TY - JOUR
T1 - Granular impact cratering by liquid drops
T2 - Understanding raindrop imprints through an analogy to asteroid strikes
AU - Zhao, Runchen
AU - Zhang, Qianyun
AU - Tjugito, Hendro
AU - Cheng, Xiang
PY - 2015/1/13
Y1 - 2015/1/13
N2 - When a granular material is impacted by a sphere, its surface deforms like a liquid yet it preserves a circular crater like a solid. Although the mechanism of granular impact cratering by solid spheres is well explored, our knowledge on granular impact cratering by liquid drops is still very limited. Here, by combining high-speed photography with high-precision laser profilometry, we investigate liquid-drop impact dynamics on granular surface and monitor the morphology of resulting impact craters. Surprisingly, we find that despite the enormous energy and length difference, granular impact cratering by liquid drops follows the same energy scaling and reproduces the same crater morphology as that of asteroid impact craters. Inspired by this similarity, we integrate the physical insight from planetary sciences, the liquidmarblemodel from fluid mechanics, and the concept of jamming transition from granular physics into a simple theoretical framework that quantitatively describes all of the main features of liquid-drop imprints in granular media. Our study sheds light on the mechanisms governing raindrop impacts on granular surfaces and reveals a remarkable analogy between familiar phenomena of raining and catastrophic asteroid strikes.
AB - When a granular material is impacted by a sphere, its surface deforms like a liquid yet it preserves a circular crater like a solid. Although the mechanism of granular impact cratering by solid spheres is well explored, our knowledge on granular impact cratering by liquid drops is still very limited. Here, by combining high-speed photography with high-precision laser profilometry, we investigate liquid-drop impact dynamics on granular surface and monitor the morphology of resulting impact craters. Surprisingly, we find that despite the enormous energy and length difference, granular impact cratering by liquid drops follows the same energy scaling and reproduces the same crater morphology as that of asteroid impact craters. Inspired by this similarity, we integrate the physical insight from planetary sciences, the liquidmarblemodel from fluid mechanics, and the concept of jamming transition from granular physics into a simple theoretical framework that quantitatively describes all of the main features of liquid-drop imprints in granular media. Our study sheds light on the mechanisms governing raindrop impacts on granular surfaces and reveals a remarkable analogy between familiar phenomena of raining and catastrophic asteroid strikes.
KW - Granular impact cratering
KW - Jamming
KW - Liquid impacts
KW - Liquid marble
UR - http://www.scopus.com/inward/record.url?scp=84920972463&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84920972463&partnerID=8YFLogxK
U2 - 10.1073/pnas.1419271112
DO - 10.1073/pnas.1419271112
M3 - Article
C2 - 25548187
AN - SCOPUS:84920972463
SN - 0027-8424
VL - 112
SP - 342
EP - 347
JO - Proceedings of the National Academy of Sciences of the United States of America
JF - Proceedings of the National Academy of Sciences of the United States of America
IS - 2
ER -