Saudi Analogs · NASA Space Apps 2026
Explore Earth's planetary analogues in Saudi Arabia.
Craters, lava tubes, volcanic fields, dunes, sinkholes and salt flats that resemble the Moon and Mars, each backed by published evidence and matched to the problems past missions actually hit.
Find a test site
Tell us what you need to test. We point you to the Saudi site.
Pick where your mission is going, the terrain you need and what you are testing. Results are ranked by how many of your needs a site meets, then by the strength of its published evidence.
Virtual field visit
Walk the terrain, then see it as the Moon or Mars.
Pick a site, switch the surface between Earth, Moon and Mars, and turn on a dust storm. Use Walk mode to stand at ground level.
Pick a route to see its length and slope. Turn on Compare and press Drive to ride the same route on Earth and on the Moon or Mars at once. On a VR headset browser with WebXR, an Enter VR button appears and puts you on the route at real scale. Full headset support with base-building tools is our next step. Slope ratings are illustrative until our rover mobility criterion is final.
Compare splits the view: the site on Earth beside the same ground as the Moon or Mars. Move the Sun to see how much ground falls into shadow; on the Moon the Sun skims 1.5° above the horizon, as at the south-pole base sites. Orbit: drag to rotate, scroll or pinch to zoom. Walk: W A S D or arrow keys, drag to look. Drive: ride along the selected rover route. On the public site each terrain is built from real SRTM elevation with satellite imagery on top; elsewhere an illustrated model is shown.
The problem
Missions keep failing to the same environments.
Dust, cold, darkness and loose ground have ended or crippled missions for sixty years. Testing on Earth helps only if the test site reproduces the right combination of conditions.
Can we predict how space systems degrade under repeated environmental stress, and point to the Earth sites where those scenarios can be tested before launch?
Mission replay
Watch a mission fail. Then find where to test the fix.
Step through what happened, using figures NASA published at the time. Each replay ends with the Saudi site and season that reproduce the same stress.
Candidate analog sites
Saudi analog sites, backed by published evidence.
Every value below comes from a cited study. We do not calculate similarity percentages; each site shows its evidence grade, what was measured, and what was not proven. Candidates are sites our team proposed that still need published evidence.
Illustrated relief map · satellite imagery loads on the public site
Pin colour: blue Moon, red Mars · darker = stronger evidence (grade A → C) · dashed = candidate
Start here
What would you like to do?
Choose the destination, terrain and test. Get ranked Saudi sites.
→To scaleAl Wahbah beside a lunar south-pole crater, at the same scale.
→3D tourReal terrain seen as Earth, Moon or Mars, with rover routes and VR.
→Mission replaysHow dust, sand and rocks ended missions, and where to test the fix.
→Test planningCombine stresses into a test scenario and weigh site readiness.
→About & sourcesMethod, limits, judging criteria, 20 references and the team.
To scale
Al Wahbah next to a lunar south-pole crater.
Shackleton, a candidate area for a permanent Moon base, is about ten times wider. Shape matters too: depth ÷ diameter tells you how steep the walls are.
Simplified profiles from published diameter and depth. Sources: LRO / LOLA for Shackleton; published surveys for Al Wahbah, to be checked against NASADEM.
Engineering readiness score
Weigh what matters for your mission.
Each criterion is scaled 0–100 and multiplied by its weight. Missing criteria are left out and the weights re-normalised, and coverage tells you how much of the score rests on real data. Scores below are sample values for the demo.
Test scenario planner
Choose a system and the stresses. Get a site and a season.
The planner combines two or more environmental factors and returns Saudi sites and months where they occur together, linked to the mission failure they would help prevent.
Weather data alone cannot prove material resistance. A real test still needs samples and instruments on site. Seasons are indicative and still need NASA POWER records for each site.
How it works
From satellite pixels to a test plan.
Discover
Find under-documented craters, sinkholes and cavities from imagery and literature.
Measure
Diameter, depth and rim slope from NASADEM / SRTM elevation (≈30 m).
Compare
Match to lunar and Martian features using Moon Trek, Mars Trek, LRO Diviner and HiRISE.
Score
Weighted readiness across stability, mobility, thermal, light and shelter.
Recommend
Pair sites and seasons with a system and the failures it must survive.
Limits of the analog
What the desert cannot reproduce.
Being clear about differences makes the results credible.
1 g on Earth, 0.17 g on the Moon, 0.38 g on Mars. Soil and wheel behaviour change with it.
No air on the Moon and 0.6 % of Earth's pressure on Mars. Heat moves very differently.
Earth's magnetic field and air block most of what reaches lunar and Martian surfaces.
Al Wahbah is about 2 km wide. Shackleton crater at the lunar south pole is about 21 km.
SRTM's ≈30 m pixels can miss small pits and skylights. Higher-resolution sources will be cited separately.
Lunar regolith is sharp and electrostatically charged. Desert sand is rounded by wind.
Judging criteria
How ASTRIX answers each criterion.
Points engineers to a real Saudi site and season for tests that could have helped Opportunity, InSight and Spirit.
See Mission replay 02CreativityThe same ground seen as Earth, Moon and Mars, side by side, with a movable Sun and a rover-route VR preview. Failures are linked to places, not only to terrain.
Try Compare 03Validity20 cited studies with evidence grades, published measurements only, no invented similarity scores, and stated limits for every site.
See To scale 04RelevanceAnswers the challenge directly: Saudi analogs for lunar south-pole base sites and for Mars, with low-angle polar lighting.
See the sites 05PresentationOne public link that runs in any browser and walks from problem to recommended test in under five minutes.
Back to homeReferences
Sources
Studies cited on this page, with links to the original publisher. NASA data on this page: GIBS imagery layers (VIIRS true colour, MODIS land surface temperature, ASTER GDEM relief) and SRTM elevation for the 3D terrain. NASA data for the next comparison step: Moon Trek, Mars Trek, Earthdata Search, NASA POWER, NASADEM / SRTM, LRO Diviner and HiRISE.
Team ASTRIX