Galaxies · Constellation 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.

Right Ascension (J2000.0)12h 50m 53.06s
Declination (J2000.0)+41° 07′ 13.6″
Primary ClassificationDouble-ringed SAB(r)ab starburst galaxy (M94 / Canes Venatici I Group anchor)
Best Observing SeasonSpring to Early Summer (March–July)

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 Cat's Eye Galaxy (Messier 94 / NGC 4736)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Integrated visual magnitude (V)8.24 mag± 0.06 magIntegrated CCD aperture photometrydefinitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Distance in light-years15000000 ly± 500000 lyHST Tip of the Red Giant Branch (TRGB: 4.61 ± 0.15 Mpc)definitiveSH0ES Local Distance Ladder Hubble Constant
Apparent major axis11.2 arcmin± 0.5 arcminOptical isophotal dimensions including outer ring (11.2′ × 9.1′)definitiveRevised New General Catalogue and Index Catalogue (RNGC/IC)
Heliocentric recession velocity308 km/s± 1 km/sTHINGS H I 21-cm synthesis velocity fielddefinitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Hubble Space Telescope TRGB star counts determine M94's distance to ±3.2% (4.61 ± 0.15 Mpc / 15.0 ± 0.5 Mly), making it the dominant central galaxy of the nearby Canes Venatici I Cloud.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Cat's Eye Galaxy (Messier 94 / NGC 4736) at RA 12h 50m 53.06s, Dec +41° 07′ 13.6″ within Canes Venatici, 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 (Canes Venatici) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 89° 40°N Lat 19° 30°S Lat RA: 12h 50m 53.06s Dec: +41° 07′ 13.6″ Epoch: J2000.0 · V = 8.24 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Discovered by Pierre Méchain on March 22, 1781, and cataloged by Charles Messier two days later, Messier 94 (NGC 4736, often called the Cat's Eye or Croc's Eye Galaxy) is the gravitational centerpiece of the nearby Canes Venatici I Cloud just 15.0 million light-years from Earth. Viewed nearly face-on, M94 is famous for its concentric double-ring architecture spanning roughly 50,000 light-years across its outer pseudoring.

Surrounding M94's intense LINER nucleus is a dazzling inner starburst ring roughly 70 arcseconds (~5,000 light-years) in diameter, where an oval distortion in the central stellar bulge acts like a cosmic paddle, driving an outward-propagating resonance wave that compresses gas into a continuous necklace of young blue star clusters and H II regions. Multi-wavelength ultraviolet (GALEX) and infrared (Spitzer) imaging further showed that the faint 11-arcminute outer ring is not a closed tidal loop, but a pair of tightly wound, star-forming spiral arms containing ~10% of the galaxy's young stellar mass.

In 2008 deep H I 21-centimeter rotation curves of M94 sparked intense astrophysical debate when researchers noted that its outer gas rotation speed drops off faster than in typical spiral galaxies, suggesting either a strongly warped outer gas disk or an unusually low-concentration dark-matter halo.

Practical Visual Observing Guide

Minimum Instrument7×50 or 10×50 binoculars; 60 mm telescope
Recommended Magnification80×–180×
Best Evening SeasonSpring to Early Summer (March–July)
  • Forms the northern vertex of a flat isosceles triangle about 2.8° northwest of the line connecting Cor Caroli (α CVn) and Chara (β CVn).
  • Because its inner 1′ starburst ring and core have one of the highest surface brightnesses of any Messier galaxy, M94 is easily visible in 7×50 binoculars and looks almost like a bright globular cluster in small refractors.
  • In a 150–250 mm telescope at 120×–180×, the blazing central core is surrounded by a distinct, sharp-edged 2′ inner ring fading into a ghostly outer halo.

Catalog Cross-Identifications & Aliases

Common Aliases: M94 · NGC 4736 · UGC 7996 · Croc's Eye Galaxy

Cross-Catalog Identifiers for Cat's Eye Galaxy (Messier 94 / NGC 4736)
Catalog AuthorityIdentifier
MESSIERM 94
NGCNGC 4736
SIMBADM 94
WIKIDATAQ14058
Related Object · Canes Venatici

Sunflower Galaxy (Messier 63 / NGC 5055)

J2000 coordinates, TRGB distance (29.3 Mly), magnitude 8.59, flocculent spiral arms, warped H I disk, and observing guide for Messier 63 (NGC 5055).

Related Object · Canes Venatici

Messier 106 (NGC 4258 Megamaser Anchor)

J2000 coordinates, geometric maser distance (24.7 Mly), magnitude 8.41, anomalous synchrotron arms, Seyfert 2 core, and observing guide for M106.

Related Object · Coma Berenices

Black Eye Galaxy (Messier 64 / NGC 4826)

J2000 coordinates, TRGB distance (17.3 Mly), magnitude 8.52, dark absorbing dust hood, counter-rotating gas disk, and observing guide for Messier 64.

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

  • 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