*Hideo Sagawa1, Takahiro Iino2, Takashi Tsukagoshi3 (1.Kyoto Sangyo University, 2.Tokyo University of Agriculture and Technology, 3.National Astronomical Observatory of Japan)
Session information
[J] Poster
P (Space and Planetary Sciences ) » P-CG Complex & General
[P-CG24] New Developments of Planetary Sciences with ALMA
Wed. May 29, 2019 3:30 PM - 5:00 PM Poster Hall (International Exhibition Hall8, Makuhari Messe)
convener:Takayuki Muto(Division of Liberal Arts, Kogakuin University), Munetake Momose(The College of Science, Ibaraki University), Hideo Sagawa(Faculty of Science, Kyoto Sangyo University), Masumi Shimojo(National Astronomical Observatory of Japan)
The Atacama Large Millimeter/Submillimeter Array (ALMA) starated its science operation in 2011, and long-baseline observations have become available since 2014. With its high sensitivity and resolution, ALMA has provided us with qualitatively new information on star and planet formation and small bodies in our Solar System. For example, in the observations of protoplanetary disks, ring-like structures have been commonly found and the structures with the scale of several-AU are discovered in several systems. In our solar system, 60km pixel-scale non-uniform brightness distribution and the rotation of the asteroid Juno are detected. Spatially-resolved thermal mapping of Europa icy surface enables us to search for thermal anomaly in possible plume source regions. As of Cycle 4, Solar observations are available, enabling us, for example, to determine the physical parameters of plasmoid quantitatively. In this session, we overview the latest results of ALMA observations in the field of planetary sciences. We also accept any theoretical and experimental works that are closely related to the observations and discuss the impact on the planetary science community.
*Soon Kang-Lou1, Munetake Momose1, Takayuki Muto2, Takashi Tsukagoshi3, Akimasa Kataoka3, Tomoyuki Hanawa4, Misato Fukagawa3, Kazuya Saigo3, Hiroshi Shibai5 (1.Ibaraki University, 2.Kogakuin University, 3.National Astronomical Observatory of Japan, 4.Chiba University, 5.Osaka University)
*Masayuki Yamaguchi1,2, Kazunori Akiyama3,2, Akimasa Kataoka2,6, Takashi Tsukagoshi2, Takayuki Muto4, Shiro Ikeda5, Misato Fukagawa2, Mareki Honma2,6, Ryohei Kawabe2,1,6 (1.The University of Tokyo, 2.National Astronomical Observatory of Japan, 3.Massachusetts Institute of Technology, Haystack Observatory, 4.Kogakuin University, 5.The Institute of Statistical Mathematics, 6. Graduate University for Advanced Studies)
*Mihoko Konishi1,2, Jun Hashimoto1,2, Hauyu Liu3, Ruobing Dong4, Takayuki Muto5 (1.Astrobiology Center, National Institute of Natural Science, 2.National Astronomical Observatory of Japan, 3.Institute of Astronomy and Astrophysics, Academia Sinica, 4.University of Victoria, 5.Kogakuin University)
*Jun Hashimoto1, Mihoko Konishi1, Taichi Uyama2, Christian Ginski3, Matthias Samland4 (1.AstroBiology Center, National Institutes of Natural Sciences, 2.University of Tokyo, 3.University of Amsterdam, 4.Max Planck Institute for Astronomy)
*Takayuki Muto1, Jun Hashimoto2, Takashi Tsukagoshi3, Mihoko Konishi3, Tomoyuki Kudo3 (1.Division of Liberal Arts, Kogakuin University, 2.Astrobiology Center, 3.NAOJ)