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Messier 106

Date vum Messier 106
Iwwerlagerung vun enger Foto (giel) mat Biller aus dem Radio- (violett), IR- (rout) a Röntgenberäich (blo).(Spitzer-Foto)
Stärebild Canes Venatici (CVn)
Positioun (Equinoxe: J2000.0)
Rektaszensioun 12h 18m 57.54s
Deklinatioun + 47° 18' 14.3"[1]
Ausgesinn
Hubble SAB(s)bc;LINER Sy1.9[1]
magV +8,3 mag[2]
magB +9,1 mag[2]
Flächenhellegkeet +13,5 mag[2]
Wénkelduerchmiesser 17.0x6.5[1]
Gehéiert zu Ursa-Major-Grupp
Coma-Sculptor-Grupp
Canes-Venatici-II-Grupp oder
Canes-Venatici-I-Grupp
Physikalesch Daten
Distanz 24 Millioune Lj
Routverrécklung (1494 ± 10)  10−6[1]
Heliozentresch radial relativ Vitess +462 ± 27
Mass ?
Geschicht
Entdecker Pierre Méchain
Entdeckungsjoer 1781
Katalogbezeechnungen
Messier 106, NGC 4258, UGC 7353, PGC 39600, MCG +8-22-104, VV 448, ZWG 244.3, ZWG 243.67, VV 448, h 1175, H 5.43, GC 2841

De Messier 106 (oder NGC 4258) ass eng Spiralgalaxie mat enger Gréisst vu 17.4' × 6.6' an enger visueller Magnitude vu +8.40m ag am Stärebild Canes Venatici.

Den M106 ass eng Galaxie, deen an der Hubble-Sequenz dem Typ Sbp zougewise gëtt, woubäi de p fir engl.: peculiar, d. h. kurious steet. Verschidden Auteure ginn den Typ och mat SABbc un, also tëscht normaler Spiral a Balke-Spiral. Mat enger Distanz vu ronn 24 Millioune Liichtjoer läit d'Galaxie an der Géigend vu ville Galaxiëgruppen.

De Kär vun der Galaxie ass aktiv an als Radioquell zanter den 1950er Jore bekannt.

Kaart vum Stärebild Canes Venatici (Juegdhënn)

Portal Astronomie

Commons: Messier 106 – Biller, Videoen oder Audiodateien

Referenzen

[Quelltext änneren]
  1. 1,0 1,1 1,2 1,3 SIMBAD
  2. 2,0 2,1 2,2 Students for the Exploration and Development of Space
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Messier 106
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