Japan Geoscience Union Meeting 2023

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-CG Complex & General

[P-CG18] Future missions and instrumentation for space and planetary science

Mon. May 22, 2023 10:45 AM - 12:00 PM 105 (International Conference Hall, Makuhari Messe)

convener:Shoichiro Yokota(Graduate School of Science, Osaka University), Naoya Sakatani(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Kazunori Ogawa(Japan Aerospace Exploration Agency), Masaki Kuwabara(Rikkyo University), Chairperson:Kazunori Ogawa(Japan Aerospace Exploration Agency)

11:00 AM - 11:15 AM

[PCG18-02] Development status of the seismic observation system onboard the Titan landing mission DragonFly

*Satoshi Tanaka1, Hiroaki Shiraishi1, Takefumi Mitani1, Taichi Kawamura2, Hideki Murakami3, Ryuhei Yamada6, Shun-ichi Kamata7, Jun Kimura5, Hiroyuki Kurokawa9, Kiwamu Nishida4, Yasuhito Sekine9, Takeshi Tsuji4, Keisuke Onodera4, Ralph Lorenz8 (1.Institute of Space and Astronautical Science, 2.Institut de Physique du Globe de Paris , 3.Kochi University, 4.University of Tokyo, 5.Osaka University, 6.University of Aizu, 7.Hokkaido University, 8.Johns Hopkins University, 9.Tokyo Institute of Technology)

Keywords:seismic observation, DragonFly mission, Titan

The Saturn satellite Titan takeoff and landing mission "Dragonfly" is a medium-scale mission selected as the fourth mission of NASA's New Frontiers Program in 2019. Dragonfly is scheduled to launch in 2027 and deploy a drone-like takeoff and landing vehicle on Titan around 2034 to conduct chemical analysis, meteorological and geophysical observations at multiple landing sites to investigate the precursors of life and evolutionary processes.
In July 2022, a plan to equip this mission with a seismometer developed by ISAS for lunar exploration was approved as a strategic overseas joint project, and full-scale development has started.
The Japanese side will be responsible for the seismometer, preamplifier, and windshield cover, which constitute the main part of the package (DraGMet SEIS) for observing seismic motions. The seismometer was initially developed for operation at -20°C in the lunar surface layer and will be modified to develop a seismometer that can operate in the Titan surface environment (1.5 atm, -180°C). For this purpose, we have developed a chamber that can be tested in an environment that simulates Titan's surface environment, and the operation of the seismometer and preamplifier has been confirmed.
As of February 2023 we had completed manufacturing of the EM (Engineered Model) and had begun testing for delivery to the U.S. After completing testing using the EM model by the middle of this year, FM manufacturing will begin, with flight model delivers scheduled for March 2024.
This presentation will report on the latest development and review process status.