We examined the Al-Mg isotope systematics of plagioclase in a FeO-poor ferromagnesian Wild 2 particle (0092,7,81,1,0; named Pyxie) using a similar to 2 mu m spot. Three analyses show average Al-27/Mg-24 ratio of similar to 65 and excess delta Mg-26* value of +0.1 +/- 4.5%0 (2 sigma), indicating no resolvable Mg-26 excess in the particle. The inferred initial (Al-26/Al-27)(0) ratio of plagioclase in Pyxie is estimated as (-0.6 +/- 4.5) x 10(-6) with an upper limit of 4 x 10(-6). The result is very similar to that of the FeO-rich ferromagnesian particle "Iris" (Ogliore et al., 2012). Assuming homogeneous distribution of Al-26 in the early solar system, Pyxie formed at least 2.6 Ma after the oldest Ca-Al-rich inclusions. This minimum formation age is marginally younger than formation ages of most chondrules in type similar to 3.0 chondrites but comparable with those of Mg# < 98 chondrules in CR3 chondrites. Considered in conjunction with similar oxygen isotope ratios between Pyxie (and Iris) and Mg# < 98 chondrules in CR3 chondrites, it is inferred that the ferromagnesian Wild 2 particles and Mg# < 98 chondrules in CR3 chondrites formed late in local disk environments that had similar oxygen isotope ratios and redox states. (C) 2014 Elsevier B.V. All rights reserved.