TECHLYMPICS MALAYSIA · WORLD ENGINEERING CHALLENGE 2026

AQUILA

An autonomous rover that hunts for water on Mars — not where it used to be, but where it briefly appears every dawn.

MISSION PROFILE
TargetEquatorial caldera frost sites
Launch vehicleFalcon Heavy
Mass~330 kg
Dimensions2.2 × 2.5 × 2.2 m
PowerSolar + EDS dust shielding
MobilityReconfigurable wheel–track
01 — MISSION BRIEF

Current rovers ask what Mars was. AQUILA asks what it is right now.

Curiosity and Perseverance study ancient rock for signs of past habitability. AQUILA is built for a different, forward-looking question — where is usable water today, for the missions that come after this one.

THE GAP

Water hides, and only shows itself briefly

In 2024, scientists confirmed frost forming on equatorial volcano calderas — but only for a few hours after sunrise before it evaporates. No mission has been built to specifically watch for this window.

THE RISK

Single-sensor readings get it wrong

Radar alone can mistake a rock layer for ice. Confirming the 2024 frost discovery took cross-referencing three independent datasets — a process AQUILA runs onboard, in real time.

02 — SENSOR SUITE

Three readings. One confirmed site.

No single instrument gets to make the call — a candidate site is only logged when all three independently agree.

01 / GPR

Ground-Penetrating Radar

Underside-mounted array scans continuously while driving, mapping subsurface layers down to several metres.

LAST SCAN → 1.2m, ice-like reflection
02 / NEUTRON

Neutron Spectrometer

Fires neutrons into the ground and reads the bounce-back to detect hydrogen — the telltale sign of water ice.

LAST SCAN → elevated hydrogen signal
03 / OPTICAL

Dawn Frost Camera

Mast-mounted camera watches caldera terrain at sunrise for the brief water-frost signature — AQUILA's original contribution.

LAST SCAN → frost visible, dawn window active
✓ 3 / 3 SENSORS AGREE — SITE LOGGED, BEACON DROPPED 94%
03 — MOBILITY

Reconfigurable wheel–track system

Toggle the states below — this is a real DARPA-developed mechanism, adapted here to solve a documented Mars failure.

Wheel Mode — hard ground

Round profile for fast, efficient travel across rocky terrain. This is AQUILA's default driving state.

Triggered by: default state
04 — SPEC SHEET

Sized against a real reference mission

Based on ESA's Rosalind Franklin rover — closest real analog in power source, drill depth, and instrument mix.

Mass~330 kg
Length × Width × Height2.2 m × 2.5 m × 2.2 m
Power sourceSolar array + electrodynamic dust shield
Drill depth2 m subsurface reach
Mobility6-wheel rocker-bogie, reconfigurable wheel–track
Primary sensorsGPR · Neutron spectrometer · Dawn frost camera
NavigationStereo navcams, hazcams, IMU, sun sensor
CommsUHF relay via orbiter
Launch vehicleFalcon Heavy
05 — STANDOUT INNOVATIONS

What no current rover does

A

Dawn-timed scanning schedule

Power-heavy scans are scheduled specifically around the 07:00 frost window, instead of running on a fixed daily cycle like current missions.

B

Live probability heatmap

Instead of a binary detected / not-detected flag, AQUILA outputs a confidence-scored water map future colony planners can use directly.

C

Physical beacon markers

Since frost is only visible at dawn, confirmed sites get a dropped beacon so future missions can return without re-scanning from scratch.

D

Wheel–track failure prevention

Wheel-slip sensors trigger automatic reconfiguration into track mode — solving the exact failure that stranded NASA's Spirit rover in 2009.