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AsteriaStar
Open cluster · Triangulum Australe

NGC 6025

Deep skyC 95NGC 6025

Scientific overview

NGC 6025 is an open cluster in the constellation Triangulum Australe. It shines at apparent magnitude 5.1 and spans about 11.4 arcminutes of sky.

Observation guide

Difficulty
Binoculars
Recommended equipment
10×50 binoculars or any small telescope
Best observed
Summer (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
Triangulum Australe
RA / Dec
16.0549h / -60.4314°
Hemisphere
Southern
Season
Summer

Precision measurements

Distances and velocities from SIMBAD · NGC 6025

Distance2,446 lySIMBAD · catalogued
Physical size (major axis)8.111816 lySIMBAD · derived
Radial velocity8.468 ± 0.619 km/sSIMBAD · measured
Right ascension (ICRS)240.779167 degSIMBAD · measured
Declination (ICRS)-60.43 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 750 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.

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.