Galaxy · Sculptor

C70 NGC 300

Magnitude
8.1
Season
Autumn
Difficulty
Hard
Star-hop chart
C700.0° field0° rotation
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Imaging reference
NGC 300 (C70) Galaxy

Observer's guide

About NGC 300

NGC 300 (C70) is catalogued as a galaxy in Sculptor. Its J2000 position is RA 00:54:53, Dec -37:41:04, corresponding to 13.7227 degrees RA and -37.6842 degrees Dec. The local catalogue places it about 3,900,000 light-years away. Its referenced angular extent is approximately 20.89 by 13.49 arcminutes.

Observing tips

StarWatchr rates this as a hard target at magnitude 8.1. It is associated with autumn observing, with midnight placement typically strongest around September. From 52 degrees north its theoretical meridian altitude is about 0.3 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 GiG. SIMBAD records the morphology as Sc. A published radial velocity value is 146 km/s. The SIMBAD record currently connects it to 1628 bibliographic references.

Its roughly 20.9 arcminute span suits a medium field of view. Use the listed 20.89 by 13.49 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 C70 are kept separate from practical observing guidance.

Coordinates (J2000/ICRS)
RA 13.722694° · Dec -37.684213°
SIMBAD classification
GiG
Morphology
Sc
Angular extent
20.89′ × 13.49′
Position angle
114°
Surface brightness
22.85 mag/arcsec²
Radial velocity
146 km/s
Redshift
0.00048712
Linked bibliography
1,628 references
Best midnight placement
September
Observable latitude range
-90° to 52.3°

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

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24-hour altitude profile

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