- SEARCHING FOR THE EVOLVED CRUST OF OXIDIZED ASTEROIDS. J. M. Sunshine1 (jess@astro.umd.edu), J. M. D. Day2
- DECONVOLVING TERRESTRIAL ALTERATION MINERAL SPECTRAL SIGNATURES FROM METEORITE REFLECTANCE MEASUREMENTS
- SPACE WEATHERING OF ROCK SURFACE WITHOUT REGOLITH: LABORATORY SIMULATION OF SPECTRAL CHANGE, S. Sasaki1
- OPTICAL PROPERTIES OF MARTIAN DUNITE NWA 2737: A RECORD OF MARTIAN PROCESSES. C.M. Pieters1
- IN-FLIGHT CALIBRATION OF THE HAYABUSA NEAR INFRARED SPECTROMETER (NIRS). , F. Vilas 2
- AN ATTEMPT OF RESTRICTING OLIVINE BANDS IN THE MODIFIED GAUSSIAN MODEL. T. Nimura1,2
- DERIVING THE DISTRIBUTION OF ORDINARY CHONDRITE (H, L, LL)-LIKE MATERIALS IN ASTEROIDS FROM THEIR VISIBLE AND NEAR-INFRARED REFLECTANCE SPECTROSCOPY. T.
- How much of the S-type asteroids are made of ordinary chondrite materials, and why are they so highly space-weathered? T. Hiroi1
- DETECTION OF A LARGE VARIATION IN THE DEGREE OF SPACE WEATHERING ON THE SURFACE OF ITOKAWA BY HAYABUSA/AMICA OBSERVATIONS. M. Ishiguro
- SYNCHROTRON-BASED INFRARED MICROSPECTROSCOPY AS A USEFUL TOOL TO STUDY HYDRATION STATES OF METEORITE CONSTITUENTS. L. V. Moroz1
- SPECTRAL IDENTIFICATION OF MAJOR AND MINOR CONSTITUENTS OF MARTIAN METEORITE ALH 84001 AND THE IMPORTANCE FOR REMOTE SENSING ON MARS. J. L. Bishop1
- MSSBAUER AND SYNCHROTRON MICROXANES ANALYSIS OF NWA2737. M.C. McCanta1 , A.H. Treiman1
- IMPORTANCE OF OLIVINE IN S-ASTEROID SPACE WEATHERING. T. Hiroi1 and S. Sasaki2
- PIGEONITE MASQUERADING AS OLIVINE AT MARS: FIRST RESULTS FROM MARS SPECTROSCOPY CONSORTIUM. C. M. Pieters1
- THE TAGISH LAKE METEORITE AS A POSSIBLE SAMPLE FROM A T OR D TYPE ASTEROID. T. , A. Kanno2
- ORIGIN OF SURFACE ALBEDO/COLOR VARIATION ON RUBBLE-PILE ITOKAWA: S. Sasaki1 , N. Hirata3
- REFLECTANCE SPECTROSCOPY OF MARTIAN IMPACT GLASS SIMULANTS. L. V. Moroz1, 2 , A. T. Basilevsky4
- SIMULATION OF IMPACT MELTING EFFECT ON OPTICAL PROPERTIES OF MARTIAN REGOLITH. A. T. Basilevsky1
- POSSIBLE METEORITE ANALOGS FOR ASTEROID 1989ML TARGET OF MUSES-C ASTEROID SAMPLE RETURN MISSION
- DISCOVERY OF THE FIRST D-ASTEROID SPECTRAL COUNTERPART: TAGISH LAKE METEORITE. T. Hiroi1
- LABORATORY SIMULATION OF SPACE WEATHERING: A TRANSMISSION ELECTRON MICROSCOPIC STUDY -MICROSTRUCTURES OF THE LASER IRRADIATED SAMPLES K. Nakamura1
- The Tagish Lake Meteorite: First Sample from the D Asteroids Takahiro Hiroi1*
- EFFECTS OF MICROSECOND PULSE LASER IRRADIATION ON VIS-NIR REFLECTANCE SPECTRUM OF CARBONACEOUS CHONDRITE SIMULANT: IMPLICATIONS FOR MARTIAN
- HED METEORITES: GROUND TRUTH TO INVESTIGATE PETROGENESIS ON VESTA. C. M. Pieters1
- WHAT ARE THE P-TYPE ASTEROIDS MADE OF? T. Hiroi1 , C. M. Pieters1
- NEAR-INFRARED SPECTRA OF MARTIAN PYROXENE SEPARATES: FIRST RESULTS FROM MARS SPECTROSCOPY CONSORTIUM. J. M. Sunshine (sunshinej@saic.com)1
- REFLECTANCE SPECTRA OF CM2 CHONDRITE MIGHEI IRRADIATED WITH PULSED LASER AND IMPLICATIONS FOR LOW-ALBEDO ASTEROIDS AND MARTIAN MOONS. L.V. Moroz1
- RELAB (REFLECTANCE EXPERIMENT LABORATORY): A NASA MULTIUSER SPECTROSCOPY FACILITY. Carl M. Pieters
- CHANGE OF ASTEROID REFLECTANCE SPECTRA BY SPACE WEATHERING: PULSE LASER IRRADIATION ON METEORITE SAMPLES. S. Sasaki1
- INTEGRATED SPECTROSCOPIC STUDIES OF MIL03346. M.D. Dyar1 , C.M. Pieters2
- METEORITE WIS91600: A NEW SAMPLE RELATED TO A D-OR T-TYPE ASTEROID. T. Hiroi1 , C. M. Pieters1
- INTEGRATED SPECTROSCOPIC STUDIES OF HYDROUS SULFATE MINERALS. M.D. Dyar1 , J.L. Bishop2
- OBSERVATIONS WITH NEAR INFRARED SPECTROMETER FOR HAYABUSA MISSION IN THE CRUISING PHASE. M. Abe1
- A NEW SCHEME FOR ESTIMATING THE DEGREE OF SPACE WEATHERING THROUGH VISIBLE MULTIBAND SPECTROSCOPY USING AN ECAS-TYPE FILTER SYSTEM SUCH AS HAYABUSA
- PRELIMINARY RESULTS FROM THE HAYABUSA NEAR INFRARED SPECTROMETER (NIRS) OF ASTEROID (25143) ITOKAWA. M. Abe1
- BROWN AND CLEAR OLIVINE IN CHASSIGNITE NWA 2737: WATER AND DEFORMATION. A.H. , M. McCanta1
- The S-type asteroid ordinary chondrite controversy and discoveries by the Hayabusa mission to asteroid 25143 Itokawa. T. Hiroi1
- COORDINATED SPECTROSCOPIC AND PETROLOGIC INVESTIGATION OF LAP 04840: FIRST RESULTS OF INFRARED, THERMAL AND RAMAN SPECTROSCOPY. R. Klima1
- LUNAR ROCK AND MINERAL CHARACTERIZATION CONSORTIUM (LRMCC): LINKS TO GLOBAL SCIENCE AND EXPLORATION. C. M. Pieters1
- AN INTEGRATED MODEL UTILIZING THE MODIFIED GAUSSIAN MODEL, A MINERAL-MIXING MODEL, AND A SPACE-WEATHERING MODEL. T. Nimura1,2
- MINERAL COMPOSITIONS OF THE BRIGHT RAYED CRATERS AND LUNAR FAR-SIDE CRUST REVEALED BY THE CONTINUOUS VIS-NIR SPECTRA BY SPECTRAL PROFILER ON
- REPRODUCING VISIBLE AND NEAR-INFRARED REFLECTANCE SPECTRA OF LUNAR ROCKS DIRECTLY FROM THEIR END-MEMBER SPECTRA: IMPORTANCE OF ILMENITE IN
- COORDINATED LABORATORY STUDIES OF METEORITES SUPPORTING ROSETTA MISSION'S ASTEROID FLYBY TARGET: 2867 STEINS. L.A. McFadden1
- SPECTROSCOPIC OBSERVATIONS OF ASTERIOD 4 VESTA FROM 1.9 TO 3.5 MICRON: EVIDENCE OF HYDRATED AND/OR HYDROXYLATED MINERALS. S. Hasegawa1
- NEAR-INFRAREDPHOTOMETRYOFASTEROID25143 ITOKAWABYTHENIRSONBOARDHAYABUSA. K. Kitazato1,2, B.E. Clark3, M. Abe2, S. Abe4, Y. Takagi5, and T. Hiroi6, 1Department of Earth and Planetary Sci-
- INTEGRATED SPECTROSCOPIC STUDIES OF ANYHDROUS SULFATE MINERALS. M. D. Lane1 , M. D. Dyar3
- HOW DOES SPACE WEATHERING DEPEND ON THE SURFACE CONDITION OF AIRLESS BODIES (ASTEROIDS, THE MOON, AND MERCURY)? S. Sasaki1
- SIMULATION OF SPACE WEATHERING BY NANOSECOND PULSE LASER HEATING AND PROTON IMPLANTATION: DIFFERENCE OF OLIVINE AND PYROXENE SAMPLES. M. Yamada
- CHARACTERISTICS AND CURRENT STATUS OF NEAR INFRARED SPECTROMETER FOR HAYABUSA MISSION. M. Abe1
- SEARCHING FOR THE PARENT BODIES OF METEORITES THROUGH REFLECTANCE SPECTROSCOPY: CURRENT STATE. T. Hiroi, Dept. of Geological
- AN IMPROVED SPECTROSCOPIC MODEL FOR SPACE WEATHERING THROUGH THE FORMATION OF A VAPOR DEPOSITION LAYER CONTAINING NANOPHASE REDUCED IRON
- THERMAL INFRARED SPECTROSCOPY OF A SYNTHETIC OLIVINE SERIES (FORSTERITE-FAYALITE) AND INTERPRETATION OF THE NILI FOSSAE, SYRTIS MAJOR, AND ISIDIS REGIONS
- THE LUNAR ROCK AND MINERAL CHARACTERIZATION CONSORTIUM (LRMCC): INTEGRATED ANALYSES AND MINERAL ENDMEMBERS FROM MARE BASALTS. P. J. Isaacson1
- SPECTRAL PROPERTIES OF SIMULATED MARTIAN IMPACT GLASSES. L. V. Moroz1 , A. T. Basilev-
- Photometric and Near-IR Spectroscopic Observations of a D-type Asteroid, 773 Irmintraud, by SUBARU / IRCS
- IMPROVED SCHEME OF MODIFIED GAUSSIAN DECONVOLUTION FOR REFLECTANCE SPECTRA OF LUNAR SOILS. T. Hiroi, C. M. Pieters, and S. K. Noble, Dept. of Geological Sciences, Brown
- SPECTROSCOPY OF IMPACTED SERPENTINE: IMPLICATIONS FOR ASTEROID SURFACES. A. S. Rivkin, Mas-sachusetts Institute of Technology, Cambridge MA 02139, USA, (asrivkin@mit.edu), T. Hiroi, Brown University, Providence RI,
- Antarctic Meteorites 22, National Institute of Polar Research, Tokyo (June 10-12, 1997) ORIGIN OF VESTA-LIKE ASTEROIDS SUGGESTED FROM PLANETARY
- SURFACE MATERIAL ANALYSIS OF S-TYPE ASTEROIDS: REMOVING THE SPACE WEATHERING EFFECT FROM REFLECTANCE SPECTRUM. Y. Ueda1
- THE ORIGIN OF BROWN OLIVINE IN MARTIAN DUNITE C. M. Pieters1
- EXTRACTING QUANTITATIVE DATA FROM LUNAR SOIL SPECTRA. S. K. Noble1,* , C. M. Pieters1
- EXPANDING THE MODIFIED GAUSSIAN MODEL TO INCLUDE THE SPACE WEATHERING EFFECTS: ESTIMATION OF THE WEATHERING DEGREES OF PULSE-LASER TREATED OLIVINE SAMPLES. Y.
- MODIFIED GAUSSIAN DECONVOLUTION OF REFLECTANCE SPECTRA OF LUNAR SOILS. T. Hiroi and C. M. Pieters, Dept. of Geological Sciences, Brown University, Providence, RI 02912, U. S. A. (takahiro_hiroi@brown.edu).
- INITIAL RESULTS OF MGM ANALYSIS ON APOLLO 17 SOIL SUITE. S. K. Noble , C. M. Pieters
- PETROGRAPHIC, CHEMICAL AND SPECTROSCOPIC DATA ON THERMALLY METAMORPHOSED CARBONACEOUS CHONDRITES. E. K. Tonui1
- CURRENT STATUS AND FIRST SCIENTIFIC RESULTS OF SELENE SPECTRAL PROFILER. T. Ma-, M. Ohtake2
- CHANGES OF BAND I CENTER AND BAND II/BAND I AREA RATIO IN REFLECTANCE SPECTRA OF OLIVINE-PYROXENE MIXTURES DUE TO THE SPACE WEATHERING AND GRAIN SIZE EFFECTS.
- OPTICAL PROPERTIES AND ABUNDANCES OF MINERALS AND GLASSES IN THE 10 TO 45 MICRON SIZE FRACTION OF MARE SOILS: PART II Carl M. Pieters1
- Fig. 1. MGM deconvolutons of natural log reflectance spectra of Hamlet LL4 chondrite samples of three differ-
