Session Details
[P-PS04][EJ] New developments of planetary sciences with ALMA
Wed. May 24, 2017 9:00 AM - 10:30 AM JST
Wed. May 24, 2017 12:00 AM - 1:30 AM UTC
Wed. May 24, 2017 12:00 AM - 1:30 AM UTC
A04 Tokyo Bay Makuhari Hall
convener:Munetake Momose(The College of Science, Ibaraki University), Hiroshi Kobayashi(Department of Physics, Nagoya University), Masumi Shimojo(National Astronomical Observatory of Japan), Hideko Nomura(Department of Earth and Planetary Sciences, Tokyo Institute of Technology), Chairperson:Munetake MOMOSE(The College of Science, Ibaraki University)
The Atacama Large Millimeter/Submillimeter Array (ALMA) starated its science operation in 2011. Thanks to its high sensitivity and mapping capability, ALMA has revealed detailed structure of nearby protoplanetary disks, providing us with new informations about the formation of a planetary system in general. Long-baseline campaign observations made in 2014 brought us spectacular images. Ring-gap structure in the disk around the young star HL Tau is discovered with 4au resolution, while non-uniform brightness distribution of the asteroid Juno is mapped with 60km pixel-size in the image. These results demonstrate that ALMA will be a powerful tool for exploring disks around young stars and objects in the solar system.
Furthermore, the solar observation mode has been offered to the community since Cycle 4. This session will accept not only the observational studies with ALMA but also any theoretical and experimental works that are closely related to the observations, and planetary sciences with the ALMA will be discussed comprehensively.
Furthermore, the solar observation mode has been offered to the community since Cycle 4. This session will accept not only the observational studies with ALMA but also any theoretical and experimental works that are closely related to the observations, and planetary sciences with the ALMA will be discussed comprehensively.
[PPS04-02]millimeter-wave polarization as a tool of investigating the planet formation★Invited papers
*Akimasa Kataoka1,3, Takashi Tsukagoshi2, Munetake Momose2, Hiroshi Nagai3, Takayuki Muto4, Cornelis Dullemond1, Adriana Pohl1,5, Misato Fukagawa6, Hiroshi Shibai7, Tomoyuki Hanawa8, Koji Murakawa9 (1.Heidelberg University, 2.Ibaraki Univerisity, 3.National Astronomical Observatory of Japan, 4.Kogakuin University, 5.Max-Planck Institute for Astronomy, 6.Nagoya University, 7.Osaka University, 8.Chiba University, 9.Osaka Sangyo University)
[PPS04-03]Submillimeter multi-wavelength observations for the protoplanetary disk around a young star TW Hya with ALMA
*Takashi Tsukagoshi1, Hideko Nomura2, Takayuki Muto3, Ryohei Kawabe4,9,10, Daiki Ishimoto2,5, Kazuhiro Kanagawa6, Satoshi Okuzumi2, Shigeru Ida2, Catherine Walsh11,7, Tom Millar8 (1.Ibaraki University, 2.Tokyo Institute of Technology, 3.Kogakuin University, 4.National Astronomical Observatory of Japan, 5.Kyoto University, 6.University of Szczecin, 7.Leiden University, 8.Queen's University Belfast, 9.The Graduate University for Advanced Studies, 10.University of Tokyo, 11.University of Leeds)
[PPS04-04]Impacts of ALMA observations of protoplanetary disks on planet formation theory
*Sanemichi Takahashi1, Shuichiro Inutsuka2 (1.Tohoku University, 2.Nagoya University)
[PPS04-05]Observation proposal for solar system bodies by using the ALMA
*Seitaro Urakawa1, Tomohiko Sekiguchi2 (1.Japan Spaceguard Association, 2.Hokkaido University of Education)
[PPS04-06]Solar chromospheric dynamics by ALMA observations★Invited papers
*Takaaki Yokoyama1, Haruhisa Iijima2, Masumi Shimojo3, Takenori Okamoto3 (1.School of Science, The University of Tokyo, 2.ISEE, Nagoya University, 3.Chile Observatory, NAOJ)