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Globular cluster · Aquila

NGC 6760

Deep skyNGC 6760

Scientific overview

NGC 6760 is a globular cluster in the constellation Aquila. It shines at apparent magnitude 9.78 and spans about 5.4 arcminutes of sky.

Observation guide

Difficulty
Medium telescope
Recommended equipment
≈ 150–200 mm telescope
Best observed
Summer (evening sky)
Best hemisphere
Both (equatorial)

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
Aquila
RA / Dec
19.1867h / 1.0305°
Hemisphere
Both
Season
Summer

Precision measurements

Distances and velocities from SIMBAD · NGC 6760

Radial velocity-1.6 ± 1.7 km/sSIMBAD · measured
Right ascension (ICRS)287.80025 degSIMBAD · measured
Declination (ICRS)1.030472 degSIMBAD · measured
Full field-level provenance
  • Radial velocity: Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · rvz_radvel · 2018MNRAS.478.1520B · direct catalogue measurement · retrieved 2026-07-11
  • Right ascension (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · ra · 2006MNRAS.365.1357D · direct catalogue measurement · retrieved 2026-07-11
  • Declination (ICRS): Centre de données astronomiques de Strasbourg (CDS) · SIMBAD · basic · dec · 2006MNRAS.365.1357D · 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 6709NGC 6709Open cluster6.78.7
NGC 6755NGC 6755Open cluster7.56
Phantom Streak NebulaNGC 6741Planetary nebula11.50.13

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.