Strocera

Lunar dust mitigation.

Apollo-traceable simulant for dust-mitigation research on landers, suits, and lunar surface hardware.

STROCERA / / / Regolithia / / / Space
[ 01 ]The challenge

Lunar dust is fine, electrostatically charged, and abrasive, and its real behaviour can only be studied against a regolith analogue with documented mineralogical fidelity. Generic dust does not transfer.

Schematic, illustrativeRegolithia
[ 02 ]The Strocera approach

Regolithia delivers Highland and Mare references at phase match 96.4 % and 99.2 %, supplied as a sub-75 µm silicate powder with alternative size fractions on request for the test campaign. Detailed test-specific specifications available on request. Bring the operating conditions and we will scope the engagement.

Full Regolithia spec
[ 03 ]Specifications for this use case
Property
Value
Method
Phase match, Highland (RGS-H1)
96.4 %
4 modelled phases; XRD and SEM-EDS
Phase match, Mare (RGS-M1)
99.2 %
4 modelled phases; XRD and SEM-EDS
Dv(10/50/90), Highland
2.93 / 8.84 / 74.0 µm
Laser diffraction, wet mode
Dv(10/50/90), Mare
3.29 / 10.4 / 74.1 µm
Laser diffraction, wet mode
Size cut
< 75 µm mesh
Sieve
Alternative size fractions
On request
[ 04 ]Validation status
Lab-validated

Apollo-traceable feedstock; campaign-specific dust profiles configured on request.

[ 05 ]Customer profile

Dust-mitigation engineers for landers, EVA suits, and lunar surface hardware.

[ 06 ]Adjacent use cases

Engineers working on this often also evaluate:

Bring your specification for Lunar dust mitigation.

Tell us the operating conditions. We'll formulate Regolithia to your application, and ship simulant matched to your particle specification and volume.