VASTWARDCelestial Atlas
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Oberon

Outer, heavily cratered major moon of Uranus

The outermost major Uranian moon, preserving old craters, dark crater floors and a mountain rising at the limb.

Atlas data reviewed
Editorial stage
Published
Visibility
Public
Voyager 2 reconstructed-color image of Oberon with bright-ray craters, dark crater floors and a mountain at the limb.Direct observation
Voyager 2's best Oberon image, with color reconstructed from violet, clear and green filters.

Official reconstructed-color spacecraft image. Features smaller than about 12 km are unresolved, and only one viewing geometry is represented.

NASA/JPL
Vastward explanation

What this world is

Oberon's surface is an old impact record. Some craters have bright rays, some floors are unusually dark, and a roughly 6 km mountain is visible at the edge of the Voyager image.

Why it looks this way now

Voyager 2 directly recorded the cratered surface and mountain. A 2023 thermal model permits a residual briny ocean, while current activity and the dark crater material remain unresolved.

02

Where it sits

The outermost and second-largest of Uranus' five major moons, beyond Titania.

How to read this mapTwo-scale location · Solar System to the Uranus moons

Swipe sideways to inspect the full map

Two-scale location · Solar System to the Uranus moonsThe left panel places Uranus in planetary order; the right places Oberon among the profiled Uranus moon orbits.Scale one · Solar SystemUranusPlanet 7 from the SunSunScale two · Uranus moon systemUranusOberonProfiled orbit 5 of 5Mean distance · 583,511 km
Blue marks the current moon and orbit

Oberon is 5 of 5 profiled Uranus moons by distance, at a mean center distance of about 583,511 km.

Muted lines and dots show system context

The left panel locates Uranus, dashed lines mark the scale change, and muted orbits and dots represent other profiled moons on the right. Titania is the adjacent profiled moon inside; it is the outermost profiled moon in the system.

The figure uses two linked scales and compares only the same-system moons currently profiled by Vastward; orbit spacing, body sizes and marker positions are compressed for teaching.
03

Read the numbers

Reference values retain their units, context, evidence state and published uncertainty.

Physical measurements

Mean radiusglobal mean
761.4kmCalculated measurementThe mean radius is about 0.438 times the radius of Earth's Moon.

Irregular moons have no single true radius; the mean radius is an equal-volume comparison.

Published uncertainty: ± 2.6 km

JPL tabulated uncertainty for the adopted mean radius.

Massglobal mean
3.075978E21kgCalculated measurementMass is not read from a scale. Motion under gravity constrains GM, from which mass is derived.

Calculated from JPL GM with a conventional gravitational constant, then rounded for display.

Approximate value

Derived from JPL's gravitational parameter GM and a conventional gravitational constant, then rounded.

Mean densityglobal mean
1.6640g/cm³Calculated measurementSimilar to Titania within uncertainty, consistent with a mixed rocky and water-rich body.

This is a whole-body average and cannot by itself prove the composition of every interior layer.

Published uncertainty: ± 0.05 g/cm³

JPL tabulated uncertainty for the adopted mean density.

Reference gravitysurface
0.35413m/s²Calculated measurementRepresentative surface gravity is about 3.61% of Earth's.

Shape, terrain and local mass distribution make real gravity vary by location.

Approximate value

Calculated from the adopted GM and mean radius. Irregular shape and local terrain can change the actual value.

Temperaturesurface
-188°CScientific modelThis is a broad sunlit reference, not the temperature of every crater floor and shadow.

Sparse thermal sampling and extreme seasons leave the full temperature range poorly constrained.

Approximate value

Approximate sunlit upper reference near 85 K for Uranian moon terrain. It is not a measured global mean and does not represent polar night.

Orbit and rotation

Average distancesystem reference
583,511kmCalculated measurementThis is a representative center-to-center distance between Oberon and Uranus.

The real distance changes around an elliptical orbit.

Approximate value

Rounded orbital distance from the moon center to the planet center. The real orbit is not a perfect circle.

Rotation periodrelative to distant stars
13.463237Earth daysCalculated measurementTidal locking makes one rotation take nearly the same time as one orbit around the planet.

This is a sidereal rotation, not a local sunrise-to-sunrise solar day.

Approximate value

Rounded synchronous rotation period. The same hemisphere normally faces the primary planet.

Orbital periodrelative to distant stars
13.463237Earth daysCalculated measurementThis reports the time for one orbit, not a claim that the path is perfectly circular.

A rounded sidereal period is used for the beginner-facing display.

Approximate value

Rounded sidereal orbital period.

04

Atmosphere and inside

Atmosphere

Oberon has no persistent atmosphere. Crater-floor darkness is a surface-material question, not weather.

Surface and interior

Oberon likely mixes rock and water-rich material beneath an ancient crust. A residual salty ocean is allowed by modeling, not confirmed.

  1. 1
    Modeled rock and water-rich interior

    Density supports a mixed interior with a substantial rocky fraction and water-rich material.

    Scientific model
  2. 2
    Possible residual briny ocean

    Thermal evolution modeling allows a salty liquid layer, but it has not been directly detected.

    Scientific model
  3. 3
    Ancient cratered ice-rich crust

    Voyager images directly show bright-ray craters, dark crater floors and a mountain at the limb.

    Direct observation
05

How we know

Images constrain size, orbital and radio tracking constrain GM, and spectra and thermal emission constrain materials. Every number retains its method and limitation.

  1. 01

    Spacecraft imaging and shape reconstruction

    Repeated views reveal the limb, terrain, crater record and the shape used to estimate size.

    Where this method stops

    Lighting, viewing angle and incomplete coverage can hide topography. A mosaic is not a single untouched photograph.

    Direct observation
  2. 02

    Radio tracking and orbital dynamics

    Engineers measure spacecraft motion and moon orbits, solve for GM, and then derive mass and gravity.

    Where this method stops

    The result depends on trajectory coverage and a dynamical model. Very small moons leave weaker gravitational signatures.

    Calculated measurement
  3. 03

    Spectroscopy and thermal sensing

    The spectrum and thermal glow constrain surface materials, gases and representative temperature.

    Where this method stops

    A spectrum samples the visible surface or atmosphere. It does not directly photograph deep interior layers.

    Direct observation
06

Evidence key

Direct observation
An instrument or sample recorded the phenomenon, with processing still disclosed.
Calculated measurement
Observed motion or signal is converted into a physical quantity using equations and reference constants.
Scientific model
A tested interpretation that fits observations but is not directly imaged or sampled.
Vastward explanation
Original beginner-facing synthesis, traceable to the source records but not itself a measurement.
Artist visualization
An interpretive image, not observational evidence.
07

Missions and instruments

Active

Voyager 2

Voyager 2 returned the only close Oberon image, revealing its ancient impact record, dark deposits and limb mountain.

Official mission
Instruments
  • Imaging Science SubsystemImages the limb, terrain, color differences and time-dependent surface changes.
  • Spacecraft radio scienceMeasures Doppler and range changes that constrain trajectory, gravity and mass.
  • Infrared Interferometer Spectrometer and RadiometerSeparates light by wavelength to constrain composition, gases and temperature.
08

Official source trail

Links below are the exact records used for this profile. Access dates are retained with the content.

  1. 01

    NASA Science · official-page

    Oberon

    Source updated
    No source update date published
    Access checked
    2026-07-31
    Open official source
  2. 02

    NASA Jet Propulsion Laboratory, Solar System Dynamics · dataset

    Planetary Satellite Physical Parameters

    Source updated
    No source update date published
    Access checked
    2026-07-31
    Open official source
  3. 03

    NASA Science Photojournal · image

    Oberon at Voyager Closest Approach

    Source updated
    No source update date published
    Access checked
    2026-07-31
    Open official source
  4. 04

    NASA Science · official-page

    Voyager mission

    Source updated
    No source update date published
    Access checked
    2026-07-31
    Open official source
  5. 05

    NASA Technical Reports Server · research-paper

    Uranus Satellites: Surface Properties

    Source updated
    No source update date published
    Access checked
    2026-07-31
    Open official source
  6. 06

    NASA Jet Propulsion Laboratory · official-page

    New Study of Uranus' Large Moons Shows 4 May Hold Water

    Source updated
    No source update date published
    Access checked
    2026-07-31
    Open official source
09

Continue exploring

Atlas is a starting point. Use these relationships to move into explanation, experiment and mission thinking.