Galaxies · Constellation Pisces

Phantom Galaxy (Messier 74 / NGC 628)

J2000 coordinates, TRGB/SN distance (31.9 Mly), magnitude 9.46, face-on grand-design spiral arms, JWST dust filaments, and observing guide for M74.

Right Ascension (J2000.0)01h 36m 41.75s
Declination (J2000.0)+15° 47′ 00.5″
Primary ClassificationFace-on grand-design SA(s)c spiral galaxy (M74 Group dominant member)
Best Observing SeasonAutumn (September–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 Phantom Galaxy (Messier 74 / NGC 628)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Integrated visual magnitude (V)9.46 mag± 0.1 magWide-field integrated CCD photometrydefinitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Distance in light-years31900000 ly± 1000000 lyHST Tip of the Red Giant Branch (TRGB) + SN 2013ej photospheric distance (9.77 ± 0.32 Mpc)definitiveSH0ES Local Distance Ladder Hubble Constant
Apparent major axis10.5 arcmin± 0.4 arcminOptical isophotal dimensions (10.5′ × 9.5′)definitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Heliocentric recession velocity657 km/s± 1 km/sTHINGS H I 21-cm synthesis velocity fielddefinitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: HST Tip of the Red Giant Branch (TRGB) measurements and Type II-P supernova (SN 2003gd and SN 2013ej) expanding-photosphere analyses converge on 9.77 ± 0.32 Mpc (31.9 ± 1.0 Mly) for M74.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Phantom Galaxy (Messier 74 / NGC 628) at RA 01h 36m 41.75s, Dec +15° 47′ 00.5″ within Pisces, 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 (Pisces) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 66° 40°N Lat 44° 30°S Lat RA: 01h 36m 41.75s Dec: +15° 47′ 00.5″ Epoch: J2000.0 · V = 9.46 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Discovered by Pierre Méchain in late September 1780 and confirmed by Charles Messier three weeks later, Messier 74 (NGC 628) is one of the finest textbook examples of a face-on grand-design SA(s)c spiral galaxy in the local universe. Located 31.9 million light-years away in Pisces and tilted less than 7 degrees from a true face-on orientation, M74 spans ~95,000 light-years across and contains roughly 100 billion stars.

In August 2022, images of M74 from the James Webb Space Telescope's Mid-Infrared Instrument (MIRI) became an instant icon of modern astronomy: stripped of optical starlight, M74's two logarithmic spiral arms appeared as a glowing, skeletal filigree of polycyclic aromatic hydrocarbon dust lanes honeycombed with gigantic cavernous bubbles carved out by overlapping generations of stellar winds and supernovae, with a nuclear star cluster stripped completely bare of gas at the center.

M74 has hosted three prominent core-collapse supernovae in the 21st century—Type Ic SN 2002ap (a hypernova associated with gamma-ray burst physics), Type II-P SN 2003gd, and SN 2013ej—and harbors an ultraluminous quasi-periodic X-ray source (CXOU J013651.1+154547) suspected to be an intermediate-mass black hole of ~10,000 solar masses.

Practical Visual Observing Guide

Minimum Instrument100–130 mm telescope under dark skies (300 mm+ to trace spiral arms)
Recommended Magnification40×–80× (avoid high magnification that dims the disk)
Best Evening SeasonAutumn (September–December)
  • Easy to point to—just 1.3° east-northeast of Eta Piscium (η Psc, magnitude 3.6)—yet notorious among Messier Marathon runners as the hardest object to spot at twilight, earning its nickname the 'Phantom Galaxy'.
  • Because its 9.5-magnitude light is spread over a 10.5′ × 9.5′ face-on disk, its surface brightness is a very low ~23.2 mag/arcsec²; dark skies (Bortle 1–4) and low magnification (40×–70×) are mandatory.
  • In a 300–400 mm (12–16 inch) telescope under pristine autumn skies, averted vision traces the two sweeping spiral arcs and faint H II knots winding outward from the small pinpoint core.

Catalog Cross-Identifications & Aliases

Common Aliases: M74 · NGC 628 · UGC 1149 · Phantom Galaxy

Cross-Catalog Identifiers for Phantom Galaxy (Messier 74 / NGC 628)
Catalog AuthorityIdentifier
MESSIERM 74
NGCNGC 628
SIMBADM 74
WIKIDATAQ13999
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Triangulum Galaxy (Messier 33 / NGC 598)

Coordinates, Cepheid/maser distance (859 kpc / 2.80 Mly), low surface brightness (23.0 mag/arcsec²), NGC 604 H II region, and observing guide for M33.

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Pinwheel Galaxy (Messier 101 / NGC 5457)

J2000 coordinates, Cepheid/TRGB distance (21.6 Mly), magnitude 7.86, giant H II regions, SN 2011fe & SN 2023ixf, and observing guide for M101.

Related Object · Coma Berenices

Coma Pinwheel Galaxy (Messier 99 / NGC 4254)

J2000 coordinates, Tully-Fisher distance (49.6 Mly), magnitude 9.86, asymmetric one-armed spiral, VIRGOHI21 gas tail, and observing guide for M99.

Reference Guide

Bortle Dark-Sky Scale & Sky Brightness Guide

Reference guide to the 9-class Bortle Dark-Sky Scale, zenith Sky Quality Meter (SQM) readings in mag/arcsec², naked-eye limiting magnitude, and light pollution.

Scientific Sources & Dataset Provenance

  • Revised New General Catalogue and Index Catalogue (RNGC/IC) (2024/2026 edition): Steinicke, W. 2010, Observing and Cataloguing Nebulae and Star Clusters (Cambridge Univ. Press); Verga, M. OpenNGC (CC-BY-SA 4.0 / data tables) — Wolfgang Steinicke / OpenNGC
  • 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)
  • 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