Skip to main content
. Author manuscript; available in PMC: 2016 Jul 15.
Published in final edited form as: Earth Planet Sci Lett. 2015 Jun 15;420:45–54. doi: 10.1016/j.epsl.2015.03.028

Fig. 6.

Fig. 6

The available energy resulting from 26Al decay is shown in (a) versus time for a canonical (26Al/27Al)0 and that the (26Al/27Al)0 for the APB, while the same figure is shown expanded in (b) indicating also the allowable time window of APB accretion. APB accretion is assumed to occur while sufficient energy is available for large scale melting to satisfy the differentiated character of angrites. The required energy for melting and respective temperatures are from Hevey and Sanders (2006).