Research

Uniting for SCIENCE to understand the nature of nature

On the contrary, in Japan, we often see the word "science" paired with "technology", as in "kagaku-gijitsu" ("science technology"). From thousands of years ago, Western culture which has found significant value in questioning the mechanism of nature itself, has put the greatest emphasis on science itself rather than science technology. However, the biggest purpose of science that has come to be recognized in Japan is to become the direct benefit to people's lives and to create "technology" (to bring efficiency and good profit). As a result, in Japan, the mindset that does not first and foremost value "science as a tool to explore the causality and mechanisms of the natural phenomenon" has been spread, and eventually only "science technology" came to be primarily valued. This inevitability is understandable in the historical context. After the Second World War, Japan has rapidly reconstructed and achieved huge economic growth mainly through drastic industrialization and urbanization. However, I have been drawn to science to engaged in "science", and I want to continue in this path in the future, rather than the tendency for "science and technology". In addition and through my own work, I hope to promote the value, fun and appeal of pure science to Japan and the world.
One of the most important and fundamental questions of science is the "origin/s of life". Again, I am a planetary scientist and, in particular, working on the icy moons orbiting giant planets, e.g., Europa and Ganymede in the Jovian system, and Enceladus in the Saturnian system. Through several previous exploration missions, in several icy moons it has been considered that a vast liquid ocean exists beneath the icy crust. The subsurface ocean does not consist only of pure water but some minerals and organics which could be important compounds as building blocks of life are dissolved. Finally scientists are considering that the icy moon and its subsurface ocean may have a potential for harboring extraterrestrial (ET) life. The important point is not to search for ET life but to explore and find an evolutionary path from simple organics to life in the ET environment.
Recently, for example, glycine, the simplest amino acid, was confirmed to be present on comet 81P/Wild 2 from samples returned by NASA's Stardust spacecraft. We now know that biological components are present in the Universe and this first detection of extraterrestrial glycine suggests that amino acids can be formed by abiotic processes in the Universe.
However, further chemical environmental information and subsequent evolution toward functional biopolymers remain unclear. In order to push forward investigation of ET habitability, we need further chemical and environmental information and need to get together various experts from across the world. And eventually I believe we will be able to shed light on the essence of astrobiology.
To tackle seriously one of the biggest questions in nature, we have to unite beyond the boundaries of the various research fields and each expertise to maximize research progress and benefit by intensively concentrating resources on it. Eventually, I believe that exploring both the origins and evolution of the Earth and other planets/moons and the origins and evolution of life/lives will lead to creating a new field, "Bioplanetology". And personally, I hope and will continue to work so that "science" for understanding natural phenomena will take firmer root on Japanese soil and in the world.
Icy Worlds: Extra-terrestrial oceans, extra-terrestrial habitats, and extra-terrestrial life
I have been studying the surface tectonics, interior structure, chemical composition, and their evolution of the icy satellites, which belong to giant planets using computer simulation and observational data analyses, in particular. In addition, interior evolution of terrestrial Moon and its evolution is also my interest in a viewpoint of comparative understandings between icy and rocky bodies. Ultimately, I'd like to explain how planets and satellites have evolved to the current states, how did they diverge on their evolutionm and what is conditions for emerging an extra-terrestrial life.I participated in the exploration mission projects, SELENE/KAGUYA, Japanese lunar mission from 2007 to 2009. Now I'm a member of LIDAR (Laser Altimeter) team on the HAYABUSA-2 mission which has been launched in December 2014 to C-type asteroid "Ryugu", and GALA (Ganymede Laser Altimeter) team on the JUICE (JUpiter ICy moons Explorer) mission which has been successfully launched to the Jupiter system in 2023.
Stability of the subsurface ocean in the icy bodies

Surface geology and icy tectonics of icy bodies

Dynamo activity in the planetary core

Astrobiology

Also, we investigate chemical evolution in the icy moon's environment. In particular, we perform thermodynamic calculations (e.g., free energy) for polymerization of amino acids and other building bloks of life.