Double & Multiple Stars · Constellation Aquarius

Zeta Aquarii (ζ¹ & ζ² Aquarii)

Coordinates, Hipparcos distance (92 ly), 487-year twin F-star binary orbit (2.4″ in 2026), and observing guide for Zeta Aquarii.

Right Ascension (J2000.0)22h 28m 49.69s
Declination (J2000.0)-00° 01′ 11.9″
Primary ClassificationHierarchical triple system of two F-type stars and an astrometric companion
Best Observing SeasonLate Summer to Autumn (August–December)

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 Zeta Aquarii (ζ¹ & ζ² Aquarii)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Combined apparent visual magnitude (V)3.65 mag± 0.01 magJohnson UBV photometry (ζ² Aqr = 4.36 mag, ζ¹ Aqr = 4.53 mag)definitiveHipparcos New Reduction Catalog
Trigonometric parallax35.48 mas± 1.07 masHipparcos New Reduction + interferometric orbit (28.18 ± 0.85 pc / 91.9 ly) (J2000.0)definitiveHipparcos New Reduction Catalog
Visual binary orbital period (ζ¹–ζ²)177875 d± 3650 dSpeckle & adaptive-optics orbit (487 ± 10 yr, a = 3.50″, e = 0.43)high-confidenceSIMBAD Astronomical Database (CDS)
Visual angular separation (2026 epoch)0.04 arcmin± 0.002 arcminOrbital ephemeris (~2.4 arcseconds in 2026, widening after 1978 periastron)definitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Astrometric perturbations with a 25.95-year period first noticed by Kaj Strand in 1942 were confirmed by adaptive-optics imaging in 2010 to come from a 0.40-solar-mass M0 V red dwarf (ζ¹ Aquarii B) orbiting ζ¹ Aquarii at 9.7 AU.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Zeta Aquarii (Water Jar Twin F-Star Binary) at RA 22h 28m 49.69s, Dec -00° 01′ 11.9″ within Aquarius, 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 (Aquarius) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 50° 40°N Lat 60° 30°S Lat RA: 22h 28m 49.69s Dec: -00° 01′ 11.9″ Epoch: J2000.0 · V = 3.65 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Zeta Aquarii (55 Aquarii) sits at the exact center of the three-pointed 'Water Jar' Y-asterism of northern Aquarius and just 1.2 arcminutes south of the celestial equator (declination −00° 01′ 12″; due to axial precession, it crossed from the Southern into the Northern Celestial Hemisphere in 2004). First recorded as a double star by Christian Mayer in 1777 and independently by William Herschel in 1779, Zeta Aquarii shines at combined visual magnitude 3.65 at a distance of 28.18 ± 0.85 parsecs (91.9 light-years).

In the eyepiece, Zeta Aquarii resembles an autumn version of Porrima (Gamma Virginis): two nearly equal, creamy yellow-white stars—Zeta² Aquarii (magnitude 4.36, spectral type F3 V, ~1.4 solar masses) and Zeta¹ Aquarii (magnitude 4.53, spectral type F6 IV subgiant, ~1.4 solar masses)—orbiting their common center of mass every 487 years along an inclined ellipse.

Having passed through its closest visual separation (1.67 arcseconds) around 1978, the pair has now opened to ~2.4 arcseconds in 2026 along position angle ~156° and will continue widening over the next two centuries toward 5.0 arcseconds. High-contrast infrared adaptive optics also resolved a third component, Zeta¹ Aquarii B, an M0 V red dwarf orbiting Zeta¹ Aquarii every 25.95 years.

Practical Visual Observing Guide

Minimum InstrumentNaked eye; 60–80 mm telescope at 120×+ splits the 2.4″ twin pair
Recommended Magnification120×–180×
Best Evening SeasonLate Summer to Autumn (August–December)
  • Locate the compact Y-shaped Water Jar of Aquarius south of the head of Pegasus; Zeta Aquarii is the central vertex where the three branches of the Y meet.
  • At 2.4 arcseconds separation of two equal 4.4- and 4.5-magnitude stars, Zeta Aquarii is a superb benchmark test for a 60–80 mm refractor at 120×–160×, producing two touching or cleanly split figure-8 Airy disks.

Catalog Cross-Identifications & Aliases

Common Aliases: ζ Aquarii · ζ¹ & ζ² Aquarii · HD 213051 / HD 213052 · HIP 110960 · 55 Aquarii

Cross-Catalog Identifiers for Zeta Aquarii (ζ¹ & ζ² Aquarii)
Catalog AuthorityIdentifier
HIPHIP 110960
HDHD 213051
SIMBAD* zet Aqr
WIKIDATAQ13068
Related Object · Virgo

Porrima (Gamma Virginis Twin F0V Binary)

Coordinates, Hipparcos distance (38.1 ly), 169-year eccentric F0V+F0V visual binary orbit (3.4″ in 2026), and observing guide for Porrima.

Related Object · Lyra

Epsilon Lyrae (The Double Double Star)

Coordinates, Gaia DR3 distance (160 ly), 208″ wide pair and 2.3″/2.4″ tight sub-pairs, and telescope resolution test guide for Epsilon Lyrae.

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

Celestial Coordinates (RA & Dec) Explained

Practical reference to J2000 equatorial coordinates: Right Ascension (RA in hours, minutes, seconds), Declination (Dec in degrees), and sexagesimal conversion.

Scientific Sources & Dataset Provenance