Chisato Okamoto
Kobe University
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Featured researches published by Chisato Okamoto.
Icarus | 2018
Ayako Suzuki; Chisato Okamoto; Kosuke Kurosawa; Toshihiko Kadono; Sunao Hasegawa; Takayuki Hirai
Abstract Impact-cratering processes on small bodies are thought to be mainly controlled by the local material strength because of their low surface gravity, and craters that are as large as the parent bodies should be affected by the target curvature. Although cratering processes on planar surfaces in the strength-controlled regime have been studied extensively, the mechanism by which target curvature affects the cratering processes remains unclear. Herein, we report on a series of impact experiments that used spherical targets with various diameters. The resultant craters consisted of a deep circular pit and an irregular-shaped spall region around the pit, which is consistent with the features reported in a number of previous cratering experiments on planar surfaces. However, the volume and radius of the craters increased with the normalized curvature. The results indicate that the increase in the spall-region volume and radius mainly contributes to the increase in the whole crater volume and radius, although the volume, depth, and radius of pits remain constant with curvature. The results of our model indicate that the geometric effect due to curvature (i.e., whereby the distance from the equivalent center to the target free surface is shorter for higher curvature values) contributes to increases in the cratering efficiency. Our results suggest that the impactors that produce the largest craters (basins) on some asteroids are thus smaller than what is estimated by current scaling laws, which do not take into account the curvature effects.
EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference | 2009
Masahiko Arakawa; Yo‐ichiro Uchiyama; Chisato Okamoto
We conducted impact experiments of simulated rimmed chondrules at the impact velocity from 10 cm/s to 80 m/s to obtain the sticking velocity and the restitution coefficients. The porosity of the rim was changed from 70% to 90% with the thickness of 5 mm while the rim was composed of sub‐micron silica particles, and a glass ball with the size of 10 mm was used as a chondrule analogue. As a result, we found that the upper limit of the sticking velocity, vc, varied with the porosity.
Space Science Reviews | 2017
Masahiko Arakawa; Koji Wada; Takanao Saiki; Toshihiko Kadono; Yasuhiko Takagi; K. Shirai; Chisato Okamoto; Hajime Yano; M. Hayakawa; Satoru Nakazawa; Naru Hirata; Masanori Kobayashi; Patrick Michel; Martin Jutzi; H. Imamura; Kazunori Ogawa; Naoya Sakatani; Yuichi Iijima; Rie Honda; Ko Ishibashi; H. Hayakawa; Hirotaka Sawada
Space Science Reviews | 2017
Takanao Saiki; H. Imamura; Masahiko Arakawa; Koji Wada; Yasuhiko Takagi; M. Hayakawa; Kei Shirai; Hajime Yano; Chisato Okamoto
Acta Astronautica | 2013
Takanao Saiki; Hirotaka Sawada; Chisato Okamoto; Hajime Yano; Yasuhiko Takagi; Yasuhiro Akahoshi; Makoto Yoshikawa
Meteoritics & Planetary Science | 2009
Chisato Okamoto; Masahiko Arakawa
Icarus | 2012
Koji Dohi; Masahiko Arakawa; Chisato Okamoto; Sunao Hasegawa; Minami Yasui
Space Science Reviews | 2017
Ryuji Okazaki; Hirotaka Sawada; Shinji Yamanouchi; Shogo Tachibana; Yayoi N. Miura; Kanako Sakamoto; Yoshinori Takano; Masanao Abe; S.-I. Itoh; Keita Yamada; Hikaru Yabuta; Chisato Okamoto; Hajime Yano; Takaaki Noguchi; Tomoki Nakamura; Keisuke Nagao
Space Science Reviews | 2017
Hirotaka Sawada; Ryuji Okazaki; Shogo Tachibana; Kanako Sakamoto; Yoshinori Takano; Chisato Okamoto; Hajime Yano; Yayoi N. Miura; Masanao Abe; Sunao Hasegawa; Takaaki Noguchi; Hayabusa Smp Team
Icarus | 2008
Chisato Okamoto; Masahiko Arakawa