
NGC 4605 - Wikipedia
NGC 4605 is a dwarf barred spiral galaxy [6] in the constellation Ursa Major, located at a distance of 18.1 ± 0.3 megalight-years from the Milky Way. [5] Physically it is similar in size and in B-band absolute magnitude to the Large Magellanic Cloud. [6] It is a possible member of either the M81 Galaxy Group or the Messier 101 Group. [9]
NGC 4605 - 维基百科,自由的百科全书
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NGC 4605 - Galaxy in Ursa Major | TheSkyLive.com
NGC 4605 is a Galaxy in the Ursa Major constellation. NGC 4605 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Given its B magnitude of 10.94, NGC 4605 is visible with the help of a telescope having an aperture of 6 inches (150mm) or more.
NGC 4605 - 维基百科,自由的百科全书 - zh.wikipedia.org
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NGC 4605 - 維基百科,自由的百科全書 - zh.wikipedia.org
維基百科 Discord 、 IRC 、 LINE 、 QQ 及 Telegram 等 各平臺交流群 歡迎大家加入。 NGC 4605 是位於 星座 大熊座 方向上的一個 螺旋星系。 ^ The scale of the Universe. ESA/Hubble …
NGC 4605 — Wikipédia
NGC 4605 est une petite galaxie spirale barrée rapprochée et située dans la constellation de la Grande Ourse. Sa vitesse par rapport au fond diffus cosmologique est de 259 ± 9 km/s, ce qui correspond à une distance de Hubble de 3,82 ± 0,30 Mpc (∼12,5 millions d' al) 1.
NGC 4605 - NASA Science
2023年11月3日 · The newly-formed stars in NGC 4605 are being used to investigate how interactions between galaxies affect the formation, evolution, and behavior of the stars within, how bright stellar nurseries come together to form stellar clusters and stellar associations, and how these stars evolve over time.
NGC 4605 Galaxy (UGC 7831) Facts & Distance - Universe Guide
NGC 4605 is a Spiral Galaxy located in the constellation of Ursa Major in the northern hemisphere. NGC 4605's distance from Earth is 15,922,954.36 light years. NGC 4605 is called NGC 4605 in the New General Catalogue (NGC).
NGC 4605 - 百度百科
NGC 4605是位于大熊座方向上的一个螺旋星系。 视星等10.9。
Hubble Eyes a Scale of the Universe - NASA Science
2023年11月3日 · The newly-formed stars in NGC 4605 are being used to investigate how interactions between galaxies affect the formation, evolution, and behavior of the stars within, how bright stellar nurseries come together to form stellar clusters and stellar associations, and how these stars evolve over time.
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