Galaxies · Constellation Serpens

Hoag's Object (PGC 54559)

J2000 coordinates, distance (613 Mly), magnitude 16.00, golden E0 core inside detached blue star-forming ring, and observing guide for Hoag's Object.

Right Ascension (J2000.0)15h 17m 14.20s
Declination (J2000.0)+21° 35′ 08.0″
Primary ClassificationUnique detached circular ring galaxy surrounding a spherical E0 core
Best Observing SeasonLate Spring to Summer (May–August)

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 Hoag's Object (PGC 54559)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Integrated visual magnitude (V)16 mag± 0.15 magHST WFPC2 & deep CCD integrated photometrydefinitiveSIMBAD Astronomical Database (CDS)
Distance in light-years613000000 ly± 20000000 lyOptical & H I 21-cm cosmological redshift (z = 0.0425, 188 ± 6 Mpc)high-confidenceSIMBAD Astronomical Database (CDS)
Apparent diameter (outer blue ring)0.75 arcmin± 0.05 arcminHST WFPC2 outer ring diameter (45″ × 45″ = 0.75′)definitiveSIMBAD Astronomical Database (CDS)
Heliocentric recession velocity12740 km/s± 15 km/sOptical core absorption & WSRT H I 21-cm ring spectroscopydefinitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Identical +12,740 km/s radial velocities in both the golden E0 core and the outer blue ring prove they are a single bound galaxy at 188 ± 6 Mpc (613 ± 20 Mly), with ~3% distance uncertainty from the Hubble constant calibration.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Hoag's Object (PGC 54559 Polar Ring Galaxy) at RA 15h 17m 14.20s, Dec +21° 35′ 08.0″ within Serpens, 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 (Serpens) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 72° 40°N Lat 38° 30°S Lat RA: 15h 17m 14.20s Dec: +21° 35′ 08.0″ Epoch: J2000.0 · V = 16 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

When astronomer Arthur Hoag discovered this object in 1950 on photographic plates of Serpens Caput, its geometry was so uncanny that he initially proposed it was either a planetary nebula or the first gravitational Einstein ring produced by a foreground galaxy lensing a background quasar. Positioned 613 million light-years (188 megaparsecs) away, Hoag's Object (PGC 54559) consists of an almost perfectly spherical 24,000-light-year-wide core of ancient, golden-yellow stars encircled—across a 35,000-light-year empty gap—by a detached, symmetric ring of luminous blue OB star clusters spanning 120,000 light-years in outer diameter.

In 1974 and 1987 spectroscopists proved that the golden inner sphere and the blue outer ring share the exact same recession velocity (+12,740 km/s) and therefore belong to a single extraordinary galaxy. Unlike the Cartwheel Galaxy, Hoag's Object has no nearby 'bullet' intruder galaxy, its central core is a slow-rotating triaxial E0 spheroid rather than a disk, and no luminous spokes connect the core to the ring.

Modern cosmological hydrodynamical simulations and Westerbork 21-centimeter H I observations suggest that the ancient central elliptical core formed over 10 billion years ago, and subsequently accreted a massive 2-billion-year-old ring of cold atomic hydrogen gas directly along a cosmic web filament (or dissolved an early triaxial stellar bar that swept all outer gas into an outer resonance ring). Remarkably, in Hubble Space Telescope images of Hoag's Object, a second, even more distant ring galaxy (SDSS J151713.93+213516.8) can be seen shining right through the empty dark gap at the one-o'clock position between Hoag's core and ring!

Practical Visual Observing Guide

Minimum Instrument450 mm+ telescope for visual core detection; 200 mm+ + cooled CMOS camera for ring
Recommended Magnification300×–450× (visual); deep-sky CMOS astrophotography target
Best Evening SeasonLate Spring to Summer (May–August)
  • Located in northern Serpens Caput, 1.8° northeast of Beta Serpentis (β Ser).
  • At magnitude 16.0 and 613 million light-years distance, visually spotting the 6-arcsecond central core of Hoag's Object requires a 450–600 mm (18–24 inch) telescope at 300×–450× under pristine dark skies.
  • For backyard astrophotographers with 200–350 mm telescopes, capturing the distinct golden core and 45-arcsecond blue ring of Hoag's Object is one of the ultimate deep-field trophies.

Catalog Cross-Identifications & Aliases

Common Aliases: Hoag's Object · PGC 54559 · PRC D-51

Cross-Catalog Identifiers for Hoag's Object (PGC 54559)
Catalog AuthorityIdentifier
SIMBADNAME Hoag's Object
WIKIDATAQ14084
Related Object · Sculptor

Cartwheel Galaxy (ESO 350-40 Ring Galaxy)

J2000 coordinates, distance (489 Mly), magnitude 15.20, bullseye collisional ring, JWST dust spokes, ultraluminous X-ray sources, and observing guide.

Related Object · Canes Venatici

Cat's Eye Galaxy (Messier 94 / NGC 4736)

J2000 coordinates, TRGB distance (15.0 Mly), magnitude 8.24, blazing inner starburst ring, outer pseudoring, and observing guide for Messier 94.

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

Proper Motion, Radial Velocity & Redshift

How astronomers combine tangential proper motion (mas/yr), Doppler radial velocity (km/s), and cosmological redshift (z) to reconstruct 3D space motion.

Scientific Sources & Dataset Provenance

  • SIMBAD Astronomical Database (CDS) (2026-10 release): Wenger, M., et al. 2000, A&AS, 143, 9 (The SIMBAD astronomical database) — Centre de Données astronomiques de Strasbourg
  • SH0ES Local Distance Ladder Hubble Constant (2022 Baseline Cepheid + SN Ia): Riess, A. G., et al. 2022, ApJL, 934, L7 (A Comprehensive Measurement of the Local Value of the Hubble Constant) — SH0ES Collaboration (HST / JWST)