Author/Authors :
T. Okada، نويسنده , , M. Kato، نويسنده , , K. Shirai، نويسنده , , Y. Yamamoto، نويسنده , , T. Matsuda، نويسنده , , H. Tsunemi، نويسنده , , S. Kitamoto، نويسنده ,
Abstract :
X-ray fluorescence spectrometry of a near-earth asteroid has been planned to determine major elemental composition of the asteroid surface and its regional variation from the MUSES-C orbiter, which will be launched in 2002 by the M-V vehicle. We present the characteristics of the XRS instrument and its observation plan during the mission. We numerically simulated x-ray fluorescence spectrometry of asteroid that rotates in 19-hour period and has surface geologic anomaly and we investigated achievable spatial resolution through the XRS observation during the asteroid rendezvous phase.