BibTex format
@article{Miljković:2014:10.1016/j.epsl.2014.08.026,
author = {Miljkovi, K and Collins, GS and Bland, PA},
doi = {10.1016/j.epsl.2014.08.026},
journal = {Earth and Planetary Science Letters},
pages = {285--286},
title = {Reply to comment on: “Supportive comment on: “Morphology and population of binary asteroid impact craters”, by K. Miljkovi, G.S. Collins, S. Mannick and P.A. Bland – An updated assessment”},
url = {http://dx.doi.org/10.1016/j.epsl.2014.08.026},
volume = {405},
year = {2014}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - In Miljkovi et al. (2013) we resolved the apparent contradiction that while 15% of the Near Earth Asteroid (impactor) population are binaries, only 2–4% of craters formed on Earth and Mars (target planet) are doublet craters. Using 3D hydrocode simulations to explore the physics of binary impacts, we showed that only 2% of binary asteroid impacts produced well-separated doublets, while the rest covered morphologies ranging from overlapping to elliptical or even circular. We then generated a complete classification dataset to aid in the identification of the (sometimes subtle) morphological characteristics consistent with a binary asteroid impact. We thank Schmieder et al. (2013) for providing additional detailed geochronological constraints which indicate that our lower bound of 2% doublet craters on Earth may in fact be ≤1.5%.
AU - Miljkovi,K
AU - Collins,GS
AU - Bland,PA
DO - 10.1016/j.epsl.2014.08.026
EP - 286
PY - 2014///
SN - 0012-821X
SP - 285
TI - Reply to comment on: “Supportive comment on: “Morphology and population of binary asteroid impact craters”, by K. Miljkovi, G.S. Collins, S. Mannick and P.A. Bland – An updated assessment”
T2 - Earth and Planetary Science Letters
UR - http://dx.doi.org/10.1016/j.epsl.2014.08.026
UR - http://hdl.handle.net/10044/1/18602
VL - 405
ER -