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M 70

Globular Cluster M70 (NGC 6681), class V, in Sagittarius

Right Ascension 18 : 43.2 (h:m)
Declination -32 : 18 (deg:m)
Distance 29.4 (kly)
Visual Brightness 7.9 (mag)
Apparent Dimension 7.8 (arc min)

Discovered 1780 by Charles Messier.

Appearing approximately as bright and big as its neighbor M69, globular star cluster M70 is indeed only a little more luminous and little bigger, and a bit more remote (29,400 light years). Both are quite close to the galactic center, so they are both subject to quite strong tidal gravitational forces. As it is also at about the same southern declination, it is a difficult object from Paris where Messier observed it.

M70 is 7.8 arc minutes in apparent angular and roughly 65 light years in linear diameter, its bright visual core being only about 4'. It is rapidly receding from us, at about 200 km/sec. Only 2 variables are known in this stellar swarm.

The core of M70 is of extreme density, as it has undercone a core collapse somewhen in its history, similar to at least 21 and perhaps up to 29 of the 147 known Milky Way globulars, including M15, M30, and possibly M62.

Globular cluster M70 became famous in 1995 when the great comet Hale-Bopp was discovered near it by Alan Hale and Thomas Bopp as they were observing this globular.

  • Historical Observations and Descriptions of M70
  • More images of M70
  • Amateur images of M70

  • SIMBAD Data of M70
  • NED Data of M70
  • Observing Reports for M70 (IAAC Netastrocatalog)

    Hartmut Frommert (spider@seds.org)
    Christine Kronberg (smil@lrz.uni-muenchen.de)

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    Last Modification: 9 Dec 1999, 22:58 MET