Flight Phase QSO-Low Approach
Altitude to Surface 1,240 m
Relative Speed 0.34 m/s
Delta-V Consumed 142.6 m/s
Sample Yield 12.4 g
Mission Status Sample Capsule Sealed for Earth Return
NAV-CAM & ORBITAL RADAR • SCALE: 1px = 4.2m • MARS TIDAL FRAME Tgt: Stickney Flank (-1.2°, 45.8°W)
PHOBOS MASS: 1.0659×10¹⁶ kg
SURFACE GRAV: 0.0057 m/s²
ESCAPE VEL: 11.39 m/s
RADAR CONTACT: ACTIVE
DESCENT STABLE: Press [THROTTLES] or Arrow Keys to steer
MMX Guidance & RCS QSO-LOCKED
Phobos resides deep inside Mars' Hill Sphere. Rather than an unstable Keplerian orbit, MMX maintains a retro-grade Quasi-Satellite Orbit (QSO). Use thruster burns below to modulate relative descent vectors.
DESCENT CRITERIA:
• Safe Touchdown Speed: < 0.50 m/s
• Phobos Escape Speed: 11.39 m/s
• Total Delta-V Budget: 450 m/s
• Touchdown Velocity: 0.18 m/s
Regolith Mass Spectrometry (RAMS) SAMPLE ANALYZED

Real-time NIR reflectance & laser ablation spectrum from core sample retrieved at Stickney Crater Flank. Resolves the 28-year planetary debate: Captured Carbonaceous Asteroid vs. Giant Impact Martian Ejecta.

Primitive Carbonaceous Chondrite
68%
Hydrated phyllo-silicates & organics
Martian Ejecta Silicates
32%
Pyroxene-olivine from ancient impact
Japan's 28-Year Mars Exploration Arc 1998 — 2026
1998
Nozomi (Planet-B) Launch: Japan’s first Mars orbiter launched by ISAS. A valve anomaly during earth flyby starved propellant reserves; despite valiant course corrections, insertion failed in Dec 2003.
2010
Hayabusa 1 & 2 Asteroid Mastery: JAXA perfects microgravity touch-and-go sampling at Itokawa and Ryugu, building the sample capsule heritage that underpins MMX.
2026
MMX (Martian Moons eXploration): Japan returns to Mars after a 28-year gap. The probe enters Quasi-Satellite Orbit around Phobos, conducts landings, and returns the first pristine Martian system samples to Earth.
SCIENTIFIC OBJECTIVE: Confirm if Mars' moons originated from a mega-impact (proto-Mars + giant impactor) or are captured outer solar system asteroids trapped by gas drag.
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