Morphology and population of binary asteroid impact cratersFrom the pop sci write up I found:
1. Katarina Miljković (a)
2. Gareth S. Collins (a)
3. Sahil Mannick (a)
4. Philip A. Bland (b)
a. Department of Earth Sciences and Engineering, Imperial College London, South Kensington Campus, SW7 2AZ London, United Kingdom
b. Department of Applied Geology, Curtin University, GPO Box U1987, Perth, WA 6845, Australia
Observational data show that in the Near Earth Asteroid (NEA) region 15% of asteroids are binary. However, the observed number of plausible doublet craters is 2–4% on Earth and 2–3% on Mars. This discrepancy between the percentage of binary asteroids and doublets on Earth and Mars may imply that not all binary systems form a clearly distinguishable doublet crater owing to insufficient separation between the binary components at the point of impact. We simulate the crater morphology formed in close binary asteroid impacts in a planetary environment and the range of possible crater morphologies includes: single (circular or elliptical) craters, overlapping (tear-drop or peanut shaped) craters, as well as clearly distinct, doublet craters. While the majority of binary asteroids impacting Earth or Mars should form a single, circular crater, about one in four are expected to form elongated or overlapping impact craters and one in six are expected to be doublets. This implies that doublets are formed in approximately 2% of all asteroid impacts on Earth and that elongated or overlapping binary impact craters are under-represented in the terrestrial crater record. The classification of a complete range of binary asteroid impact crater structures provides a template for binary asteroid impact crater morphologies, which can help in identifying planetary surface features observed by remote sensing.
"The Chicxulub crater shows some important asymmetries. It is worth considering that it was formed by a binary asteroid," Miljkovic told New Scientist.Someone ought to explain asteroid nomenclature to the New Scientist, btw.