Moons · Space Codex

Deimos

A 15 km lump of dark rock that circles Mars every 30 hours.

Mars's small, smooth outer moon

  • Last reviewed 10 Oct 2026
  • 3 sources

At a glance

Deimos at a glance, with sources
MeasureValueSource
Dimensions15 × 12 × 11 kmNASA Science: Deimos (opens in a new tab)NASA Science: Deimos (opens in a new tab)
Mean radius6.2 kmJPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mass1.44 × 10¹⁵ kgDerived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Surface gravity2.5 mm/s²Derived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Escape velocity6 m/sDerived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mean density1.471 g/cm³JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Distance from Mars's centre23,457 kmJPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Orbital period30.3 hours (1.2625 days)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Orbital inclination1.8°JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Regolith depthPossibly about 100 mNASA Science: Deimos (opens in a new tab)NASA Science: Deimos (opens in a new tab)
Largest craterAbout 2.3 km acrossNASA Science: Deimos (opens in a new tab)NASA Science: Deimos (opens in a new tab)
Discovered11 Aug 1877 by Asaph HallNASA Science: Deimos (opens in a new tab)NASA Science: Deimos (opens in a new tab)

Key points

A thick blanket of dust softens its craters, giving it a smoother face than Phobos.

  • About 15 km across, smaller than many cities
  • Covered by dust possibly 100 m deep
  • Slowly drifting away from Mars

Surface

Deimos has no grooves and only small, partly buried craters. Its slightly reddish, dark surface resembles C-type asteroids. Debris knocked off by impacts can briefly form a thin ring around Mars before it falls back as dust.

Orbit

Unlike Phobos, Deimos orbits outside the synchronous distance, so tides push it slowly outward instead of drawing it in. From the Martian surface it would look like a bright star, rising in the east and taking more than two days to cross the sky.

What we still don't know

Whether Deimos shares Phobos's origin. MMX will observe it during its survey of the Martian system.

Missions

  1. 2005–

    Mars Reconnaissance Orbiter

    NASAActive

    HiRISE camera and relay for surface missions.

  2. Launch 19 Oct 2026

    H3 F10 from Tanegashima at 19:41 UTC (window to 7 Nov). Phobos operations 2027–2030, sample return 2031.

    Mission page (opens in a new tab)

First-hand · our 3D model

How we render it

Deimos is a displaced triaxial mesh at its measured 15 × 12 × 11 km proportions, long axis towards Mars. Its surface map is our own procedural work, smoother than Phobos to suggest its deep dust blanket.

It is drawn at about 1.6% of Mars's radius, enlarged from its true 0.18% so it stays visible. It orbits in Mars's equatorial frame, inclined 1.8°, with a 1.26-day period kept in true ratio to its neighbours, and keeps one face towards Mars.

Moon sizes and orbits are compressed so a whole system fits on screen, but never reordered: each moon is drawn at 0.72 × (true size ratio)^0.6 of its planet, capped so no large moon is drawn bigger than it really is, and orbit distances are log-compressed into a band that clears the planet's rings. Orbital periods keep their true ratios, every moon is tidally locked, and on lighter devices only the two largest moons of each planet are drawn.

Sources

  1. NASA Science: Deimos (opens in a new tab)
  2. JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
  3. JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)

Last reviewed against these sources. Built from public NASA, ESA and JPL data; not affiliated with or endorsed by any agency.