PLANETARY SCIENCE:
Peering into Stardust
A. G. G. M. Tielens
Stardust--the tiny interstellar dust grains that predate the formation of the solar system--are generally believed to have an anomalous isotopic composition. But as Tielens explains in his Perspective, some presolar grains may not have an anomalous isotopic composition despite similar texture, structure, and morphology. He highlights the results of Messenger et al., who found that only 6 out of 1000 GEMS particles (glass with embedded metal and sulfides)--widely believed to represent stardust--have an anomalous isotopic composition. The study suggests that the particles have been processed in the early solar system, leaving no trace of their stardust origin.
The author is at the Space Organization of the Netherlands (SRON)-Kapteyn Astronomical Institute, 9700 AV Groningen, Netherlands. E-mail: tielens{at}astro.rug.nl. This article was written while the author was at the Miller Institute and Astronomy Department, University of California, Berkeley, CA 94720, USA.