Using Gauss’s theorem, we estimated the mass deficiencies of the Chicxulub impact structure (Yucatan, Mexico) from its gravity anomaly. The mass deficiency obtained from the residual gravity anomaly map ranges between 1.06 × 1016 and 1.67 × 1016 kg. Because the gravity anomaly has approximately radial symmetry, we also estimated the mass deficiency from selected profiles. In this way, we obtained slightly lower mass deficiency (6.16 × 1015 to 1.35 × 1016 kg). The central gravity high, which is supposed to be associated with the central structural high, has a mean excess mass of 1.93 × 1014 kg. By assuming a mean density contrast of 100 kg/m3 between the country rock and the sedimentary and brecciated rocks, we estimated the equivalent total mass (1.60 × 1017 to 4.34 × 1017 kg) and volume (6.16 × 1013 to 1.67 × 1014 m3) of breccias and sedimentary rocks responsible for the gravity anomaly. These figures represent lower bounds on the mass and volume ejected from the impact crater. They represent estimates made from geophysical principles and data, and compare well with independent estimates based on other principles such as scaling relations. According to actual estimations of the sulfur dioxide mass generated by the Cretaceous‐Tertiary impact and our results, only a small fraction (about 1%) of the anhydrite in the target strata was vaporized.

No abstract