Wide-field (～8' x 8') and deep near-infrared (JHK_s bands) polarization images of the Orion Nebula are presented. These data revealed various circumstellar structures as infrared reflection nebulae (IRNe) around young stellar objects (YSOs), both massive and low-mass. We found the IRN around both IRc2 and BN to be very extensive, suggesting that there might be two extended ( > 0.7 pc) bipolar/monopolar IRNe in these sources. We discovered at least 13 smaller scale (～0.01-0.1 pc) IRNe around less massive YSOs, including the famous source θ~2 Ori C. We also suggest the presence of many unresolved ( < 690 AU) systems around low-mass YSOs and young brown dwarfs showing possible intrinsic polarizations. Wide-field infrared polarimetry is thus demonstrated to be a powerful technique in revealing IRNe and hence potential disk/outflow systems among high-mass to substellar YSOs.
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