Fig. 2: SEM BSE images of a hollow Fe-Ni metal bleb.
From: Pinpointing the thermal history of lunar basaltic meteorites in a nutshell
a Fe-Ni-rich glass (dotted lines) located between the outer border of the rim and the nearby phases (mostly plagioclase glass), and within the free space left by the large internal cavity. b Close-up view of the square shown in (a) focusing on the globular melting features within the rim and at the interface between the rim and the Fe-Ni-rich glass (see also Fig. S4).
