
NGC 420 - 维基百科,自由的百科全书 - zh.wikipedia.org
是 双鱼座 的一个 星系。
NGC 420 - 维基百科,自由的百科全书
NGC 420 是 雙魚座 的一個 星系。
NGC 420 - Wikipedia
NGC 420 is a lenticular galaxy of type S0 located in the constellation Pisces. It was discovered on September 12, 1784 by William Herschel . It was described by Dreyer as "faint, pretty small, round, brighter middle."
NGC 420 - Lenticular Galaxy in Pisces | TheSkyLive.com
NGC 420 is a Lenticular Galaxy in the Pisces constellation. NGC 420 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 13.4, NGC 420 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.
NGC 420 - Wikiwand
NGC 420 is a lenticular galaxy of type S0 located in the constellation Pisces. It was discovered on September 12, 1784 by William Herschel. It was described by ...
NGC 420 - Wikipedia, entziklopedia askea.
NGC 420 galaxia bat da, Pisces konstelazioan [1]. William Herschelek aurkitu zuen 1784ko irailaren 12an [2].
NGC 420 — Wikipédia
NGC 420 est une galaxie lenticulaire située dans la constellation des Poissons. Sa vitesse par rapport au fond diffus cosmologique est de 4 716 ± 23 km/s, ce qui correspond à une distance de Hubble de 69,6 ± 4,9 Mpc (∼227 millions d'al) [1]. NGC 420 a été découverte par l'astronome germano-britannique William Herschel en 1784.
NGC 420 Galaxy Facts (UGC 752) & Distance - Dungeon Guide
NGC 420 is a Spiral Galaxy located in the constellation of Pisces in the equatorial region. NGC 420's distance from Earth is 207,869,244.20 light years. NGC 420 is called NGC 420 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.
Category : NGC 420 - Wikimedia
Media in category "NGC 420" The following 5 files are in this category, out of 5 total.
NGC 420 – Wikipedia
NGC 420 ist eine Linsenförmige Galaxie vom Hubble-Typ S0 im Sternbild Fische auf der Ekliptik. Sie ist schätzungsweise 231 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 130.000 Lichtjahren.