetic susceptibili
ty is high (similar to 55 x 10(-6) SI units), indicating a large compo
nent of silicate basement has been incorporated into this breccia, and
(2) an evaporite-rich, low susceptibility impact breccia similar in c
haracter to the evaporite-rich breccias observed at the PEMEX drill si
tes further out. The upper breccia was encountered at similar to 226 m
below the surface and is similar to 125 m thick; the lower breccia is
immediately subjacent and is >240 m thick. This two-breccia sequence
is typical of the suevite-Bunte breccia sequence found within other we
ll preserved impact craters. The suevitic upper unit is not present at
UNAM-6. Instead, a >240 m thick evaporite-rich breccia unit, similar
to the lower breccia at UNAM-7, was encountered at a depth of similar
to 280 m. The absence of an upper breccia equivalent at UNAM-6 suggest
s some portion of the breccia sequence has been removed by erosion. Th
is is consistent with interpretations that place the high-standing cra
ter rim at 130-150 km from the center. Consequently, the stratigraphic
observations and magnetic susceptibility records on the upper and low
er breccias (depth and thickness) support a similar to 300 km diameter
crater model.