This anomalous abundance is attributed to the decay of its parent 26 Al in the inclusions, and researchers conclude that such meteorites were formed in the solar nebula before the 26 Al had decayed.
Kelimpahan anomali ini disebabkan oleh peluruhan induknya 26Al dalam inklusi, dan para peneliti menyimpulkan bahwa meteorit semacam itu terbentuk di nebula surya sebelum 26Al meluruh.