Japan Geoscience Union Meeting 2015

Presentation information


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

[P-CG30] New Progress toward the Understanding of Small Solar System Bodies

Tue. May 26, 2015 2:15 PM - 4:00 PM A02 (APA HOTEL&RESORT TOKYO BAY MAKUHARI)

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), Chair:Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University)

3:00 PM - 3:15 PM

[PCG30-07] Can Hayabusa-2 reveal the distribution of organics on asteroid surface?

*Kohei KITAZATO1, Ayaka FUJIWARA1, Akiko NAKAMURA2, Makiko OHTAKE3, Masanao ABE3 (1.University of Aizu, 2.Kobe University, 3.JAXA/ISAS)

Keywords:Hayabusa-2, asteroids, organics, photometric properties

Japanese asteroidal mission "Hayabusa-2" aims at bringing back samples of a C-type asteroid to the Earth, which is expected to extend our knowledge about the early evolution of the solar system and the origin of Earth's life through the on-ground analysis of the returned samples. To maximize its scientific outputs, it is important to reveal the distributions of hydrated minerals and organics on the asteroid surface by remote sensing. Although we can examine the distribution of hydrated minerals by using the near-infrared spectrometer on-board the Hayabusa-2 spacecraft, the method to examine that of organics has not been established yet. Since the total amounts of carbon including carbonaceous meteorites show a clear negative correlation with their absolute reflectance in visible, the absolute reflectance might become a useful index for estimating the organics content. However, the absolute reflectance also depends on the physical properties such as particle size and porosity. Then, we considered discerning the organics content and particle size by using the photometric properties in addition to the absolute reflectance, and performed an experiment to verify this idea using analog materials of asteroid surface. The samples that we used are dunite and humic acid as silicate and organics analogs, respectively. We measured the photometric properties of (1) silicate-organics mixtures and (2) dunite samples with different particle size in the phase angle range of 5-60 degrees. The measurements were performed with a gonio-spectrometer developed in University of Aizu. As a result, in the case of increasing the organics content, the reflectance becomes lower and backward scattering becomes stronger. While in the case of increasing the particle size, the reflectance becomes lower and forward scattering becomes stronger. Also we found that those variations could be matched with the predictions from a theoretical model. Thus, we conclude that it is possible to discern the organics content and particle size based on the absolute reflectance and photometric properties. We need more experiments to examine the effect of space weathering.