JpGU-AGU Joint Meeting 2026

セッション情報

[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS08] Science of Venus in the post-VEx/Akatsuki era

2026年5月29日(金) 15:30 〜 17:00 303 (幕張メッセ国際会議場)

座長:Lee Yeon Joo(Institute for Basic Science)、Kleinboehl Armin(NASA Jet Propulsion Laboratory)

On 18 September 2025, the Akatsuki team transmitted the "termination of telecommunication" command to the spacecraft, thereby officially ending the operation of Akatsuki which has been and still is in the Venus' orbit since December 2015. ESA's Venus Express (in orbit from April 2006 till December 2014) and Akatsuki together had greatly advanced our knowledge about the Venusian atmosphere, with the focus of VEx being primarily chemistry and Akatsuki's focus being almost exclusively dynamics. The planetary science community in the world gained a strong momentum to further investigate Earth's twin sister: Two of the upcoming three Venus missions, NASA's VERITAS and ESA's EnVision, are more focused on the geology, interior and evolution of the solid body with the synthetic aperture radar and other tools. Another NASA mission DAVINCI will sense both the atmosphere and the surface by a descent probe. Other recent developments include the approval of the Venus Orbiter Mission (VOM) by the Indian government; the upgrade of Chinese VOICE mission to a Venus sample return mission, and announcement of the first private sector Venus mission, Venus Life Finder.
This momentum is driven by the analytical studies based on all previous Venus missions, numerical simulations (recently with data assimilation), ground-based observations, as well as laboratory experiments. This session will therefore cover all aspects of Venus science, derived observationally or theoretically, from its interior over the surface and atmosphere to the surrounding plasma environment and including possible implications for exoplanets. Contributions at all levels, from early-career researchers to experts, are all welcome.

16:15 〜 16:35

*Ignacio Romeo1, Alberto Jimenez Diaz2, Marina Mendiburu Eliçabe3, Isabel Egea Gonzalez4, Rebecca M. Hahn5, Paul K. Byrne5, Jon F. Kirby6, Julia Alvarez Lozano1, Javier Ruiz1 (1. Departamento de Geodinámica, Estratigrafía y Paleontología. Universidad Complutense de Madrid. 28040 Madrid, Spain, 2. Departamento de Biología y Geología, Física y Química Inorgánica, ESCET, Universidad Rey Juan Carlos, Móstoles, Madrid, 28933, Spain, 3. Departamento de Estadística e Investigación Operativa. Universidad Complutense de Madrid. 28040 Madrid, Spain, 4. Departamento de Física Aplicada, Escuela Superior de Ingeniería, Universidad de Cádiz, 11519, Puerto Real, Cádiz, Spain, 5. Department of Earth, Enviromental and Planetary Sciences, Washington University in St. Louis, 6. Geodesy & Earth Observation, DTU Space, Technical University of Denmark, 2800 Kongens Lyngby, Denmark)

16:35 〜 16:55

*西山 学1,2、鈴木 雄大3,4、宇野 慎介5,2、青木 翔平2、岩中 達郎2,5、今村 剛2、藤井 友香6、Müller Thomas7、田口 真8、神山 徹9、Barraud Océane1、D’Amore Mario1、Helbert Jörn10、Adeli Solmaz1、Hiesinger Harald11 (1. ドイツ航空宇宙センター(DLR)、2. 東京大学、3. 宇宙科学研究所、4. ボストン大学、5. 理化学研究所、6. 国立天文台、7. Max-Planck-Institut Für Extraterrestrische Physik、8. 立教大学、9. 産業技術総合研究所、10. European Space Research and Technology Centre (ESTEC/ESA)、11. Universität Münster)

Discussion (16:55 〜 17:00)

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