Solar System Worlds · Constellation Jupiter System (Ecliptic)

Europa (Jupiter II)

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.

Right Ascension (J2000.0)06h 00m 07.20s
Declination (J2000.0)+23° 00′ 00.0″
Primary ClassificationGalilean silicate moon with young water-ice shell and global subsurface ocean
Best Observing SeasonWhenever Jupiter is near opposition

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.

Astrometric, Photometric, and Physical Parameters for Europa (Jupiter II)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Opposition visual magnitude (V)5.29 mag± 0.05 magJPL planetary satellite photometry (geometric albedo = 0.67)definitiveNASA/JPL Solar System Dynamics & Planetary Fact Sheets
Orbital period around Jupiter3.551181 d± 0.000001 dGalilean 1:2:4 Laplace resonance ephemeris (semi-major axis = 671,100 km / 9.39 R_Jup)definitiveNASA/JPL Solar System Dynamics & Planetary Fact Sheets
Mean solid radius0.245 R⊕± 0.0002 R⊕Galileo spacecraft limb imaging (1,560.8 ± 0.5 km, 90% of Moon's radius)definitiveNASA/JPL Solar System Dynamics & Planetary Fact Sheets
Satellite mass0.008035 M⊕± 0.000001 M⊕Galileo & Juno flyby radio-Doppler tracking (4.7998 × 10^22 kg)definitiveNASA/JPL Solar System Dynamics & Planetary Fact Sheets
Measurement Uncertainties & Competing Solutions: While magnetometer induction measurements from the Galileo spacecraft prove a conductive saltwater ocean exists beneath Europa's ice shell, the exact thickness of the overlying solid ice crust remains debated between 'thin-shell' models (3–5 km) and 'thick-convective-shell' models (15–25 km), which NASA's Europa Clipper radar aims to measure directly.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Europa (Jupiter II Subsurface Ocean World) at RA 06h 00m 07.20s, Dec +23° 00′ 00.0″ within Jupiter System (Ecliptic), 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.

J2000 Equatorial Sky Position (Jupiter System (Ecliptic)) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 73° 40°N Lat 37° 30°S Lat RA: 06h 00m 07.20s Dec: +23° 00′ 00.0″ Epoch: J2000.0 · V = 5.29 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Europa (Jupiter II), the smallest of the four Galilean moons discovered by Galileo Galilei in January 1610, has a diameter of 3,121.6 kilometers (slightly smaller than Earth's Moon) and orbits Jupiter every 3.5512 days at a distance of 671,100 kilometers. Locked in a 1:2:4 Laplace orbital resonance with inner Io (1.769 days) and outer Ganymede (7.155 days), Europa's orbit is forced into a non-zero eccentricity (e = 0.009), flexing its interior through continuous tidal dissipation.

With a geometric albedo of 0.67, Europa's water-ice surface is one of the brightest and smoothest solid surfaces in the Solar System, crisscrossed by dark reddish-brown lineae (fractures) and chaotic ice-raft terrains while virtually devoid of large impact craters—indicating a surface geologic age of only 40 to 90 million years. During the late 1990s, the Galileo spacecraft detected an induced magnetic field inside Europa as Jupiter's tilted magnetosphere swept past it, providing the strongest geophysical evidence for a global liquid saltwater ocean ~60 to 150 kilometers deep containing roughly twice the liquid water volume of all Earth's oceans combined.

In 2023 the James Webb Space Telescope's NIRSpec instrument mapped Europa's surface and discovered that crystalline and amorphous carbon dioxide (CO2) ice is concentrated inside Tara Regio, a geologically young 'chaos terrain' where warm subsurface ocean brines have recently upwelled through the ice shell—proving that Europa's internal ocean contains bio-essential carbon.

Practical Visual Observing Guide

Minimum Instrument7×50 binoculars to spot Europa beside Jupiter; 60–100 mm telescope for transits & shadows
Recommended Magnification120×–220×
Best Evening SeasonWhenever Jupiter is near opposition
  • At visual magnitude 5.29, Europa is theoretically bright enough to see with the naked eye if it were not lost in the glare of magnitude −2.8 Jupiter (maximum elongation ~3.5 arcminutes).
  • Any 7×50 or 10×50 binocular splits Europa from Jupiter near eastern or western elongation, and any 60–150 mm telescope at 120×–200× lets you watch Europa transit across Jupiter's disk, cast its crisp black shadow onto the clouds, and disappear into Jupiter's shadow during eclipses.

Catalog Cross-Identifications & Aliases

Common Aliases: Jupiter II

Cross-Catalog Identifiers for Europa (Jupiter II)
Catalog AuthorityIdentifier
WIKIDATAQ3143
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Reference Guide

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.

Reference Guide

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
  • JWST / MAST Science Archive & Mission Documentation (Cycle 1–4 Public Releases (2022–2026)): Rigby, J., et al. 2023, PASP, 135, 048001 (The Science Performance of JWST as Characterized in Commissioning) — NASA / ESA / CSA / STScI