Spiral Galaxy · Canes Venatici

M106 NGC 4258

Magnitude
8.4
Season
Spring
Difficulty
Hard
Star-hop chart
M1060.0° field0° rotation
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Imaging reference
NGC 4258 (M106) Spiral Galaxy

Observer's guide

About NGC 4258

NGC 4258 (M106) is catalogued as a spiral galaxy in Canes Venatici. Its J2000 position is RA 12:18:57.50, Dec +47:18:14.3, corresponding to 184.7401 degrees RA and 47.3037 degrees Dec. The local catalogue places it about 25,000,000 light-years away. Its referenced angular extent is approximately 17.78 by 6.92 arcminutes.

Observing tips

StarWatchr rates this as a hard target at magnitude 8.4. It is associated with spring observing, with midnight placement typically strongest around March. From 52 degrees north its theoretical meridian altitude is about 85.3 degrees; local horizons and the live altitude chart determine the practical window.

A small telescope under reasonably dark skies is a good starting point; use the live altitude chart to choose its highest point.

What to expect

The SIMBAD classification for the matched source is Sy2. SIMBAD records the morphology as SAB. A published radial velocity value is 506.8 km/s. The SIMBAD record currently connects it to 2540 bibliographic references.

At roughly 17.8 arcminutes across, it benefits from a narrower field and adequate image scale. Use the listed 17.78 by 6.92 arcminute extent to check framing, and treat catalogue magnitude as integrated brightness rather than a direct measure of visual contrast.

Sourced catalogue data

Scientific record

Measurements for M106 are kept separate from practical observing guidance.

Coordinates (J2000/ICRS)
RA 184.740083° · Dec 47.303719°
SIMBAD classification
Sy2
Morphology
SAB
Angular extent
17.78′ × 6.92′
Surface brightness
22.25 mag/arcsec²
Radial velocity
506.8 km/s
Redshift
0.00169195
Linked bibliography
2,540 references
Best midnight placement
March
Observable latitude range
-42.7° to 90°

Source: SIMBAD astronomical database (CDS, Strasbourg) (ODbL; checked 2026-08-09). Catalogue values may change when new measurements are published.

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