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Messier 70

Globular cluster in the constellation Sagittarius


Globular cluster in the constellation Sagittarius

FieldValue
nameMessier 70
image[[Image:Messier70-HST-Potw1215a.jpg300px]]
captionGlobular cluster Messier 70 by Hubble Space Telescope; 3.3 view
epochJ2000
classV
constellationSagittarius
ra
dec
dist_ly29.4 kly
appmag_v7.9
size_v
mass_msol
radius_ly34 ly
radius_tidal_arcminsec
metal_fe–1.35
age12.80 Gyr
namesGCl 101, M70, NGC 6681

Messier 70 or M70, also known as NGC 6681, is a globular cluster of stars to be found in the south of Sagittarius. It was discovered by Charles Messier in 1780. The famous comet Hale–Bopp was discovered near this cluster in 1995.

It is about 29,400 light years away from Earth and around 2 kpc from the Galactic Center. It is roughly the same size and luminosity as its neighbour in space, M69. M70 has a very small core radius of 0.068 pc and a half-light radius of 55.80 pc. This cluster has undergone core collapse, leaving it centrally concentrated with the luminosity distribution following a power law.

There are two distinct stellar populations in the cluster, with each displaying unique abundances. These likely represent different generations of stars. Five known variable stars lie within its broadest radius, the tidal radius, all of which are RR Lyrae variables. The cluster may have two blue stragglers near the core.

References and footnotes

| access-date=2018-12-04 | postscript=. }}

| editor1-first=S. G. | editor1-last=Djorgovski | editor2-first=G. | editor2-last=Meylan

| display-authors=1 | postscript=.

| display-authors=1 | postscript=.

| display-authors=1

| display-authors=1 | journal=The Astronomical Journal

| access-date=2006-11-17 }}

| display-authors=1 | journal=The Astrophysical Journal

References

  1. "Messier 70".
  2. distance × sin( diameter_angle / 2 ) = 34 ly. radius
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