Japan Geoscience Union Meeting 2014

Presentation information

International Session (Oral)

Symbol P (Space and Planetary Sciences) » P-PS Planetary Sciences

[P-PS02_28AM2] Mars

Mon. Apr 28, 2014 11:00 AM - 12:10 PM 418 (4F)

Convener:*Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Masaki Ishiwatari(Department of Cosmosciences, Graduate school of Science, Hokkaido University), Ayako Matsuoka(Research Division for Space Plasma, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Yoshiyuki O. Takahashi(Center for Planetary Science), Sho Sasaki(Department of Earth and Space Sciences, School of Science, Osaka University), Hideaki Miyamoto(The University Museum, The University of Tokyo), Chair:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)

11:00 AM - 11:25 AM

[PPS02-06] Life Detection Microscope: Search for Microbes on the Mars Surface with a Fluorescent Microscope

*Akihiko YAMAGISHI1, Takehiko SATOH2, Keigo ENYA2, Atsuo MIYAKAWA1, Satoshi SASAKI3, Yoshitaka YOSHIMURA4, Hajime HONDA5, Hirohide DEMURA6, Eiichi IMAI5, Tomohiro USUI7, Kazuhisa FUJITA8, Genya ISHIGAMI9, Takashi OZAWA8, Sohsuke OHNO10, Sho SASAKI11, Hideaki MIYAMOTO12 (1.Tokyo University of Pharmacy and Life Sciences, 2.ISAS/JAXA, 3.Tokyo University of Technology, 4.Tamagawa University, 5.Nagaoka Univ. Tech., 6.The University of Aizu, 7.Tokyo Institute of Technology, 8.JAXA, 9.Keio University, 10.Chiba Institute of Technology, 11.Osaka University, 12.The University of Tokyo)

Keywords:Mars, Life search, Fluorescence microscope, Microbe, Organic compounds

Past trial of direct detection of life on Mars by 1970's Viking mission reported a negative conclu-sion, whereas numbers of circumstances provided by recent Mars exploration missions in the last dec-ade indicate that there are good reasons to perform another life detection program.Here we propose Life Detection Microscope that has much higher sensitivity than the instrument onboard Viking. Indeed Life Detection Microscope (LDM) that we propose here could detect less than 104 cells in 1 gram clay. Our life detecting instru-ment has the sensitivity that is three orders of mag-nitude higher than the one onboard Viking that issued the negative conclusion. LDM is capable of identifying what we think to be the most fundamen-tal features that a cell should possess to constitute life.Our Investigation Goals are:1: High-resolution characterization of regolith and dust particles.2: Search for any type of organic compounds in Mars surface samples. The compounds include cells, other biological materials, and abiotic polycyclic aromatic hydrocarbon (PAH).3: Identify cell-like structure in which organic compounds are enveloped by membrane, which may represent Martian life.