activity
20162022
most citedHayabusa2 Extended Mission: New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period

60 citations · 89 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202217 cited

A global system of furrows on Ganymede indicative of their creation in a single impact event

Naoyuki Hirata, Ryo Suetsugu, Keiji Ohtsuki

Furrows are a concentric system of tectonic troughs, and are the oldest recognizable surface feature on Ganymede. We analyzed the distribution of furrows utilizing Voyager and Gali…

astro-ph.IM202160 cited

Hayabusa2 Extended Mission: New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period

M. Hirabayashi, Y. Mimasu, N. Sakatani +41

Hayabusa2 is the Japanese Asteroid Return Mission and targeted the carbonaceous asteroid Ryugu, conducted by the Japan Aerospace Exploration Agency (JAXA). The goal of this mission…

astro-ph.EP201912 cited

Crater-ray formation through mutual collisions of hypervelocity-impact induced ejecta particles

Toshihiko Kadono, Ayako I. Suzuki, Rintaro Matsumura +4

We investigate the patterns observed in ejecta curtain induced by hypervelocity impact (2-6 km/s) with a variety of the size and shape of target particles. We characterize the patt…

astro-ph.EP2019

Pattern of Impact-Induced Ejecta from Granular Targets with Large Inclusions

Toshihiko Kadono, Ryo Suetsugu, Dai Arakawa +4

We performed impact experiments to observe patterns in an ejecta curtain with targets consisting of small sand particles and large inclusions comparable to or smaller than the size…

astro-ph.EP2018

Collisional Disruption of Planetesimals in the Gravity Regime with iSALE Code: Comparison with SPH code for Purely Hydrodynamic Bodies

Ryo Suetsugu, Hidekazu Tanaka, Hiroshi Kobayashi +1

In most of the previous studies related to collisional disruption of planetesimals in the gravity regime, Smoothed Particle Hydrodynamics (SPH) simulations have been used. On the o…

astro-ph.EP2016

Capture of planetesimals by waning circumplanetary gas disks

Ryo Suetsugu, Keiji Ohtsuki

When gas giant protoplanets grow sufficiently massive, circumplanetary disks would form. While solid bodies captured by the circumplanetary disks likely contribute to the growth of…