Compositional groups are defined in residue from Stardust craters (1-9 Dc) by qualitative EDS. These compositional groups are being further studied by a FIB-SEM technique to determine representative residue compositions
The Stardust Interstellar Preliminary Examination team analyzed thirteen Al foils from the NASA Star...
A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine ...
International audienceThe Stardust Interstellar Preliminary Examination team analyzed thirteen Al fo...
We describe results from a new technique using dual beam FIB/SEM with which impact residues can be e...
Implications for the Wild-2 dust distribution of the statistical results obtained by SEM-EDS from ne...
Over the last decade, silica aerogel tracks and aluminum foil craters on the Stardust collector have...
We will present preliminary results on the nature and size frequency distribution of microcraters th...
The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...
Introduction: Preliminary Examination (PE) of the Stardust cometary collector revealed many tracks i...
In January 2006, the sample return capsule from NASA s Stardust spacecraft successfully returned to ...
The known encounter velocity (6.1kms{sup -1}) between the Stardust spacecraft and the dust emanating...
The known encounter velocity (6.1kms-1) and particle incidence angle (perpendicular) between the Sta...
Stardust Track 121 terminal grains contain Fe-oxide. These are consistent with the presence of hydro...
The NASA Stardust mission collected samples of particles in the tail of the Jupiter-family comet Wil...
Prior to their retrieval from low Earth orbit (LEO), the individual solar cells that make up the 'V2...
The Stardust Interstellar Preliminary Examination team analyzed thirteen Al foils from the NASA Star...
A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine ...
International audienceThe Stardust Interstellar Preliminary Examination team analyzed thirteen Al fo...
We describe results from a new technique using dual beam FIB/SEM with which impact residues can be e...
Implications for the Wild-2 dust distribution of the statistical results obtained by SEM-EDS from ne...
Over the last decade, silica aerogel tracks and aluminum foil craters on the Stardust collector have...
We will present preliminary results on the nature and size frequency distribution of microcraters th...
The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...
Introduction: Preliminary Examination (PE) of the Stardust cometary collector revealed many tracks i...
In January 2006, the sample return capsule from NASA s Stardust spacecraft successfully returned to ...
The known encounter velocity (6.1kms{sup -1}) between the Stardust spacecraft and the dust emanating...
The known encounter velocity (6.1kms-1) and particle incidence angle (perpendicular) between the Sta...
Stardust Track 121 terminal grains contain Fe-oxide. These are consistent with the presence of hydro...
The NASA Stardust mission collected samples of particles in the tail of the Jupiter-family comet Wil...
Prior to their retrieval from low Earth orbit (LEO), the individual solar cells that make up the 'V2...
The Stardust Interstellar Preliminary Examination team analyzed thirteen Al foils from the NASA Star...
A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine ...
International audienceThe Stardust Interstellar Preliminary Examination team analyzed thirteen Al fo...