VESTA LAB
LIGHT
SITE
SOURCE / LIMITS
Global elevation is derived offline from the DLR/PDS Dawn FC2 HAMO stereo radius DTM (64 pixels/degree, about 69.5 m/pixel) and stored in static shared-edge terrain packs. Broad surface brightness comes from the Dawn FC HAMO clear-filter mosaic. Source longitudes are converted from the legacy Dawn-Claudia frame to the current IAU Claudia Double Prime frame. Display colour, fine grain, rocks, hazards, routes, missions, and the fictional rover are synthetic educational layers. No live API is used. Not endorsed by NASA, USGS, DLR, or the Dawn mission; not for mission planning or navigation.
LOADING VESTA TERRAIN…
ROVER TELEMETRY
RISK GO
SLOPE 0.0 deg
POSITION 0, 0
SPEED 0.0 sim-m/s
MODE
MANUAL
RISK
GO
SLOPE
0.0 deg
BATTERY
100%
SPEED
0.0 sim-m/s
HEADING
000
POSITION
0, 0
MISSION
T+00:00
MISSION OBJECTIVES
0/3
ROUTE PLAN
0 WAYPOINTS
LOCAL PATCH
VESTA LOCATION
HEADLIGHT
FLIGHT PHASE PARKED