NGC 5986
| Kugelsternhaufen NGC 5986 | |
|---|---|
| Aufnahme des Hubble-Weltraumteleskops | |
| AladinLite | |
| Sternbild | Wolf |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 15h 46m 03,4s [1] |
| Deklination | −37° 47′ 10″ [1] |
| Erscheinungsbild | |
| Konzentrationsklasse | VII [2] |
| Helligkeit (visuell) | 7,6 mag [3] |
| Winkelausdehnung | 9,6' [3] |
| Physikalische Daten | |
| Rotverschiebung | (308 ± 20)e-6 [4] |
| Radialgeschwindigkeit | (92,3 ± 5,9) km/s [4] |
| Entfernung | 29,4 kLj |
| Masse | 330.000 M☉ |
| Gezeitenradius | 215 Lj |
| Alter | 12,2 Mrd. Jahre |
| Metallizität [Fe/H] | -1,54 |
| Geschichte | |
| Entdeckung | James Dunlop |
| Entdeckungsdatum | 10. Mai 1826 |
| Katalogbezeichnungen | |
| NGC 5986 • C 1542-376 • GCl 37 • ESO 329-018 • Dun 552 • GC 4132 • Bennett 70, h 3611 | |
NGC 5986 ist die Bezeichnung eines Kugelsternhaufens im Sternbild Wolf. NGC 5986 hat einen Durchmesser von 9,5' und eine scheinbare Helligkeit von 7,6 mag.
Das Objekt wurde am 10. Mai 1826 von James Dunlop entdeckt.[5]
Literatur
- König, Michael & Binnewies, Stefan: Bildatlas der Sternhaufen & Nebel. Stuttgart: Kosmos 2023, S. 368.
Einzelnachweise
- ↑ NASA/IPAC EXTRAGALACTIC DATABASE
- ↑ Harlow Shapley, Helen B. Sawyer: A Classification of Globular Clusters. In: Harvard College Observatory Bulletin. Band 849, 1927, S. 11–14, bibcode:1927BHarO.849...11S.
- ↑ a b SEDS: NGC 5986
- ↑ SIMBAD Query
- ↑ Seligman
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