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AsteriaStar
Supernova remnant · Taurus

Crab Nebula

M 1

Deep skyM 1NGC 1952

Scientific overview

Crab Nebula is a supernova remnant in the constellation Taurus. It shines at apparent magnitude 8.4 and spans about 8 arcminutes of sky.

Observation guide

Difficulty
Small telescope
Recommended equipment
≈ 80–100 mm 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
Taurus
RA / Dec
5.5755h / 22.0145°
Hemisphere
Northern
Season
Winter

Precision measurements

Distances and velocities from SIMBAD · M 1

Distance6,523 lySIMBAD · catalogued
Physical size (major axis)15.180007 lySIMBAD · derived
Physical size (minor axis)7.590004 lySIMBAD · derived
Right ascension (ICRS)83.6324 degSIMBAD · measured
Declination (ICRS)22.0174 degSIMBAD · measured
Full field-level provenance
  • Distance: Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · mesDistance · dist · 1973PASP...85..579T · catalogued value · source value 2 kpc · 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
  • Physical size (minor 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
  • Right ascension (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · ra · 2022A&A...661A..38P · direct catalogue measurement · retrieved 2026-07-11
  • Declination (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · dec · 2022A&A...661A..38P · 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 (′)
NGC 1746NGC 1746Open cluster6.118
NGC 1647NGC 1647Open cluster6.427
NGC 1807NGC 1807Open cluster75.4
NGC 1817NGC 1817Open cluster7.79.3
Hind's NebulaNGC 1555Reflection nebula9.981.82
Barnard's Merope NebulaReflection nebula25.7
Maia NebulaNGC 1432H II region60
Merope NebulaNGC 1435Nebula30

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.