Skip to content
AsteriaStar
Nebula · Dorado

NGC 2014

Deep skyNGC 2014

Scientific overview

NGC 2014 is a nebula in the constellation Dorado. It shines at apparent magnitude 8.97 and spans about 5.1 arcminutes of sky.

Observation guide

Difficulty
Small telescope
Recommended equipment
≈ 80–100 mm telescope
Best observed
Winter (S. evening sky)
Best hemisphere
Southern

Guidance follows standard observing practice, derived from the object's real magnitude and position. A dark, moonless sky always helps.

Location in the sky

Constellation
Dorado
RA / Dec
5.5389h / -67.6898°
Hemisphere
Southern
Season
Winter

Precision measurements

Distances and velocities from SIMBAD · NGC 2014

Right ascension (ICRS)83.1 degSIMBAD · measured
Declination (ICRS)-67.688333 degSIMBAD · measured
Full field-level provenance
  • Right ascension (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · ra · 1999AJ....117..238B · direct catalogue measurement · retrieved 2026-07-11
  • Declination (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · dec · 1999AJ....117..238B · direct catalogue measurement · retrieved 2026-07-11

Physical size is derived from the OpenNGC angular size and the catalogued distance (small-angle: size = angle × distance). This is a Galactic object: its Doppler shift is shown as a radial velocity, not a cosmological redshift. Fields a source did not provide are omitted, never invented.

ObjectTypeMagSize (′)
30 Dor ClusterC 103 · NGC 2070H II region7.2516
NGC 2074NGC 2074Cluster with nebulosity8.54
NGC 1955NGC 1955H II region8.874
NGC 1850NGC 1850Globular cluster8.963
NGC 1553NGC 1553Lenticular galaxy9.316.25
NGC 1747NGC 1747Open cluster9.374.4
NGC 1763NGC 1763Cluster with nebulosity9.45.2
NGC 2042NGC 2042Open cluster9.584.5

Sources

The primary and reference sources this topic draws on.

  • OpenNGCOpenNGC (M. Verga) — NGC/IC, Messier, and Caldwell catalogue data

    Openly-licensed deep-sky catalogue: object types, positions, magnitudes, sizes, morphology, and cross-identifiers.