49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1210.pdf ORIGINS OF HIGH-TEMPERATURE FLUIDS IN THE GOSHOGAKE MUD VOLCANO FIELD, TOHOKU, NORTHERN JAPAN: CHEMICAL AND ISOTOPIC STUDIES OF GAS AND WATER. R. Ishimaru1, N. Miyake1, G. Komatsu2, K. Kawai3, M. Kobayashi4, H. Sakuma5, T. Matsui1 1Planetary Exploration Research Center (PERC), Chiba Institute of Technology (Chitech) (2-17-1 Tsudanuma, Narashino, Chiba 275-0016, Japan;
[email protected]), 2International Research School of Planetary Sciences, Università d'Annunzio (Viale Pindaro 42, 65127 Pescara, Italy), 3Department of Earth and Planetary Science, School of Science, University of Tokyo (Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan), 4Department of Earth and Planetary Environmental Sci- ence, School of Science, University of Tokyo (Hongo 7-3-1, Bunkyo, Tokyo 113-0033, Japan), 5Reseach Center for Functional Materials, National Institute for Materials Science (1-1 Namiki, Tsukuba, 305-0044 Japan). Introduction: Mud volcanoes occur everywhere Gas sampling and laboratory analysis. Gases were in various geological settings on the Earth [e.g., 1] and, collected with a custom-made sampling device for possibly, on other planetary bodies, such as Mars [e.g., laboratory measurement of the gas species. The com- 2] and Enceladus ocean floor. Their surface terrains position analysis of the gas samples in the chamber are formed by mud ascending and erupting, together was conducted using Gas Chromatography (GS) in the with water and gas, from depths. Therefore, mud vol- laboratory. The GC analyses are made in two ways: cano is one of the most suitable landforms for explor- qualitative and quantitative analyses.