Terrestrial planet

Mercury

The innermost planet is a dense, cratered world with almost no atmosphere and extreme temperature contrast.

Mercury: loading local 3D asset.

Physics Snapshot

Planet order
1 from the Sun
Planet class
Inner terrestrial planet
Mean distance
0.387 AU
Revolution period
87.9691 Earth days
Rotation period
58.646 Earth days
Relative rotation speed
0.256 deg/s display
Mean temperature
167 C mean; about -170 to 430 C surface range
Atmosphere
No stable atmosphere; only a surface-bounded exosphere.
Main gases
Oxygen, sodium, hydrogen, helium, potassium, calcium, and magnesium atoms in a very thin exosphere.
Surface / cloud pressure
Effectively vacuum at the surface.
Ocean status
No liquid oceans. Permanently shadowed polar craters can preserve water ice.
Perihelion / closest
0.307499 AU (46.00 million km)
Aphelion / farthest
0.466697 AU (69.82 million km)
Orbit ellipse
0.205630
Mean/reference radius
2,439.7 km
Gravity definition
3.70 m/s²
Escape velocity
4.25 km/s
Day length
176 Earth days
Known moons
0
Mission record
Mariner 10, MESSENGER, and ESA-JAXA BepiColombo provide the main spacecraft record.

What Scientists Watch

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

  • High iron fraction suggests a large metallic core relative to its radius.
  • Solar tides and general relativity measurably shape its perihelion precession.
  • Permanently shadowed polar craters can trap volatile ice despite the planet's proximity to the Sun.

Exploration note: Mariner 10, MESSENGER, and ESA-JAXA BepiColombo provide the main spacecraft record.

Atmosphere and oceans

Gases, temperature, and liquids

Atmosphere
No stable atmosphere; only a surface-bounded exosphere.
Main gases
Oxygen, sodium, hydrogen, helium, potassium, calcium, and magnesium atoms in a very thin exosphere.
Pressure
Effectively vacuum at the surface.
Surface / cloud temperature
About -170 to 430 C, with a mean near 167 C because of extreme day-night contrast.
Oceans and liquids
No liquid oceans. Permanently shadowed polar craters can preserve water ice.
Stable surface liquids
None stable at the surface.

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

Mercury: loading local 3D asset.

This viewer loads the local asset-backed model for Mercury 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

  • Caloris Basin, Rembrandt basin, and globally distributed impact plains dominate the relief map.
  • Lobate scarps cut across craters and plains, recording planetary contraction as the large metallic core cooled.
  • Permanently shadowed polar craters are cold traps where radar-bright ice deposits are plausible.

Interior and field

Core, mantle, and magnetism

Crust
Thin silicate crust scarred by impacts and tectonic scarps
Mantle
Relatively thin silicate mantle compared with the size of the core
Outer core
Large molten iron-rich shell that powers the global dynamo
Inner core
Solid iron-rich center inferred from libration and density constraints

Orbital characteristics

Detailed orbit solution

Epoch
J2000
Perihelion
0.307499 AU (46.00 million km)
Aphelion
0.466697 AU (69.82 million km)
Semi-major axis
0.387098 AU (57.91 million km)
Eccentricity
0.205630
Sidereal period
87.9691 Earth days
Synodic period
115.88 Earth days
Average orbital speed
47.36 km/s
Inclination
7.005 deg to the ecliptic
Longitude of ascending node
48.331 deg
Argument of perihelion
29.124 deg

Physical characteristics

Bulk properties and rotation

Mean radius
2,439.7 km
Flattening
Effectively zero
Surface area
74.8 million km²
Volume
60.83 billion km³
Mass
3.3011 × 10²³ kg
Mean density
5.427 g/cm³
Surface gravity
3.70 m/s²
Escape velocity
4.25 km/s
Sidereal rotation
58.646 Earth days
Solar day
176 Earth days
Equatorial rotation speed
About 3.0 m/s
Axial tilt
0.034 deg
Geometric albedo
0.106

Atmosphere profile

Pressure, composition, and temperature

Surface pressure
Near-vacuum exosphere
Composition
Oxygen, sodium, hydrogen, helium, potassium, calcium, and magnesium atoms
Thermal state
Mean near 167 C, with day-side peaks above 400 C and night-side lows below -170 C

Field review

Magnetic field, core behavior, and crater context

  • Mercury has a real global magnetic field, but it is weak compared with Earth and offset northward from the planet's center.
  • Its magnetosphere is compressed by the solar wind, so reconnection and particle precipitation can be studied close to the Sun.
Caloris BasinRembrandtRaditladiEminescu

Moon catalog

Moons Available

Confirmed count: 0

No natural moons confirmed.

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