EGU23-4751, updated on 22 Feb 2023
https://doi.org/10.5194/egusphere-egu23-4751
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Major results from the Hisaki mission and future perspectives

Fuminori Tsuchiya1, Yasumasa Kasaba1, Ichiro Yoshikawa2, Go Murakami3, Atsushi Yamazaki3, Kazuo Yoshioka2, Tomoki Kimura4, Chihiro Tao5, Ryoichi Koga6, Hajime Kita7, Kei Masunaga3, Masato Kagitani1, Shotaro Sakai1, and Masaki Kuwabara8
Fuminori Tsuchiya et al.
  • 1Tohoku University, Sendai, Japan
  • 2The University of Tokyo, Kashiwa, Japan
  • 3SAS/JAXA, Sagamihara, Japan
  • 4Tokyo University of Science, Tokyo, Japan
  • 5NICT, Koganei, Japan
  • 6Nagoya University, Nagoya, Japan
  • 7Tohoku Institute of Technology, Sendai, Japan
  • 8Rikkyo University, Tokyo, Japan

Hisaki is an earth orbiting extreme ultraviolet spectroscope dedicated for observing solar system planets. Thanks to its monitoring capability, Hisaki has carried out unprecedented continuous observation of Io plasma torus, Jovian aurora, and Mars and Venus upper atmosphere since December 2013. One of notable phenomena observed by Hisaki is significant enhancements of neutral gas (sodium and oxygen) from Io occurred in the spring of 2015. Hisaki revealed that not only the plasma source, but transport, heating, and loss processes of magnetospheric plasma were influenced by the variation in the neutral source input. The presentation will include related topics from recent Hisaki publication. Since the autumn of 2016, the Juno spacecraft was in the orbit around Jupiter. Hisaki monitored activities of Jovian aurora and the plasma torus in the Juno era. These datasets will provide opportunities to compare in-situ observation by Juno with the global view by Hisaki. 
JAXA approved the Hisaki mission period by the end of March 2023. As a future remote observation platform, we are going to propose a UV space telescope, LAPYUTA (Life-environmentology, Astronomy, and PlanetarY Ultraviolet Telescope Assembly), a Japanese-leading mission using heritages of UV instruments for planetary science (e.g., Hisaki) and space telescope techniques for astronomy. One of goals of this mission is dynamics of our solar system planets and moons as the most quantifiable archetypes of extraterrestrial habitable environments in the universe. Water plume that gushes from the subsurface ocean of Galilean moons and tenuous atmosphere which is generated by bombardment of energetic charged particles to the surface are primary targets of LAPYUTA. As the plume activity and the atmosphere are not stable, continuous monitoring with high spatial resolution is essential. The icy moon's plume and ambient space will be deeply explored with the spacecraft by NASA's and ESA's icy moon missions in 2020s-2030s. The complementary remote sensing by LAPYUTA will visualize their global structure and temporal dynamics.

How to cite: Tsuchiya, F., Kasaba, Y., Yoshikawa, I., Murakami, G., Yamazaki, A., Yoshioka, K., Kimura, T., Tao, C., Koga, R., Kita, H., Masunaga, K., Kagitani, M., Sakai, S., and Kuwabara, M.: Major results from the Hisaki mission and future perspectives, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-4751, https://doi.org/10.5194/egusphere-egu23-4751, 2023.