Implications for the Wild-2 dust distribution of the statistical results obtained by SEM-EDS from nearly 300 impact craters on aluminium foils of the Stardust sample tray assembly
Aluminium foils exposed to impact during the passage of the Stardust spacecraft through the coma of ...
The NASA Stardust spacecraft deployed two collector trays, one dedicated to the collection of dust f...
Preliminary Examination (PE) of the Stardust cometary collector revealed material embedded in aeroge...
We will present preliminary results on the nature and size frequency distribution of microcraters th...
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...
Over the last decade, silica aerogel tracks and aluminum foil craters on the Stardust collector have...
Introduction: Preliminary Examination (PE) of the Stardust cometary collector revealed many tracks i...
Compositional groups are defined in residue from Stardust craters (1-9 Dc) by qualitative EDS. These...
In January 2006, the sample return capsule from NASA s Stardust spacecraft successfully returned to ...
Aluminum foils of the Stardust cometary dust collector are peppered with impact features of a wide r...
The known encounter velocity (6.1 kms(-1)) and particle incidence angle (perpendicular) between the ...
The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...
Impact ionisation detectors on a suite of spacecraft have shown the direction, velocity, flux and ma...
From 1999 to 2006 the NASA Stardust mission collected cometary particles from the Wild 2 comet and i...
Aluminium foils exposed to impact during the passage of the Stardust spacecraft through the coma of ...
The NASA Stardust spacecraft deployed two collector trays, one dedicated to the collection of dust f...
Preliminary Examination (PE) of the Stardust cometary collector revealed material embedded in aeroge...
We will present preliminary results on the nature and size frequency distribution of microcraters th...
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...
Over the last decade, silica aerogel tracks and aluminum foil craters on the Stardust collector have...
Introduction: Preliminary Examination (PE) of the Stardust cometary collector revealed many tracks i...
Compositional groups are defined in residue from Stardust craters (1-9 Dc) by qualitative EDS. These...
In January 2006, the sample return capsule from NASA s Stardust spacecraft successfully returned to ...
Aluminum foils of the Stardust cometary dust collector are peppered with impact features of a wide r...
The known encounter velocity (6.1 kms(-1)) and particle incidence angle (perpendicular) between the ...
The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...
Impact ionisation detectors on a suite of spacecraft have shown the direction, velocity, flux and ma...
From 1999 to 2006 the NASA Stardust mission collected cometary particles from the Wild 2 comet and i...
Aluminium foils exposed to impact during the passage of the Stardust spacecraft through the coma of ...
The NASA Stardust spacecraft deployed two collector trays, one dedicated to the collection of dust f...
Preliminary Examination (PE) of the Stardust cometary collector revealed material embedded in aeroge...