NGC 366

NGC 366
Podaci posmatranja
Epoha: J2000.0
SazviježđeKasiopeja[1]
Rektascenzija1sat. 6m 25,9s [2]
Deklinacija+62° 13' 44'' [2]
Tipotvoreno zvjezdano jato (II3p) [2]
Prividne dimenzijeNajveći prečnik: 4,00 u.m.
Ostale oznake
OCL 316[2][3]
Karta
Portal
Portal
Portal Astronomija

NGC 366 je otvoreno zvjezdano jato i nalazi se u sazviježđu Kasiopeja. Prvo otkriće je napravio John Frederick William Herschel 27. oktobra 1829. godine.[2][4][5]

Najbliži NGC/IC objekti

Sljedeći spisak sadrži deset najbližih NGC/IC objekata.[a]

Ime Udaljenost od NGC 366
(uglovnih minuta)[3][a] 		Rektascenzija (J2000)[3] Deklinacija (astronomija) (J2000)[3] Tip[3]
NGC 358 0,38 1sat. 5m 10,8s +62° 1' 16'' trostruka zvijezda (*3)
NGC 381 0,8 1sat. 8m 20,0s +61° 35' 0'' otvoreno zvjezdano jato (III2p)
IC 63 2,18 0sat. 59m 29,0s +60° 54' 40'' emisijska maglina (EN)
IC 59 2,49 0sat. 57m 28,5s +61° 8' 37'' emisijska maglina (EN)
NGC 433 3,03 1sat. 15m 9,2s +60° 7' 33'' otvoreno zvjezdano jato (III2p)
NGC 436 4,17 1sat. 15m 58,0s +58° 48' 42'' otvoreno zvjezdano jato (I3m)
NGC 457 5,12 1sat. 19m 33,0s +58° 17' 42'' otvoreno zvjezdano jato (I3r)
NGC 225 5,73 0sat. 43m 36,0s +61° 46' 0'' otvoreno zvjezdano jato (III1p)
NGC 559 5,87 1sat. 29m 31,0s +63° 18' 6'' otvoreno zvjezdano jato (II2m)
IC 11 6,55 0sat. 52m 53,8s +56° 37' 30'' emisijska maglina (EN)

Također pogledajte

Bilješke

Reference

  1. ^ (en) seds.org Arhivirano 6. 1. 2014. na Wayback Machine
  2. ^ a b c d e (en)(de) Entdeckung und Katalogisierung von Nebeln und Sternhaufen. "Wolfgang Steinicke-ov revizirani NGC i IC katalog". Arhivirano s originala, 18. 7. 2013. Pristupljeno 10. 4. 2013.
  3. ^ a b c d e (en) Rezultati za NGC 366. "NASA/IPAC Extragalactic Database".
  4. ^ Spisak posmatrača na Wolfgang Steinicke-om sajtu.
  5. ^ Young, C., Sid. Mess. II, 252 (1883-84).

Literatura

Vanjski linkovi

NGC 366

NGC katalog


Nedovršeni članak NGC 366 koji govori o svemiru treba dopuniti. Dopunite ga prema pravilima Wikipedije. Koordinate: Nebeska mapa 1h 6m 25.9s, +62° 13′ 44″

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