Lat/Lon: 0.0000, 0.0000

Map Layers

Slope Classes
πŸš€ 2Β°
Ice Probability
THEMIS Thermal Inertia
Ocean Level
MCD Surface Weather β“˜

About this layer

Climatological averages from the Mars Climate Database β€” not real-time observations. Read each value as a long-term mean for the selected season and time of day.

  • Ls (areocentric solar longitude) is the season angle. 0Β° = northern spring equinox, 90Β° = northern summer solstice, 180Β° = northern autumn equinox, 270Β° = northern winter solstice.
  • LTST is local true solar time in 2-hour steps.
  • Grid is 5.625Β° Γ— 3.75Β° (~330 Γ— 220 km). Position inside one cell does not change the value.
  • Wind is the climatological mean surface wind vector, not gusts or instantaneous flow. It drives the Monte Carlo cloud drift.

Limitations: coarse grid, one dust scenario at a time, no storm-scale events. Use for planning context, not final engineering numbers.

β“˜
Ls (season) β“˜ 0–30Β° Β· N. spring
LTST (hour) β“˜ 02:00
Opacity 70%
Default
Satellite (zoom 3+)
No basemap
TerrainWhere it is safe to land
Safety limitsFail these β†’ cell excluded (red, dashed border)
Max landing elevation β“˜ βˆ’2000 m
βˆ’5000m βˆ’4000m βˆ’3000m βˆ’2000m βˆ’1000m 0m
Cells above this turn red (excluded). Moves the green/red boundary β€” NASA baseline: βˆ’2000m.
Thermal Inertia safe range β“˜ 200–800 TIU
0 100 200 350 500 800 1400 TIU
Cells outside this range β†’ excluded (red). Only applies where THEMIS data exists.
Terrain steepnessRight handle excludes (red). Left handle only hides.
Terrain Steepness β“˜ 0–15Β°
0Β° 5Β° 10Β° 15Β° πŸš€ 2Β°
Steeper than the right handle is excluded (red). Flatter than the left handle is hidden, not marked unsafe. NASA hard limit: 15Β°; Starship target: 2Β°.
View filtersOutside these β†’ cell hidden from view (not marked unsafe)
|Latitude| range 0–90Β°
0Β° 30Β° 60Β° 90Β°
NASA solar power limit: ≀30Β°. Starship may tolerate more.
Shown elevation band βˆ’6000β€“βˆ’1000m
βˆ’6000m βˆ’4000m βˆ’2000m βˆ’1000m
Hides safe cells outside this band (does not mark them unsafe). Deeper = denser atmosphere.
Excluded cells (dashed red border) fail a safety limit: elevation, slope >15Β°, craters, or thermal inertia.
Opacity: 80%

Mars Exploration Service

Interactive map of Martian (sub)surface

About us

100 km
Credits | Map: marscarto.com

Sources

Basemap
Default
OpenPlanetaryMap - MOLA global terrain tiles
Satellite
NASA/JPL/MSSS/The Murray Lab - CTX Global Mosaic
Data
Craters
Robbins & Hynek (2012), global Mars impact crater database β‰₯1 km
Sub-km Craters
Lagain, A. et al. (2021), Nature Communications, doi: 10.1038/s41467-021-26648-3
Topography
OpenPlanetaryMap - Mars Topography Contours
Hydrography
Goudge, T. A. et al. (2021), Nature, doi: 10.1038/s41586-021-03860-1
Lava Tube Caves
USGS Mars Global Cave Candidate Catalog
Subsurface Ice (SWIM)
Morgan, G. A., Putzig, N. E., et al. (2025), Planet. Sci. J., doi: 10.3847/PSJ/ad9b24
Thermal Inertia (THEMIS)
Putzig, N. E., et al. (2013), MARSTHERM, AGU Abstract P43C-2023 β€” underlying data: NASA/JPL-Caltech/Arizona State University (THEMIS)
HiRISE Imagery
NASA/JPL/University of Arizona/USGS/Esri - MRO HiRISE Uncontrolled Mosaic
Atmosphere / Climate (MCD)
Mars Climate Database (c) LMD/LATMOS/OU/IAA/ESA/CNES. F. Forget, E. Millour, M. Vals, V. Zakharov, T. Pierron (LMD) and S.R. Lewis (OU)
Analyzing this area…