Interplanetary dust particles.

By J. Bradley, S. Sandford, R. Walker. 2003

266 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/77953a1e01ef6ec7e907c9311bcdd5724f1fc838

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Citations in the corpus

• Thermal infrared (vibrational) spectroscopy of Mg–Fe olivines: A review and applications to determining the composition of planetary surfaces (2010, methodology): “For example, microscopic TIR spectroscopy has been used in the classification of chondritic IDPs, establishing that there are three primary classes, one of which is dominated by olivine (c.f., Bradley, 2004).”
• Ultra-primitive interplanetary dust particles from the comet 26P/Grigg–Skjellerup dust stream collection (2009, background): “It is highly debated whether GEMS are (Bradley et al., 1999; Keller et al., 2000) or are not (Keller and Messenger, 2004, 2008) of presolar origin too.”
• Chondrules and the Protoplanetary Disk (2011, background): “…and nearly isotropic comets and laboratory studies of cometary IDPs show that comets, like chondrite matrices, contain submicrometer crystals of FeO-poor olivines and pyroxenes and amorphous silicate grains of comparable size (Bradley 2003, Harker et al. 2005, Nuth et al. 2005, Wooden et al. 2006).”
• Redox Conditions in the Solar Nebula: Observational, Experimental, and Theoretical Constraints (2008, methodology): “The mean mole fraction of fayalite, XFa , in olivine is 0.05 to 0.10 in CI and CM chondrites, ~0.07 in chondrules of CV chondrites, 0.38 in R chondrites, ~0.50 in the matrices of CO and CV chondrites (Brearley and Jones 1998), and ~0.10 in interplanetary dust particles (Rietmeijer 1998).”
• The nature of molecular cloud material in interplanetary dust (2004, background): “Interplanetary dust particles (IDPs) collected in the Ea stratosphere are fragments of asteroids and comets th largely unsampled by collected meteorites (Bradley et al. 1988).”