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Palomar 5

Globular cluster in the constellation Serpens


Globular cluster in the constellation Serpens

FieldValue
namePalomar 5
imagePal5_-_SDSS_DR14_(panorama).jpg
epochJ2000
classXII
constellationSerpens
ra{{cite web
titleSIMBAD Astronomical Database
workResults for Palomar 5
urlhttp://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Palomar+5&submit=SIMBAD+search
access-date2006-11-17}}
dec
dist_ly76 kly
appmag_v+11.75
size_v6.9
radius_ly76 ly
mass_msol
ageGyr{{cite journal
authorMartell, S. L.
author2Smith, G. H.
author3Grillmair, C. J.
titleA New Age Measurement for Palomar 5
journalAmerican Astronomical Society, 201st AAS Meeting, #07.11; Bulletin of the American Astronomical Society
volume34
date2002
pages1103
bibcode2002AAS...201.0711M
notesErroneously thought to be a dwarf galaxy
namesUGC 9792, GCl 32

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

Palomar 5 is a globular cluster in the constellation Serpens and a member of the Palomar Globular Clusters group. It was discovered by Walter Baade in 1950, and independently found again by Albert George Wilson in 1955. After the initial name of Serpens, it was subsequently catalogued as Palomar 5.

There is a process of disruption acting on this cluster because of the gravitation of the Milky Way – in fact there are many stars leaving this cluster in the form of a stellar stream. The stream has a mass of 5000 solar masses and is 30,000 light years long. The cluster is currently 60.6 kly from the Galactic Center. It shows a noticeable amount of flattening, with an aspect ratio of 0.62 ± 0.23 between its semimajor axis and semiminor axis.

References

References

  1. distance × sin( diameter_angle / 2 ) = 76 ly. radius
  2. Ibata, Rodrigo. (April 2007). "The Ghosts of Galaxies Past". Scientific American.
  3. (November 2007). "A 1.4 GHz Arecibo Survey for Pulsars in Globular Clusters". The Astrophysical Journal.
  4. (October 2010). "Morphological Distortion of Galactic Globular Clusters". The Astrophysical Journal.
  5. (November 2011). "Young Radio Pulsars in Galactic Globular Clusters". The Astrophysical Journal.
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