Terrestrial planet

Mars

Mars preserves river valleys, lake deposits, volcanic provinces, polar caps, and a thin CO2 atmosphere.

Mars: loading local 3D asset.

Physics Snapshot

Planet order
4 from the Sun
Planet class
Inner terrestrial planet
Mean distance
1.524 AU
Revolution period
686.98 Earth days
Rotation period
24 h 37 m 22 s
Relative rotation speed
14.620 deg/s display
Mean temperature
-63 C average; about -125 to +20 C surface range
Atmosphere
Thin carbon-dioxide atmosphere with global dust, clouds, and strong seasonal pressure changes.
Main gases
About 95% carbon dioxide, 2.7% nitrogen, 1.6% argon, with oxygen, carbon monoxide, and water vapor traces.
Surface / cloud pressure
About 6 millibar average surface pressure, less than 1% of Earth sea-level pressure.
Ocean status
No stable surface ocean today; ancient lakes, river systems, possible northern seas, polar ice, and subsurface ice are key evidence.
Perihelion / closest
1.3814 AU (206.65 million km)
Aphelion / farthest
1.6660 AU (249.26 million km)
Orbit ellipse
0.0934
Mean/reference radius
3,389.5 km
Gravity definition
3.71 m/s²
Escape velocity
5.03 km/s
Day length
24 h 39 m 35 s
Known moons
2
Mission record
Viking, Pathfinder, Spirit, Opportunity, Curiosity, MAVEN, InSight, Perseverance, Ingenuity, Tianwen-1/Zhurong, Hope, and Mars Express.

What Scientists Watch

Classification: Inner terrestrial planet. Mercury through Mars are inner rocky worlds; Jupiter through Neptune are outer giants.

  • Ancient habitability is studied through clay, carbonate, sulfate, and delta deposits.
  • Dust, thin air, and low gravity make landing and surface operations unusually hard.
  • Perseverance caches selected samples while Curiosity studies Gale crater's layered history.

Exploration note: Viking, Pathfinder, Spirit, Opportunity, Curiosity, MAVEN, InSight, Perseverance, Ingenuity, Tianwen-1/Zhurong, Hope, and Mars Express.

Atmosphere and oceans

Gases, temperature, and liquids

Atmosphere
Thin carbon-dioxide atmosphere with global dust, clouds, and strong seasonal pressure changes.
Main gases
About 95% carbon dioxide, 2.7% nitrogen, 1.6% argon, with oxygen, carbon monoxide, and water vapor traces.
Pressure
About 6 millibar average surface pressure, less than 1% of Earth sea-level pressure.
Surface / cloud temperature
About -63 C average, with local surface temperatures from roughly -125 to +20 C.
Oceans and liquids
No stable surface ocean today; ancient lakes, river systems, possible northern seas, polar ice, and subsurface ice are key evidence.
Stable surface liquids
Liquid water is not stable for long at the surface; transient brines are possible in special conditions.

Interpretation note

How to read these values

Rocky worlds list surface conditions directly. Jupiter, Saturn, Uranus, and Neptune do not have hard surfaces, so temperature and pressure are referenced to atmospheric levels such as the 1-bar cloud region.

Ocean status separates the planet itself from its moons. Several outer-planet moons are major ocean-world targets even when the parent planet has no surface ocean.

3D asset view

Rotatable planet model

Mars: loading local 3D asset.

This viewer loads the local asset-backed model for Mars and applies the sidereal axis tilt and relative rotation direction for study. Drag to rotate, wheel to zoom, and open full screen for close inspection.

Elevation and relief

Topography map notes

  • Elevation maps are dominated by the Tharsis rise, Olympus Mons, Valles Marineris, Hellas Planitia, and the low northern plains.
  • The crust preserves cratered highlands in the south and smoother younger volcanic and sedimentary provinces in the north.
  • Landing-site geomorphology at Gale, Jezero, and Elysium links basin history, volcanism, sediment transport, and climate shifts.

Interior and field

Core, mantle, and magnetism

Crust
Basaltic crust with hemispheric topographic dichotomy
Mantle
Silicate mantle that fed giant shield volcanoes and long-lived magmatism
Core
Large liquid iron-sulfur core inferred from seismology and moment-of-inertia constraints

Orbital characteristics

Detailed orbit solution

Epoch
J2000
Perihelion
1.3814 AU (206.65 million km)
Aphelion
1.6660 AU (249.26 million km)
Semi-major axis
1.523679 AU (227.94 million km)
Eccentricity
0.0934
Sidereal period
686.98 Earth days
Synodic period
779.94 Earth days
Average orbital speed
24.07 km/s
Inclination
1.850 deg to the ecliptic
Longitude of ascending node
49.578 deg
Argument of perihelion
286.502 deg

Physical characteristics

Bulk properties and rotation

Mean radius
3,389.5 km
Flattening
0.00589
Surface area
144.8 million km²
Volume
163.18 billion km³
Mass
6.4171 × 10²³ kg
Mean density
3.933 g/cm³
Surface gravity
3.71 m/s²
Escape velocity
5.03 km/s
Sidereal rotation
24 h 37 m 22 s
Solar day
24 h 39 m 35 s
Equatorial rotation speed
241 m/s
Axial tilt
25.19 deg
Geometric albedo
0.170

Atmosphere profile

Pressure, composition, and temperature

Surface pressure
About 6 millibar
Composition
About 95.3% carbon dioxide, 2.7% nitrogen, 1.6% argon, with trace oxygen and water vapor
Surface temperature
About -63 C average
Water inventory
Polar ice, buried ice, hydrated minerals, and strong evidence for ancient rivers and lakes

Field review

Magnetic field, core behavior, and crater context

  • Mars no longer has a strong global dynamo field, but orbiters map intense remanent crustal magnetization in ancient terrains.
  • Its weak present-day magnetosphere allows substantial solar-wind interaction with the upper atmosphere and ongoing escape processes.
Hellas PlanitiaJezeroGaleIsidis

Moon catalog

Moons Available

Confirmed count: 2

Phobos, Deimos.

Data note: rotation values are sidereal periods. For solar orbits this guide uses perihelion and aphelion; those are the Sun-orbit equivalents of closest and farthest orbital distance. Gravity is surface or equatorial gravity for rocky planets and a reference-level value for giant planets, so rounded fact sheets may differ slightly. Moon counts can change when new satellites are confirmed.

Data basis

How these values are normalized

Orbital elements are presented in a J2000-style reference format. Rotation values use sidereal periods unless a solar day is explicitly named. For giant planets, pressure, temperature, and gravity are reference-level values because there is no solid surface to stand on.

Audit note

How to read discrepancies

Compact summary boxes, environment notes, and detailed fact tables are now aligned to the same field guide data blocks. This consistency pass was updated on May 5, 2026. Small differences can still appear when a quantity is rounded for readability, when a rocky-planet surface value is contrasted with a giant-planet reference level, or when moon counts change after new confirmations.

Mathematical model

Planet rotation and scale model

Planet meshes are procedural study models: radius, axial tilt, and rotation come from catalog fields, while surface textures are visual aids. The mathematical model does not infer planet shape from a picture.

Rotation phase

\[\theta(t)=\theta_0+\frac{2\pi t}{P_{\mathrm{rot}}}\]

The displayed spin angle advances from the body's rotation period P_rot. Retrograde rotation is represented by the sign of P_rot.

Axial tilt

\[\mathbf{r}_{\mathrm{tilted}}=R_z(\varepsilon)\,\mathbf{r}_{\mathrm{body}}\]

The spin axis is tilted by an explicit obliquity epsilon. The proof is a rigid-body rotation matrix, not an artist-drawn axis.

Scale contract

\[R_{\mathrm{scene}}=k\,R_{\mathrm{catalog}}\]

Scene radius is a scalar multiple of catalog radius unless the user chooses a readability mode. The page states when visual radius is bounded so the model is not mistaken for exact visual scale.

Verification standard: the rendered object must be reproducible from stated equations, catalog parameters, or explicit geometric transforms. Visual reference images may inform presentation only; they are not the source of orbital positions, field vectors, accretion-disk gradients, timing, or engineering layout.

Limitations: browser scenes may use bounded scale, compressed distances, simplified two-body dynamics, schematic transfer curves, or educational approximations where full numerical ephemerides, CFD, finite-element models, or general-relativistic ray tracing are outside the page scope. Those simplifications are part of the model contract, not hidden image-based construction.

Open the full site-wide mathematical verification policy