Sombrero Galaxy vs Whirlpool Galaxy

Similar magnitudes, different propositions. The Sombrero (M104, NGC 4594) records 8.59 and the Whirlpool (M51, NGC 5194) 8.36, a difference too small to matter at the eyepiece. Extent is what separates them: M51 spreads across 13.71 arcminutes against 8.45 for M104, so the Sombrero concentrates its light to about 13.0 magnitudes per square arcminute where the Whirlpool falls to 13.8. The edge-on Sombrero consequently holds together under mediocre skies as a bright spindle bisected by its dust lane, while M51's face-on spiral arms demand darkness and aperture before they emerge from the background.

Property comparison

Property Sombrero Galaxy Whirlpool Galaxy
Object type Galaxy Galaxy
Catalogue designation NGC 4594 NGC 5194
Integrated magnitude 8.59 8.36
Apparent size 8.4′ (8.45′) 14′ (13.71′)
Mean surface brightness 13.0 mag/arcmin² 13.8 mag/arcmin²
Position (J2000) RA 12h, Dec -11° RA 13h, Dec +47°
Sky region Southern sky Far northern sky

Mean surface brightness is derived from the integrated magnitude and the apparent diameter; higher values mean a fainter, more diffuse surface.

Full data for each object: Sombrero Galaxy · Whirlpool Galaxy

Key differences

Key Differences

  • Magnitudes are close: 8.36 for M51 against 8.59 for M104.
  • M51 spans 13.71 arcminutes against 8.45 for M104, about 1.6 times wider.
  • M104 has the higher surface brightness, near 13.0 magnitudes per square arcminute against 13.8.
  • M104 lies at declination −11°, M51 at +47° — nearly 60 degrees apart in the sky.
  • M104 presents edge-on with a dust lane; M51 presents face-on with its companion NGC 5195.

Frequently asked questions

Frequently Asked Questions

Which galaxy shows more detail in a small telescope?
M104. Its higher surface brightness near 13.0 magnitudes per square arcminute keeps the dust lane visible in apertures around 150 mm, while the spiral structure of M51 typically needs 200 mm and a dark sky.
Are they visible at the same time of year?
Both are spring objects, but their declinations differ sharply — M51 at +47° passes near the zenith for northern observers while M104 at −11° stays low in the south.
Which is brighter?
M51, marginally, at magnitude 8.36 against 8.59. The 0.23-magnitude gap is far less important than the difference in how widely each spreads that light.
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