The bulk of the comet 81P/Wild 2 (hereafter Wild 2) samples returned to Earth by the Stardust spacecraft appear to be weakly constructed mixtures of nanometer-scale grains, with occasional much larger (over 1 micrometer) ferromagnesian silicates, Fe-Ni sulfides, Fe-Ni metal, and accessory phases. The very wide range of olivine and low-Ca pyroxene compositions in comet Wild 2 requires a wide range of formation conditions, probably reflecting very different formation locations in the protoplanetary disk. The restricted compositional ranges of Fe-Ni sulfides, the wide range for silicates, and the absence of hydrous phases indicate that comet Wild 2 experienced little or no aqueous alteration. Less abundant Wild 2 materials include a refractory...
The presence of crystalline silicates in the comae of comets, inferred through infrared observations...
The bulk of the Wild 2 samples appear to be weakly-constructed mixtures of nanometerscale grains wit...
We have used synchrotron Fe-XANES, XRS, microRaman, and SEM-TEM analyses of Stardust track 41 slice ...
The bulk of the comet 81P/Wild 2 (hereafter Wild 2) samples returned to Earth by the Stardust spacec...
The bulk of the comet 81P/Wild 2 ( hereafter Wild 2) samples returned to Earth by the Stardust space...
The nature of cometary solids is of fundamental importance to our understanding of the early solar n...
The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to ...
The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to ...
The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to ...
Infrared spectra of material captured from comet 81P/Wild 2 by the Stardust spacecraft reveal indige...
The mineralogy of comet 81P/Wild 2 particles, collected in aerogel by the Stardust mission, has been...
We measured the elemental compositions of material from 23 particles in aerogel and from residue in ...
The fragile structure of chondritic-porous interplanetary dust particles (CP-IDPs) and their minimal...
We have used synchrotron Fe-XANES, XRS, micro Raman, and SEM-TEM analyses of Stardust track 41 slice...
The fragile structure of chondritic-porous interplanetary dust particles (CP-IDPs) and their minimal...
The presence of crystalline silicates in the comae of comets, inferred through infrared observations...
The bulk of the Wild 2 samples appear to be weakly-constructed mixtures of nanometerscale grains wit...
We have used synchrotron Fe-XANES, XRS, microRaman, and SEM-TEM analyses of Stardust track 41 slice ...
The bulk of the comet 81P/Wild 2 (hereafter Wild 2) samples returned to Earth by the Stardust spacec...
The bulk of the comet 81P/Wild 2 ( hereafter Wild 2) samples returned to Earth by the Stardust space...
The nature of cometary solids is of fundamental importance to our understanding of the early solar n...
The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to ...
The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to ...
The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to ...
Infrared spectra of material captured from comet 81P/Wild 2 by the Stardust spacecraft reveal indige...
The mineralogy of comet 81P/Wild 2 particles, collected in aerogel by the Stardust mission, has been...
We measured the elemental compositions of material from 23 particles in aerogel and from residue in ...
The fragile structure of chondritic-porous interplanetary dust particles (CP-IDPs) and their minimal...
We have used synchrotron Fe-XANES, XRS, micro Raman, and SEM-TEM analyses of Stardust track 41 slice...
The fragile structure of chondritic-porous interplanetary dust particles (CP-IDPs) and their minimal...
The presence of crystalline silicates in the comae of comets, inferred through infrared observations...
The bulk of the Wild 2 samples appear to be weakly-constructed mixtures of nanometerscale grains wit...
We have used synchrotron Fe-XANES, XRS, microRaman, and SEM-TEM analyses of Stardust track 41 slice ...