activity
20162021
most citedJetting during oblique impacts of spherical impactors

28 citations · 57 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202128 cited

Jetting during oblique impacts of spherical impactors

Shigeru Wakita, Brandon Johnson, C. Adeene Denton +1

During the early stages of an impact a small amount material may be jetted and ejected at speeds exceeding the impact velocity. Jetting is an important process for producing melt d…

astro-ph.EP20196 cited

Aggregate Growth and Internal structures of Chondrite Parent Bodies Forming from Dense Clumps

Yuji Matsumoto, Shigeru Wakita, Yasuhiro Hasegawa +1

Major components of chondrites are chondrules and matrix. Measurements of the volatile abundance in Semarkona chondrules suggest that chondrules formed in a dense clump that had a…

astro-ph.EP2019

The Properties of Planetesimal Collisions under Jupiter's Perturbation and the Application to Chondrule Formation via Impact Jetting

Shoichi Oshino, Yasuhiro Hasegawa, Shigeru Wakita +1

Understanding chondrule formation provides invaluable clues about the origin of the solar system. Recent studies suggest that planetesimal collisions and the resulting impact melts…

astro-ph.EP201919 cited

Fates of hydrous materials during planetesimal collisions

Shigeru Wakita, Hidenori Genda

Hydrous minerals are found on the surfaces of asteroids, but their origin is not clear. If their origin is endogenic, the hydrous minerals that were formed in the inner part of a p…

astro-ph.EP2018

Abundances of ordinary chondrites in thermally evolving planetesimals

S. Wakita, Y. Hasegawa, T. Nozawa

Chondrites are one of the most primitive objects in the solar system, and keep the record of the degree of thermal metamorphism experienced in their parent bodies. This thermal his…

astro-ph.EP20174 cited

Chondrule Accretion with a Growing Protoplanet

Yuji Matsumoto, Shoichi Oshino, Yasuhiro Hasegawa +1

Chondrules are primitive materials in the Solar System. They are formed in the first about 3 Myr of the Solar System's history. This timescale is longer than that of Mars formation…