Menu

M19

NGC 6273

Ammasso globulare Eccezionale (80/100)
M19 GlobularCluster Ophiuchus Visibile Livello 3 Medium telescope (6-8") - Higher magnification helpful
Mappa stellare Aggiungi alla lista Aggiungi al piano
Torna al catalogo

Proprietà

Magnitudine 6.8
Dimensione angolare 7.5′
Distanza 28700 ly
Globular Cluster [Distance: 28700 ly]

Posizione e identificatori

RA 17h 02m 37.7s
Dec -26° 16' 04.6"
Costellazione Ophiuchus
Catalogo M19

Visibilità

Imposta una località nelle impostazioni per vedere i dati di visibilità.

Immagine survey

Caricamento immagine survey…

Su M19

Descrizione

M19 is one of the most oblate (flattened) globular clusters known, located about 28,700 light-years from Earth in Ophiuchus. It lies very close to the galactic center — only about 6,500 light-years from it — and the Milky Way's tidal forces are likely responsible for its elongated shape. The cluster contains several hundred thousand stars.

Consigli per l'osservazione

Located about 8 degrees due east of Antares. Appears as a small, oval fuzzy patch in binoculars. A 4-inch telescope shows a bright, slightly elongated glow. Resolving stars requires 8 inches or more. Look carefully for the elongated shape — M19 is visibly non-circular even in moderate apertures. Best observed from June through August.

Storia

Discovered by Charles Messier on June 5, 1764. He described it as a 'nebula without stars.' William Herschel resolved it into stars and noted its elliptical shape. Modern studies confirm it is one of the most flattened globular clusters in the Milky Way.

Curiosità

M19's oblateness (ellipticity of about 0.3) is remarkable among globular clusters, which are typically quite round. Its proximity to the galactic center subjects it to intense tidal forces that distort its shape. The cluster is heavily reddened by interstellar dust, losing about 1.5 magnitudes of brightness.

Foto della comunità (1)

Credit: Doug Williams, REU Program / NOIRLAB / NSF / AURA. License: CC BY-SA 4.0. (Wikimedia Commons)

Credit: Doug Williams, REU Program / NOIRLAB / NSF / AURA. License: CC BY-SA 4.0. (Wikimedia Commons)

Skybred Feb 28, 2026