Ganymede
Reference data for Jupiter's moon Ganymede: 5,268 km diameter, 7.15-day orbit, intrinsic magnetosphere, subsurface ocean, and JUICE target.
Provenance-Backed Scientific Measurements
Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.
| Parameter | Value | Uncertainty | Method & Epoch | Quality Status | Source Archive |
|---|---|---|---|---|---|
| Opposition Magnitude (V) | 4.61 mag | ± 0.15 mag | JPL Horizons DE440/441 planetary and satellite ephemeris solution | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Sidereal Orbital Period | 7.154553 d | ± 0.000001 d | Outer anchor of the 4:2:1 Laplace resonance with Io and Europa. | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Jovicentric Semi-Major Axis | 0.007155 AU | ± 0.000001 AU | Mean orbital radius of 1,070,400 km (14.97 Jupiter radii). | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Mean Volumetric Radius | 0.4135 R⊕ | ± 0.0001 R⊕ | Mean radius of 2,634.1 km (diameter 5,268.2 km—8% wider than Mercury). | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Mass | 0.0248 M⊕ | ± 0.00001 M⊕ | 1.4819 × 10²³ kg (2.02 times the mass of Earth's Moon). | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Opposition Angular Diameter | 0.0295 arcmin | ± 0.0033 arcmin | JPL Horizons DE440/441 planetary and satellite ephemeris solution | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots Ganymede (Jupiter III) — Largest Moon Profile at RA 04h 55m 10.00s, Dec +22° 05′ 10.0″ within Taurus, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.
Astrophysical Context & Structure
Measuring 5,268.2 kilometers across—8 percent larger in diameter than the planet Mercury and three-quarters the size of Mars—Ganymede (Jupiter III) reigns as the largest and most massive satellite in the Solar System. Orbiting 1.07 million kilometers from Jupiter every 7.155 days, it serves as the outer anchor of the three-body Laplace resonance with Io and Europa. Its low bulk density of 1.936 grams per cubic centimeter reflects an almost equal 50-50 split by mass between silicate rock and water ice, differentiated into one of the lowest moment-of-inertia factors (0.3115) of any solid Solar System body.
During its close flybys in 1996, NASA's Galileo spacecraft made the astonishing discovery that Ganymede possesses its own permanent dipole magnetic field (~720 nanoteslas at the equator), carving a mini-magnetosphere inside Jupiter's vast magnetosphere and generating ultraviolet oxygen auroral ovals around Ganymede's poles. This intrinsic dynamo arises from convection inside a liquid iron-iron sulfide core. Furthermore, Hubble measurements of how those auroral ovals rock back and forth in Jupiter's time-varying magnetic field confirmed the presence of a global, electrically conductive saltwater ocean ~100 kilometers thick sandwiched beneath a 150-kilometer icy crust.
Ganymede's surface is split between ancient, dark, clay-rich cratered regions (such as Galileo Regio) and younger, brighter swaths of tectonically faulted grooved terrain (sulci). In the 2030s, the European Space Agency's Jupiter Icy Moons Explorer (JUICE) will become the first spacecraft to enter orbit around a moon other than Earth's, mapping Ganymede's ocean and magnetosphere in detail.
Practical Visual Observing Guide
- At magnitude V = 4.61 and elongations up to 5.9 arcminutes from Jupiter, Ganymede is bright enough to be glimpsed with the naked eye by sharp-sighted observers when Jupiter is masked behind a building or tree limb.
- Subtends up to 1.8 arcseconds at opposition; 8-inch to 14-inch amateur telescopes under steady seeing resolve its disk and even capture broad albedo patches (Galileo Regio vs. Osiris ray system) via lucky imaging.
- Its large shadow is the easiest Galilean moon shadow to spot crossing Jupiter's cloud belts in small 60 mm to 80 mm refractors.
Catalog Cross-Identifications & Aliases
Common Aliases: Jupiter III · Largest Solar System Moon
| Catalog Authority | Identifier |
|---|---|
| SIMBAD | Ganymede |
Related Objects, Comparisons & Guides
Callisto (Jupiter IV) — Outer Galilean Moon
Reference data for Jupiter's moon Callisto: 4,821 km diameter, 16.69-day non-resonant orbit, Valhalla multi-ring basin, and internal ocean.
Europa (Jupiter II Subsurface Ocean World)
Orbital parameters (3.551 d around Jupiter in 1:2:4 Laplace resonance), magnitude 5.29, icy shell & subsurface ocean, and observing guide for Europa.
Io (Jupiter I) — Volcanic Galilean Moon Data
Reference data for Jupiter's moon Io: 1.77-day resonant orbit, over 400 active sulfur-silicate volcanoes, plasma torus, and transit timings.
Angular Size, Separation & Field of View
How angular diameter (degrees, arcminutes, arcseconds), spherical angular separation, and small-angle physical diameter relate to telescope field of view.
Apparent vs Absolute Magnitude Explained
Understand the logarithmic Pogson astronomical magnitude scale, apparent visual magnitude (m), absolute magnitude (M at 10 parsecs), and bolometric corrections.
Scientific Sources & Dataset Provenance
- NASA/JPL Solar System Dynamics & Planetary Fact Sheets (DE441 (2021/2026)): Park, R. S., et al. 2021, AJ, 161, 105 (The JPL Planetary and Lunar Ephemerides DE440 and DE441) — NASA Jet Propulsion Laboratory / GSFC