218 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Tokyo Institute of TechnologyJP129 papers
- The University of TokyoJP34 papers
- National Astronomical Observatory of JapanJP24 papers
- Japan Aerospace Exploration AgencyJP11 papers
- Centre National de la Recherche ScientifiqueFR10 papers
- RIKEN Center for Computational ScienceJP10 papers
- Institute of Space and Astronautical ScienceJP8 papers
- Life Science InstituteJP8 papers
- California Institute of TechnologyUS7 papers
- Hungarian Academy of SciencesHU7 papers
- Kyoto UniversityJP7 papers
- Nagoya UniversityJP7 papers
8 papers · 1 filter
Particle-particle Particle-tree Code for Planetary System Formation with Individual Cut-off Method: GPLUM
Yota Ishigaki, Junko Kominami, Junichiro Makino +2
In a standard theory of the formation of the planets in our Solar System, terrestrial planets and cores of gas giants are formed through accretion of kilometer-sized objects (plane…
Thermal Conductivity of CaSiO Perovskite at Lower Mantle Conditions
Zhen Zhang, Dong-Bo Zhang, Kotaro Onga +4
Thermal conductivity () of mantle minerals is a fundamental property in geodynamic modeling. It controls the style of mantle convection and the time scale of the mantle and core…
Microlensed Radio Emission from Exoplanets
Yuta Shiohira, Yuka Terada, Den Mukuno +2
In this paper, we investigate the detectability of radio emission from exoplanets, especially hot Jupiters, which are magnified by gravitational microlensing. Because hot Jupiters…
SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
Yutaka Hirai, Michiko S. Fujii, Takayuki R. Saitoh
Most stars are formed as star clusters in galaxies, which then disperse into galactic disks. Upcoming exascale supercomputational facilities will enable performing simulations of g…
The effect of high nitrogen pressures on the habitable zone and an appraisal of greenhouse states
Ramses M. Ramirez
The habitable zone is the main tool that mission architectures utilize to select potentially habitable planets for follow up spectroscopic observation. Given its importance, the pr…
Uranian Satellite Formation by Evolution of a Water Vapor Disk Generated by a Giant Impact
Shigeru Ida, Shoji Ueta, Takanori Sasaki +1
The ice-giant planet Uranus likely underwent a giant impact, given that its spin axis is tilted by 98 degrees. That its satellite system is equally inclined and prograde suggests t…
Impact Ejecta near the Impact Point Observed using Ultra-high-speed Imaging and SPH Simulations, and a Comparison of the Two Methods
Takaya Okamoto, Kosuke Kurosawa, Hidenori Genda +1
High-speed impact ejecta at velocities comparable to the impact velocity are expected to contribute to material transport between planetary bodies and deposition of ejecta far from…
Earth-Like: An education & outreach tool for exploring the diversity of planets like our own
Elizabeth J. Tasker, Kana Ishimaru, Nicholas Guttenberg +1
Earth-Like is an interactive website and twitter bot that allows users to explore changes in the average global surface temperature of an Earth-like planet due to variations in the…