Cool Stars 14 - Submitted Abstract # 302 This version created on 05 October 2006 The SPICA mission and the MIR-coronagraph for SPICA Keigo Enya, ISAS/JAXA Shinichro Tanaka, Univ. of Tokyo, Japan Lyu Abe, NAOJ Takao Nakagawa, ISAS/JAXA Hirokazu Kataza, ISAS/JAXA Olivier Guyon, SUBARU/NAOJ Melanie Venet, Univ. of Nice, France Takashi Miyata, IoA, Univ. of Tokyo, Japan Shigeyuki Sako, IoA, Univ. of Tokyo, Japan Naoshi Murakami, NAOJ Jun Nishikawa, NAOJ Motohide Tamura, NAOJ Kenta Fujita, Univ. of Kobe, Japan Yoich Itoh, Univ. of Kobe, Japan SPICA working group We introduce the Space Infrared Telescope for Cosmology and Astrophysics(SPICA) mission and the mid-infrared coronagraph for SPICA. SPICA is the next generation mission of space telescope for infrared astronomy following to AKARI. 3.5 m telescope will be cooled down to 4.5 K for observation at 5-200 micron wavelength. The launch of the SPICA is planed to be middle of 2010th. We are developing an mid-infrared coronagraph for the SPICA mission. First, binary pupil masks were studied as a safe solution because of their robustness. Laboratory experiment with the checkerboard-type binary masks were performed using visible light. Achieved contrast averaged in the dark region of the point spread function was 1.1 * 10^-7 without wave front control. Study of Phase induced amplitude apodization (PIAA) and Prolate Apodized Lyot Coronagraph (PALC) are undergoing for challenging solutions. We are developing cryogenic tip-tilt mirror system and deformable mirror for SPICA. ----------------------------------