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Samples of Stars Beyond the Solar System: Silicate Grains in Interplanetary Dust
Scott Messenger,1Lindsay P. Keller,2Frank J. Stadermann,1Robert M. Walker,1Ernst Zinner1
We have identified six circumstellar silicate grains within
interplanetary dust particles (IDPs). Their extrasolar originsare
demonstrated by their extremely anomalous oxygen isotopiccompositions.
Three 17O-rich grains appear to originate from red giant or
asymptoticgiant branch stars. One 16O-rich grain may be
from a metal-poor star. Two 16O-poor grains have unknown
stellar sources. One of the grainsis forsterite, and two are amorphous
silicate "GEMS" (glass withembedded metal and sulfides), which is
consistent with astronomicalidentifications of crystalline and
amorphous silicates in theoutflows of evolved stars. These
observations suggest cometaryorigins of these IDPs and underscore
the perplexing absence ofsilicates among circumstellar dust
grains from meteorites.
1 Laboratory for Space Sciences and Physics
Department, Washington University, St. Louis, MO 63130, USA.
2 Mail Code SR, NASA Johnson Space Center, Houston,
TX 77058, USA.
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PERSPECTIVES
A. G. G. M. Tielens (4 April 2003) Science300 (5616), 68.
[DOI: 10.1126/science.1082234] |Summary »|Full Text »|PDF »
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