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• W3100691697 endingPage "L41" @default.
• W3100691697 startingPage "L41" @default.
• W3100691697 abstract "Recently acquired evidence shows that extrasolar asteroids exhibit over a factor of 100 variation in the iron to aluminum abundance ratio. This large range likely is a consequence of igneous differentiation that resulted from heating produced by radioactive decay of 26Al with an abundance comparable to that in the solar system's protoplanetary disk at birth. If so, the conventional view that our solar system began with an unusually high amount of 26Al should be discarded." @default.
• W3100691697 created "2020-11-23" @default.
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• W3100691697 date "2013-09-18" @default.
• W3100691697 modified "2023-10-14" @default.
• W3100691697 title "²⁶ Al IN THE EARLY SOLAR SYSTEM: NOT SO UNUSUAL AFTER ALL" @default.
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• W3100691697 doi "https://doi.org/10.1088/2041-8205/775/2/l41" @default.
• W3100691697 hasPublicationYear "2013" @default.
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