Resource Detailed View
The facility is designed to study the interaction of micro-grain impacts with target materials like planetary analogues, metals or interplanetary dust collector materials.
Dust grain materials from nano to micron sizes are accelerated, using a 2 MV Van-de-Graaff accelerator, to velocities between 1 and 60 km/s.
The accelerator can be operated in a single-shot mode and in a continuous mode.
Keywords (11):
atmospheric dust
Bepicolombo
comet nuclei
cometary dust
Comets
DUST
interplanetary dust
PLANETS
Rosetta
TNA-facility
Ulysses
Bepicolombo
comet nuclei
cometary dust
Comets
DUST
interplanetary dust
PLANETS
Rosetta
TNA-facility
Ulysses
Science Cases (2):
SC4.3 - Distant activity, outbursts, splitting and disruption of cometary nuclei
SC4.4 - Comet Churyumov-Gerasimenko outgassing
SC4.4 - Comet Churyumov-Gerasimenko outgassing




