Japan Geoscience Union Meeting 2016

Presentation information

International Session (Oral)

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

[P-CG10] Small Solar System Bodies: General and Mars Satellite Sample Return Mission

Sun. May 22, 2016 3:30 PM - 5:00 PM 104 (1F)

Convener:*Taishi Nakamoto(Tokyo Institute of Technology), Kiyoshi Kuramoto(Department of Cosmosciences, Graduate School of Sciences, Hokkaido University), Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University), MASATERU ISHIGURO(Department of Physics and Astronomy, Seoul National University), Masahiko Arakawa(Graduate School of Science, Kobe University), Masanao Abe(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Tomoko Arai(Planetary Exploration Research Center, Chiba Institute of Technology), Sho Sasaki(Department of Earth and Space Sciences, School of Science, Osaka University), Chair:Tomoko Arai(Planetary Exploration Research Center, Chiba Institute of Technology)

4:45 PM - 5:00 PM


*Yuna Grace Kwon1, MASATERU ISHIGURO1, Hidekazu Hanayama2, Daisuke Kuroda3, Satoshi Honda4, Jun Takahashi4, Yoonyoung Kim1, Myung Gyoon Lee1, Young-Jun Choi5, Myung-Jin Kim5, Jeremie Vaubaillon6, Takeshi Miyaji2, Kenshi Yanagisawa3, Michitoshi Yoshida7, Kouji Ohta8, Nobuyuki Kawai9, Hideo Fukushima10, Jun-ichi Watanabe10 (1.Seoul National University, 2.Ishigakijima Astronomical Observatory, 3.Okayama Astrophysical Observatory, 4.Nishi-Harima Astronomical Observatory, 5.Korea Astronomy and Space Science Institute, 6.Observatoire de Paris, 7.Hiroshima University, 8.Kyoto University, 9.Tokyo Institute of Technology Meguro, 10.National Astronomical Observatory of Japan)

Keywords:comets, 17P/Holmes

Comets are the most pristine reservoir of the materials left over from the formation epoch of the solar system. When they are heated and expel this ancient material in their orbital motions around the Sun, we can have the opportunity to decipher the primitive information which have buried underneath the cometary surface for a long time. Herein, we present a brief overview of our observational results of a Jupiter-Family comet, 17P/Holmes, which underwent the historic outburst in 2007, to investigate its secular change in activity during 2014 perihelion passage. We performed the monitoring observation over two years, welcoming its first perihelion passage since the 2007 outburst. We analyzed the imaging data taken over two years, and found that there is a strong asymmetry of cometary activity with respect to the perihelion. Compared to the values taken right after the 2007 outburst, our results present a dust-production rate that has been utterly quenched by about five orders of magnitudes and is rather similar to that of pre-outburst inactive phase. We also found that the secular evolution of the fractional active area over the cometary surface had drastically dropped by about two orders of magnitudes in only one orbital revolution around the Sun. All of our results indicate that 17P/Holmes has entered upon an inactive phase far more rapidly than the prediction of the previous researches, and from this we conjecture that a surficial dust layer (~7 – 10 cm in depth) of the comet play a dominant role as an insulator of sublimation of subsurface water ice from the solar irradiation.