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NGC 5897

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Globular cluster in the constellation Libra
NGC 5897
The globular cluster NGC 5897 imaged with an amateur telescope.
Observation data (J2000 epoch)
ClassXI
ConstellationLibra
Right ascension15 17 24.40
Declination−21° 00′ 36.4″
Distance24.1 kly
(7.4 kpc)
Apparent magnitude (V)8.52
Physical characteristics
Radius6.3' x 6.3'
Metallicity [ Fe / H ] {\displaystyle {\begin{smallmatrix}\left\end{smallmatrix}}}  = -2.04±0.15 dex
Other designationsGCl 33, C 1514-208
See also: Globular cluster, List of globular clusters

NGC 5897 is a globular cluster in the constellation Libra. This satellite of the Milky Way, which is quite remote (located about 41,000 light years away), has a diameter of over 170 light years. With its Shapley–Sawyer Concentration Class of XI, it has very low star density even in its center.

The stars of the cluster have only 0.91% of the Sun's metallicity, while the abundance of elements produced by the alpha process is roughly 5 times larger. This means that the cluster formed in a time before the galaxy formed a disk and spiral arms. However, some of the stars are apparently younger, indicating multiple star-forming epochs.

NGC 5897 has a diameter of 12.6 arcminutes and an apparent magnitude of 8.5.

References

  1. Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin, 849 (849): 11–14, Bibcode:1927BHarO.849...11S.
  2. ^ "NGC 5897". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 January 2017.
  3. ^ "NGC 5897". Retrieved 7 January 2016.
  4. ^ Koch, Andreas; McWilliam, Andrew (2014), "The chemical composition of a regular halo globular cluster: NGC 5897", Astronomy & Astrophysics, 565: A23, arXiv:1403.1262, doi:10.1051/0004-6361/201323119, S2CID 53958921
  5. "A Galactic Globular Clusters Database: NGC 5897". Retrieved 8 January 2017.

External links

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Constellation of Libra
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