Globular Cluster Messier 80

Messier 80
Messier 80: Image taken with the Hubble Space Telescope. © ESA/Hubble & NASA [215]


The globular cluster M 80 was discovered by Charles Messier on 4 January 1781. He wrote: «Nebula without a star, in Scorpio between the stars ρ and δ, compared to ρ for determining the position: The nebula is round, the center brilliant, looks like the core of a comet wrapped in nebula. M. Méchain saw it on 28 January 1781.» [281]

Physical Properties

About 28'000 light years away is M 80, one of the densest of the 150 known globular clusters in our Milky Way. This globular cluster contains several hundred thousand stars, which are held together by their mutual attraction. In 1860 a nova occurred in this globular cluster. Novas can arise when a nearby companion star transfers fresh hydrogen to a burned-out white dwarf. This can lead to a thermonuclear explosion on the surface of the white dwarf and a brief increase in brightness. A large number of blue stragglers were also found in the cluster, stars that are unusually young for globular clusters. [215]

Revised+Historic NGC/IC Version 22/9, © 2022 Dr. Wolfgang Steinicke [277]
Designation NGC 6093
Type GCL (II)
Right Ascension (J2000.0) 16h 17m 02.5s
Declination (J2000.0) -22° 58' 28"
Diameter 10 arcmin
Visual magnitude 7.3 mag
Metric Distance 10.000 kpc
Dreyer Description !! globular, vB, L, vmbM (var *), rrr, st 14
Identification, Remarks h 3624; GC 4173; M 80; GCL 39; ESO 516-SC11

Finder Chart

M 80 is located in the constellation Scorpius between the stars ρ Ophiuchi and δ Scorpii. It can best be observed in the months of April to August.

Finder Chart Globular Cluster Messier 80
Globular Cluster Messier 80 in constellation Scorpius. Charts created using SkySafari 6 Pro and STScI Digitized Sky Survey. Limiting magnitudes: Constellation chart ~6.5 mag, DSS2 close-ups ~20 mag. [149, 160]

Objects Within a Radius of 15°