48 citations · 70 across the 2 of their papers we have counts for
4 papers
Rotational Disruption of Porous Dust Aggregates due to Gas Flow in Protoplanetary Disks
Misako Tatsuuma, Akimasa Kataoka
We introduce a possible disruption mechanism of dust grains in planet formation by their spinning motion. This mechanism has been discussed as rotational disruption for the interst…
Tensile Strength of Porous Dust Aggregates
Misako Tatsuuma, Akimasa Kataoka, Hidekazu Tanaka
Comets are thought to have information about the formation process of our solar system. Recently, detailed information about comet 67P/Churyumov-Gerasimenko has been found by a spa…
Thermal conductivity and coordination number of compressed dust aggregates
Sota Arakawa, Misako Tatsuuma, Naoya Sakatani +1
Understanding the heat transfer mechanism within dust aggregates is of great importance for many subjects in planetary science. We calculated the coordination number and the therma…
Gravitational instability of a dust layer composed of porous silicate dust aggregates in a protoplanetary disk
Misako Tatsuuma, Shugo Michikoshi, Eiichiro Kokubo
Planetesimal formation is one of the most important unsolved problems in planet formation theory. In particular, rocky planetesimal formation is difficult because silicate dust gra…