Session Details
[P-CG30]New Progress toward the Understanding of Small Solar System Bodies
Tue. May 26, 2015 6:15 PM - 7:30 PM JST
Tue. May 26, 2015 9:15 AM - 10:30 AM UTC
Tue. May 26, 2015 9:15 AM - 10:30 AM UTC
Convention Hall 2F
Convener:*Masahiko Arakawa(Graduate School of Science, Kobe University), Taishi Nakamoto(Tokyo Institute of Technology), Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University), Masanao Abe(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), MASATERU ISHIGURO(Department of Physics and Astronomy, Seoul National University)
This session is aimed at setting up a forum to discuss how we can make progresses in our understanding of the solar system evolution with our hands on data. Presentations related to the science of the small bodies in the solar system (satellites, asteroids, comets, interplanetary dust particles, trans-Neptunian objects, and planetesimals) are invited. In addition to the extensive astronomical/remote-sensing observations and theoretical works, Hayabusa has brought us samples back from Itokawa (S-type asteroid) for unprecedentedly detailed analysis. The results of the Hayabusa sample initial analysis do prove that analysis of returned samples will play a key role in our future study of the solar system evolution. While the mission preparation of Hayabusa2, which is targeted at a more primordial asteroid than Itokawa (1999JU3, C-type), will be launched in 2014 winter, expectation of building a new gateway to biology-flavored topics via organic material and aqueous alternation analysis is ramping up. In this session, after summarizing the cutting-edge results obtained by various methods including the Hayabusa sample analysis, we will discuss the future shape of the study of the solar system evolution.
[PCG30-P01]Pre-launch calibration and the first image data of the optical navigation camera of Hayabusa 2
*Seiji SUGITA1, Shingo KAMEDA2, Hirotaka SAWADA3, Hidehiko SUZUKI4, Manabu YAMADA5, Rie HONDA6, Tomokatsu MOROTA7, Chikatoshi HONDA8, Kazunori OGAWA3, Kei SHIRAI3, Yuichi IIJIMA3, Yuichiro CHO2, Akito TAKEI2, Hiroshi OKUMURA2, Tatsuya YASUDA2, Kazuo SHIBAZAKI2, Masaki SATO2, Shota IKEZAWA2, Tomoki NAKAMURA8, Takahiro HIROI9, Shunichi KAMATA10, Sumire KOGA1, ONC, Science team 3 (1.University of Tokyo, 2.Rikkyo University, 3.JAXA, 4.Meiji University, 5.Chiba Institute of Technology, 6.Kochi University, 7.Aizu University, 8.Tohoku University, 9.Brown University, 10.UC. Santa Cruz)
[PCG30-P02]Accuracy Evaluation of Asteroid Shape Reconstruction by Structure-from-Motion Method with a asteroid scale model
*Naru HIRATA1, Fumiya IWASAKI1, SHAPE RECONSTRUCTION, Study group HAYABUSA-22 (1.ARC-Space/CAIST, The University of Aizu, 2.Hayabusa-2 project)
[PCG30-P03]Results of the development for NIRS3: the Near Infrared Spectrometer on Hayabusa-2
*Takahiro IWATA1, Kohei KITAZATO2, Masanao ABE1, Takehiko ARAI1, Yusuke NAKAUCHI3, Tomoki NAKAMURA4, Takahiro HIROI5, Takahito OSAWA6, Moe MATSUOKA4, Shuji MATSUURA1 (1.Institute of Space and Astronautical Science, JAXA, 2.University of Aizu, 3.Graduate University for Advanced Studies, 4.Tohoku University, 5.Brown University, 6.JAEA)
[PCG30-P04]Initial operation of Hayabusa-2 laser altimeter (LIDAR)
*Hirotomo NODA1, Takahide MIZUNO2, Noriyuki NAMIKI1, Hiroki SENSHU3, Ryuhei YAMADA1, Naru HIRATA4, Makoto SHIZUGAMI5 (1.RISE project, NAOJ, 2.Japan Aerospace Exploration Agency, 3.Planetary Exploration Research Center, Chiba Institute of Technology, 4.Dep. of Computer Science and Engineering, Univ. of Aizu, 5.Mizusawa VLBI Observatory, NAOJ)
[PCG30-P05]Present status of curation of Hayabusa-returned samples
*Toru YADA1, Masanao ABE1, Masayuki UESUGI1, Yuzuru KAROUJI1, Aiko NAKATO1, Kazuya KUMAGAI1, Tatsuaki OKADA1 (1.Japan Aerospace Exploration Agency)
[PCG30-P06]Statistical analyses of lineaments on Phobos: implications to their formational processes and orbital environment
*Hiroshi KIKUCHI1, Hideaki MIYAMOTO1 (1.The University Museum, The University of Tokyo)
[PCG30-P07]MU radar head echo observations of the 2012 October Draconid outburst
*Yasunori FUJIWARA1, Johan Kero2, Makoto ABO3, Csilla Szasz2, Takuji NAKAMURA4 (1.SOKENDAI, 2.Swedish Institute of Space Physics, 3.Tokyo Metropolitan University, 4.National Institute of Polar Research)
[PCG30-P08]Prediction of Phoenicid
Takehiro SAITO1, *Isao SATO1, Shinsuke ABE1 (1.Nihon University)