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AsteriaStar
Open cluster · Perseus

NGC 1582

Deep skyNGC 1582

Scientific overview

NGC 1582 is an open cluster in the constellation Perseus. It shines at apparent magnitude 7 and spans about 7.8 arcminutes of sky.

Observation guide

Difficulty
Binoculars
Recommended equipment
10×50 binoculars or any small telescope
Best observed
Winter (N. evening sky)
Best hemisphere
Northern

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
Perseus
RA / Dec
4.5297h / 43.7848°
Hemisphere
Northern
Season
Winter

Precision measurements

Distances and velocities from SIMBAD · NGC 1582

Distance3,242 lySIMBAD · catalogued
Physical size (major axis)7.355852 lySIMBAD · derived
Radial velocity-21.45 ± 0.521 km/sSIMBAD · measured
Right ascension (ICRS)67.985 degSIMBAD · measured
Declination (ICRS)43.718056 degSIMBAD · measured
Full field-level provenance
  • Distance: Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · mesDistance · dist · 2021A&A...651A.104P · distance indicator: paral · catalogued value · source value 994 pc · retrieved 2026-07-11
  • Physical size (major axis): Centre de données astronomiques de Strasbourg (CDS) · derived (OpenNGC angular size × SIMBAD distance) · physical size = angular size × distance (small-angle); angular size from OpenNGC, distance from SIMBAD mesDistance · derived · retrieved 2026-07-11
  • Radial velocity: Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · rvz_radvel · 2023A&A...674A..37G · direct catalogue measurement · retrieved 2026-07-11
  • Right ascension (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · ra · 2021A&A...647A..19T · direct catalogue measurement · retrieved 2026-07-11
  • Declination (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · dec · 2021A&A...647A..19T · 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 (′)
h Persei ClusterNGC 869Open cluster3.714.4
chi Persei ClusterNGC 884Open cluster3.810.5
California NebulaNGC 1499Nebula5160
M 34M 34 · NGC 1039Open cluster5.222.5
NGC 1545NGC 1545Open cluster6.24.2
NGC 1528NGC 1528Open cluster6.49.6
NGC 1444NGC 1444Open cluster6.63.6
NGC 1342NGC 1342Open cluster6.76.3

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.