Jupiter
JPL orbital parameters (5.2038 AU, 11.862 yr), opposition magnitude −2.94, 50.1″ angular disk, Galilean moons, and observing guide for Jupiter.
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 |
|---|---|---|---|---|---|
| Maximum opposition visual magnitude (V) | -2.94 mag | -2.94 to -1.66 mag | JPL planetary ephemeris photometry (varies from −2.94 at perihelic opposition to −1.66 at conjunction) | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Orbital semi-major axis | 5.2038 AU | ± 0.0001 AU | JPL DE441 planetary ephemeris (e = 0.0489) | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Sidereal orbital period | 4332.59 d | ± 0.01 d | JPL DE441 ephemeris (11.862 Julian years; synodic opposition period = 398.88 d) | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Planetary mass | 317.828 M⊕ | ± 0.001 M⊕ | Juno/Galileo spacecraft radio-Doppler tracking (1.89813 × 10^27 kg) | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Equatorial 1-bar radius | 11.209 R⊕ | ± 0.001 R⊕ | Radio occultation & imaging (71,492 km equatorial vs 66,854 km polar) | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
| Peak opposition equatorial diameter | 0.835 arcmin | 0.497 to 0.835 arcmin | Spans 50.1 arcseconds at perihelic opposition down to 29.8 arcseconds at conjunction | definitive | NASA/JPL Solar System Dynamics & Planetary Fact Sheets |
J2000 Equatorial Sky Chart & Culmination Altitude
The chart below plots Jupiter (Gas Giant & Galilean Moons) at RA 06h 00m 00.00s, Dec +23° 00′ 00.0″ within Ecliptic (Zodiac), 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
Jupiter is the fifth planet from the Sun and the gravitational titan of our Solar System, packing 317.83 Earth masses (more than 2.5 times the combined mass of all other planets) into a rapidly rotating hydrogen-helium spheroid with an equatorial diameter of 142,984 kilometers (11.21 Earth radii). Because Jupiter spins on its axis in just 9 hours 55 minutes 30 seconds—the shortest day of any planet—centrifugal forces flatten its disk by 6.49%, making its polar diameter 9,276 kilometers shorter than its equatorial diameter.
In January 1610 Galileo Galilei turned his 20× spyglass on Jupiter and discovered its four major moons—Io, Europa, Ganymede, and Callisto—revolving in a miniature Copernican plane around the planet, providing the first direct observational proof that not all celestial bodies orbit Earth. NASA's Juno spacecraft, orbiting Jupiter since 2016, has used high-precision gravity harmonics to show that Jupiter does not have a small, sharp rocky core, but rather a 'dilute' or fuzzy core of heavy elements dissolved into metallic hydrogen across nearly half the planet's radius.
Jupiter's dynamic ammonia-hydrosulfide cloud deck is divided into bright upwelling 'zones' and dark descending 'belts,' anchored by the Great Red Spot—an anticyclonic vortex larger than Earth that has persisted in the South Equatorial Belt for at least 190 to 350 years.
Practical Visual Observing Guide
- Shining between magnitude −1.7 and −2.94, Jupiter outshines every star in the sky and is surpassed only by the Moon, Venus, and occasionally Mars at perihelic opposition.
- Even steadily held 7×50 or 10×50 binoculars resolve the four Galilean moons (magnitudes 4.6 to 5.7) shifting positions from night to night.
- In any 60–150 mm telescope at 120×–220×, you can observe the North and South Equatorial Belts, the polar flattening, the Great Red Spot rotating across the disk, and black pinhole shadow transits cast by Io, Europa, Ganymede, and Callisto onto the cloud tops.
Catalog Cross-Identifications & Aliases
Common Aliases: Jove · Sol V
| Catalog Authority | Identifier |
|---|---|
| WIKIDATA | Q319 |
Related Objects, Comparisons & Guides
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.
Saturn (Ringed Giant & Cassini Division)
JPL orbital parameters (9.5826 AU, 29.457 yr), ring tilt cycle, Cassini Division resolution, and telescope observing guide for Saturn.
Titan (Saturn VI Nitrogen-Atmosphere Moon)
Orbital parameters (15.945 d around Saturn), visual magnitude 8.4, 1.45-bar N2/CH4 atmosphere, hydrocarbon lakes, and observing guide for Titan.
Mars (Terrestrial Planet & Opposition Cycle)
JPL orbital parameters (1.5237 AU, 686.98 d), 780-day synodic opposition cycle, 25.1″ maximum disk, and telescope observing guide for Mars.
51 Pegasi b (Dimidium First Hot Jupiter)
Coordinates, Gaia DR3 distance (15.46 pc), 4.2308-day orbital period, Nobel-winning radial-velocity discovery, and observing guide for 51 Pegasi b.
Solar System Planets & Moons Opposition Guide
How to observe Jupiter, Saturn, Mars, Titan, and Europa around opposition using high magnification, atmospheric dispersion control, and transit timing.
Suburban & Urban Light-Pollution Targets Guide
Practical observing guide to high-surface-brightness targets—planets, double stars, open clusters, and planetary nebulae—that cut through Bortle 6–8 skyglow.
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