Japanese/English September 10, 2009 |
A research paper co-authored by faculty members of the University of Aizu,
affiliated to CAIST/ARC-Space (the Research Center for Advanced Information Science
and Technology / the Aizu Research Cluster for Space Science), was published in
a British science journal, "Nature" issued on September 10, 2009.
(The University of Aizu Campus News)
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In this paper, our faculty members made
contributions through provision of spectral-analyzer software to estimate mineral
composition from reflected spectrum of the lunar surface materials and analysis
on how the crusts of the lunar highland were exposed in the inside of lunar craters.
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The relevant faculty members of the University
have been a part of the team of LISM (Lunar Imager/SpectroMeter) since the early
planning stages of the KAGUYA project. They participated in development and
tests of mission instruments and software development for data analysis.
They conducted research on means of data compression to send image data observed by
the Multi-band Imager (MI) efficiently, and developed software for operation of
observation instruments. The results from the University's research were used to
obtain observational data for LISM. With the Grant-in-Aid for Scientific Research,
the University started research on a lunar surface GIS (Geographic Information
System) server which can visualize data observed by KAGUYA two years ago.
To promote further research and development of analytical software, the University
newly recruited young researchers with great experience gained in the KAGUYA project
to CAIST/ARC-Space established in April of this year.
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The University will carry out further analysis
to acquire more scientific output from the observational data obtained by KAGUYA in
cooperation with JAXA and other related research institutions, and will also promote
software development aiming at more efficient and accurate analysis.
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- Co-authors of the research paper from the University of Aizu
- Professor Noriaki Asada, the Multimedia Systems Laboratory
- Assistant Professor Hirohide Demura, the Multimedia Systems Laboratory and CAIST/ARC-Space
- Assistant Professor Naru Hirata, the Multimedia Systems Laboratory and CAIST/ARC-Space
- Assistant Professor Yoshiko Ogawa, CAIST/ARC-Space
- Assistant Professor Chikatoshi Honda, CAIST/ARC-Space
- Assistant Professor Kohei Kitazato, CAIST/ARC-Space
- Assistant Lecturer Junya Terazono, the Database Systems Laboratory and CAIST/ARC-Space
- Lead author and co-authors of the research paper invited to the University of Aizu Graduate School as adjunct professors
- Dr. Makiko Ohtake, JAXA (Lead author)
- Dr. Junichi Haruyama, JAXA
- Dr. Yasuhiro Yokota, JAXA
- Dr. Tomokatsu Morota, JAXA
- Dr. Akira Sasaki, the National Astronomical Observatory of Japan
- *Listed in order of the chapters
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The research paper was based on observational data obtained by the Multiband
Imager onboard "KAGUYA" (SELENE). As a result of analyzing the mineral
distribution on the entire lunar surface observed by the Multiband Imager onboard
the lunar orbiting satellite "SELENE" (KAGUYA), this paper clarified for
the first time in the world that anorthosite (*1) consisting of nearly 100% anorthite
was widely distributed in the lunar highland crust. JAXA provides more details about
the research at its official Press Release site.
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Multiband Imager (MI) is one of the observation instruments onboard "KAGUYA". This is one of
three optical observation instruments (TC: Terrain Camera, SP: Spectral Profiler and
MI) installed on "KAGUYA". This article is recognized as the first research
achievement on the Moon using MI observational data. It is written by a lead author,
Assistant Professor Makiko Ohtake, Department of Planetary Science, Institute of Space
and Astronautical Science, Japan Aerospace Exploration Agency, Principal Investigator of
MI Observation Instrument Team (Adjunct Professor of the University of Aizu Graduate School) and
31 other researchers of the team from both Japan and other countries.
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(*1) A white igneous rock rich in minerals called anorthite made of calcium, aluminum, silicon, and oxygen is called anorthosite.
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